Sample records for paper-ice composite insulating

  1. Mechanical Characteristics of Resin-Coated Papers and their Electrical Breakdown Characteristics in Composite Insulation Systems with Insulation Oil

    NASA Astrophysics Data System (ADS)

    Kurihara, Takashi; Takahashi, Toshihiro; Mizutani, Yoshinobu; Suzuki, Hiroshi; Okamoto, Tatsuki; Ogura, Nobuyuki; Iwamoto, Kazuyoshi; Kitagawa, Setsuo

    Three types of resin-coated papers were investigated; kraft papers and heat-resistant kraft papers partially covered with epoxy resin, and a kraft paper covered with phenol resin; those were laminated to certain thickness. They were thermally degraded at 120°C for 240 to 1320 hours, and their mechanical characteristics such as tensile strength and average polymerization degree were measured. As a result, it was found that the tensile strength of the first and second resin-coated papers was larger than that of the pressboard, but the tensile strength of the third one was smaller. As the effect of the heating time, it was found that the tensile strength of the first resin-coated paper decreased down to that of pressboards after 500 hours of heating time while those of the second and third ones almost retained the initial values after 1320 hours of the heating time. Then, electrical breakdown characteristics of composite insulation systems with a resin-coated paper and insulation oil were investigated. In the system, an oil-filled gap was artificially introduced between a resin-coated paper and a plane electrode to induce partial discharges (PDs) at the same location. PDs occurred before breakdowns and it was found that their PD inception electric field strength was almost as high as that of the pressboard and the effect of the heating time was negligible. It was also found that the electrical breakdown field strength has similar characteristics to those of the PD inception field strength; negligible effects of the type of resin-coated papers and the heating time. Electrical breakdown occurred at the oil-filled gap and the edge of a high voltage electrode.

  2. 2. Ice Plant interior, east section, looking north. Insulated walls ...

    Library of Congress Historic Buildings Survey, Historic Engineering Record, Historic Landscapes Survey

    2. Ice Plant interior, east section, looking north. Insulated walls and ceiling are sheathed in fir. Note condenser coils on ceiling. - Curtis Wharf, Ice Plant, O & Second Streets, Anacortes, Skagit County, WA

  3. Natural ageing of EPDM composite insulators

    DOE Office of Scientific and Technical Information (OSTI.GOV)

    Vlastos, A.E.; Sherif, E.

    1990-01-01

    Long-rod composite insulators, with weather sheds (sheds) made of ethylene propylene rubbers (EPDM), were exposed for many years to HVAC and HVDC under realistic conditions and natural pollution. The change of their properties with time and their aging was studied. The results show that the insulator shed material undergoes a slow degradation process and loses successively its water repelling properties which initially make the EPDM composite insulators superior to inorganic glass and porcelain insulator. The outdoor degradation of the shed material depends on the electric stress, in the environmental factors (such as pollution, rain, salt-laden fog, and UV-radiation from sun)more » and on the materials and fillers used in the construction of the composite insulators. A thorough macro- and microscopic study of the EPDM composite insulator sheds illustrates the differences of the surface state of EPDM insulators of different makes in which different basic material compositions and fillers are used. The poor performance of aged EPDM composite insulators compared to inorganic insulators depends on the design and on environmental factors.« less

  4. Preparation and properties of the multi-layer aerogel thermal insulation composites

    NASA Astrophysics Data System (ADS)

    Wang, Miao; Feng, Junzong; Jiang, Yonggang; Zhang, Zhongming; Feng, Jian

    2018-03-01

    Multi-layer insulation materials possess low radiation thermal conductivity, and excellent thermal insulation property in a vacuum environment. However, the spacers of the traditional multi-layer insulation materials are mostly loose fibers, which lead to more sensitive to the vacuum environmental of serviced. With the vacuum degree declining, gas phases thermal convection increase obviously, and the reflective screen will be severe oxidation, all of these make the thermal insulation property of traditional multi-layer insulation deteriorate, thus limits its application scope. In this paper, traditional multi-layer insulation material is combined with aerogel and obtain a new multi-layer aerogel thermal insulation composite, and the effects of the number, thickness and type of the reflective screens on the thermal insulation properties of the multi-layer composites are also studied. The result is that the thermal insulation property of the new type multi-layer aerogel composites is better than the pure aerogel composites and the traditional multi-layer insulation composites. When the 0.01 mm stainless steel foil as the reflective screen, and the aluminum silicate fiber and silica aerogel as the spacer layer, the layer density of composite with the best thermal insulation property is one layer per millimeter at 1000 °C.

  5. Composite Flexible Blanket Insulation

    NASA Technical Reports Server (NTRS)

    Kourtides, Demetrius A. (Inventor); Pitts, William C. (Inventor); Goldstein, Howard E. (Inventor); Sawko, Paul M. (Inventor)

    1991-01-01

    Composite flexible multilayer insulation systems (MLI) were evaluated for thermal performance and compared with the currently used fibrous silica (baseline) insulation system. The systems described are multilayer insulations consisting of alternating layers of metal foil and scrim ceramic cloth or vacuum metallized polymeric films quilted together using ceramic thread. A silicon carbide thread for use in the quilting and the method of making it are also described. These systems are useful in providing lightweight insulation for a variety of uses, particularly on the surface of aerospace vehicles subject to very high temperatures during flight.

  6. Development of High Performance Composite Foam Insulation with Vacuum Insulation Cores

    DOE Office of Scientific and Technical Information (OSTI.GOV)

    Biswas, Kaushik; Desjarlais, Andre Omer; SmithPhD, Douglas

    Development of a high performance thermal insulation (thermal resistance or R-value per inch of R-12 hr-ft2- F/Btu-in or greater), with twice the thermal resistance of state-of-the-art commercial insulation materials ( R6/inch for foam insulation), promises a transformational impact in the area of building insulation. In 2010, in the US, the building envelope-related primary energy consumption was 15.6 quads, of which 5.75 quads were due to opaque wall and roof sections; the total US consumption (building, industrial and transportation) was 98 quads. In other words, the wall and roof contribution was almost 6% of the entire US primary energy consumption. Buildingmore » energy modeling analyses have shown that adding insulation to increase the R-value of the external walls of residential buildings by R10-20 (hr-ft2- F/Btu) can yield savings of 38-50% in wall-generated heating and cooling loads. Adding R20 will require substantial thicknesses of current commercial insulation materials, often requiring significant (and sometimes cost-prohibitive) alterations to existing buildings. This article describes the development of a next-generation composite insulation with a target thermal resistance of R25 for a 2 inch thick board (R12/inch or higher). The composite insulation will contain vacuum insulation cores, which are nominally R35-40/inch, encapsulated in polyisocyanurate foam. A recently-developed variant of vacuum insulation, called modified atmosphere insulation (MAI), was used in this research. Some background information on the thermal performance and distinguishing features of MAI has been provided. Technical details of the composite insulation development and manufacturing as well as laboratory evaluation of prototype insulation boards are presented.« less

  7. Composite flexible insulation for thermal protection of space vehicles

    NASA Technical Reports Server (NTRS)

    Kourtides, Demetrius A.; Tran, Huy K.; Chiu, S. Amanda

    1991-01-01

    A composite flexible blanket insulation (CFBI) system considered for use as a thermal protection system for space vehicles is described. This flexible composite insulation system consists of an outer layer of silicon carbide fabric, followed by alumina mat insulation, and alternating layers of aluminized polyimide film and aluminoborosilicate scrim fabric. A potential application of this composite insulation would be as a thermal protection system for the aerobrake of the aeroassist space transfer vehicle (ASTV). It would also apply to other space vehicles subject to high convective and radiative heating during atmospheric entry. The thermal performance of this composite insulation as exposed to a simulated atmospheric entry environment in a plasma arc test facility is described. Other thermophysical properties which affect the thermal response of this composite insulation is included. It shows that this composite insulation is effective as a thermal protection system at total heating rates up to 30.6 W/sq cm.

  8. Composite flexible insulation for thermal protection of space vehicles

    NASA Astrophysics Data System (ADS)

    Kourtides, Demetrius A.; Tran, Huy K.; Chiu, S. Amanda

    1992-09-01

    A composite flexible blanket insulation (CFBI) system considered for use as a thermal protection system for space vehicles is described. This flexible composite insulation system consists of an outer layer of silicon carbide fabric, followed by alumina mat insulation, and alternating layers of aluminized polyimide film and aluminoborosilicate scrim fabric. A potential application of this composite insulation would be as a thermal protection system for the aerobrake of the Aeroassist Space Transfer Vehicle (ASTV). It would also apply to other space vehicles subject to high convective and radiative heating during atmospheric entry. The thermal performance of this composite insulation as exposed to a simulated atmospheric entry environment in a plasma arc test facility is described. Other thermophysical properties which affect the thermal response of this system are also described. Analytical modeling describing the thermal performance of this composite insulation is included. It shows that this composite insulation is effective as a thermal protection system at total heating rates up to 30.6 W/sq cm.

  9. Thermal Performance of Composite Flexible Blanket Insulations for Hypersonic Aerospace Vehicles

    NASA Technical Reports Server (NTRS)

    Kourtides, Demetrius A.

    1993-01-01

    This paper describes the thermal performance of a Composite Flexible Blanket Insulation (C.F.B.I.) considered for potential use as a thermal protection system or thermal insulation for future hypersonic vehicles such as the National Aerospace Plane (N.A.S.P.). Thermophysical properties for these insulations were also measured including the thermal conductivity at various temperatures and pressures and the emissivity of the fabrics used in the flexible insulations. The thermal response of these materials subjected to aeroconvective heating from a plasma arc is also described. Materials tested included two surface variations of the insulations, and similar insulations coated with a Protective Ceramic Coating (P.C.C.). Surface and backface temperatures were measured in the flexible insulations and on Fibrous Refractory Composite Insulation (F.R.C.I.) used as a calibration model. The uncoated flexible insulations exhibited good thermal performance up to 35 W/sq cm. The use of a P.C.C. to protect these insulations at higher heating rates is described. The results from a computerized thermal analysis model describing thermal response of those materials subjected to the plasma arc conditions are included. Thermal and optical properties were determined including thermal conductivity for the rigid and flexible insulations and emissivity for the insulation fabrics. These properties were utilized to calculate the thermal performance of the rigid and flexible insulations at the maximum heating rate.

  10. High temperature insulation barrier composite

    NASA Technical Reports Server (NTRS)

    Onstott, Joseph W. (Inventor)

    1989-01-01

    A composite material suitable for providing insulation for the nozzle structure of the Space Shuttle and other similar surfaces is disclosed. The composite layer is comprised of an outer skin layer of nickel chromium and an interleaved inner region comprising a top layer of nickel chromium foil which acts as a primary convective shield. There are at least two layers of alumina batting adjacent to the layers of silicon carbide fabric. An additional layer of nickel chromium foil is used as a secondary convective shield. The composite is particularly advantageous for use as nozzle insulation because of its ability to withstand high reentry temperatures, its flexibility, oxidation resistance, low conductivity, and light weight.

  11. Composite flexible blanket insulation

    NASA Technical Reports Server (NTRS)

    Kourtides, Demetrius A. (Inventor); Lowe, David M. (Inventor)

    1994-01-01

    An improved composite flexible blanket insulation is presented comprising top silicon carbide having an interlock design, wherein the reflective shield is composed of single or double aluminized polyimide and wherein the polyimide film has a honeycomb pattern.

  12. Influence of copper on the by-products of different oil-paper insulations

    NASA Astrophysics Data System (ADS)

    Hao, Jian; Liao, Ruijin; Chen, George; Ma, Chao

    2011-08-01

    Transformer failure caused by the corrosion of copper material in transformer attracts great attention of researchers and engineers. In this paper, Karamay No. 25 naphthenic mineral oil, Karamay No. 25 paraffinic mineral oil, Kraft paper and copper were used to compose four combinations of oil-paper insulation samples. The ageing by-products and dielectric properties of the four combinations of oil-paper insulation samples were compared after they were thermally aged at 130°C. The influence of copper on the by-products and dielectric properties of different oil-paper insulations was obtained. The results show that copper can accelerate the ageing rate of insulation oils and reduce their AC breakdown voltage. The content of copper substance dissolved in insulating oil increases with ageing time at first and then decreases. The paper aged in the oil-paper insulation sample with copper has higher moisture content than the one without copper. Results of energy dispersive spectroscopy (EDS) in the scanning electron microscope (SEM) show that there is copper product deposited on the surface of insulation paper. The insulation oil and paper aged in the oil-paper insulation sample with copper have higher dielectric loss and conductivity than that without copper.

  13. Ceramic insulation/multifoil composite for thermal protection of reentry spacecraft

    NASA Technical Reports Server (NTRS)

    Pitts, W. C.; Kourtides, D. A.

    1989-01-01

    A new type of insulation blanket called Composite Flexible Blanket Insulation is proposed for thermal protection of advanced spacecraft in regions where the maximum temperature is not excessive. The blanket is a composite of two proven insulation materials: ceramic insulation blankets from Space Shuttle technology and multilayer insulation blankets from spacecraft thermal control technology. A potential heatshield weight saving of up to 500 g/sq m is predicted. The concept is described; proof of concept experimental data are presented; and a spaceflight experiment to demonstrate its actual performance is discussed.

  14. Primary spectrum and composition with IceCube/IceTop

    NASA Astrophysics Data System (ADS)

    Gaisser, Thomas K.; IceCube Collaboration

    2016-10-01

    IceCube, with its surface array IceTop, detects three different components of extensive air showers: the total signal at the surface, GeV muons in the periphery of the showers and TeV muons in the deep array of IceCube. The spectrum is measured with high resolution from the knee to the ankle with IceTop. Composition and spectrum are extracted from events seen in coincidence by the surface array and the deep array of IceCube. The muon lateral distribution at the surface is obtained from the data and used to provide a measurement of the muon density at 600 meters from the shower core up to 30 PeV. Results are compared to measurements from other experiments to obtain an overview of the spectrum and composition over an extended range of energy. Consistency of the surface muon measurements with hadronic interaction models and with measurements at higher energy is discussed.

  15. High temperature insulation for ceramic matrix composites

    DOEpatents

    Merrill, Gary B.; Morrison, Jay Alan

    2001-01-01

    A ceramic composition is provided to insulate ceramic matrix composites under high temperature, high heat flux environments. The composition comprises a plurality of hollow oxide-based spheres of various dimensions, a phosphate binder, and at least one oxide filler powder, whereby the phosphate binder partially fills gaps between the spheres and the filler powders. The spheres are situated in the phosphate binder and the filler powders such that each sphere is in contact with at least one other sphere. The spheres may be any combination of Mullite spheres, Alumina spheres, or stabilized Zirconia spheres. The filler powder may be any combination of Alumina, Mullite, Ceria, or Hafnia. Preferably, the phosphate binder is Aluminum Ortho-Phosphate. A method of manufacturing the ceramic insulating composition and its application to CMC substrates are also provided.

  16. High temperature insulation for ceramic matrix composites

    DOEpatents

    Merrill, Gary B.; Morrison, Jay Alan

    2000-01-01

    A ceramic composition is provided to insulate ceramic matrix composites under high temperature, high heat flux environments. The composite comprises a plurality of hollow oxide-based spheres of varios dimentions, a phosphate binder, and at least one oxide filler powder, whereby the phosphate binder partially fills gaps between the spheres and the filler powders. The spheres are situated in the phosphate binder and the filler powders such that each sphere is in contact with at least one other sphere. The spheres may be any combination of Mullite spheres, Alumina spheres, or stabilized Zirconia spheres. The filler powder may be any combination of Alumina, Mullite, Ceria, or Hafnia. Preferably, the phosphate binder is Aluminum Ortho-Phosphate. A method of manufacturing the ceramic insulating composition and its application to CMC substates are also provided.

  17. High temperature insulation for ceramic matrix composites

    DOEpatents

    Merrill, Gary B.; Morrison, Jay Alan

    2004-01-13

    A ceramic composition is provided to insulate ceramic matrix composites under high temperature, high heat flux environments. The composition comprises a plurality of hollow oxide-based spheres of various dimensions, a phosphate binder, and at least one oxide filler powder, whereby the phosphate binder partially fills gaps between the spheres and the filler powders. The spheres are situated in the phosphate binder and the filler powders such that each sphere is in contact with at least one other sphere. The spheres may be any combination of Mullite spheres, Alumina spheres, or stabilized Zirconia spheres. The filler powder may be any combination of Alumina, Mullite, Ceria, or Hafnia. Preferably, the phosphate binder is Aluminum Ortho-Phosphate. A method of manufacturing the ceramic insulating composition and its application to CMC substrates are also provided.

  18. Surface structural changes of naturally aged silicone and EPDM composite insulators

    DOE Office of Scientific and Technical Information (OSTI.GOV)

    Vlastos, A.E.; Gubanski, S.M.

    1991-04-01

    In a long-term outdoor test with high direct and alternating voltages, silicone and EPDM rubber composite insulators have, at the beginning, shown a superior performance to that of glass and porcelain insulators. In the long-term test, however, the silicone rubber composite insulator has, in spite of the ageing of both insulator types, kept its good performance, while the performance of the EPDM rubber composite insulator was drastically deteriorated. In order to get a better insight into results obtained, the wettability and the surface structural changes of the insulators were studied by the drop deposition method (using a goniometer) and bymore » advanced techniques such as SEM, ESCA, FTIR and SIMS respectively. The results show that the differences in performance have to be found in the differences in the surface structural changes and in the dynamic ability of the surface to compensate the ageing.« less

  19. Composition and process for making an insulating refractory material

    DOEpatents

    Pearson, A.; Swansiger, T.G.

    1998-04-28

    A composition and process are disclosed for making an insulating refractory material. The composition includes calcined alumina powder, flash activated alumina powder, an organic polymeric binder and a liquid vehicle which is preferably water. Starch or modified starch may also be added. A preferred insulating refractory material made with the composition has a density of about 2.4--2.6 g/cm{sup 3} with reduced thermal conductivity, compared with tabular alumina. Of importance, the formulation has good abrasion resistance and crush strength during intermediate processing (commercial sintering) to attain full strength and refractoriness.

  20. High-pressure dielectric-strength tests on PPP (PPLP) insulation. Final report. [Paper-polypropylene film-paper

    DOE Office of Scientific and Technical Information (OSTI.GOV)

    Hata, R.; Hirose, M.; Nagai, T.

    1983-06-01

    The objectives of this project were to establish the effects of fluid pressure on the impulse and ac breakdown strengths of PPP (PPLP) (paper-polypropylene film-paper) insulation. Two thicknesses of PPP (PPLP), which was developed jointly by Sumitomo Electric Industries, Ltd. and Tomoegawa Paper Co., Ltd. and produced by the latter company, were tested with dodecylebenzene (DDB) of the alkylbenzene family as dielectric fluid. Appropriate flat/model cells as employed for previous breakdown tests on paper-oil insulation were used, suitable for test pressures up to 20 kg/cm/sup 2/ abs. (2.0 MN/m/sup 2/ or 284 psi). Impulse and ac breakdown tests were performedmore » at a series of applied pressures, at room temperature and 90/sup 0/C. The results were analyzed and are presented in comparison with previously published data on paper-oil cable insulation.« less

  1. A review of vacuum insulation research and development in the Building Materials Group of the Oak Ridge National Laboratory

    DOE Office of Scientific and Technical Information (OSTI.GOV)

    Kollie, T.G.; McElroy, D.L.; Fine, H.A.

    This report is a summary of the development work on flat-vacuum insulation performed by the Building Materials Group (BMG) in the Metals and Ceramics Division of the Oak Ridge National Laboratory (ORNL) during the last two years. A historical review of the technology of vacuum insulation is presented, and the role that ORNL played in this development is documented. The ORNL work in vacuum insulation has been concentrated in Powder-filled Evacuated Panels (PEPs) that have a thermal resistivity over 2.5 times that of insulating foams and seven times that of many batt-type insulations, such as fiberglass. Experimental results of substitutingmore » PEPs for chlorofluorocarbon (CFC) foal insulation in Igloo Corporation ice coolers are summarized. This work demonstrated that one-dimensional (1D) heat flow models overestimated the increase in thermal insulation of a foam/PEP-composite insulation, but three-dimensional (3D) models provided by a finite-difference, heat-transfer code (HEATING-7) accurately predicted the resistance of the composites. Edges and corners of the ice coolers were shown to cause the errors in the 1D models as well as shunting of the heat through the foam and around the PEPs. The area of coverage of a PEP in a foam/PEP composite is established as an important parameter in maximizing the resistance of such composites. 50 refs., 27 figs,. 22 tabs.« less

  2. Composite multilayer insulations for thermal protection of aerospace vehicles

    NASA Technical Reports Server (NTRS)

    Kourtides, Demetrius A.; Pitts, William C.

    1989-01-01

    Composite flexible multilayer insulation systems (MLI), consisting of alternating layers of metal foil and scrim cloth or insulation quilted together using ceramic thread, were evaluated for thermal performance and compared with a silica fibrous (baseline) insulation system. The systems studied included: (1) alternating layers of aluminoborosilicate (ABS) scrim cloth and stainless steel foil, with silica, ABS, or alumina insulation; (2) alternating layers of scrim cloth and aluminum foil, with silica or ABS insulation; (3) alternating layers of aluminum foil and silica or ABS insulation; and (4) alternating layers of aluminum-coated polyimide placed on the bottom of the silica insulation. The MLIs containing aluminum were the most efficient, measuring as little as half the backface temperature increase of the baseline system.

  3. Properties of radiation stable insulation composites for fusion magnet

    NASA Astrophysics Data System (ADS)

    Wu, Zhixiong; Huang, Rongjin; Huang, Chuanjun; Li, Laifeng

    2017-09-01

    High field superconducting magnets made of Nb3Al will be a suitable candidate for future fusion device which can provide magnetic field over 15T without critical current degradation caused by strain. The higher magnetic field and the larger current will produce a huge electromagnetic force. Therefore, it is necessary to develop high strength cryogenic structural materials and electrical insulation materials with excellent performance. On the other hand, superconducting magnets in fusion devices will experience significant nuclear radiation exposure during service. While typical structural materials like stainless steel and titanium have proven their ability to withstand these conditions, electrical insulation materials used in these coils have not fared as well. In fact, recent investigations have shown that electrical insulation breakdown is a limiting factor in the performance of high field magnets. The insulation materials used in the high field fusion magnets should be characterized by excellent mechanical properties, high radiation resistivity and good thermal conductivity. To meet these objectives, we designed various insulation materials based on epoxy resins and cyanate ester resins and investigated their processing characteristic and mechanical properties before and after irradiation at low temperature. In this paper, the recent progress of the radiation stable insulation composites for high field fusion magnet is presented. The materials have been irradiated by 60Co γ-ray irradiation in air at ambient temperature with a dose rate of 300 Gy/min. The total doses of 1 MGy, 5 MGy and 10 MGy were selected to the test specimens.

  4. Composition and process for making an insulating refractory material

    DOEpatents

    Pearson, Alan; Swansiger, Thomas G.

    1998-04-28

    A composition and process for making an insulating refractory material. The composition includes calcined alumina powder, flash activated alumina powder, an organic polymeric binder and a liquid vehicle which is preferably water. Starch or modified starch may also be added. A preferred insulating refractory material made with the composition has a density of about 2.4-2.6 g/cm.sup.3 with reduced thermal conductivity, compared with tabular alumina. Of importance, the formulation has good abrasion resistance and crush strength during intermediate processing (commercial sintering) to attain full strength and refractoriness, good abrasion resistance and crush strength.

  5. Thermal Response Of Composite Insulation

    NASA Technical Reports Server (NTRS)

    Stewart, David A.; Leiser, Daniel B.; Smith, Marnell; Kolodziej, Paul

    1988-01-01

    Engineering model gives useful predictions. Pair of reports presents theoretical and experimental analyses of thermal responses of multiple-component, lightweight, porous, ceramic insulators. Particular materials examined destined for use in Space Shuttle thermal protection system, test methods and heat-transfer theory useful to chemical, metallurgical, and ceramic engineers needing to calculate transient thermal responses of refractory composites.

  6. Thermal Insulation System for Non-Vacuum Applications Including a Multilayer Composite

    NASA Technical Reports Server (NTRS)

    Fesmire, James E. (Inventor)

    2017-01-01

    The thermal insulation system of the present invention is for non-vacuum applications and is specifically tailored to the ambient pressure environment with any level of humidity or moisture. The thermal insulation system includes a multilayered composite including i) at least one thermal insulation layer and at least one compressible barrier layer provided as alternating, successive layers, and ii) at least one reflective film provided on at least one surface of the thermal insulation layer and/or said compressible barrier layer. The different layers and materials and their combinations are designed to provide low effective thermal conductivity for the system by managing all modes of heat transfer. The thermal insulation system includes an optional outer casing surrounding the multilayered composite. The thermal insulation system is particularly suited for use in any sub-ambient temperature environment where moisture or its adverse effects are a concern. The thermal insulation system provides physical resilience against damaging mechanical effects including compression, flexure, impact, vibration, and thermal expansion/contraction.

  7. POROSITY AND BAND-STRENGTH MEASUREMENTS OF MULTI-PHASE COMPOSITE ICES

    DOE Office of Scientific and Technical Information (OSTI.GOV)

    Bossa, Jean-Baptiste; Fransen, Coen; Cazaux, Stéphanie

    2015-11-20

    We use experimental mid-infrared optical constants and extended effective medium approximations to determine the porosity and the band strengths of multi-phase composite ices grown at 30 K. A set of porous H{sub 2}O:CH{sub 4} ices are taken as a prototypical example. As a benchmark and proof of concept, the stoichiometry of the ice constituents is retreived with good accuracy from the refractive indices and the extinction coefficients of the reference binary ice mixtures with known compositions. Accurate band strengths are then calculated from experimental mid-infrared spectra of complex ices. We notice that the presence of pores has only a smallmore » effect on the overall band strengths, whereas a water dilution can considerably alter them. Different levels of porosity are observed depending on the abundance of methane used as a gas contaminant premixed with water prior to background deposition. The absorption profiles are also found to vary with deposition rate. To explain this, we use Monte Carlo simulations and we observe that the deposition rate strongly affects the pore size distribution as well as the ice morphology through reorganization processes. Extrapolated to genuine interstellar ices, the methodology presented in this paper can be used to evaluate the porosity and to quantify the relative abundances from observational data.« less

  8. Composite Behavior of a Novel Insulated Concrete Sandwich Wall Panel Reinforced with GFRP Shear Grids: Effects of Insulation Types.

    PubMed

    Kim, JunHee; You, Young-Chan

    2015-03-03

    A full-scale experimental program was used in this study to investigate the structural behavior of novel insulated concrete sandwich wall panels (SWPs) reinforced with grid-type glass-fiber-reinforced polymer (GFRP) shear connectors. Two kinds of insulation-expanded polystyrene (EPS) and extruded polystyrene (XPS) with 100 mm thickness were incased between the two concrete wythes to meet the increasing demand for the insulation performance of building envelope. One to four GFRP shear grids were used to examine the degree of composite action of the two concrete wythes. Ten specimens of SWPs were tested under displacement control subjected to four-point concentrated loads. The test results showed that the SWPs reinforced with GFRP grids as shear connectors developed a high degree of composite action resulting in high flexural strength. The specimens with EPS foam exhibited an enhanced load-displacement behavior compared with the specimens with XPS because of the relatively stronger bond between insulation and concrete. In addition, the ultimate strength of the test results was compared to the analytical prediction with the mechanical properties of only GRFP grids. The specimens with EPS insulation presented higher strength-based composite action than the ones with XPS insulation.

  9. Composite Behavior of a Novel Insulated Concrete Sandwich Wall Panel Reinforced with GFRP Shear Grids: Effects of Insulation Types

    PubMed Central

    Kim, JunHee; You, Young-Chan

    2015-01-01

    A full-scale experimental program was used in this study to investigate the structural behavior of novel insulated concrete sandwich wall panels (SWPs) reinforced with grid-type glass-fiber-reinforced polymer (GFRP) shear connectors. Two kinds of insulation-expanded polystyrene (EPS) and extruded polystyrene (XPS) with 100 mm thickness were incased between the two concrete wythes to meet the increasing demand for the insulation performance of building envelope. One to four GFRP shear grids were used to examine the degree of composite action of the two concrete wythes. Ten specimens of SWPs were tested under displacement control subjected to four-point concentrated loads. The test results showed that the SWPs reinforced with GFRP grids as shear connectors developed a high degree of composite action resulting in high flexural strength. The specimens with EPS foam exhibited an enhanced load-displacement behavior compared with the specimens with XPS because of the relatively stronger bond between insulation and concrete. In addition, the ultimate strength of the test results was compared to the analytical prediction with the mechanical properties of only GRFP grids. The specimens with EPS insulation presented higher strength-based composite action than the ones with XPS insulation. PMID:28787978

  10. Rocket motors incorporating basalt fiber and nanoclay compositions and methods of insulating a rocket motor with the same

    NASA Technical Reports Server (NTRS)

    Gajiwala, Himansu M. (Inventor)

    2011-01-01

    An insulation composition that comprises at least one nitrile butadiene rubber, basalt fibers, and nanoclay is disclosed. Further disclosed is an insulation composition that comprises polybenzimidazole fibers, basalt fibers, and nanoclay. The basalt fibers may be present in the insulation compositions in a range of from approximately 1% by weight to approximately 6% by weight of the total weight of the insulation composition. The nanoclay may be present in the insulation compositions in a range of from approximately 5% by weight to approximately 10% by weight of the total weight of the insulation composition. Rocket motors including the insulation compositions and methods of insulating a rocket motor are also disclosed.

  11. Research on breakdown characteristics of oil-paper insulation in compound field at different temperatures

    NASA Astrophysics Data System (ADS)

    Li, L.; Chen, M. Y.; Zhu, X. C.; Gao, Z. W.; Zhang, H. D.; Li, G. X.; Zhang, J.; Yu, C. L.; Feng, Y. M.

    2018-01-01

    The breakdown characteristics of oil-paper insulation in AC, DC and compound field at different temperatures were studied. The breakdown mechanism of oil-paper insulation at different temperatures and in AC and DC electric fields was analyzed. The breakdown characteristic mechanisms of the oil-paper insulation in the compound field at different temperatures were obtained: the dielectric strength of oil-paper compound insulation is changed gradually from dependence on oil dielectric strength to dependence on paperboard dielectric strength at low temperature. The dielectric strength of oil-paper compound insulation is always related to the oil dielectric strength closely at high temperature with decrease of AC content.

  12. Insulator coated magnetic nanoparticulate composites with reduced core loss and method of manufacture thereof

    NASA Technical Reports Server (NTRS)

    Zhang, Yide (Inventor); Wang, Shihe (Inventor); Xiao, Danny (Inventor)

    2004-01-01

    A series of bulk-size magnetic/insulating nanostructured composite soft magnetic materials with significantly reduced core loss and its manufacturing technology. This insulator coated magnetic nanostructured composite is comprises a magnetic constituent, which contains one or more magnetic components, and an insulating constituent. The magnetic constituent is nanometer scale particles (1-100 nm) coated by a thin-layered insulating phase (continuous phase). While the intergrain interaction between the immediate neighboring magnetic nanoparticles separated by the insulating phase (or coupled nanoparticles) provide the desired soft magnetic properties, the insulating material provides the much demanded high resistivity which significantly reduces the eddy current loss. The resulting material is a high performance magnetic nanostructured composite with reduced core loss.

  13. Analysis of the possibilities of using dielectric foam in the construction of composite high voltage post-insulators

    NASA Astrophysics Data System (ADS)

    Mączka, T.; Paściak, G.; Jarski, A.; Piątek, M.

    2016-02-01

    This paper presents the construction and basic performance parameters of the innovative tubular construction of high voltage composite insulator filled with the lightweight foamed electroinsulating material. The possibility of using of the commercially available expanding foams for preparing the lightweight foamed dielectric materials was analysed. The expanding foams of silicone RTV and compositions based on epoxy resin and LSR silicone were taken into account. The lightweight foamed dielectric materials were prepared according to the own foaming technology. In this work the experimental results on the use of the selected foams for the preparing of the lightweight filling materials to the tubular structure of composite insulator of 110 kV are presented.

  14. Polyimide/Glass Composite High-Temperature Insulation

    NASA Technical Reports Server (NTRS)

    Pater, Ruth H.; Vasquez, Peter; Chatlin, Richard L.; Smith, Donald L.; Skalski, Thomas J.; Johnson, Gary S.; Chu, Sang-Hyon

    2009-01-01

    Lightweight composites of RP46 polyimide and glass fibers have been found to be useful as extraordinarily fire-resistant electrical-insulation materials. RP46 is a polyimide of the polymerization of monomeric reactants (PMR) type, developed by NASA Langley Research Center. RP46 has properties that make it attractive for use in electrical insulation at high temperatures. These properties include high-temperature resistance, low relative permittivity, low dissipation factor, outstanding mechanical properties, and excellent resistance to moisture and chemicals. Moreover, RP46 contains no halogen or other toxic materials and when burned it does not produce toxic fume or gaseous materials. The U. S. Navy has been seeking lightweight, high-temperature-resistant electrical-insulation materials in a program directed toward reducing fire hazards and weights in ship electrical systems. To satisfy the requirements of this program, an electrical-insulation material must withstand a 3-hour gas-flame test at 1,600 F (about 871 C). Prior to the development reported here, RP46 was rated for use at temperatures from -150 to +700 F (about -101 to 371 C), and no polymeric product - not even RP46 - was expected to withstand the Navy 3-hour gas-flame test.

  15. Surface water mass composition changes captured by cores of Arctic land-fast sea ice

    NASA Astrophysics Data System (ADS)

    Smith, I. J.; Eicken, H.; Mahoney, A. R.; Van Hale, R.; Gough, A. J.; Fukamachi, Y.; Jones, J.

    2016-04-01

    In the Arctic, land-fast sea ice growth can be influenced by fresher water from rivers and residual summer melt. This paper examines a method to reconstruct changes in water masses using oxygen isotope measurements of sea ice cores. To determine changes in sea water isotope composition over the course of the ice growth period, the output of a sea ice thermodynamic model (driven with reanalysis data, observations of snow depth, and freeze-up dates) is used along with sea ice oxygen isotope measurements and an isotopic fractionation model. Direct measurements of sea ice growth rates are used to validate the output of the sea ice growth model. It is shown that for sea ice formed during the 2011/2012 ice growth season at Barrow, Alaska, large changes in isotopic composition of the ocean waters were captured by the sea ice isotopic composition. Salinity anomalies in the ocean were also tracked by moored instruments. These data indicate episodic advection of meteoric water, having both lower salinity and lower oxygen isotopic composition, during the winter sea ice growth season. Such advection of meteoric water during winter is surprising, as no surface meltwater and no local river discharge should be occurring at this time of year in that area. How accurately changes in water masses as indicated by oxygen isotope composition can be reconstructed using oxygen isotope analysis of sea ice cores is addressed, along with methods/strategies that could be used to further optimize the results. The method described will be useful for winter detection of meteoric water presence in Arctic fast ice regions, which is important for climate studies in a rapidly changing Arctic. Land-fast sea ice effective fractionation coefficients were derived, with a range of +1.82‰ to +2.52‰. Those derived effective fractionation coefficients will be useful for future water mass component proportion calculations. In particular, the equations given can be used to inform choices made when

  16. Basalt fiber and nanoclay compositions, articles incorporating the same, and methods of insulating a rocket motor with the same

    NASA Technical Reports Server (NTRS)

    Gajiwala, Himansu M. (Inventor)

    2010-01-01

    An insulation composition that comprises at least one nitrile butadiene rubber, basalt fibers, and nanoclay is disclosed. Further disclosed is an insulation composition that comprises polybenzimidazole fibers, basalt fibers, and nanoclay. The basalt fibers may be present in the insulation compositions in a range of from approximately 1% by weight to approximately 6% by weight of the total weight of the insulation composition. The nanoclay may be present in the insulation compositions in a range of from approximately 5% by weight to approximately 10% by weight of the total weight of the insulation composition. Rocket motors including the insulation compositions and methods of insulating a rocket motor are also disclosed.

  17. ION COMPOSITION ELUCIDATION (ICE)

    EPA Science Inventory



    Ion Composition Elucidation (ICE) utilizes selected ion recording with a double focusing mass spectrometer to simultaneously determine exact masses and relative isotopic abundances from mass peak profiles. These can be determined more accurately and at higher sensitivity ...

  18. Cosmic ray spectrum and composition from three years of IceTop and IceCube

    NASA Astrophysics Data System (ADS)

    Rawlins, K.; IceCube Collaboration

    2016-05-01

    IceTop is the surface component of the IceCube Observatory, composed of frozen water tanks at the top of IceCube’s strings. Data from this detector can be analyzed in different ways with the goal of measuring cosmic ray spectrum and composition. The shower size S125 from IceTop alone can be used as a proxy for primary energy, and unfolded into an all-particle spectrum. In addition, S125 from the surface can be combined with high-energy muon energy loss information from the deep IceCube detector for those air showers which pass through both. Using these coincident events in a complementary analysis, both the spectrum and mass composition of primary cosmic rays can be extracted in parallel using a neural network. Both of these analyses have been performed on three years of IceTop and IceCube data. Both all-particle spectra as well as individual spectra for elemental groups are presented.

  19. Foam/Aerogel Composite Materials for Thermal and Acoustic Insulation and Cryogen Storage

    NASA Technical Reports Server (NTRS)

    Williams, Martha K. (Inventor); Smith, Trent M. (Inventor); Fesmire, James E. (Inventor); Sass, Jared P. (Inventor); Weiser, Erik S. (Inventor)

    2011-01-01

    The invention involves composite materials containing a polymer foam and an aerogel. The composite materials have improved thermal insulation ability, good acoustic insulation, and excellent physical mechanical properties. The composite materials can be used, for instance, for heat and acoustic insulation on aircraft, spacecraft, and maritime ships in place of currently used foam panels and other foam products. The materials of the invention can also be used in building construction with their combination of light weight, strength, elasticity, ability to be formed into desired shapes, and superior thermal and acoustic insulation power. The materials have also been found to have utility for storage of cryogens. A cryogenic liquid or gas, such as N.sub.2 or H.sub.2, adsorbs to the surfaces in aerogel particles. Thus, another embodiment of the invention provides a storage vessel for a cryogen.

  20. Foam/aerogel composite materials for thermal and acoustic insulation and cryogen storage

    NASA Technical Reports Server (NTRS)

    Smith, Trent M. (Inventor); Fesmire, James E. (Inventor); Williams, Martha K. (Inventor); Sass, Jared P. (Inventor); Weiser, Erik S. (Inventor)

    2010-01-01

    The invention involves composite materials containing a polymer foam and an aerogel. The composite materials have improved thermal insulation ability, good acoustic insulation, and excellent physical mechanical properties. The composite materials can be used, for instance, for heat and acoustic insulation on aircraft, spacecraft, and maritime ships in place of currently used foam panels and other foam products. The materials of the invention can also be used in building construction with their combination of light weight, strength, elasticity, ability to be formed into desired shapes, and superior thermal and acoustic insulation power. The materials have also been found to have utility for storage of cryogens. A cryogenic liquid or gas, such as N.sub.2 or H.sub.2, adsorbs to the surfaces in aerogel particles. Thus, another embodiment of the invention provides a storage vessel for a cryogen.

  1. Composite Behavior of Insulated Concrete Sandwich Wall Panels Subjected to Wind Pressure and Suction.

    PubMed

    Choi, Insub; Kim, JunHee; Kim, Ho-Ryong

    2015-03-19

    A full-scale experimental test was conducted to analyze the composite behavior of insulated concrete sandwich wall panels (ICSWPs) subjected to wind pressure and suction. The experimental program was composed of three groups of ICSWP specimens, each with a different type of insulation and number of glass-fiber-reinforced polymer (GFRP) shear grids. The degree of composite action of each specimen was analyzed according to the load direction, type of the insulation, and number of GFRP shear grids by comparing the theoretical and experimental values. The failure modes of the ICSWPs were compared to investigate the effect of bonds according to the load direction and type of insulation. Bonds based on insulation absorptiveness were effective to result in the composite behavior of ICSWP under positive loading tests only, while bonds based on insulation surface roughness were effective under both positive and negative loading tests. Therefore, the composite behavior based on surface roughness can be applied to the calculation of the design strength of ICSWPs with continuous GFRP shear connectors.

  2. Composite Behavior of Insulated Concrete Sandwich Wall Panels Subjected to Wind Pressure and Suction

    PubMed Central

    Choi, Insub; Kim, JunHee; Kim, Ho-Ryong

    2015-01-01

    A full-scale experimental test was conducted to analyze the composite behavior of insulated concrete sandwich wall panels (ICSWPs) subjected to wind pressure and suction. The experimental program was composed of three groups of ICSWP specimens, each with a different type of insulation and number of glass-fiber-reinforced polymer (GFRP) shear grids. The degree of composite action of each specimen was analyzed according to the load direction, type of the insulation, and number of GFRP shear grids by comparing the theoretical and experimental values. The failure modes of the ICSWPs were compared to investigate the effect of bonds according to the load direction and type of insulation. Bonds based on insulation absorptiveness were effective to result in the composite behavior of ICSWP under positive loading tests only, while bonds based on insulation surface roughness were effective under both positive and negative loading tests. Therefore, the composite behavior based on surface roughness can be applied to the calculation of the design strength of ICSWPs with continuous GFRP shear connectors. PMID:28788001

  3. Exploring Insulation with Ice Hands

    ERIC Educational Resources Information Center

    Taylor, Neil; Taylor, Subhashni; Littledyke, Michael

    2017-01-01

    Students often hold misconceptions about insulation, largely because they put on clothes to keep themselves warm--at least in winter in the cooler regions of Australia. The following activity is designed to identify students' misconceptions about insulation and provide an engaging, evidence-based activity to help address these misconceptions using…

  4. Heat insulation performance, mechanics and hydrophobic modification of cellulose-SiO2 composite aerogels.

    PubMed

    Shi, Jianjun; Lu, Lingbin; Guo, Wantao; Zhang, Jingying; Cao, Yang

    2013-10-15

    Cellulose-SiO2 composite hydrogel was prepared by combining the NaOH/thiourea/H2O solvent system and the immersion method with controlling the hydrolysis-fasculation rate of tetraethyl orthosilicate (TEOS). The hydrophobic composite aerogels were obtained through the freeze-drying technology and the cold plasma modification technology. Composite SiO2 could obviously reduce the thermal conductivity of cellulose aerogel. The thermal conductivity could be as low as 0.026 W/(mK). The thermal insulation mechanism of the aerogel material was discussed. Composite SiO2 reduced hydrophilicity of cellulose aerogel, but environmental humidity had a significant influence on heat insulation performance. After hydrophobic modification using CCl4 as plasma was conducted, the surface of composite aerogel was changed from hydrophilic to hydrophobic and water contact angle was as high as 132°. The modified composite aerogel still kept good heat insulation performance. This work provided a foundation for the possibility of applying cellulose-SiO2 composite aerogel in the insulating material field. Copyright © 2013 Elsevier Ltd. All rights reserved.

  5. Fibrous-Ceramic/Aerogel Composite Insulating Tiles

    NASA Technical Reports Server (NTRS)

    White, Susan M.; Rasky, Daniel J.

    2004-01-01

    Fibrous-ceramic/aerogel composite tiles have been invented to afford combinations of thermal-insulation and mechanical properties superior to those attainable by making tiles of fibrous ceramics alone or aerogels alone. These lightweight tiles can be tailored to a variety of applications that range from insulating cryogenic tanks to protecting spacecraft against re-entry heating. The advantages and disadvantages of fibrous ceramics and aerogels can be summarized as follows: Tiles made of ceramic fibers are known for mechanical strength, toughness, and machinability. Fibrous ceramic tiles are highly effective as thermal insulators in a vacuum. However, undesirably, the porosity of these materials makes them permeable by gases, so that in the presence of air or other gases, convection and gas-phase conduction contribute to the effective thermal conductivity of the tiles. Other disadvantages of the porosity and permeability of fibrous ceramic tiles arise because gases (e.g., water vapor or cryogenic gases) can condense in pores. This condensation contributes to weight, and in the case of cryogenic systems, the heat of condensation undesirably adds to the heat flowing to the objects that one seeks to keep cold. Moreover, there is a risk of explosion associated with vaporization of previously condensed gas upon reheating. Aerogels offer low permeability, low density, and low thermal conductivity, but are mechanically fragile. The basic idea of the present invention is to exploit the best features of fibrous ceramic tiles and aerogels. In a composite tile according to the invention, the fibrous ceramic serves as a matrix that mechanically supports the aerogel, while the aerogel serves as a low-conductivity, low-permeability filling that closes what would otherwise be the open pores of the fibrous ceramic. Because the aerogel eliminates or at least suppresses permeation by gas, gas-phase conduction, and convection, the thermal conductivity of such a composite even at

  6. Hydrophobic Characteristics of Composite Insulators in Simulated Inland Arid Desert Environment

    NASA Astrophysics Data System (ADS)

    Khan, Yasin; Al-Arainy, Abdulrehman Ali; Malik, Nazar Hussain; Qureshi, Muhammad Iqbal

    2010-06-01

    Presently along with traditional insulators i.e. glass and porcelain, etc., the polymeric insulators are also used world widely. These polymeric insulators are very sensitive to various environmental parameters e.g. UV radiations, heat, etc. The UV radiation level in the central region of Saudi Arabia is high as compared to the recommended IEC-61109 standard for the accelerated aging of the composite insulators. In this study, thermoplastic elastomer (TPE) and Ethylene Propylene Diene Monomer (EPDM) insulators were subjected to accelerated aging stress as per IEC standard as well as modified IEC standard simulating the inland arid desert's atmospheric conditions. The hydrophobic characteristics were studied by measuring the contact angle along the insulator surface before and after the accelerated aging of the samples. It was found that TPE loses its hydrophobic properties more as compared to EPDM insulator. This loss was proportional to the intensity of UV irradiation. The rate of recovery is also low for both the tested materials as compared to Silicone Rubber insulators.

  7. Estimation of composite hydraulic resistance in ice-covered alluvial streams

    NASA Astrophysics Data System (ADS)

    Ghareh Aghaji Zare, Soheil; Moore, Stephanie A.; Rennie, Colin D.; Seidou, Ousmane; Ahmari, Habib; Malenchak, Jarrod

    2016-02-01

    Formation, propagation, and recession of ice cover introduce a dynamic boundary layer to the top of rivers during northern winters. Ice cover affects water velocity magnitude and distribution, water level and consequently conveyance capacity of the river. In this research, total resistance, i.e., "composite resistance," is studied for a 4 month period including stable ice cover, breakup, and open water stages in Lower Nelson River (LNR), northern Manitoba, Canada. Flow and ice characteristics such as water velocity and depth and ice thickness and condition were measured continuously using acoustic techniques. An Acoustic Doppler Current Profiler (ADCP) and Shallow Water Ice Profiling Sonar (SWIPS) were installed simultaneously on a bottom mount and deployed for this purpose. Total resistance to the flow and boundary roughness are estimated using measured bulk hydraulic parameters. A novel method is developed to calculate composite resistance directly from measured under ice velocity profiles. The results of this method are compared to the measured total resistance and to the calculated composite resistance using formulae available in literature. The new technique is demonstrated to compare favorably to measured total resistance and to outperform previously available methods.

  8. Cryogenic Insulation Systems

    NASA Technical Reports Server (NTRS)

    Augustynowicz, S. D.; Fesmire, J. E.; Wikstrom, J. P.

    1999-01-01

    The results of a comparative study of cryogenic insulation systems performed are presented. The key aspects of thermal insulation relative to cryogenic system design, testing, manufacturing, and maintenance are discussed. An overview of insulation development from an energy conservation perspective is given. Conventional insulation materials for cryogenic applications provide three levels of thermal conductivity. Actual thermal performance of standard multilayer insulation (MLI) is several times less than laboratory performance and often 10 times worse than ideal performance. The cost-effectiveness of the insulation system depends on thermal performance; flexibility and durability; ease of use in handling, installation, and maintenance; and overall cost including operations, maintenance, and life cycle. Results of comprehensive testing of both conventional and novel materials such as aerogel composites using cryostat boil-off methods are given. The development of efficient, robust cryogenic insulation systems that operate at a soft vacuum level is the primary focus of this paper.

  9. Effects of Electrical Insulation Breakdown Voltage And Partial Discharge

    NASA Astrophysics Data System (ADS)

    Bahrim, F. S.; Rahman, N. F. A.; Haris, H. C. M.; Salim, N. A.

    2018-03-01

    During the last few decades, development of new materials using composite materials has been of much interest. The Cross-linked Polyethylene (XLPE) which is insulated power cables has been widely used. This paper describes the theoretical analysis, fundamental experiments and application experiments for the XLPE cable insulation. The composite that has been tested is a commercial XLPE and Polypropylene with 30% fiber glass. The results of breakdown strength and partial discharge (PD) behavior described the insulating performance of the composite.

  10. The Effect of Volcanic Ash Composition on Ice Nucleation Affinity

    NASA Astrophysics Data System (ADS)

    Genareau, K. D.; Cloer, S.; Primm, K.; Woods, T.; Tolbert, M. A.

    2017-12-01

    Understanding the role that volcanic ash plays in ice nucleation is important for knowledge of lightning generation in both volcanic plumes and in clouds developing downwind from active volcanoes. Volcanic ash has long been suggested to influence heterogeneous ice nucleation following explosive eruptions, but determining precisely how composition and mineralogy affects ice nucleation affinity (INA) is poorly constrained. For the study presented here, volcanic ash samples with different compositions and mineral/glass contents were tested in both the deposition and immersion modes, following the methods presented in Schill et al. (2015). Bulk composition was determined with X-ray fluorescence (XRF), grain size distribution was determined with laser diffraction particle size analysis (LDPSA), and mineralogy was determined with X-ray diffraction (XRD) and scanning electron microscopy (SEM). Results of the deposition-mode experiments reveal that there is no relationship between ice saturation ratios (Sice) and either mineralogy or bulk ash composition, as all samples have similar Sice ratios. In the immersion-mode experiments, frozen fractions were determined from -20 °C to -50 °C using three different amounts of ash (0.5, 1.0, and 2.0 wt% of slurry). Results from the immersion freezing reveal that the rhyolitic samples (73 wt% SiO2) nucleate ice at higher temperatures compared to the basaltic samples (49 wt% SiO2). There is no observed correlation between frozen fractions and mineral content of ash samples, but the two most efficient ice nuclei are rhyolites that contain the greatest proportion of amorphous glass (> 90 %), and are enriched in K2O relative to transition metals (MnO and TiO2), the latter of which show a negative correlation with frozen fraction. Higher ash abundance in water droplets increases the frozen fraction at all temperatures, indicating that ash amount plays the biggest role in ice nucleation. If volcanic ash can reach sufficient abundance (

  11. Grain Surface Chemistry and the Composition of Interstellar Ices

    NASA Technical Reports Server (NTRS)

    Tielens, A. G. G. M.

    2006-01-01

    Submicron sized dust grains are an important component of the interstellar medium. In particular they provide surface where active chemistry can take place. At the low temperatures (-10 K) of the interstellar medium, colliding gas phase species will stick, diffuse, react, and form an icy mantle on these dust grains. This talk will review the principles of grain surface chemistry and delineate important grain surface routes, focusing on reactions involving H, D, and O among each other and with molecules such as CO. Interstellar ice mantles can be studied through the fundamental vibrations of molecular species in the mid-infrared spectra of sources embedded in or located behind dense molecular clouds. Analysis of this type of data has provided a complex view of the composition of these ices and the processes involved. Specifically, besides grain surface chemistry, the composition of interstellar ices is also affected by thermal processing due to nearby newly formed stars. This leads to segregation between different ice components as well as outgassing. The latter results in the formation of a so-called Hot Core region with a gas phase composition dominated by evaporated mantle species. Studies of such regions provide thus a different view on the ice composition and the chemical processes involved. Interstellar ices can also be processed by FUV photons and high energy cosmic ray ions. Cosmic ray processing likely dominates the return of accreted species to the gas phase where further gas phase reactions can take place. These different chemical routes towards molecular complexity in molecular clouds and particularly regions of star formation will be discussed.

  12. HYDROPHOBIC CHARACTERISTICS OF COMPOSITE INSULATORS IN SIMULATED INLAND ARID DESERT ENVIRONMENT

    DOE Office of Scientific and Technical Information (OSTI.GOV)

    Khan, Yasin; Al-Arainy, Abdulrehman Ali; Malik, Nazar Hussain

    2010-06-15

    Presently along with traditional insulators i.e. glass and porcelain, etc., the polymeric insulators are also used world widely. These polymeric insulators are very sensitive to various environmental parameters e.g. UV radiations, heat, etc. The UV radiation level in the central region of Saudi Arabia is high as compared to the recommended IEC-61109 standard for the accelerated aging of the composite insulators. In this study, thermoplastic elastomer (TPE) and Ethylene Propylene Diene Monomer (EPDM) insulators were subjected to accelerated aging stress as per IEC standard as well as modified IEC standard simulating the inland arid desert's atmospheric conditions. The hydrophobic characteristicsmore » were studied by measuring the contact angle along the insulator surface before and after the accelerated aging of the samples. It was found that TPE loses its hydrophobic properties more as compared to EPDM insulator. This loss was proportional to the intensity of UV irradiation. The rate of recovery is also low for both the tested materials as compared to Silicone Rubber insulators.« less

  13. Determination of threshold and maximum operating electric stresses for selected high voltage insulations. Task 2: Investigation of oil-filled paper insulated cables

    NASA Astrophysics Data System (ADS)

    Sosnowski, M.; Eager, G. S., Jr.

    1983-06-01

    Threshold voltage of oil-impregnated paper insulated cables are investigaed. Experimental work was done on model cables specially manufactured for this project. The cables were impregnated with mineral and with synthetic oils. Standard impulse breakdown voltage tests and impulse voltage breakdown tests with dc prestressing were performed at room temperature and at 1000C. The most important result is the finding of very high level of threshold voltage stress for oil-impregnated paper insulated cables. This threshold voltage is approximately 1.5 times higher than the threshold voltage or crosslinked polyethylene insulated cables.

  14. Wettability of naturally aged silicone and EPDM composite insulators

    DOE Office of Scientific and Technical Information (OSTI.GOV)

    Gubanski, S.M.; Vlastos, A.E.

    1990-07-01

    This paper reports the wettability of aged surfaces and of the bulk of naturally aged silicone and EPDM insulator housings and of silicone elastomer insulator coatings studied. The samples were taken either directly from the insulators or treated by exposing them to corona discharges and/or to saline pollution. The results show that the contact angles of the silicone rubber insulator surfaces are larger than the contact angles of the RTV silicone rubber coating and of the EPDM rubber insulator surfaces, especially when the surfaces are aged. When the insulators were exposed to corona discharges, the contact angles of the siliconemore » rubber insulators are reduced but after the exposure they recover with time. The contact angles of the EPDM rubber insulators, however, after the exposure, continue to reduce. When exposed to artificial saline pollution, the silicone rubber insulators show a limited recovery of their contact angles with time, while, when exposed to corona discharge, they show a recovery of the contact angle after the exposure. The time for recovery is dependent on the exposure time to the corona discharges.« less

  15. Fibrous refractory composite insulation. [shielding reusable spacecraft

    NASA Technical Reports Server (NTRS)

    Leiser, D. B.; Goldstein, H. E.; Smith, M. (Inventor)

    1979-01-01

    A refractory composite insulating material was prepared from silica fibers and aluminosilicate fibers in a weight ratio ranging from 1:19 to 19:1, and about 0.5 to 30% boron oxide, based on the total fiber weight. The aluminosilicate fiber and boron oxide requirements may be satisfied by using aluminoborosilicate fibers and, in such instances, additional free boron oxide may be incorporated in the mix up to the 30% limit. Small quantities of refractory opacifiers, such as silicon carbide, may be also added. The composites just described are characterized by the absence of a nonfibrous matrix.

  16. Advanced Booster Composite Case/Polybenzimidazole Nitrile Butadiene Rubber Insulation Development

    NASA Technical Reports Server (NTRS)

    Gentz, Steve; Taylor, Robert; Nettles, Mindy

    2015-01-01

    The NASA Engineering and Safety Center (NESC) was requested to examine processing sensitivities (e.g., cure temperature control/variance, debonds, density variations) of polybenzimidazole nitrile butadiene rubber (PBI-NBR) insulation, case fiber, and resin systems and to evaluate nondestructive evaluation (NDE) and damage tolerance methods/models required to support human-rated composite motor cases. The proposed use of composite motor cases in Blocks IA and II was expected to increase performance capability through optimizing operating pressure and increasing propellant mass fraction. This assessment was to support the evaluation of risk reduction for large booster component development/fabrication, NDE of low mass-to-strength ratio material structures, and solid booster propellant formulation as requested in the Space Launch System NASA Research Announcement for Advanced Booster Engineering Demonstration and/or Risk Reduction. Composite case materials and high-energy propellants represent an enabling capability in the Agency's ability to provide affordable, high-performing advanced booster concepts. The NESC team was requested to provide an assessment of co- and multiple-cure processing of composite case and PBI-NBR insulation materials and evaluation of high-energy propellant formulations.

  17. 7 CFR 58.647 - Composition requirements for ice cream.

    Code of Federal Regulations, 2014 CFR

    2014-01-01

    ... 7 Agriculture 3 2014-01-01 2014-01-01 false Composition requirements for ice cream. 58.647 Section 58.647 Agriculture Regulations of the Department of Agriculture (Continued) AGRICULTURAL MARKETING... requirements for ice cream. See § 58.605(a). ...

  18. 7 CFR 58.647 - Composition requirements for ice cream.

    Code of Federal Regulations, 2013 CFR

    2013-01-01

    ... 7 Agriculture 3 2013-01-01 2013-01-01 false Composition requirements for ice cream. 58.647 Section 58.647 Agriculture Regulations of the Department of Agriculture (Continued) AGRICULTURAL MARKETING... requirements for ice cream. See § 58.605(a). ...

  19. 7 CFR 58.647 - Composition requirements for ice cream.

    Code of Federal Regulations, 2011 CFR

    2011-01-01

    ... 7 Agriculture 3 2011-01-01 2011-01-01 false Composition requirements for ice cream. 58.647 Section 58.647 Agriculture Regulations of the Department of Agriculture (Continued) AGRICULTURAL MARKETING... requirements for ice cream. See § 58.605(a). ...

  20. 7 CFR 58.647 - Composition requirements for ice cream.

    Code of Federal Regulations, 2012 CFR

    2012-01-01

    ... 7 Agriculture 3 2012-01-01 2012-01-01 false Composition requirements for ice cream. 58.647 Section 58.647 Agriculture Regulations of the Department of Agriculture (Continued) AGRICULTURAL MARKETING... requirements for ice cream. See § 58.605(a). ...

  1. 7 CFR 58.647 - Composition requirements for ice cream.

    Code of Federal Regulations, 2010 CFR

    2010-01-01

    ... 7 Agriculture 3 2010-01-01 2010-01-01 false Composition requirements for ice cream. 58.647 Section 58.647 Agriculture Regulations of the Department of Agriculture (Continued) AGRICULTURAL MARKETING... requirements for ice cream. See § 58.605(a). ...

  2. Measurement of dielectric properties at low temperatures: application to the study of magnetoresistive manganite/ insulating oxide bulk composites

    NASA Astrophysics Data System (ADS)

    Vanderbemden, P.; Rivas-Murias, B.; Lovchinov, V.; Vertruyen, B.

    2010-11-01

    In this paper, we report low temperature dielectric measurements of bulk composite electroceramic samples containing a colossal magnetoresistive (CMR) manganite phase (La0.7Ca0.3MnO3 [abbreviated LCMO]) and an insulating phase (Mn3O4). Details of the experimental system are given and possible experimental artefacts due to moisture are outlined. For a LCMO volume fraction of ~ 16%, the permittivity of the LCMO/ Mn3O4 composite at T = 50 K is found to be much higher than that of pure Mn3O4 and magnetic field dependent. This effect is related to an extrinsic space charge polarization mechanism between the insulating phase (Mn3O4) and the conducting magnetoresistive phase (LCMO).

  3. Production and characterization of a composite insulation material from waste polyethylene teraphtalates

    DOE Office of Scientific and Technical Information (OSTI.GOV)

    Kurtulmus, Erhan; Karaboyacı, Mustafa; Yigitarslan, Sibel

    2013-12-16

    The pollution of polyethylene teraphtalate (PET) is in huge amounts due to the most widely usage as a packaging material in several industries. Regional pumice has several desirable characteristics such as porous structure, low-cost and light-weight. Considering the requirements approved by the Ministry of Public Works on isolation, composite insulation material consisting of PET and pumice was studied. Sheets of composites differing both in particle size of pumice and composition of polymer were produced by hot-molding technique. Characterization of new composite material was achieved by measuring its weight, density, flammability, endurance against both to common acids and bases, and tomore » a force applied, heat insulation and water adsorption capacity. The results of the study showed that produced composite material is an alternative building material due to its desirable characteristics; low weight, capability of low heat conduction.« less

  4.  Thermal Insulation System Made of Wood and Paper for Use in Residential Construction

    Treesearch

    Zoltán Pásztory; Tibor Horváth; Samuel V. Glass; Samuel L. Zelinka

    2015-01-01

    This article introduces an insulation system that takes advantage of the low thermal conductivity of still air and is made of wood and paper. The insulation, called the Mirrorpanel, is constructed as a panel of closely spaced layers of coated paper and held together in a frame of wood or fiberboard. Panels have been fabricated and tested at the laboratory scale, whole...

  5. Insulating Cryogenic Pipes With Frost

    NASA Technical Reports Server (NTRS)

    Stephenson, J. G.; Bova, J. A.

    1985-01-01

    Crystallized water vapor fills voids in pipe insulation. Small, carefully controlled amount of water vapor introduced into dry nitrogen gas before it enters aft fuselage. Vapor freezes on pipes, filling cracks in insulation. Ice prevents gaseous nitrogen from condensing on pipes and dripping on structure, in addition to helping to insulate all parts. Industrial applications include large refrigeration plants or facilities that use cryogenic liquids.

  6. Research on breakdown characteristics of converter transformer oil-paper insulation under compound electric field in alpine region

    NASA Astrophysics Data System (ADS)

    Xu, C.; Gao, Z. W.; Lan, S.; Guo, H. X.; Gong, M. C.

    2018-01-01

    In the paper, existing research and operating experience was summarized. On the basis, the particularity of oil-paper insulation operation condition for converter transformer was combined for studying the influence of temperature on oil-paper insulation field intensity distribution of converter transformers under different AC contents within wide temperature scope (-40°C∼105°C). The law of temperature gradients on space charge accumulation was analyzed. The breakdown or flashover characteristics of typical oil-paper compound insulation structure under the action of DC, AC and AC-DC superposition voltage at different temperatures were explored. The design principles of converter transformer oil-paper insulation structures in alpine region was proposed. The principle was adjusted and optimized properly according to the operation temperature scope and withstood AC-DC proportion. The reliability of transformer operation was improved on the one hand, and the insulating medium can be rationally utilized for reducing the manufacturing cost of the transformer on the other hand.

  7. Thermal Aging Characteristics of Insulation Paper in Mineral Oil under Overloaded Operating Transformers

    NASA Astrophysics Data System (ADS)

    Miyagi, Katsunori; Oe, Etsuo; Yamagata, Naoki; Miyahara, Hideyuki

    A sudden capacity increase in demand during the summer peak, or in contingencies such as malfunctioning transformers, may cause overload for normal transformers. In this paper, on the basis of examples of overloaded transformer operation in distributing substations, thermal aging testing in oil was carried out under various overload patterns, such as short time overload and long time overload, but with the winding insulation paper's life loss kept constant. From the results, various characteristics such as mean degree of polymerization and productions of furfural and (CO2+CO), and their effects on the life loss of the insulation paper were obtained.

  8. ION COMPOSITION ELUCIDATION (ICE): AN INVESTIGATIVE ...

    EPA Pesticide Factsheets

    Ion Composition Elucidation (ICE) often leads to identification of compounds and provides high quality evidence for tracking compounds to their sources. Mass spectra for most organic compounds are not found in mass spectral libraries used to tentatively identify analytes. In addition, multiple matches are common. Ion Composition Elucidation provides the numbers of atoms of each element in the ions in the mass spectrum, greatly limiting the number of possible compounds that could produce the mass spectrum. Review of chemical and commercial literature then limits the number of possible compounds to one or a few that can be purchased to confirm tentative compound identifications by comparison of mass spectra and chromatographic retention times. Ion Composition Elucidation is conceptually simple relative to other analytical techniques and more easily explained to a judge or jury. It is based on sums of the exact masses of atoms and their isotopic abundances. Several applications of ICE are demonstrated for ultra-trace-level compounds in an extract of the effluent from a tertiary sewage treatment plant including: (i) measurement of five values to determine an ion's composition and to generate evidence for the compound's identity, (ii) rejection of incorrect library matches, (iii) rapid screening for a target compound in an extract, and (iv) a strategy for tracking unidentified compounds to their sources. The research focused on in the subtasks is the development and

  9. Use of high temperature insulation for ceramic matrix composites in gas turbines

    DOEpatents

    Morrison, Jay Alan; Merrill, Gary Brian; Ludeman, Evan McNeil; Lane, Jay Edgar

    2001-01-01

    A ceramic composition for insulating components, made of ceramic matrix composites, of gas turbines is provided. The composition comprises a plurality of hollow oxide-based spheres of various dimensions, a phosphate binder, and at least one oxide filler powder, whereby the phosphate binder partially fills gaps between the spheres and the filler powders. The spheres are situated in the phosphate binder and the filler powders such that each sphere is in contact with at least one other sphere and the arrangement of spheres is such that the composition is dimensionally stable and chemically stable at a temperature of approximately 1600.degree. C. A stationary vane of a gas turbine comprising the composition of the present invention bonded to the outer surface of the vane is provided. A combustor comprising the composition bonded to the inner surface of the combustor is provided. A transition duct comprising the insulating coating bonded to the inner surface of the transition is provided. Because of abradable properties of the composition, a gas turbine blade tip seal comprising the composition also is provided. The composition is bonded to the inside surface of a shroud so that a blade tip carves grooves in the composition so as to create a customized seal for the turbine blade tip.

  10. An active bacterial community linked to high chl-a concentrations in Antarctic winter-pack ice and evidence for the development of an anaerobic sea-ice bacterial community.

    PubMed

    Eronen-Rasimus, Eeva; Luhtanen, Anne-Mari; Rintala, Janne-Markus; Delille, Bruno; Dieckmann, Gerhard; Karkman, Antti; Tison, Jean-Louis

    2017-10-01

    Antarctic sea-ice bacterial community composition and dynamics in various developmental stages were investigated during the austral winter in 2013. Thick snow cover likely insulated the ice, leading to high (<4 μg l -1 ) chlorophyll-a (chl-a) concentrations and consequent bacterial production. Typical sea-ice bacterial genera, for example, Octadecabacter, Polaribacter and Glaciecola, often abundant in spring and summer during the sea-ice algal bloom, predominated in the communities. The variability in bacterial community composition in the different ice types was mainly explained by the chl-a concentrations, suggesting that as in spring and summer sea ice, the sea-ice bacteria and algae may also be coupled during the Antarctic winter. Coupling between the bacterial community and sea-ice algae was further supported by significant correlations between bacterial abundance and production with chl-a. In addition, sulphate-reducing bacteria (for example, Desulforhopalus) together with odour of H 2 S were observed in thick, apparently anoxic ice, suggesting that the development of the anaerobic bacterial community may occur in sea ice under suitable conditions. In all, the results show that bacterial community in Antarctic sea ice can stay active throughout the winter period and thus possible future warming of sea ice and consequent increase in bacterial production may lead to changes in bacteria-mediated processes in the Antarctic sea-ice zone.

  11. Cosmic ray spectrum, composition, and anisotropy measured with IceCube

    NASA Astrophysics Data System (ADS)

    Tamburro, Alessio

    2014-04-01

    Analysis of cosmic ray surface data collected with the IceTop array of Cherenkov detectors at the South Pole provides an accurate measurement of the cosmic ray spectrum and its features in the "knee" region up to energies of about 1 EeV. IceTop is part of the IceCube Observatory that includes a deep-ice cubic kilometer detector that registers signals of penetrating muons and other particles. Surface and in-ice signals detected in coincidence provide clear insights into the nuclear composition of cosmic rays. IceCube already measured an increase of the average primary mass as a function of energy. We present preliminary results on both IceTop-only and coincident events analysis. Furthermore, we review the recent measurement of the cosmic ray anisotropy with IceCube.

  12. Cryogenic Insulation System for Soft Vacuum

    NASA Technical Reports Server (NTRS)

    Augustynowicz, S. D.; Fesmire, J. E.

    1999-01-01

    The development of a cryogenic insulation system for operation under soft vacuum is presented in this paper. Conventional insulation materials for cryogenic applications can be divided into three levels of thermal performance, in terms of apparent thermal conductivity [k-value in milliwatt per meter-kelvin (mW/m-K)]. System k-values below 0.1 can be achieved for multilayer insulation operating at a vacuum level below 1 x 10(exp -4) torr. For fiberglass or powder operating below 1 x 10(exp -3) torr, k-values of about 2 are obtained. For foam and other materials at ambient pressure, k-values around 30 are typical. New industry and aerospace applications require a versatile, robust, low-cost thermal insulation with performance in the intermediate range. The target for the new composite insulation system is a k-value below 4.8 mW/m-K (R-30) at a soft vacuum level (from 1 to 10 torr) and boundary temperatures of approximately 77 and 293 kelvin (K). Many combinations of radiation shields, spacers, and composite materials were tested from high vacuum to ambient pressure using cryostat boiloff methods. Significant improvement over conventional systems in the soft vacuum range was demonstrated. The new layered composite insulation system was also shown to provide key benefits for high vacuum applications as well.

  13. Cosmic ray composition and energy spectrum from 1-30 PeV using the 40-string configuration of IceTop and IceCube

    NASA Astrophysics Data System (ADS)

    IceCube Collaboration; Abbasi, R.; Abdou, Y.; Ackermann, M.; Adams, J.; Aguilar, J. A.; Ahlers, M.; Altmann, D.; Andeen, K.; Auffenberg, J.; Bai, X.; Baker, M.; Barwick, S. W.; Baum, V.; Bay, R.; Beattie, K.; Beatty, J. J.; Bechet, S.; Becker, J. K.; Becker, K.-H.; Bell, M.; Benabderrahmane, M. L.; BenZvi, S.; Berdermann, J.; Berghaus, P.; Berley, D.; Bernardini, E.; Bertrand, D.; Besson, D. Z.; Bindig, D.; Bissok, M.; Blaufuss, E.; Blumenthal, J.; Boersma, D. J.; Bohm, C.; Bose, D.; Böser, S.; Botner, O.; Brayeur, L.; Brown, A. M.; Bruijn, R.; Brunner, J.; Buitink, S.; Caballero-Mora, K. S.; Carson, M.; Casey, J.; Casier, M.; Chirkin, D.; Christy, B.; Clevermann, F.; Cohen, S.; Cowen, D. F.; Silva, A. H. Cruz; Danninger, M.; Daughhetee, J.; Davis, J. C.; De Clercq, C.; Descamps, F.; Desiati, P.; de Vries-Uiterweerd, G.; DeYoung, T.; Díaz-Vélez, J. C.; Dreyer, J.; Dumm, J. P.; Dunkman, M.; Eagan, R.; Eisch, J.; Ellsworth, R. W.; Engdegård, O.; Euler, S.; Evenson, P. A.; Fadiran, O.; Fazely, A. R.; Fedynitch, A.; Feintzeig, J.; Feusels, T.; Filimonov, K.; Finley, C.; Fischer-Wasels, T.; Flis, S.; Franckowiak, A.; Franke, R.; Frantzen, K.; Fuchs, T.; Gaisser, T. K.; Gallagher, J.; Gerhardt, L.; Gladstone, L.; Glüsenkamp, T.; Goldschmidt, A.; Goodman, J. A.; Góra, D.; Grant, D.; Groß, A.; Grullon, S.; Gurtner, M.; Ha, C.; Ismail, A. Haj; Hallgren, A.; Halzen, F.; Hanson, K.; Heereman, D.; Heimann, P.; Heinen, D.; Helbing, K.; Hellauer, R.; Hickford, S.; Hill, G. C.; Hoffman, K. D.; Hoffmann, R.; Homeier, A.; Hoshina, K.; Huelsnitz, W.; Hulth, P. O.; Hultqvist, K.; Hussain, S.; Ishihara, A.; Jacobi, E.; Jacobsen, J.; Japaridze, G. S.; Jlelati, O.; Johansson, H.; Kappes, A.; Karg, T.; Karle, A.; Kiryluk, J.; Kislat, F.; Kläs, J.; Klein, S. R.; Köhne, J.-H.; Kohnen, G.; Kolanoski, H.; Köpke, L.; Kopper, C.; Kopper, S.; Koskinen, D. J.; Kowalski, M.; Krasberg, M.; Kroll, G.; Kunnen, J.; Kurahashi, N.; Kuwabara, T.; Labare, M.; Laihem, K.; Landsman, H.; Larson, M. J.; Lauer, R.; Lesiak-Bzdak, M.; Lünemann, J.; Madsen, J.; Maruyama, R.; Mase, K.; Matis, H. S.; McNally, F.; Meagher, K.; Merck, M.; Mészáros, P.; Meures, T.; Miarecki, S.; Middell, E.; Milke, N.; Miller, J.; Mohrmann, L.; Montaruli, T.; Morse, R.; Movit, S. M.; Nahnhauer, R.; Naumann, U.; Nowicki, S. C.; Nygren, D. R.; Obertacke, A.; Odrowski, S.; Olivas, A.; Olivo, M.; O'Murchadha, A.; Panknin, S.; Paul, L.; Pepper, J. A.; de los Heros, C. Pérez; Pieloth, D.; Pirk, N.; Posselt, J.; Price, P. B.; Przybylski, G. T.; Rädel, L.; Rawlins, K.; Redl, P.; Resconi, E.; Rhode, W.; Ribordy, M.; Richman, M.; Riedel, B.; Rodrigues, J. P.; Rothmaier, F.; Rott, C.; Ruhe, T.; Rutledge, D.; Ruzybayev, B.; Ryckbosch, D.; Salameh, T.; Sander, H.-G.; Santander, M.; Sarkar, S.; Saba, S. M.; Schatto, K.; Scheel, M.; Scheriau, F.; Schmidt, T.; Schmitz, M.; Schoenen, S.; Schöneberg, S.; Schönherr, L.; Schönwald, A.; Schukraft, A.; Schulte, L.; Schulz, O.; Seckel, D.; Seo, S. H.; Sestayo, Y.; Seunarine, S.; Smith, M. W. E.; Soiron, M.; Soldin, D.; Spiczak, G. M.; Spiering, C.; Stamatikos, M.; Stanev, T.; Stasik, A.; Stezelberger, T.; Stokstad, R. G.; Stößl, A.; Strahler, E. A.; Ström, R.; Sullivan, G. W.; Taavola, H.; Taboada, I.; Tamburro, A.; Ter-Antonyan, S.; Tilav, S.; Toale, P. A.; Toscano, S.; Usner, M.; van Eijndhoven, N.; van der Drift, D.; Van Overloop, A.; van Santen, J.; Vehring, M.; Voge, M.; Walck, C.; Waldenmaier, T.; Wallraff, M.; Walter, M.; Wasserman, R.; Weaver, Ch.; Wendt, C.; Westerhoff, S.; Whitehorn, N.; Wiebe, K.; Wiebusch, C. H.; Williams, D. R.; Wissing, H.; Wolf, M.; Wood, T. R.; Woschnagg, K.; Xu, C.; Xu, D. L.; Xu, X. W.; Yanez, J. P.; Yodh, G.; Yoshida, S.; Zarzhitsky, P.; Ziemann, J.; Zilles, A.; Zoll, M.

    2013-02-01

    The mass composition of high energy cosmic rays depends on their production, acceleration, and propagation. The study of cosmic ray composition can therefore reveal hints of the origin of these particles. At the South Pole, the IceCube Neutrino Observatory is capable of measuring two components of cosmic ray air showers in coincidence: the electromagnetic component at high altitude (2835 m) using the IceTop surface array, and the muonic component above ˜1 TeV using the IceCube array. This unique detector arrangement provides an opportunity for precision measurements of the cosmic ray energy spectrum and composition in the region of the knee and beyond. We present the results of a neural network analysis technique to study the cosmic ray composition and the energy spectrum from 1 PeV to 30 PeV using data recorded using the 40-string/40-station configuration of the IceCube Neutrino Observatory.

  14. Evaluation of cryogenic insulation materials and composites for use in nuclear radiation environments

    NASA Technical Reports Server (NTRS)

    Bullock, R. E.

    1972-01-01

    The following subjects are studied: (1) composite materials tests; (2) test of liquid level sensors and fission couples; (3) test of valve-seal materials; (4) boron epoxy composites; (5) radiation analysis of explosive materials and bifuels for RNS applications; and (6) test of thermal insulation.

  15. Recent Progress in Electrical Insulation Techniques for HTS Power Apparatus

    NASA Astrophysics Data System (ADS)

    Hayakawa, Naoki; Kojima, Hiroki; Hanai, Masahiro; Okubo, Hitoshi

    This paper describes the electrical insulation techniques at cryogenic temperatures, i.e. Cryodielectrics, for HTS power apparatus, e.g. HTS power transmission cables, transformers, fault current limiters and SMES. Breakdown and partial discharge characteristics are discussed for different electrical insulation configurations of LN2, sub-cooled LN2, solid, vacuum and their composite insulation systems. Dynamic and static insulation performances with and without taking account of quench in HTS materials are also introduced.

  16. Thermal performance of multilayer insulations. [gas evacuation characteristics of three selected multilayer insulation composites

    NASA Technical Reports Server (NTRS)

    Keller, C. W.; Cunnington, G. R.; Glassford, A. P.

    1974-01-01

    Experimental and analytical studies were conducted in order to extend previous knowledge of the thermal performance and gas evacuation characteristics of three selected multilayer insulation (MLI) composites. Flat plate calorimeter heat flux measurements were obtained for 20- and 80- shield specimens using three representative layer densities over boundary temperatures ranging from 39 K (70 R) to 389 K (700 R). Laboratory gas evacuation tests were performed on representative specimens of each MLI composite after initially purging them with helium, nitrogen, or argon gases. In these tests, the specimens were maintained at temperatures between 128 K (230 R) and 300 K (540 R). Based on the results of the laboratory-scale tests, a composite MLI system consisting of 112 unperforated, double-aluminized Mylar reflective shields and 113 water preconditioned silk net spacer pairs was fabricated and installed on a 1.22-m-(4-ft-) diameter calorimeter tank.

  17. Thermal Insulation Strips Conserve Energy

    NASA Technical Reports Server (NTRS)

    2009-01-01

    Launching the space shuttle involves an interesting paradox: While the temperatures inside the shuttle s main engines climb higher than 6,000 F hot enough to boil iron for fuel, the engines use liquid hydrogen, the second coldest liquid on Earth after liquid helium. Maintained below 20 K (-423 F), the liquid hydrogen is contained in the shuttle s rust-colored external tank. The external tank also contains liquid oxygen (kept below a somewhat less chilly 90 K or -297 F) that combines with the hydrogen to create an explosive mixture that along with the shuttle s two, powdered aluminum-fueled solid rocket boosters allows the shuttle to escape Earth s gravity. The cryogenic temperatures of the main engines liquid fuel can cause ice, frost, or liquefied air to build up on the external tank and other parts of the numerous launch fueling systems, posing a possible debris risk when the ice breaks off during launch and causing difficulties in the transfer and control of these cryogenic liquid propellants. Keeping the fuel at the necessary ultra-cold temperatures while minimizing ice buildup and other safety hazards, as well as reducing the operational maintenance costs, has required NASA to explore innovative ways for providing superior thermal insulation systems. To address the challenge, the Agency turned to an insulating technology so effective that, even though it is mostly air, a thin sheet can prevent a blowtorch from igniting a match. Aerogels were invented in 1931 and demonstrate properties that make them the most extraordinary insulating materials known; a 1-inch-thick piece of aerogel provides the same insulation as layering 15 panes of glass with air pockets in between. Derived from silica, aluminum oxide, or carbon gels using a supercritical drying process - resulting in a composition of almost 99-percent air - aerogels are the world s lightest solid (among 15 other titles they hold in the Guinness World Records), can float indefinitely on water if treated to be

  18. Densification control and analysis of outer shell of new high-temperature vacuum insulated composite

    NASA Astrophysics Data System (ADS)

    Wang, Yang; Chen, Zhaofeng; Jiang, Yun; Yu, Shengjie; Xu, Tengzhou; Li, Binbin; Chen, Zhou

    2017-11-01

    A novel high temperature vacuum insulated composite with low thermal conductivity composed of SiC foam core material and sealing outer shell is discussed, which will have a great potential to be used as thermal protection system material. In this composite, the outer shell is the key to maintain its internal vacuum, which is consisted of 2.5D C/C and SiC coating. So the densification processes of outer shell, including 2.5D braiding process, chemical vapor infiltration (CVI) pyrolytic carbon (PyC) process, polymer infiltration and pyrolysis (PIP) glassy carbon (GC) process and chemical vapor deposition (CVD) SiC process, are focused in this paper. The measuring result of the gas transmission quantity of outer shell is only 0.14 cm3/m2 · d · Pa after 5 times CVD processes, which is two order of magnitude lower than that sample deposited one time. After 10 times thermal shock cycles, the gas transmission quantity increases to 1.2 cm3/m2 · d · Pa. The effective thermal conductivity of high temperature vacuum insulated composite ranged from 0.19 W m-1 K-1 to 0.747 W m-1 K-1 within the temperature from 20 °C to 900 °C. Even after 10 thermal shock cycles, the variation of the effective thermal conductivity is still consistent with that without treatments.

  19. High friction on ice provided by elastomeric fiber composites with textured surfaces

    NASA Astrophysics Data System (ADS)

    Rizvi, R.; Naguib, H.; Fernie, G.; Dutta, T.

    2015-03-01

    Two main applications requiring high friction on ice are automobile tires and footwear. The main motivation behind the use of soft rubbers in these applications is the relatively high friction force generated between a smooth rubber contacting smooth ice. Unfortunately, the friction force between rubber and ice is very low at temperatures near the melting point of ice and as a result we still experience automobile accidents and pedestrian slips and falls in the winter. Here, we report on a class of compliant fiber-composite materials with textured surfaces that provide outstanding coefficients of friction on wet ice. The fibrous composites consist of a hard glass-fiber phase reinforcing a compliant thermoplastic polyurethane matrix. The glass-fiber phase is textured such that it is aligned transversally and protruding out of the elastomer surface. Our analysis indicates that the exposed fiber phase exhibits a "micro-cleat" effect, allowing for it to fracture the ice and increase the interfacial contact area thereby requiring a high force to shear the interface.

  20. Development of advanced materials composites for use as insulations for LH2 tanks

    NASA Technical Reports Server (NTRS)

    Lemons, C. R.; Salmassy, O. K.

    1973-01-01

    A study of thread-reinforced polyurethane foam and glass fabric liner, serving as internally bonded insulation for space shuttle LH2 tanks, is reported. Emphasis was placed on an insulation system capable of reentry and multiple reuse in the shuttle environment. The optimized manufacturing parameters associated with each element of the composite are established and the results, showing successful completion of subscale system evaluation tests using the shuttle flight environmental requirements, are given.

  1. Macroporous Calcium Phosphate/Chitosan Composites Prepared via Unidirectional Ice Segregation and Subsequent Freeze-Drying

    PubMed Central

    Aranaz, Inmaculada; Martínez-Campos, Enrique; Moreno-Vicente, Carolina; Civantos, Ana; García-Arguelles, Sara; del Monte, Francisco

    2017-01-01

    Calcium phosphate chitosan-based composites have gained much interest in recent years for biomedical purposes. In this paper, three-dimensional calcium phosphate chitosan-based composites with different mineral contents were produced using a green method called ice segregation induced self-assembly (ISISA). In this methodology, ice crystals were used as a template to produce porous structures from an aqueous solution of chitosan (CS) and hydroxyapatite (Hap) also containing acetic acid (pH = 4.5). For better characterization of the nature of the inorganic matter entrapped within the resulting composite, we performed either oxygen plasma or calcination processes to remove the organic matter. The nature of the phosphate salts was studied by XRD and NMR studies. Amorphous calcium phosphate (ACP) was identified as the mineral phase in the composites submitted to oxygen plasma, whereas crystalline Hap was obtained after calcination. SEM microscopy revealed the formation of porous structures (porosity around 80–85%) in the original composites, as well as in the inorganic matrices obtained after calcination, with porous channels of up to 50 µm in diameter in the former case and of up to 20 µm in the latter. The biocompatibility of the composites was assessed using two different cell lines: C2C12GFP premyoblastic cells and MC3T3 preosteoblastic cells. PMID:28772874

  2. Surface ices and the atmospheric composition of Pluto

    NASA Technical Reports Server (NTRS)

    Owen, Tobias C.; Roush, Ted L.; Cruikshank, Dale P.; Elliot, James L.; Young, Leslie A.; De Bergh, Catherine; Schmitt, Bernard; Geballe, Thomas R.; Brown, Robert H.; Bartholomew, Mary J.

    1993-01-01

    Observations of the 1.4- to 2.4-micrometer spectrum of Pluto reveal absorptions of carbon monoxide and nitrogen ices and confirm the presence of solid methane. Frozen nitrogen is more abundant than the other two ices by a factor of about 50; gaseous nitrogen must therefore be the major atmospheric constituent. The absence of carbon dioxide absorptions is one of several differences between the spectra of Pluto and Triton in this region. Both worlds carry information about the composition of the solar nebula and the processes by which icy planetesimals formed.

  3. Anti-icing properties of superhydrophobic ZnO/PDMS composite coating

    NASA Astrophysics Data System (ADS)

    Yang, Chao; Wang, Fajun; Li, Wen; Ou, Junfei; Li, Changquan; Amirfazli, Alidad

    2016-01-01

    We present the excellent anti-icing performance for a superhydrophobic coating surface based on ZnO/polydimethylsiloxane (ZnO/PDMS) composite. The superhydrophobic ZnO/PDMS coating surface was prepared by a facile solution mixing, drop coating, room-temperature curing and surface abrading procedure. The superhydrophobic ZnO/PDMS composite coating possesses a water contact angle of 159.5° and a water sliding angle of 8.3° at room temperature (5 °C). The anti-icing properties of the superhydrophobic coating were investigated by continuously dropping cold-water droplets (about 0 °C) onto the pre-cooled surface using a home-made apparatus. The sample was placed at different tilting angle (0° and 10°) and pre-cooled to various temperatures (-5, -10 and -15 °C) prior to measure. The pure Al surface was also studied for comparison. It was found that icing accretion on the surface could be reduced apparently because the water droplets merged together and slid away from the superhydrophobic surface at all of the measuring temperatures when the surface is horizontally placed. In addition, water droplet slid away completely from the superhydrophobic surface at -5 and -10 °C when the surface is tilted at 10°, which demonstrates its excellent anti-icing properties at these temperatures. When the temperature decreased to -15 °C, though ice accretion on the tilted superhydrophobic coating surface could not be avoided absolutely, the amount of ice formed on the surface is very small, which indicated that the coating surface with superhydrophobicity could significantly reduce ice accumulation on the surface at very low temperature (-15 °C). Importantly, the sample is also stable against repeated icing/deicing cycles. More meaningfully, once the superhydrophobic surface is damaged, it can be repaired easily and rapidly.

  4. Multifunctional carbon nano-paper composite

    NASA Astrophysics Data System (ADS)

    Zhang, Zhichun; Chu, Hetao; Wang, Kuiwen; Liu, Yanjv; Leng, Jinsong

    2013-08-01

    Carbon Nanotube (CNT), for its excellent mechanical, electrical properties and nano size, large special surface physical property, become the most promising material. But carbon nanotube can still fabricated in micro dimension, and can't be made into macro size, so to the carbon nanotube filled composite can't explore the properties of the CNT. Carbon nano-paper is made of pure CNT, with micro pore, and it turn micro sized CNT into macro shaped membrane. Based on the piezo-resistivity and electrical conductivity of the carbon nano-paper, we used the carbon nano-paper as functional layers fabricate functional composite, and studies its strain sensing, composite material deicing and shape memory polymer (SMP) material electric actuation performance. The results shown that the resin can pregnant the nano paper, and there was good bond for nano paper and composite. The functional composite can monitoring the strain with high sensitivity comparing to foil strain gauge. The functional composite can be heated via the carbon nano paper with low power supply and high heating rate. The composite has good deicing and heat actuation performance to composite material. For the good strain sensing, electric conductivity and self-heating character of the carbon nano-paper composite, it can be used for self sensing, anti lightning strike and deicing of composite materials in aircrafts and wind turbine blades.

  5. Thermal Performance Of Space Suit Elements With Aerogel Insulation For Moon And Mars Exploration

    NASA Technical Reports Server (NTRS)

    Tang, Henry H.; Orndoff, Evelyne S.; Trevino, Luis A.

    2006-01-01

    Flexible fiber-reinforced aerogel composites were studied for use as insulation materials of a future space suit for Moon and Mars exploration. High flexibility and good thermal insulation properties of fiber-reinforced silica aerogel composites at both high and low vacuum conditions make it a promising insulation candidate for the space suit application. This paper first presents the results of a durability (mechanical cycling) study of these aerogels composites in the context of retaining their thermal performance. The study shows that some of these Aerogels materials retained most of their insulation performance after up to 250,000 cycles of mechanical flex cycling. This paper also examines the problem of integrating these flexible aerogel composites into the current space suit elements. Thermal conductivity evaluations are proposed for different types of aerogels space suit elements to identify the lay-up concept that may have the best overall thermal performance for both Moon and Mars environments. Potential solutions in mitigating the silica dusting issue related to the application of these aerogels materials for the space suit elements are also discussed.

  6. Importance of Chemical Composition of Ice Nuclei on the Formation of Arctic Ice Clouds

    NASA Astrophysics Data System (ADS)

    Keita, Setigui Aboubacar; Girard, Eric

    2016-09-01

    Ice clouds play an important role in the Arctic weather and climate system but interactions between aerosols, clouds and radiation remain poorly understood. Consequently, it is essential to fully understand their properties and especially their formation process. Extensive measurements from ground-based sites and satellite remote sensing reveal the existence of two Types of Ice Clouds (TICs) in the Arctic during the polar night and early spring. TICs-1 are composed by non-precipitating small (radar-unseen) ice crystals of less than 30 μm in diameter. The second type, TICs-2, are detected by radar and are characterized by a low concentration of large precipitating ice crystals ice crystals (>30 μm). To explain these differences, we hypothesized that TIC-2 formation is linked to the acidification of aerosols, which inhibits the ice nucleating properties of ice nuclei (IN). As a result, the IN concentration is reduced in these regions, resulting to a lower concentration of larger ice crystals. Water vapor available for deposition being the same, these crystals reach a larger size. Current weather and climate models cannot simulate these different types of ice clouds. This problem is partly due to the parameterizations implemented for ice nucleation. Over the past 10 years, several parameterizations of homogeneous and heterogeneous ice nucleation on IN of different chemical compositions have been developed. These parameterizations are based on two approaches: stochastic (that is nucleation is a probabilistic process, which is time dependent) and singular (that is nucleation occurs at fixed conditions of temperature and humidity and time-independent). The best approach remains unclear. This research aims to better understand the formation process of Arctic TICs using recently developed ice nucleation parameterizations. For this purpose, we have implemented these ice nucleation parameterizations into the Limited Area version of the Global Multiscale Environmental Model

  7. Breakdown Characteristic Analysis of Paper- Oil Insulation under AC and DC Voltage

    NASA Astrophysics Data System (ADS)

    Anuar, N. F.; Jamail, N. A. M.; Rahman, R. A.; Kamarudin, M. S.

    2017-08-01

    This paper presents the study of breakdown characteristic of Kraft paper insulated with two different types of insulating fluid, which are Palm oil and Coconut oil. Palm oil and Coconut oil are chosen as the alternative fluid to the transformer oil because it has high potential and environmentally-friendly. The Segezha Kraft papers with various thicknesses (65.5 gsm, 75 gsm, 85gsm, 90 gsm) have been used in this research. High Voltage Direct Current (HVDC), High Voltage Alternating Current (HVAC) and carbon track and severity analysis is conducted to observe the sample of aging Kraft paper. These samples have been immersed using Palm oil and Coconut oil up to 90 days to observe the absorption rate. All samples started to reach saturation level at 70 days of immersion. HVDC and HVAC breakdown experiments have been done after the samples had reached the saturation level based on normal condition, immersed in Palm oil and immersed in Coconut oil. All samples immersed in liquid show different breakdown voltage reading compared to normal condition. The analysis of carbon track and severity on surface has been done using Analytical Scanning Electron Microscope (SEM) Analysis. The results of the experiment show that the sample of Kraft paper immersed in Palm oil was better than Coconut oil immersed sample. Therefore the sample condition was the main factor that determines the value of breakdown voltage test. Introduction

  8. The Effects of Snow Depth Forcing on Southern Ocean Sea Ice Simulations

    NASA Technical Reports Server (NTRS)

    Powel, Dylan C.; Markus, Thorsten; Stoessel, Achim

    2003-01-01

    The spatial and temporal distribution of snow on sea ice is an important factor for sea ice and climate models. First, it acts as an efficient insulator between the ocean and the atmosphere, and second, snow is a source of fresh water for altering the already weak Southern Ocean stratification. For the Antarctic, where the ice thickness is relatively thin, snow can impact the ice thickness in two ways: a) As mentioned above snow on sea ice reduces the ocean-atmosphere heat flux and thus reduces freezing at the base of the ice flows; b) a heavy snow load can suppress the ice below sea level which causes flooding and, with subsequent freezing, a thickening of the sea ice (snow-to-ice conversion). In this paper, we compare different snow fall paramterizations (incl. the incorporation of satellite-derived snow depth) and study the effect on the sea ice using a sea ice model.

  9. Experimental and analytical study of the DC breakdown characteristics of polypropylene laminated paper with a butt gap condition considering the insulation design of superconducting cable

    NASA Astrophysics Data System (ADS)

    Seo, In-jin; Choi, Won; Seong, Jae-gyu; Lee, Bang-wook; Koo, Ja-yoon

    2014-08-01

    It has been reported that the insulation design under DC stress is considered as one of the critical factors in determining the performance of high-voltage direct current (HVDC) superconducting cable. Therefore, it is fundamentally necessary to investigate the DC breakdown characteristics of the composite insulation system consisting of liquid nitrogen (LN2)/polypropylene-laminated-paper (PPLP). In particular, the insulation characteristics under DC polarity reversal condition should be verified to understand the polarity effect of the DC voltage considering the unexpected incidents taking place at line-commutated-converters (LCC) under service at a DC power grid. In this study, to examine the variation of DC electric field strength, the step voltage and polarity reversal breakdown tests are performed under DC stress. Also, we investigate the electric field distributions in a butt gap of the LN2/PPLP condition considering the DC polarity reversal by using simulation software.

  10. Using of Aerogel to Improve Thermal Insulating Properties of Windows

    NASA Astrophysics Data System (ADS)

    Valachova, Denisa; Zdrazilova, Nada; Panovec, Vladan; Skotnicova, Iveta

    2018-06-01

    For the best possible thermal-technical properties of building structures it is necessary to use materials with very low thermal conductivity. Due to the increasing thermal-technical requirements for building structures, the insulating materials are developed. One of the modern thermal insulating materials is so-called aerogel. Unfortunately, this material is not used in the field of external thermal insulation composite systems because of its price and its properties. The aim of this paper is to present possibilities of using this insulating material in the civil engineering - specifically a usage of aerogel in the production of windows.

  11. Structural, compositional, and sensorial properties of United States commercial ice cream products.

    PubMed

    Warren, Maya M; Hartel, Richard W

    2014-10-01

    Commercial vanilla ice cream products from the United States (full fat, low fat, and nonfat) were analyzed for their structural, behavioral (i.e., melt rate and drip-through), compositional, and sensorial attributes. Mean size distributions of ice crystals and air cells, drip-through rates, percent partially coalesced fat, percent overrun and total fat, and density were determined. A trained panel carried out sensory analyses in order to determine correlations between ice cream microstructure attributes and sensory properties using a Spectrum(TM) descriptive analysis. Analyses included melt rate, breakdown, size of ice particulates (iciness), denseness, greasiness, and overall creaminess. To determine relationships and interactions, principle component analysis and multivariate pairwise correlation were performed within and between the instrumental and sensorial data. Greasiness and creaminess negatively correlated with drip-through rate and creaminess correlated with percent total fat and percent fat destabilization. Percent fat did not determine the melt rate on a sensorial level. However, drip-through rate at ambient temperatures was predicted by total fat content of the samples. Based on sensory analysis, high-fat products were noted to be creamier than low and nonfat products. Iciness did not correlate with mean ice crystal size and drip-through rate did not predict sensory melt rate. Furthermore, on a sensorial level, greasiness positively correlated with total percent fat destabilization and mean air cell size positively correlated with denseness. These results indicate that commercial ice cream products vary widely in composition, structure, behavior, and sensory properties. There is a wide range of commercial ice creams in the United States market, ranging from full fat to nonfat. In this research we showed that these ice creams vary greatly in their microstructures, behaviors (the melt/drip-though, collapse, and/or stand up properties of ice cream

  12. Composite aerogel insulation for cryogenic liquid storage

    NASA Astrophysics Data System (ADS)

    Kyeongho, Kim; Hyungmook, Kang; Soojin, Shin; In Hwan, Oh; Changhee, Son; Hyung, Cho Yun; Yongchan, Kim; Sarng Woo, Karng

    2017-02-01

    High porosity materials such as aerogel known as a good insulator in a vacuum range (10-3 ∼ 1 Torr) was widely used to storage and to transport cryogenic fluids. It is necessary to be investigated the performance of aerogel insulations for cryogenic liquid storage in soft vacuum range to atmospheric pressure. A one-dimensional insulating experimental apparatus was designed and fabricated to consist of a cold mass tank, a heat absorber and an annular vacuum space with 5-layer (each 10 mm thickness) of the aerogel insulation materials. Aerogel blanket for cryogenic (used maximum temperature is 400K), aerogel blanket for normal temperature (used maximum temperature is 923K), and combination of the two kinds of aerogel blankets were 5-layer laminated between the cryogenic liquid wall and the ambient wall in vacuum space. Also, 1-D effective thermal conductivities of the insulation materials were evaluated by measuring boil-off rate from liquid nitrogen and liquid argon. In this study, the effective thermal conductivities and the temperature-thickness profiles of the two kinds of insulators and the layered combination of the two different aerogel blankets were presented.

  13. Test results of Thermal Ice Cap prototype and final comments. Final report

    DOE Office of Scientific and Technical Information (OSTI.GOV)

    Burley, W.

    1982-01-01

    The design and testing of an insulating cover, Ice Cap, for an ice rink are described. The radio-controlled reel system which houses, deploys, and harvests the 17,000 square feet of insulating material is essential to the success of the cover. Photographs showing the use of the system are included. (MHR)

  14. In-situ single submicron particle composition analysis of ice residuals from mountain-top mixed-phase clouds in Central Europe

    NASA Astrophysics Data System (ADS)

    Schmidt, S.; Schneider, J.; Klimach, T.; Mertes, S.; Schenk, L. P.; Curtius, J.; Kupiszewski, P.; Hammer, E.; Vochezer, P.; Lloyd, G.; Ebert, M.; Kandler, K.; Weinbruch, S.; Borrmann, S.

    2015-02-01

    This paper presents results from the "INUIT-JFJ/CLACE 2013" field campaign at the high alpine research station Jungfraujoch in January/February 2013. The chemical composition of ice particle residuals (IPR) in a size diameter range of 200-900 nm was measured in orographic, convective and non-convective clouds with a single particle mass spectrometer (ALABAMA) under ambient conditions characterized by temperatures between -28 and -4 °C and wind speed from 0.1 to 21 km h-1. Additionally, background aerosol particles in cloud free air were investigated. The IPR were sampled from mixed-phase clouds with two inlets which selectively extract small ice crystals in-cloud, namely the Counterflow Virtual Impactor (Ice-CVI) and the Ice Selective Inlet (ISI). The IPR as well as the aerosol particles were classified into seven different particle types: (1) black carbon, (2) organic carbon, (3) black carbon internally mixed with organic carbon, (4) minerals, (5) one particle group (termed "BioMinSal") that may contain biological particles, minerals, or salts, (6) industrial metals, and (7) lead containing particles. For any sampled particle population it was determined by means of single particle mass spectrometer how many of the analyzed particles belonged to each of these categories. Accordingly, between 20 and 30% of the IPR and roughly 42% of the background particles contained organic carbon. The measured fractions of minerals in the IPR composition varied from 6 to 33%, while the values for the "BioMinSal" group were between 15 and 29%. Four percent to 31% of the IPR contained organic carbon mixed with black carbon. Both inlets delivered similar results of the chemical composition and of the particle size distribution, although lead was found only in the IPR sampled by the Ice-CVI. The results show that the ice particle residual composition varies substantially between different cloud events, which indicates the influence of different meteorological conditions, such as

  15. Development of a cellulose-based insulating composite material for green buildings: Case of treated organic waste (paper, cardboard, hash)

    NASA Astrophysics Data System (ADS)

    Ouargui, Ahmed; Belouaggadia, Naoual; Elbouari, Abdeslam; Ezzine, Mohammed

    2018-05-01

    Buildings are responsible for 36% of the final energy consumption in Morocco [1-2], and a reduction of this energy consumption of buildings is a priority for the kingdom in order to reach its energy saving goals. One of the most effective actions to reduce energy consumption is the selection and development of innovative and efficient building materials [3]. In this work, we present an experimental study of the effect of adding treated organic waste (paper, cardboard, hash) on mechanical and thermal properties of cement and clay bricks. Thermal conductivity, specific heat and mechanical resistance were investigated in terms of content and size additives. Soaking time and drying temperature were also taken into account. The results reveal that thermal conductivity decreases as well in the case of the paper-cement mixture as that of the paper-clay and seems to stabilize around 40%. In the case of the composite paper-cement, it is found that, for an additives quantity exceeding 15%, the compressive strength exceeds the standard for the hollow non-load bearing masonry. However, the case of paper-clay mixture seems to give more interesting results, related to the compressive strength, for a mass composition of 15% in paper. Given the positive results achieved, it seems possible to use these composites for the construction of walls, ceilings and roofs of housing while minimizing the energy consumption of the building.

  16. Resistivity and resistivity fluctuations of thin-film platinum-aluminum oxide granular metal-insulator composites

    DOE Office of Scientific and Technical Information (OSTI.GOV)

    Mantese, J.V.

    1986-01-01

    Thin film metal-insulator composites were used to study how the resistivity and fluctuations in the resistivity were altered by changes in conduction mechanism so as to understand the source of the fluctuations and to better understand the conduction processes themselves. Metal-insulator composites were prepared by co-evaporation of platinum and aluminum oxide in a high vacuum system to create a series of films which had a range of metal volume fill fractions, p, from 23 to 100%. The samples were patterned using standard photolithographic techniques to form sample geometries of typical dimensions, length approx.40 ..mu..m, width approx.2 ..mu..m, and thickness approx.1500more » A. The resistivity rho, and power spectral density of the resistivity fluctuations, S/sub rho/(f), were measured as a function of p and temperature, T. Rho(p,T) was found to be a rapidly increasing function of decreasing p, rising monotonically by more than 7 orders of magnitude as p was decreased from 100% to 23%. For p greater than or equal to 59% the resistivity decreased linearly with decreasing temperature until limited by impurity scattering. The resistivities for the low metal fill fraction materials (P greater than or equal to 50%) increased as the temperature was reduced as expected of thermally assisted tunneling conduction in metal-insulator composites. The transition from metallic conduction to thermally assisted tunneling occurred at a critical value, p/sub c/, between 59% and 50% Pt.« less

  17. Monitoring on internal temperature of composite insulator with embedding fiber Bragg grating for early diagnosis

    NASA Astrophysics Data System (ADS)

    Chen, Wen; Tang, Ming

    2017-04-01

    The abnormal temperature rise is the precursor of the defective composite insulator in power transmission line. However no consolidated techniques or methodologies can on line monitor its internal temperature now. Thus a new method using embedding fiber Bragg grating (FBG) in fiber reinforced polymer (FRP) rod is adopted to monitor its internal temperature. To correctly demodulate the internal temperature of FRP rod from the Bragg wavelength shift of FBG, the conversion coefficient between them is deduced theoretically based on comprehensive investigation on the thermal stresses of the metal-composite joint, as well as its material and structural properties. Theoretical model shows that the conversion coefficients of FBG embedded in different positions will be different because of non-uniform thermal stress distribution, which is verified by an experiment. This work lays the theoretical foundation of monitoring the internal temperature of composite insulator with embedding FBG, which is of great importance to its health structural monitoring, especially early diagnosis.

  18. Application of composite flow laws to grain size distributions derived from polar ice cores

    NASA Astrophysics Data System (ADS)

    Binder, Tobias; de Bresser, Hans; Jansen, Daniela; Weikusat, Ilka; Garbe, Christoph; Kipfstuhl, Sepp

    2014-05-01

    Apart from evaluating the crystallographic orientation, focus of microstructural analysis of natural ice during the last decades has been to create depth-profiles of mean grain size. Several ice flow models incorporated mean grain size as a variable. Although such a mean value may coincide well with the size of a large proportion of the grains, smaller/larger grains are effectively ignored. These smaller/larger grains, however, may affect the ice flow modeling. Variability in grain size is observed on centimeter, meter and kilometer scale along deep polar ice cores. Composite flow laws allow considering the effect of this variability on rheology, by weighing the contribution of grain-size-sensitive (GSS, diffusion/grain boundary sliding) and grain-size-insensitive (GSI, dislocation) creep mechanisms taking the full grain size distribution into account [1]. Extraction of hundreds of grain size distributions for different depths along an ice core has become relatively easy by automatic image processing techniques [2]. The shallow ice approximation is widely adopted in ice sheet modeling and approaches the full-Stokes solution for small ratios of vertical to horizontal characteristic dimensions. In this approximation shear stress in the vertical plain dominates the strain. This assumption is not applicable at ice divides or dome structures, where most deep ice core drilling sites are located. Within the upper two thirds of the ice column longitudinal stresses are not negligible and ice deformation is dominated by vertical strain. The Dansgaard-Johnsen model [3] predicts a dominating, constant vertical strain rate for the upper two thirds of the ice sheet, whereas in the lower ice column vertical shear becomes the main driver for ice deformation. We derived vertical strain rates from the upper NEEM ice core (North-West Greenland) and compared them to classical estimates of strain rates at the NEEM site. Assuming intervals of constant accumulation rates, we found a

  19. Pre-cometary ice composition from hot core chemistry.

    PubMed

    Tornow, Carmen; Kührt, Ekkehard; Motschmann, Uwe

    2005-10-01

    Pre-cometary ice located around star-forming regions contains molecules that are pre-biotic compounds or pre-biotic precursors. Molecular line surveys of hot cores provide information on the composition of the ice since it sublimates near these sites. We have combined a hydrostatic hot core model with a complex network of chemical reactions to calculate the time-dependent abundances of molecules, ions, and radicals. The model considers the interaction between the ice and gas phase. It is applied to the Orion hot core where high-mass star formation occurs, and to the solar-mass binary protostar system IRAS 16293-2422. Our calculations show that at the end of the hot core phase both star-forming sites produce the same prebiotic CN-bearing molecules. However, in the Orion hot core these molecules are formed in larger abundances. A comparison of the calculated values with the abundances derived from the observed line data requires a chemically unprocessed molecular cloud as the initial state of hot core evolution. Thus, it appears that these objects are formed at a much younger cloud stage than previously thought. This implies that the ice phase of the young clouds does not contain CN-bearing molecules in large abundances before the hot core has been formed. The pre-biotic molecules synthesized in hot cores cause a chemical enrichment in the gas phase and in the pre-cometary ice. This enrichment is thought to be an important extraterrestrial aspect of the formation of life on Earth and elsewhere.

  20. Durability of crosslinked polydimethylsyloxanes: the case of composite insulators

    NASA Astrophysics Data System (ADS)

    Delor-Jestin, Florence; Tomer, Namrata S.; Pal Singh, Raj; Lacoste, Jacques

    2008-04-01

    Most applications of silicones are linked to their hydrophobic properties and (or) their high resistance to ageing (e.g. thermal ageing and photoageing). However, when placed in extreme environments, these materials can fail as in the case of epoxy/fiber glass composite powerlines insulators, where crosslinked polymethylsyloxanes (PDMSs) are used as the protective envelope (housing) of the insulator. We report on the behavior of both pure/noncrosslinked PDMSs and typical formulations used in industrial insulators, i.e. containing peroxide crosslinked PDMS, alumina trioxide hydrated (ATH) and silica. Special attention is paid on both (i) the sources of potential degradation and (ii) the best analytical methods that can be applied to the study of very complex formulations. (i) Aside from conventional types of ageing such as photo-ageing and thermal, hydrolytic, and service life ageings, treatments with acidic vapors, plasma and ozone possibly generating species from the reaction of a high electric field with air were also performed, which allowed to accelerate electrical and out-door ageings and to obtain differently aged materials. (ii) Aside from conventional analytical methods of polymer degradation such as FTIR/ATR spectroscopy and SEC, TG, hardness measurements, more specific methods like photo/DSC, TG/IR, thermoporosimetry, resistivity and density measurements were also performed to characterize the chemical and physical evolutions of polymer materials. In particular, it was found that treatment with nitric acid vapor has detrimental effects on the properties of both fire retardants (e.g. ATH) and PDMSs, affecting the hardness and resistivity of the formulated material.

  1. Polyimide-Foam/Aerogel Composites for Thermal Insulation

    NASA Technical Reports Server (NTRS)

    Williams, Martha; Fesmire, James; Sass, Jared; Smith, Trent; Weoser. Erol

    2009-01-01

    Composites of specific types of polymer foams and aerogel particles or blankets have been proposed to obtain thermal insulation performance superior to those of the neat polyimide foams. These composites have potential to also provide enhanced properties for vibration dampening or acoustic attenuation. The specific type of polymer foam is denoted "TEEK-H", signifying a series, denoted H, within a family of polyimide foams that were developed at NASA s Langley Research Center and are collectively denoted TEEK (an acronym of the inventors names). The specific types of aerogels include Nanogel aerogel particles from Cabot Corporation in Billerica, MA. and of Spaceloft aerogel blanket from Aspen Aerogels in Northborough, MA. The composites are inherently flame-retardant and exceptionally thermally stable. There are numerous potential uses for these composites, at temperatures from cryogenic to high temperatures, in diverse applications that include aerospace vehicles, aircraft, ocean vessels, buildings, and industrial process equipment. Some low-temperature applications, for example, include cryogenic storage and transfer or the transport of foods, medicines, and chemicals. Because of thermal cycling, aging, and weathering most polymer foams do not perform well at cryogenic temperatures and will undergo further cracking over time. The TEEK polyimides are among the few exceptions to this pattern, and the proposed composites are intended to have all the desirable properties of TEEK-H foams, plus improved thermal performance along with enhanced vibration or acoustic-attenuation performance. A composite panel as proposed would be fabricated by adding an appropriate amount of TEEK friable balloons into a mold to form a bottom layer. A piece of flexible aerogel blanket material, cut to the desired size and shape, would then be placed on the bottom TEEK layer and sandwiched between another top layer of polyimide friable balloons so that the aerogel blanket would become

  2. New High-Performance Droplet Freezing Assay (HP-DFA) for the Analysis of Ice Nuclei with Complex Composition

    NASA Astrophysics Data System (ADS)

    Kunert, Anna Theresa; Scheel, Jan Frederik; Helleis, Frank; Klimach, Thomas; Pöschl, Ulrich; Fröhlich-Nowoisky, Janine

    2016-04-01

    Freezing of water above homogeneous freezing is catalyzed by ice nucleation active (INA) particles called ice nuclei (IN), which can be of various inorganic or biological origin. The freezing temperatures reach up to -1 °C for some biological samples and are dependent on the chemical composition of the IN. The standard method to analyze IN in solution is the droplet freezing assay (DFA) established by Gabor Vali in 1970. Several modifications and improvements were already made within the last decades, but they are still limited by either small droplet numbers, large droplet volumes or inadequate separation of the single droplets resulting in mutual interferences and therefore improper measurements. The probability that miscellaneous IN are concentrated together in one droplet increases with the volume of the droplet, which can be described by the Poisson distribution. At a given concentration, the partition of a droplet into several smaller droplets leads to finely dispersed IN resulting in better statistics and therefore in a better resolution of the nucleation spectrum. We designed a new customized high-performance droplet freezing assay (HP-DFA), which represents an upgrade of the previously existing DFAs in terms of temperature range and statistics. The necessity of observing freezing events at temperatures lower than homogeneous freezing due to freezing point depression, requires high-performance thermostats combined with an optimal insulation. Furthermore, we developed a cooling setup, which allows both huge and tiny temperature changes within a very short period of time. Besides that, the new DFA provides the analysis of more than 750 droplets per run with a small droplet volume of 5 μL. This enables a fast and more precise analysis of biological samples with complex IN composition as well as better statistics for every sample at the same time.

  3. Single particle measurements of the chemical composition of cirrus ice residue during CRYSTAL-FACE

    NASA Astrophysics Data System (ADS)

    Cziczo, D. J.; Murphy, D. M.; Hudson, P. K.; Thomson, D. S.

    2004-02-01

    The first real-time, in situ, investigation of the chemical composition of the residue of cirrus ice crystals was performed during July 2002. This study was undertaken on a NASA WB-57F high-altitude research aircraft as part of CRYSTAL-FACE, a field campaign which sought to further our understanding of the relation of clouds, water vapor, and climate by characterizing, among other parameters, anvil cirrus formed about the Florida peninsula. A counter flow virtual impactor (CVI) was used to separate cirrus ice from the unactivated interstitial aerosol particles and evaporate condensed-phase water. Residual material, on a crystal-by-crystal basis, was subsequently analyzed using the NOAA Aeronomy Laboratory's Particle Analysis by Laser Mass Spectrometry (PALMS) instrument. Sampling was performed from 5 to 15 km altitude and from 12° to 28° north latitude within cirrus originating over land and ocean. Chemical composition measurements provided several important results. Sea salt was often incorporated into cirrus, consistent with homogeneous ice formation by aerosol particles from the marine boundary layer. Size measurements showed that large particles preferentially froze over smaller ones. Meteoritic material was found within ice crystals, indicative of a relation between stratospheric aerosol particles and tropospheric clouds. Mineral dust was the dominant residue observed in clouds formed during a dust transport event from the Sahara, consistent with a heterogeneous freezing mechanism. These results show that chemical composition and size are important determinants of which aerosol particles form cirrus ice crystals.

  4. Composition of Eocene Ice-Rafted Debris, Central Arctic Ocean

    NASA Astrophysics Data System (ADS)

    Ramstad, C.; St. John, K.

    2007-12-01

    IODP Expedition 302 drilled a 400-m sediment record which contains physical evidence of ice-rafting in the Eocene and Neogene in the Arctic (Backman et al., 2006; Moran et al., 2006, St. John, in press). An increase in the terrigenous sand abundance occurs above 246 mcd (~46 Ma), with a flux similar to that in the Neogene. Higher resolution sampling in an interval of good recovery from 246-236 mcd shows evidence of cyclic input of IRD and biogenic components that fits with Milankovitch forcing at the obliquity period (Sangiorgi et al., in press). The question remains - what areas of the Arctic were ice-covered at this early stage in the Cenozoic? To address this provenance issue the composition of the terrigenous sands (250 micron fraction) in cores 55-56X is being quantified. Grains in 75 samples are being point-counted and their compositions categorized. Quartz grains are the dominant component (greater than 10,000 grains per gram), with some being hematite-stained, and there are lesser amounts of mafic minerals. No carbonate grains are identified so far in this study. Possible sources areas for Eocene IRD are the Eastern European and Russian Arctic margins. Tracking compositional variations of the IRD over the interval of cyclic deposition, should indicate whether the cyclic IRD deposition was consistently derived from one source region or multiple regions during this time.

  5. Light, Strong Insulating Tiles

    NASA Technical Reports Server (NTRS)

    Cordia, E.; Schirle, J.

    1987-01-01

    Improved lightweight insulating silica/aluminum borosilicate/silicon carbide tiles combine increased tensile strength with low thermal conductivity. Changes in composition substantially improve heat-insulating properties of silica-based refractory tile. Silicon carbide particles act as high-emissivity radiation scatterers in tile material.

  6. Sliding temperatures of ice skates

    NASA Astrophysics Data System (ADS)

    Colbeck, S. C.; Najarian, L.; Smith, H. B.

    1997-06-01

    The two theories developed to explain the low friction of ice, pressure melting and frictional heating, require opposite temperature shifts at the ice-skate interface. The arguments against pressure melting are strong, but only theoretical. A set of direct temperature measurements shows that frictional heating is the dominant mechanism because temperature behaves in the manner predicted by the theory of frictional heating. Like snow skis, ice skates are warmed by sliding and then cool when the sliding stops. The temperature increases with speed and with thermal insulation. The sliding leaves a warm track on the ice surface behind the skate and the skate sprays warm ejecta.

  7. Investigation of Insulation Materials for Future Radioisotope Power Systems

    NASA Technical Reports Server (NTRS)

    Cornell, Peggy A.; Hurwitz, Frances I.; Ellis, David L.; Schmitz, Paul C.

    2013-01-01

    NASA's Radioisotope Power Systems (RPS) Technology Advancement Project is developing next generation high-temperature insulation materials that directly benefit thermal management and improve performance of RPS for future science missions. Preliminary studies on the use of multilayer insulation (MLI) for Stirling convertors used on the Advanced Stirling Radioisotope Generator (ASRG) have shown the potential benefits of MLI for space vacuum applications in reducing generator size and increasing specific power (W/kg) as compared to the baseline Microtherm HT (Microtherm, Inc.) insulation. Further studies are currently being conducted at NASA Glenn Research Center on candidate MLI foils and aerogel composite spacers. This paper presents the method of testing of foils and spacers and experimental results to date.

  8. The Collection of Ice in Jet A-1 Fuel Pipes

    NASA Astrophysics Data System (ADS)

    Maloney, Thomas C.

    ® and there was a lack of a preferential accumulation region downstream of a pipe bend. A greater heat transfer from the pipe increased ice accumulation for aluminum that was made rough with 80 grit sand paper, and for Teflon®. Water was shown to collect in the pipe system as the number of tests increased and the freeze temperature of either the hard or soft ice was about 0 °C. Finally, results of "stage I" tests showed that stainless steel pipe welds were a preferred sight for ice to accumulate. Repeatability was done first in stage II and the normalized pressure increase for two 3/42 un-insulated pipe tests were within 7%. Normalized pressure increase across a pipe was shown to increase as Reynolds number decreased. A 50% increase in Reynolds number led to a 40% decrease in characteristic normalized pressure increase (CNPI). Tests were done at three temperatures and ice accumulated the most at -11 °C. The CNPI at -11 °C was about three times greater than the CNPI at -7.4 °C and about sixty times greater than the CNPI at -19.4 C. A greater heat transfer from the fuel pipe increased ice accumulation. For the amount of time that the tests ran, the total normalized pressure increase was about .9 greater for an un-insulated pipe than for an insulated pipe. Contamination in the fuel increased the amount of soft ice that collected in the system. The CNPI for the more contaminated fuel was more than double the case with less contaminated fuel. Possible solutions for the prevention or decrease of ice accumulation in aircraft fuel systems based on the results of this study are insulated pipes, a change in the type of pipe material, a higher fuel flow rate and cleaner fuel. The fuel temperature could also be altered to avoid temperatures where the most ice accumulates.

  9. A Comparison of Sea Ice Type, Sea Ice Temperature, and Snow Thickness Distributions in the Arctic Seasonal Ice Zones with the DMSP SSM/I

    NASA Technical Reports Server (NTRS)

    St.Germain, Karen; Cavalieri, Donald J.; Markus, Thorsten

    1997-01-01

    Global climate studies have shown that sea ice is a critical component in the global climate system through its effect on the ocean and atmosphere, and on the earth's radiation balance. Polar energy studies have further shown that the distribution of thin ice and open water largely controls the distribution of surface heat exchange between the ocean and atmosphere within the winter Arctic ice pack. The thickness of the ice, the depth of snow on the ice, and the temperature profile of the snow/ice composite are all important parameters in calculating surface heat fluxes. In recent years, researchers have used various combinations of DMSP SSMI channels to independently estimate the thin ice type (which is related to ice thickness), the thin ice temperature, and the depth of snow on the ice. In each case validation efforts provided encouraging results, but taken individually each algorithm gives only one piece of the information necessary to compute the energy fluxes through the ice and snow. In this paper we present a comparison of the results from each of these algorithms to provide a more comprehensive picture of the seasonal ice zone using passive microwave observations.

  10. Overload characteristics of paper-polypropylene-paper cable

    DOE Office of Scientific and Technical Information (OSTI.GOV)

    Ernst, A.

    1990-09-01

    The short-time rating of PPP pipe-type cable may be lower than the equivalent paper cable sized to carry the same normal load. The ratings depend on the relative conductor sizes and the maximum allowable conductor temperatures of the insulation. The insulation thermal resistivity may be a significant parameter for overload times of approximately one hour and should be verified for PPP insulation. The thermal capacitance temperature characteristic of PPP insulation is not known. However, the overload ratings are not very sensitive to this parameter. Overload ratings are given for maximum conductor temperatures from 105 C to 130 C. Use ofmore » ratings based on temperatures greater than 105 C would require testing to determine the extent of degradation of the insulation at these higher temperatures. PPP-insulated cable will be thermally stable over a wider range of operating conditions (voltage and current) compared with paper-insulated cable. The short-circuit ratings of PPP- and paper-insulated cable systems and the positive/negative and zero sequence impedances are compared. 21 refs., 22 figs., 5 tabs.« less

  11. High temperature resistant cermet and ceramic compositions. [for thermal resistant insulators and refractory coatings

    NASA Technical Reports Server (NTRS)

    Phillips, W. M. (Inventor)

    1978-01-01

    High temperature oxidation resistance, high hardness and high abrasion and wear resistance are properties of cermet compositions particularly to provide high temperature resistant refractory coatings on metal substrates, for use as electrical insulation seals for thermionic converters. The compositions comprise a sintered body of particles of a high temperature resistant metal or metal alloy, preferably molybdenum or tungsten particles, dispersed in and bonded to a solid solution formed of aluminum oxide and silicon nitride, and particularly a ternary solid solution formed of a mixture of aluminum oxide, silicon nitride and aluminum nitride. Ceramic compositions comprising a sintered solid solution of aluminum oxide, silicon nitride and aluminum nitride are also described.

  12. Thermal insulating conformal blanket

    NASA Technical Reports Server (NTRS)

    Barney, Andrea (Inventor); Whittington, Charles A (Inventor); Eilertson, Bryan (Inventor); Siminski, Zenon (Inventor)

    2003-01-01

    The conformal thermal insulating blanket may have generally rigid batting material covered by an outer insulating layer formed of a high temperature resistant woven ceramic material and an inner insulating layer formed of a woven ceramic fiber material. The batting and insulating layers may be fastened together by sewing or stitching using an outer mold layer thread fabricated of a high temperature resistant material and an inner mold layer thread of a ceramic fiber material. The batting may be formed to a composite structure that may have a firmness factor sufficient to inhibit a pillowing effect after the stitching to not more than 0.03 inch. The outer insulating layer and an upper portion of the batting adjacent the outer insulating layer may be impregnated with a ceramic coating material.

  13. Reconstruction of Aerosol Concentration and Composition from Glacier Ice Cores

    NASA Astrophysics Data System (ADS)

    Vogel, Alexander; Dällenbach, Kaspar; El-Haddad, Imad; Wendl, Isabel; Eichler, Anja; Schwikowski, Margit

    2017-04-01

    Reconstruction of the concentration and composition of natural aerosol in an undisturbed atmosphere enables the evaluation of the understanding of aerosol-climate effects, which is currently based on highly uncertain emission inventories of the biosphere under pre-industrial conditions. Understanding of the natural state of the pre-industrial atmosphere and evaluating the atmospheric perturbations by anthropogenic emissions, and their potential feedbacks, is essential for accurate model predictions of the future climate (Boucher et al., 2013). Here, we present a new approach for the chemical characterization of the organic fraction preserved in cold-glacier ice cores. From this analysis historic trends of atmospheric organic aerosols are reconstructed, allowing new insights on organic aerosol composition and mass in the pre-industrial atmosphere, which can help to improve climate models through evaluation of our current understanding of aerosol radiative effects. We present results from a proof-of-principal study, analyzing an 800 year ice core record from the Lomonosovfonna glacier ice core, drilled in 2009 in Svalbard, Norway, using a setup that has until then only been applied on offline measurements of aerosol filter extracts (Dällenbach et al., 2016): The melted ice was nebulized and dried, such that aerosols are formed from the soluble and insoluble organic and inorganic compounds that are preserved in the ice. To improve the sensitivity, the aerosol stream was then enriched by the application of an online aerosol concentrator, before the aerosol was analyzed by electron ionization within a high resolution time-of-flight aerosol mass spectrometer (HR-ToF-AMS). We were able to demonstrate that this setup is a quantitative method toward nitrate and sulfate when internal inorganic standards of NH415NO3 and (NH4)234SO4 are added to the sample. Comparison between AMS and IC measurements of nitrate and sulfate resulted in an excellent agreement. The analysis of

  14. Under-ice melt ponds and the oceanic mixed layer

    NASA Astrophysics Data System (ADS)

    Flocco, D.; Smith, N.; Feltham, D. L.

    2017-12-01

    Under-ice melt ponds are pools of freshwater beneath the Arctic sea ice that form when melt from the surface of the sea ice percolates down through the porous sea ice. Through double diffusion, a sheet of ice can form at the interface between the ocean and the under-ice melt pond, completely isolating the pond from the mixed layer below and forming a false bottom to the sea ice. As such, they insulate the sea ice from the ocean below. It has been estimated that these ponds could cover between 5 and 40 % of the base of the Arctic sea ice, and so could have a notable impact on the mass balance of the sea ice. We have developed a one-dimensional model to calculate the thickness and thermodynamic properties of a slab of sea ice, an under-ice melt pond, and a false bottom, as these layers evolve. Through carrying out sensitivity studies, we have identified a number of interesting ways that under-ice melt ponds affect the ice above them and the rate of basal ablation. We found that they result in thicker sea ice above them, due to their insulation of the ice, and have found a possible positive feedback cycle in which less ice will be gained due to under-ice melt ponds as the Arctic becomes warmer. More recently, we have coupled this model to a simple Kraus-Turner type model of the oceanic mixed layer to investigate how these ponds affect the ocean water beneath them. Through altering basal ablation rates and ice thickness, they change the fresh water and salt fluxes into the mixed layer, as well as incoming radiation. Multi-year simulations have, in particular, shown how these effects work on longer time-scales.

  15. Investigation of Insulation Materials for Future Radioisotope Power Systems (RPS)

    NASA Technical Reports Server (NTRS)

    Cornell, Peggy A.; Hurwitz, Frances I.; Ellis, David L.; Schmitz, Paul C.

    2013-01-01

    NASA's Radioisotope Power System (RPS) Technology Advancement Project is developing next generation high temperature insulation materials that directly benefit thermal management and improve performance of RPS for future science missions. Preliminary studies on the use of multilayer insulation (MLI) for Stirling convertors used on the Advanced Stirling Radioisotope Generator (ASRG) have shown the potential benefits of MLI for space vacuum applications in reducing generator size and increasing specific power (W/kg) as compared to the baseline Microtherm HT (Microtherm, Inc.) insulation. Further studies are currently being conducted at NASA Glenn Research Center (GRC) on candidate MLI foils and aerogel composite spacers. This paper presents the method of testing of foils and spacers and experimental results to date.

  16. Alternating current breakdown voltage of ice electret

    NASA Astrophysics Data System (ADS)

    Oshika, Y.; Tsuchiya, Y.; Okumura, T.; Muramoto, Y.

    2017-09-01

    Ice has low environmental impact. Our research objectives are to study the availability of ice as a dielectric insulating material at cryogenic temperatures. We focus on ferroelectric ice (iceXI) at cryogenic temperatures. The properties of iceXI, including its formation, are not clear. We attempted to obtain the polarized ice that was similar to iceXI under the applied voltage and cooling to 77 K. The polarized ice have a wide range of engineering applications as electronic materials at cryogenic temperatures. This polarized ice is called ice electret. The structural difference between ice electret and normal ice is only the positions of protons. The effects of the proton arrangement on the breakdown voltage of ice electret were shown because electrical properties are influenced by the structure of ice. We observed an alternating current (ac) breakdown voltage of ice electret and normal ice at 77 K. The mean and minimum ac breakdown voltage values of ice electret were higher than those of normal ice. We considered that the electrically weak part of the normal ice was improved by applied a direct electric field.

  17. Physicochemical control of bacterial and protist community composition and diversity in Antarctic sea ice.

    PubMed

    Torstensson, Anders; Dinasquet, Julie; Chierici, Melissa; Fransson, Agneta; Riemann, Lasse; Wulff, Angela

    2015-10-01

    Due to climate change, sea ice experiences changes in terms of extent and physical properties. In order to understand how sea ice microbial communities are affected by changes in physicochemical properties of the ice, we used 454-sequencing of 16S and 18S rRNA genes to examine environmental control of microbial diversity and composition in Antarctic sea ice. We observed a high diversity and richness of bacteria, which were strongly negatively correlated with temperature and positively with brine salinity. We suggest that bacterial diversity in sea ice is mainly controlled by physicochemical properties of the ice, such as temperature and salinity, and that sea ice bacterial communities are sensitive to seasonal and environmental changes. For the first time in Antarctic interior sea ice, we observed a strong eukaryotic dominance of the dinoflagellate phylotype SL163A10, comprising 63% of the total sequences. This phylotype is known to be kleptoplastic and could be a significant primary producer in sea ice. We conclude that mixotrophic flagellates may play a greater role in the sea ice microbial ecosystem than previously believed, and not only during the polar night but also during summer when potential food sources are abundant. © 2015 Society for Applied Microbiology and John Wiley & Sons Ltd.

  18. Partial Model of Insulator/Insulator Contact Charging

    NASA Technical Reports Server (NTRS)

    Hogue, Michael; Calle, C. I.; Buhler, C. R.; Mucciolo, E. R.

    2005-01-01

    Two papers present a two-phase equilibrium model that partly explains insulator/ insulator contact charging. In this model, a vapor of ions within a gas is in equilibrium with a submonolayer of ions of the same species that have been adsorbed on the surface of an insulator. The surface is modeled as having localized states, each with a certain energy of adsorption for an ion. In an earlier version of the model described in the first paper, the ions do not interact with each other. Using the grand canonical ensemble, the chemical potentials of both vapor and absorbed phases are derived and equated to determine the vapor pressure. If a charge is assigned to the vapor particles (in particular, if single ionization is assumed), then the surface charge density associated with adsorbed ions can be calculated as a function of pressure. In a later version of the model presented in the second paper, the submodel of the vapor phase is extended to include electrostatic interactions between vapor ions and adsorbed ones as well as the screening effect, at a given distance from the surface, of ions closer to the surface. Theoretical values of this model closely match preliminary experimental data on the discharge of insulators as a function of pressure.

  19. Glass-mica composite: a new structural thermal-insulating material for building applications

    DOE Office of Scientific and Technical Information (OSTI.GOV)

    Low, N.M.P.

    1981-12-01

    Homogeneous, rigid glass-mica composites have been synthesized from mixtures of Canadian natural mica flakes of the phlogopite type and ground glass powders prepared from recycled soda-lime waste glasses by a simple sintering process. By means of selection of compositions and processing techniques, composites can be fabricated into products that exhibit a celular structure, a highly densified structure, and multilayer and sandwich structures. The cellular structure composite has a thermal conductivity in the range of 0.165 to 0.230 W/m /sup 0/C when measured over the temperature range 25 to 180/sup 0/C, and a compressive strength of about 0.874 MPa; the highlymore » densified composite, on the other hand, has a thermal conductivity in the range of 0.155 to 0.330 W/m /sup 0/C, a compressive strength in excess of 40 MPa, and an instantaneous coefficient of thermal expansion of 5.8 X 10/sup -6///sup 0/C at 100/sup 0/C. These glass-mica composites exhibit qualities such as insulating efficiency, safety, mechanical strength, and durability that are suitable for engineering applications in building structures or other systems.« less

  20. Advances in cryogenic foam insulations.

    NASA Technical Reports Server (NTRS)

    Lemons, C. R.; Salmassy, O. K.; Watts, C. R.

    1971-01-01

    Description of a discretely oriented thread-reinforced polyurethane foam thermal insulation system for liquid hydrogen fuel tanks. The 3-D foam and glass liner composite is designed to be adhesively bonded to the inside surface of the tank wall and to be in direct contact with liquid hydrogen. All elements of this insulation composite are capable of sustaining the loads and environmental conditions imposed by testing under simulated Space Shuttle vehicle requirements at temperatures between -423 and +350 F.

  1. Interstellar matrices: the chemical composition and evolution of interstellar ices as observed by ISO.

    PubMed

    d'Hendecourt, L; Dartois, E

    2001-03-15

    Matrix isolation techniques have been developed in the early sixties as a tool for studying the spectroscopic properties of out of equilibrium species (atoms, radicals, ions, reactive molecules), embedded in rare gas inert matrices at low temperatures. Cold interstellar grains surfaces are able to condense out gas phase molecules, routinely observed by radioastronomy. These grain 'mantles' can be considered as 'interstellar matrices'. However, these matrices are not clean and unreactive. They are made principally of dirty ices whose composition must be determined carefully to assess the importance of the solid state chemistry that takes place in the Interstellar Medium. Infrared spectroscopy, both in astronomy and in the laboratory, is the unique tool to determine the chemical composition of these ices. Astronomical spectra can directly be compared with laboratory ones obtained using classical matrix isolation techniques. Furthermore, dedicated experiments may be undertaken to further improve the understanding of the basic physico-chemical processes that take place in cosmic ices.

  2. Chemical composition, mixing state, size and morphology of Ice nucleating particles at the Jungfraujoch research station, Switzerland

    NASA Astrophysics Data System (ADS)

    Ebert, Martin; Worringen, Annette; Kandler, Konrad; Weinbruch, Stephan; Schenk, Ludwig; Mertes, Stephan; Schmidt, Susan; Schneider, Johannes; Frank, Fabian; Nilius, Björn; Danielczok, Anja; Bingemer, Heinz

    2014-05-01

    An intense field campaign from the Ice Nuclei Research Unit (INUIT) was performed in January and February of 2013 at the High-Alpine Research Station Jungfraujoch (3580 m a.s.l., Switzerland). Main goal was the assessment of microphysical and chemical properties of free-tropospheric ice-nucelating particles. The ice-nucleating particles were discriminated from the total aerosol with the 'Fast Ice Nucleation CHamber' (FINCH; University Frankfurt) and the 'Ice-Selective Inlet' (ISI, Paul Scherer Institute) followed by a pumped counter-stream virtual impactor. The separated ice-nucleating particles were then collected with a nozzle-type impactor. With the 'FRankfurt Ice nuclei Deposition freezinG Experiment' (FRIDGE), aerosol particles are sampled on a silicon wafer, which is than exposed to ice-activating conditions in a static diffusion chamber. The locations of the growing ice crystals are recorded for later analysis. Finally, with the ICE Counter-stream Virtual Impactor (ICE-CVI) atmospheric ice crystals are separated from the total aerosol and their water content is evaporated to retain the ice residual particles, which are then collected also by impactor sampling. All samples were analyzed in a high-resolution scanning electron microscope. By this method, for each particle its size, morphology, mixing-state and chemical composition is obtained. In total approximately 1700 ice nucleating particles were analyzed. Based on their chemical composition, the particles were classified into seven groups: silicates, metal oxides, Ca-rich particles, (aged) sea-salt, soot, sulphates and carbonaceous matter. Sea-salt is considered as artifact and is not regarded as ice nuclei here. The most frequent ice nucleating particles/ice residuals at the Jungfraujoch station are silicates > carbonaceous particles > metal oxides. Calcium-rich particles and soot play a minor role. Similar results are obtained by quasi-parallel measurements with an online single particle laser ablation

  3. Fluid insulation to prevent ice formation in heat exchangers

    NASA Technical Reports Server (NTRS)

    Coffinberry, G. A.

    1973-01-01

    Heat transfer surfaces were insulated to maintain air side surface temperature above freezing. Double wall tubes, with annular space between tubes, were filled with static liquid hydrogen. Low thermal conductivity of this hydrogen provided thermal resistance.

  4. Mechanically Stretchable and Electrically Insulating Thermal Elastomer Composite by Liquid Alloy Droplet Embedment.

    PubMed

    Jeong, Seung Hee; Chen, Si; Huo, Jinxing; Gamstedt, Erik Kristofer; Liu, Johan; Zhang, Shi-Li; Zhang, Zhi-Bin; Hjort, Klas; Wu, Zhigang

    2015-12-16

    Stretchable electronics and soft robotics have shown unsurpassed features, inheriting remarkable functions from stretchable and soft materials. Electrically conductive and mechanically stretchable materials based on composites have been widely studied for stretchable electronics as electrical conductors using various combinations of materials. However, thermally tunable and stretchable materials, which have high potential in soft and stretchable thermal devices as interface or packaging materials, have not been sufficiently studied. Here, a mechanically stretchable and electrically insulating thermal elastomer composite is demonstrated, which can be easily processed for device fabrication. A liquid alloy is embedded as liquid droplet fillers in an elastomer matrix to achieve softness and stretchability. This new elastomer composite is expected useful to enhance thermal response or efficiency of soft and stretchable thermal devices or systems. The thermal elastomer composites demonstrate advantages such as thermal interface and packaging layers with thermal shrink films in transient and steady-state cases and a stretchable temperature sensor.

  5. Mechanically Stretchable and Electrically Insulating Thermal Elastomer Composite by Liquid Alloy Droplet Embedment

    PubMed Central

    Jeong, Seung Hee; Chen, Si; Huo, Jinxing; Gamstedt, Erik Kristofer; Liu, Johan; Zhang, Shi-Li; Zhang, Zhi-Bin; Hjort, Klas; Wu, Zhigang

    2015-01-01

    Stretchable electronics and soft robotics have shown unsurpassed features, inheriting remarkable functions from stretchable and soft materials. Electrically conductive and mechanically stretchable materials based on composites have been widely studied for stretchable electronics as electrical conductors using various combinations of materials. However, thermally tunable and stretchable materials, which have high potential in soft and stretchable thermal devices as interface or packaging materials, have not been sufficiently studied. Here, a mechanically stretchable and electrically insulating thermal elastomer composite is demonstrated, which can be easily processed for device fabrication. A liquid alloy is embedded as liquid droplet fillers in an elastomer matrix to achieve softness and stretchability. This new elastomer composite is expected useful to enhance thermal response or efficiency of soft and stretchable thermal devices or systems. The thermal elastomer composites demonstrate advantages such as thermal interface and packaging layers with thermal shrink films in transient and steady-state cases and a stretchable temperature sensor. PMID:26671673

  6. Robust Multilayer Insulation for Cryogenic Systems

    NASA Technical Reports Server (NTRS)

    Fesmire, J. E.; Scholtens, B. F.; Augustynowicz, S. D.

    2007-01-01

    New requirements for thermal insulation include robust Multilayer insulation (MU) systems that work for a range of environments from high vacuum to no vacuum. Improved MLI systems must be simple to install and maintain while meeting the life-cycle cost and thermal performance objectives. Performance of actual MLI systems has been previously shown to be much worse than ideal MLI. Spacecraft that must contain cryogens for both lunar service (high vacuum) and ground launch operations (no vacuum) are planned. Future cryogenic spacecraft for the soft vacuum environment of Mars are also envisioned. Industry products using robust MLI can benefit from improved cost-efficiency and system safety. Novel materials have been developed to operate as excellent thermal insulators at vacuum levels that are much less stringent than the absolute high vacuum requirement of current MLI systems. One such robust system, Layered Composite Insulation (LCI), has been developed by the Cryogenics Test Laboratory at NASA Kennedy Space Center. The experimental testing and development of LCI is the focus of this paper. LCI thermal performance under cryogenic conditions is shown to be six times better than MLI at soft vacuum and similar to MLI at high vacuum. The experimental apparent thermal conductivity (k-value) and heat flux data for LCI systems are compared with other MLI systems.

  7. Composition and biodegradation of a synthetic oil spilled on the perennial ice cover of Lake Fryxell, Antarctica.

    PubMed

    Jaraula, Caroline M B; Kenig, Fabien; Doran, Peter T; Priscu, John C; Welch, Kathleen A

    2009-04-15

    A helicopter crashed in January 2003 on the 5 m-thick perennial ice cover of Lake Fryxell, spilling synthetic turbine oil Aeroshell 500. Molecular compositions of the oils were analyzed by gas chromatography-mass spectrometry and compared to the composition of contaminants in ice, meltwater, and sediments collected a year after the accident. Aeroshell 500 is based on C20-C33 Pentaerythritol triesters (PET) with C5-C10 fatty acids susbstituents and contain a number of antioxidant additives, such as tricresyl phosphates. Biodegradation of this oil in the ice cover occurs when sediments are present PETs with short fatty acids substituents are preferentially degraded, whereas long chain fatty acids seem to hinder esters from hydrolysis by esterase derived from the microbial assemblage. It remains to be seen if the microbial ecosystem can degrade tricresyl phosphates. These more recalcitrant PET species and tricresyl phosphates are likely to persist and comprise the contaminants that may eventually cross the ice cover to reach the pristine lake water.

  8. Dating an 800,000 year Antarctic ice core record using the isotopic composition of trapped air

    NASA Astrophysics Data System (ADS)

    Dreyfus, Gabrielle Boissier

    Here we measure the isotopic composition of air trapped in the European Project for Ice Coring in Antarctica Dome C (EDC) ice core, and use this geochemical information to improve the ice core agescale and our understanding of air enclosure processes. A first result is the detection of a flow anomaly in the bottom 500m of the EDC ice core using the delta18O of atmospheric oxygen (noted delta18Oatm). By tuning the measured delta18Oatm to the orbital precession signal, we correct the EDC agescale over 400-800 ka for flow-induced distortions in the duration of events. Uncertainty in delta 18Oatm phasing with respect to precession limits the accuracy of the tuned agescale to +/-6 ka. We use this improved agescale to date two 10Be peaks detected in the EDC ice core and associated with the Matuyama-Brunhes geomagnetic boundary. While the ice age of the "precursor" event agrees within uncertainty with the age of radioisotopically dated lavas, the volcanic age for the younger reversal is approximately 10 ka older than the mid-point of the 10 Be peak in the ice. Since 80% of the lavas recording the Matuyama-Brunhes reversal are located in the Central Pacific, the observed age difference may indicate that the magnetic field orientation at this location changed prior to the dipole intensity minimum recorded by the ice core 10Be, as suggested by recent geodynamo modeling. A particular challenge for ice core dating is accurately accounting for the age difference between the trapped air and surrounding ice. This gas age - ice age difference (noted Deltaage) depends on the age of the ice at the bottom of the firn. delta15N of N2 is constant in the atmosphere over the timescales considered here, so any deviation from atmospheric composition reflects fractionation processes in the firn. We show that delta15N is positively correlated with the ice deuterium content, a proxy for temperature, over the entire EDC record, and propose an accumulation-permeability-convection mechanism

  9. Ice detector

    NASA Technical Reports Server (NTRS)

    Weinstein, Leonard M. (Inventor)

    1988-01-01

    An ice detector is provided for the determination of the thickness of ice on the outer surface on an object (e.g., aircraft) independently of temperature or the composition of the ice. First capacitive gauge, second capacitive gauge, and temperature gauge are embedded in embedding material located within a hollowed out portion of the outer surface. This embedding material is flush with the outer surface to prevent undesirable drag. The first capacitive gauge, second capacitive gauge, and the temperature gauge are respectively connected to first capacitive measuring circuit, second capacitive measuring circuit, and temperature measuring circuit. The geometry of the first and second capacitive gauges is such that the ratio of the voltage outputs of the first and second capacitance measuring circuits is proportional to the thickness of ice, regardless of ice temperature or composition. This ratio is determined by offset and dividing circuit.

  10. Winter severity determines functional trait composition of phytoplankton in seasonally ice-covered lakes.

    PubMed

    Özkundakci, Deniz; Gsell, Alena S; Hintze, Thomas; Täuscher, Helgard; Adrian, Rita

    2016-01-01

    How climate change will affect the community dynamics and functionality of lake ecosystems during winter is still little understood. This is also true for phytoplankton in seasonally ice-covered temperate lakes which are particularly vulnerable to the presence or absence of ice. We examined changes in pelagic phytoplankton winter community structure in a north temperate lake (Müggelsee, Germany), covering 18 winters between 1995 and 2013. We tested how phytoplankton taxa composition varied along a winter-severity gradient and to what extent winter severity shaped the functional trait composition of overwintering phytoplankton communities using multivariate statistical analyses and a functional trait-based approach. We hypothesized that overwintering phytoplankton communities are dominated by taxa with trait combinations corresponding to the prevailing winter water column conditions, using ice thickness measurements as a winter-severity indicator. Winter severity had little effect on univariate diversity indicators (taxon richness and evenness), but a strong relationship was found between the phytoplankton community structure and winter severity when taxon trait identity was taken into account. Species responses to winter severity were mediated by the key functional traits: motility, nutritional mode, and the ability to form resting stages. Accordingly, one or the other of two functional groups dominated the phytoplankton biomass during mild winters (i.e., thin or no ice cover; phototrophic taxa) or severe winters (i.e., thick ice cover; exclusively motile taxa). Based on predicted milder winters for temperate regions and a reduction in ice-cover durations, phytoplankton communities during winter can be expected to comprise taxa that have a relative advantage when the water column is well mixed (i.e., need not be motile) and light is less limiting (i.e., need not be mixotrophic). A potential implication of this result is that winter severity promotes different

  11. Optimization of Refining Craft for Vegetable Insulating Oil

    NASA Astrophysics Data System (ADS)

    Zhou, Zhu-Jun; Hu, Ting; Cheng, Lin; Tian, Kai; Wang, Xuan; Yang, Jun; Kong, Hai-Yang; Fang, Fu-Xin; Qian, Hang; Fu, Guang-Pan

    2016-05-01

    Vegetable insulating oil because of its environmental friendliness are considered as ideal material instead of mineral oil used for the insulation and the cooling of the transformer. The main steps of traditional refining process included alkali refining, bleaching and distillation. This kind of refining process used in small doses of insulating oil refining can get satisfactory effect, but can't be applied to the large capacity reaction kettle. This paper using rapeseed oil as crude oil, and the refining process has been optimized for large capacity reaction kettle. The optimized refining process increases the acid degumming process. The alkali compound adds the sodium silicate composition in the alkali refining process, and the ratio of each component is optimized. Add the amount of activated clay and activated carbon according to 10:1 proportion in the de-colorization process, which can effectively reduce the oil acid value and dielectric loss. Using vacuum pumping gas instead of distillation process can further reduce the acid value. Compared some part of the performance parameters of refined oil products with mineral insulating oil, the dielectric loss of vegetable insulating oil is still high and some measures are needed to take to further optimize in the future.

  12. Hydrogen storage in insulated pressure vessels

    DOE Office of Scientific and Technical Information (OSTI.GOV)

    Aceves, S.M.; Garcia-Villazana, O.

    1998-08-01

    Insulated pressure vessels are cryogenic-capable pressure vessels that can be fueled with liquid hydrogen (LH{sub 2}) or ambient-temperature compressed hydrogen (CH{sub 2}). Insulated pressure vessels offer the advantages of liquid hydrogen tanks (low weight and volume), with reduced disadvantages (lower energy requirement for hydrogen liquefaction and reduced evaporative losses). This paper shows an evaluation of the applicability of the insulated pressure vessels for light-duty vehicles. The paper shows an evaluation of evaporative losses and insulation requirements and a description of the current analysis and experimental plans for testing insulated pressure vessels. The results show significant advantages to the use ofmore » insulated pressure vessels for light-duty vehicles.« less

  13. Dielectric and Insulating Technology 2005 : Reviews & Forecasts

    NASA Astrophysics Data System (ADS)

    Okamoto, Tatsuki

    This article reports the state-of-art of TC-DEI ( Technical Committee of Dielectrics and Electrical Insulation of IEEJ) activites. The activiteis are basically based on the activites of 8-10 investigation committees under TC-DEI. Recent activites were categorized into three functions in this article and remarkable activity or trend for each category is mentioned as was done in the article of 2003. Thoese are activities on asset management (AI application and insulation diagnosis), activities on new insulating and functional materials (Nano composite) and activities on new insulation technology for power tansmission (high Tc superconducting cable insulation).

  14. Dielectric and Insulating Technology 2006 : Review & Forecast

    NASA Astrophysics Data System (ADS)

    Okamoto, Tatsuki

    This article reports the state-of-art of TC-DEI ( Technical Committee of Dielectrics and Electrical Insulation of IEEJ) activites. The activiteis are basically based on the activites of 8-10 investigation committees under TC-DEI. Recent activites were categorized into three functions in this article and remarkable activity or trend for each category is mentioned as was seen in the articles of 2005. Those are activities on asset management (AI application and insulation diagnosis), activities on new insulating and functional materials (Nano composite) and activities on new insulation technology for power tansmission (high Tc superconducting cable insulation).

  15. Structural Continuum Modeling of Space Shuttle External Tank Foam Insulation

    NASA Technical Reports Server (NTRS)

    Steeve, Brian; Ayala, Sam; Purlee, T. Eric; Shaw, Phillip

    2006-01-01

    This document is a viewgraph presentation reporting on work in modeling the foam insulation of the Space Shuttle External Tank. An analytical understanding of foam mechanics is required to design against structural failure. The Space Shuttle External Tank is covered primarily with closed cell foam to: Prevent ice, Protect structure from ascent aerodynamic and engine plume heating, and Delay break-up during re-entry. It is important that the foam does not shed unacceptable debris during ascent environment. Therefore a modeling of the foam insulation was undertaken.

  16. Antifogging and icing-delay properties of composite micro- and nanostructured surfaces.

    PubMed

    Wen, Mengxi; Wang, Lei; Zhang, Mingqian; Jiang, Lei; Zheng, Yongmei

    2014-03-26

    A composite micro/nanostrucutred (MN) surface was designed using poly(vinylidene difluoride) (PVDF) polymer in combination with ZnO materials via heat-pattern-transfer and crystal-growth techniques. The surface, composed of ZnO nanohairs over PVDF microratchets (i.e., ZP-MN), displays excellent antifogging and icing-delay properties. Condensed water droplets can be easily shed from the ZP-MN surface at -5 °C for ∼1600 s via a slight wind or tilting. The droplets do not completely freeze on the ZP-MN surface at -10 °C until ∼7360 s. This investigation offers a way to design a structured surface that possesses anti-icing ability, which is significant because it can be extended to fields such as microdevices, engineering systems, and engines that operate in a cold or humid environment.

  17. Multilayer Impregnated Fibrous Thermal Insulation Tiles

    NASA Technical Reports Server (NTRS)

    Tran, Huy K.; Rasky, Daniel J.; Szalai, Christine e.; Hsu, Ming-ta; Carroll, Joseph A.

    2007-01-01

    The term "secondary polymer layered impregnated tile" ("SPLIT") denotes a type of ablative composite-material thermal- insulation tiles having engineered, spatially non-uniform compositions. The term "secondary" refers to the fact that each tile contains at least two polymer layers wherein endothermic reactions absorb considerable amounts of heat, thereby helping to prevent overheating of an underlying structure. These tiles were invented to afford lighter-weight alternatives to the reusable thermal-insulation materials heretofore variously used or considered for use in protecting the space shuttles and other spacecraft from intense atmospheric-entry heating.

  18. Understanding the Percolation Characteristics of Nonlinear Composite Dielectrics

    PubMed Central

    Yang, Xiao; Hu, Jun; Chen, Shuiming; He, Jinliang

    2016-01-01

    Nonlinear composite dielectrics can function as smart materials for stress control and field grading in all fields of electrical insulations. The percolation process is a significant issue of composite dielectrics. However, the classic percolation theory mainly deals with traditional composites in which the electrical parameters of both insulation matrix and conducting fillers are independent of the applied electric field. This paper measured the nonlinear V-I characteristics of ZnO microvaristors/silicone rubber composites with several filler concentrations around an estimated percolation threshold. For the comparison with the experiment, a new microstructural model is proposed to simulate the nonlinear conducting behavior of the composite dielectrics modified by metal oxide fillers, which is based on the Voronoi network and considers the breakdown feature of the insulation matrix for near percolated composites. Through both experiment and simulation, the interior conducting mechanism and percolation process of the nonlinear composites were presented and a specific percolation threshold was determined as 33%. This work has provided a solution to better understand the characteristics of nonlinear composite dielectrics. PMID:27476998

  19. Understanding the Percolation Characteristics of Nonlinear Composite Dielectrics

    NASA Astrophysics Data System (ADS)

    Yang, Xiao; Hu, Jun; Chen, Shuiming; He, Jinliang

    2016-08-01

    Nonlinear composite dielectrics can function as smart materials for stress control and field grading in all fields of electrical insulations. The percolation process is a significant issue of composite dielectrics. However, the classic percolation theory mainly deals with traditional composites in which the electrical parameters of both insulation matrix and conducting fillers are independent of the applied electric field. This paper measured the nonlinear V-I characteristics of ZnO microvaristors/silicone rubber composites with several filler concentrations around an estimated percolation threshold. For the comparison with the experiment, a new microstructural model is proposed to simulate the nonlinear conducting behavior of the composite dielectrics modified by metal oxide fillers, which is based on the Voronoi network and considers the breakdown feature of the insulation matrix for near percolated composites. Through both experiment and simulation, the interior conducting mechanism and percolation process of the nonlinear composites were presented and a specific percolation threshold was determined as 33%. This work has provided a solution to better understand the characteristics of nonlinear composite dielectrics.

  20. Alkali-Activated Aluminium-Silicate Composites as Insulation Materials for Industrial Application

    NASA Astrophysics Data System (ADS)

    Dembovska, L.; Bajare, D.; Pundiene, I.; Bumanis, G.

    2015-11-01

    The article reports on the study of thermal stability of alkali-activated aluminium- silicate composites (ASC) at temperature 800-1100°C. ASC were prepared by using calcined kaolinite clay, aluminium scrap recycling waste, lead-silicate glass waste and quartz sand. As alkali activator, commercial sodium silicate solution modified with an addition of sodium hydroxide was used. The obtained alkali activation solution had silica modulus Ms=1.67. Components of aluminium scrap recycling waste (aluminium nitride (AlN) and iron sulphite (FeSO3)) react in the alkali media and create gases - ammonia and sulphur dioxide, which provide the porous structure of the material [1]. Changes in the chemical composition of ASC during heating were identified and quantitatively analysed by using DTA/TG, dimension changes during the heating process were determined by using HTOM, pore microstructure was examined by SEM, and mineralogical composition of ASC was determined by XRD. The density of ASC was measured in accordance with EN 1097-7. ASC with density around 560 kg/m3 and heat resistance up to 1100°C with shrinkage less than 5% were obtained. The intended use of this material is the application as an insulation material for industrial purposes at elevated temperatures.

  1. Ice/frost detection using millimeter wave radiometry. [space shuttle external tank

    NASA Technical Reports Server (NTRS)

    Gagliano, J. A.; Newton, J. M.; Davis, A. R.; Foster, M. L.

    1981-01-01

    A series of ice detection tests was performed on the shuttle external tank (ET) and on ET target samples using a 35/95 GHz instrumentation radiometer. Ice was formed using liquid nitrogen and water spray inside a test enclosure containing ET spray on foam insulation samples. During cryogenic fueling operations prior to the shuttle orbiter engine firing tests, ice was formed with freon and water over a one meter square section of the ET LOX tank. Data analysis was performed on the ice signatures, collected by the radiometer, using Georgia Tech computing facilities. Data analysis technique developed include: ice signature images of scanned ET target; pixel temperature contour plots; time correlation of target data with ice present versus no ice formation; and ice signature radiometric temperature statistical data, i.e., mean, variance, and standard deviation.

  2. High sensitive FBG load cell for icing of overhead transmission lines

    NASA Astrophysics Data System (ADS)

    Mao, Naiqiang; Ma, Guoming; Li, Chengrong; Li, Yabo; Shi, Cheng; Du, Yue

    2017-04-01

    Heavy ice coating of overhead transmission lines created the serious threat on the safe operation of power grid. The measurement of conductor icing had been an effective and reliable methods to prevent potential risks, such as conductor breakage, insulator flashover and tower collapse. Because of the advantages of immunity to electromagnetic interference and no demand for power supply in site, the optical load cell has been widely applied in monitoring the ice coating of overhead transmission lines. In this paper, we have adopted the shearing structure with additional grooves as elastic element of load cell to detect the eccentric load. Then, two welding package fiber Bragg gratings (FBGs) were mounted onto the grooves of elastic element with a direction deviation of 90° to eliminate temperature effects on strain measurement without extra FBG. After that, to avoid the occurrence of load cell breakage in heavy load measurement, the protection part has been proposed and added to the elastic element. The results of tension experiments indicate that the resolution of the load cell is 7.78 N in the conventional measuring range (0-10 kN). And in addition, the load cell proposed in this paper also has a good performance in actual experiment in which the load and temperature change simultaneously.

  3. Polybenzoxazole-filled nitrile butadiene rubber compositions

    NASA Technical Reports Server (NTRS)

    Gajiwala, Himansu M. (Inventor); Guillot, David G. (Inventor)

    2008-01-01

    An insulation composition that comprises at least one nitrile butadiene rubber (NBR) having an acrylonitrile content that ranges from approximately 26% by weight to approximately 35% by weight and polybenzoxazole (PBO) fibers. The NBR may be a copolymer of acrylonitrile and butadiene and may be present in the insulation composition in a range of from approximately 45% by weight to approximately 56% by weight of a total weight of the insulation composition. The PBO fibers may be present in a range of from approximately 3% by weight to approximately 10% by weight of a total weight of the insulation composition. A rocket motor including the insulation composition and a method of insulating a rocket motor are also disclosed.

  4. Thermal highly porous insulation materials made of mineral raw materials

    NASA Astrophysics Data System (ADS)

    Mestnikov, A.

    2015-01-01

    The main objective of the study is to create insulating foam based on modified mineral binders with rapid hardening. The results of experimental studies of the composition and properties of insulating foam on the basis of rapidly hardening Portland cement (PC) and gypsum binder composite are presented in the article. The article proposes technological methods of production of insulating foamed concrete and its placement to the permanent shuttering wall enclosures in monolithic-frame construction and individual energy-efficient residential buildings, thus reducing foam shrinkage and improving crack-resistance.

  5. Quantifying the ice-albedo feedback through decoupling

    NASA Astrophysics Data System (ADS)

    Kravitz, B.; Rasch, P. J.

    2017-12-01

    The ice-albedo feedback involves numerous individual components, whereby warming induces sea ice melt, inducing reduced surface albedo, inducing increased surface shortwave absorption, causing further warming. Here we attempt to quantify the sea ice albedo feedback using an analogue of the "partial radiative perturbation" method, but where the governing mechanisms are directly decoupled in a climate model. As an example, we can isolate the insulating effects of sea ice on surface energy and moisture fluxes by allowing sea ice thickness to change but fixing Arctic surface albedo, or vice versa. Here we present results from such idealized simulations using the Community Earth System Model in which individual components are successively fixed, effectively decoupling the ice-albedo feedback loop. We isolate the different components of this feedback, including temperature change, sea ice extent/thickness, and air-sea exchange of heat and moisture. We explore the interactions between these different components, as well as the strengths of the total feedback in the decoupled feedback loop, to quantify contributions from individual pieces. We also quantify the non-additivity of the effects of the components as a means of investigating the dominant sources of nonlinearity in the ice-albedo feedback.

  6. How Will Sea Ice Loss Affect the Greenland Ice Sheet? On the Puzzling Features of Greenland Ice-Core Isotopic Composition

    NASA Technical Reports Server (NTRS)

    Pausata, Francesco S. R.; Legrande, Allegra N.; Roberts, William H. G.

    2016-01-01

    The modern cryosphere, Earth's frozen water regime, is in fast transition. Greenland ice cores show how fast theses changes can be, presenting evidence of up to 15 C warming events over timescales of less than a decade. These events, called Dansgaard/Oeschger (D/O) events, are believed to be associated with rapid changes in Arctic sea ice, although the underlying mechanisms are still unclear. The modern demise of Arctic sea ice may, in turn, instigate abrupt changes on the Greenland Ice Sheet. The Arctic Sea Ice and Greenland Ice Sheet Sensitivity (Ice2Ice Chttps://ice2ice.b.uib.noD) initiative, sponsored by the European Research Council, seeks to quantify these past rapid changes to improve our understanding of what the future may hold for the Arctic. Twenty scientists gathered in Copenhagen as part of this initiative to discuss the most recent observational, technological, and model developments toward quantifying the mechanisms behind past climate changes in Greenland. Much of the discussion focused on the causes behind the changes in stable water isotopes recorded in ice cores. The participants discussed sources of variability for stable water isotopes and framed ways that new studies could improve understanding of modern climate. The participants also discussed how climate models could provide insights into the relative roles of local and nonlocal processes in affecting stable water isotopes within the Greenland Ice Sheet. Presentations of modeling results showed how a change in the source or seasonality of precipitation could occur not only between glacial and modern climates but also between abrupt events. Recent fieldwork campaigns illustrate an important role of stable isotopes in atmospheric vapor and diffusion in the final stable isotope signal in ice. Further, indications from recent fieldwork campaigns illustrate an important role of stable isotopes in atmospheric vapor and diffusion in the final stable isotope signal in ice. This feature complicates

  7. Research and application of high performance GPES rigid foam composite plastic insulation boards

    NASA Astrophysics Data System (ADS)

    sun, Hongming; xu, Hongsheng; Han, Feifei

    2017-09-01

    A new type of heat insulation board named GPES was prepared by several polymers and modified nano-graphite particles, injecting high-pressure supercritical CO2. Compared with the traditional thermal insulation material, GPES insulation board has higher roundness bubble and thinner bubble wall. Repeatability and reproducibility tests show that melting knot, dimensional stability, strength and other physical properties are significantly better than traditional organic heat insulation materials. Especially the lower and more stable thermal conductivity of GPES can significantly reduce thermal insulation layer thickness. Obviously GPES is the best choice of insulation materials with the implement of 75% and higher energy efficiency standard.

  8. Optical probing of quantum Hall effect of composite fermions and of the liquid-insulator transition

    NASA Astrophysics Data System (ADS)

    Rossella, F.; Bellani, V.; Dionigi, F.; Amado, M.; Diez, E.; Kowalik, K.; Biasiol, G.; Sorba, L.

    2011-12-01

    In the photoluminescence spectra of a two-dimensional electron gas in the fractional quantum Hall regime we observe the states at filling factors ν = 4/5, 5/7, 4/11 and 3/8 as clear minima in the intensity or area emission peak. The first three states are described as interacting composite fermions in fractional quantum Hall regime. The minimum in the intensity at ν = 3/8, which is not explained within this picture, can be an evidence of a suppression of the screening of the Coulomb interaction among the effective quasi-particles involved in this intriguing state. The magnetic field energy dispersion at very low temperatures is also discussed. At low field the emission follows a Landau dispersion with a screened magneto-Coulomb contribution. At intermediate fields the hidden symmetry manifests. At high field above ν = 1/3 the electrons correlate into an insulating phase, and the optical emission behaviour at the liquid-insulator transition is coherent with a charge ordering driven by Coulomb correlations.

  9. Chemical composition and mixing-state of ice residuals sampled within mixed phase clouds

    NASA Astrophysics Data System (ADS)

    Ebert, M.; Worringen, A.; Benker, N.; Mertes, S.; Weingartner, E.; Weinbruch, S.

    2010-10-01

    During an intensive campaign at the high alpine research station Jungfraujoch, Switzerland, in February/March 2006 ice particle residuals within mixed-phase clouds were sampled using the Ice-counterflow virtual impactor (Ice-CVI). Size, morphology, chemical composition, mineralogy and mixing state of the ice residual and the interstitial (i.e., non-activated) aerosol particles were analyzed by scanning and transmission electron microscopy. Ice nuclei (IN) were identified from the significant enrichment of particle groups in the ice residual (IR) samples relative to the interstitial aerosol. In terms of number lead-bearing particles are enriched by a factor of approximately 25, complex internal mixtures with silicates or metal oxides as major components by a factor of 11, and mixtures of secondary aerosol and soot (C-O-S particles) by a factor of 2. Other particle groups (sulfates, sea salt, Ca-rich particles, external silicates) observed in the ice-residual samples cannot be assigned unambiguously as IN. Between 9 and 24% of all IR are Pb-bearing particles. Pb was found as major component in around 10% of these particles (PbO, PbCl2). In the other particles, Pb was found as some 100 nm sized agglomerates consisting of 3-8 nm sized primary particles (PbS, elemental Pb). C-O-S particles are present in the IR at an abundance of 17-27%. The soot component within these particles is strongly aged. Complex internal mixtures occur in the IR at an abundance of 9-15%. Most IN identified at the Jungfraujoch station are internal mixtures containing anthropogenic components (either as main or minor constituent), and it is concluded that admixture of the anthropogenic component is responsible for the increased IN efficiency within mixed phase clouds. The mixing state appears to be a key parameter for the ice nucleation behaviour that cannot be predicted from the separate components contained within the individual particles.

  10. Measurement of polychlorinated biphenyls in solid waste such as transformer insulation paper by supercritical fluid extraction and gas chromatography electron capture detection.

    PubMed

    Chikushi, Hiroaki; Fujii, Yuka; Toda, Kei

    2012-09-21

    In this work, a method for measuring polychlorinated biphenyls (PCBs) in contaminated solid waste was investigated. This waste includes paper that is used in electric transformers to insulate electric components. The PCBs in paper sample were extracted by supercritical fluid extraction and analyzed by gas chromatography-electron capture detection. The recoveries with this method (84-101%) were much higher than those with conventional water extraction (0.08-14%), and were comparable to those with conventional organic solvent extraction. Limit of detection was 0.0074 mg kg(-1) and measurable up to 2.5 mg kg(-1) for 0.5 g of paper sample. Data for real insulation paper by the proposed method agreed well with those by the conventional organic solvent extraction. Extraction from wood and concrete was also investigated and good performance was obtained as well as for paper samples. The supercritical fluid extraction is simpler, faster, and greener than conventional organic solvent extraction. Copyright © 2012 Elsevier B.V. All rights reserved.

  11. Snow contribution to first-year and second-year Arctic sea ice mass balance north of Svalbard

    NASA Astrophysics Data System (ADS)

    Granskog, Mats A.; Rösel, Anja; Dodd, Paul A.; Divine, Dmitry; Gerland, Sebastian; Martma, Tõnu; Leng, Melanie J.

    2017-03-01

    The salinity and water oxygen isotope composition (δ18O) of 29 first-year (FYI) and second-year (SYI) Arctic sea ice cores (total length 32.0 m) from the drifting ice pack north of Svalbard were examined to quantify the contribution of snow to sea ice mass. Five cores (total length 6.4 m) were analyzed for their structural composition, showing variable contribution of 10-30% by granular ice. In these cores, snow had been entrained in 6-28% of the total ice thickness. We found evidence of snow contribution in about three quarters of the sea ice cores, when surface granular layers had very low δ18O values. Snow contributed 7.5-9.7% to sea ice mass balance on average (including also cores with no snow) based on δ18O mass balance calculations. In SYI cores, snow fraction by mass (12.7-16.3%) was much higher than in FYI cores (3.3-4.4%), while the bulk salinity of FYI (4.9) was distinctively higher than for SYI (2.7). We conclude that oxygen isotopes and salinity profiles can give information on the age of the ice and enables distinction between FYI and SYI (or older) ice in the area north of Svalbard.Plain Language SummaryThe role of snow in sea <span class="hlt">ice</span> mass balance is largely two fold. Firstly, it can slow down growth and melt due to its high <span class="hlt">insulation</span> and high reflectance, but secondly it can actually contribute to sea <span class="hlt">ice</span> growth if the snow cover is turned into <span class="hlt">ice</span>. The latter is largely a consequence of high mass of snow on top of sea <span class="hlt">ice</span> that can push the surface of the sea <span class="hlt">ice</span> below sea level and seawater can flood the <span class="hlt">ice</span>. This mixture of seawater and snow can then freeze and add to the growth of sea <span class="hlt">ice</span>. This is very typical in the Antarctic but not believed to be so important in the Arctic. In this work we show, for the first time, that snow actually contributes significantly to the growth of Arctic sea <span class="hlt">ice</span>. This is likely a consequence of the thinning of the Arctic sea <span class="hlt">ice</span>. The conditions in the Arctic, with</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017SPIE10091E..0BW','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017SPIE10091E..0BW"><span>Laser-assisted manufacturing of super-<span class="hlt">insulation</span> materials</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wang, Zhen; Zhang, Tao; Park, Byung Kyu; Lee, Woo Il; Hwang, David</p> <p>2017-02-01</p> <p>Being lightweight materials with good mechanical and thermal properties, hollow glass micro-particles (HGMPs) have been widely studied for multiple applications. In this study, it is shown that by using reduced binder fraction diluted in solvent, enables minimal contacts among the HGMPs assisted by a natural capillary trend, as confirmed by optical and electron microscope imaging. Such material architecture fabricated in a <span class="hlt">composite</span> level proves to have enhanced thermal <span class="hlt">insulation</span> performance through quantitative thermal conductivity measurement. Mechanical strength has also been evaluated in terms of particle-binder bonding by tensile test via in-situ microscope inspection. Effect of laser treatment was examined for further improvement of thermal and mechanical properties by selective binder removal and efficient redistribution of remaining binder components. The fabricated <span class="hlt">composite</span> materials have potential applications to building <span class="hlt">insulation</span> materials for their scalable manufacturing nature, improved thermal <span class="hlt">insulation</span> performance and reasonable mechanical strength. Further studies are needed to understand mechanical and thermal properties of the resulting <span class="hlt">composites</span>, and key fabrication mechanisms involved with laser treatment of complex multi-component and multi-phase systems.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018AIPA....8e5204H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018AIPA....8e5204H"><span>Performance of waste-<span class="hlt">paper</span>/PETG wood–plastic <span class="hlt">composites</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Huang, Lijie; An, Shuxiang; Li, Chunying; Huang, Chongxing; Wang, Shuangfei; Zhang, Xiaoxiao; Xu, Mingzi; Chen, Jie; Zhou, Lei</p> <p>2018-05-01</p> <p>Wood-plastic <span class="hlt">composites</span> were prepared from polyethylene terephthalate- 1,4-cyclohexanedimethanol ester (PETG) and waste-<span class="hlt">paper</span> fiber that was unmodified, modified with alkyl-ketene-dimer (AKD), and modified with a silane-coupling agent. The mechanical properties, water absorption properties, surface structure, and thermal properties of the three prepared materials were compared. The results showed that the optimum amount of waste-<span class="hlt">paper</span> powder is 10 wt%, while that of the waste-<span class="hlt">paper</span> particles is 60-80 mesh. The use of AKD and coupling agent KH550 can reduce the water absorption of the <span class="hlt">composite</span>; however, the reductive effect of the coupling agent is better, in that it is reduced by 0.3%. Modification using a 1-wt% KH550 coupling agent can effectively increase the tensile strength of a <span class="hlt">composite</span> from 31.36 to 41.67 MPa (increase of 32.8%), while the bending strength increased from 86.47 to 98.31 MPa (increase of 13.7%). This also enhances the thermal stability of the <span class="hlt">composites</span>. With the addition of the coupling agent, the <span class="hlt">composite</span> material maintains good mechanical properties even after being immersed in water; this can enable the safe use of these <span class="hlt">composite</span> materials in outdoor environments.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20120001909','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20120001909"><span>Polyimide Foams Offer Superior <span class="hlt">Insulation</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>2012-01-01</p> <p>At Langley Research Center, Erik Weiser and his colleagues in the Advanced Materials and Processing Branch were working with a new substance for fabricating <span class="hlt">composites</span> for use in supersonic aircraft. The team, however, was experiencing some frustration. Every time they tried to create a solid <span class="hlt">composite</span> from the polyimide (an advanced polymer) material, it bubbled and foamed. It seemed like the team had reached a dead end in their research - until they had another idea. "We said, This isn t going to work for <span class="hlt">composites</span>, but maybe we could make a foam out of it," Weiser says. "That was kind of our eureka moment, to see if we could go in a whole other direction. And it worked." Weiser and his colleagues invented a new kind of polyimide foam <span class="hlt">insulation</span> they named TEEK. The innovation displayed a host of advantages over existing <span class="hlt">insulation</span> options. Compared to other commercial foams, Weiser explains, polyimide foams perform well across a broad range of temperatures, noting that the NASA TEEK foams provide effective structural <span class="hlt">insulation</span> up to 600 F and down to cryogenic temperatures. The foam does not burn or off-gas toxic fumes, and even at -423 F - the temperature of liquid hydrogen - the material stays flexible. The inventors could produce the TEEK foam at a range of densities, from 0.5 pounds per cubic foot up to 20 pounds per cubic foot, making the foam ideal for a range of applications, including as <span class="hlt">insulation</span> for reusable launch vehicles and for cryogenic tanks and lines. They also developed a unique, friable balloon format for manufacturing the foam, producing it as hollow microspheres that allowed the foam to be molded and then cured into any desired shape - perfect for <span class="hlt">insulating</span> pipes of different sizes and configurations. The team s originally unplanned invention won an "R&D 100" award, and a later form of the foam, called LaRC FPF-44 (Spinoff 2009), was named "NASA Invention of the Year" in 2007.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.P51F..10B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.P51F..10B"><span>Effect of Adsorption on <span class="hlt">Ice</span> Surfaces on the <span class="hlt">Composition</span> of Enceladus' Plumes: Partitioning of Oxygen-Bearing Organics</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bouquet, A.; Teolis, B. D.; Waite, J. H., Jr.</p> <p>2017-12-01</p> <p>Introduction: The plumes of Enceladus offer an opportunity to access a sample of water from its internal ocean. However, to gain valuable insights into the ocean's <span class="hlt">composition</span>, it is necessary to take into account any possible process that would alter the mixture between the water table and the geysers. The adsorption of refractory compounds on the <span class="hlt">ice</span> walls in the vents could partition them depending on their properties. Evaluating the effect of this fractionation is critical in anticipating which organics could be detected by a future mission. Models: We used a model using the temkin isotherm and published experimental desorption energies for our compounds of interest. The model calculates how the coverage of an <span class="hlt">ice</span> surface exposed to the flow can evolve with time and what is the final <span class="hlt">composition</span> of the adsorbed mixture is. The model considers the <span class="hlt">ice</span> walls and the <span class="hlt">ice</span> grains, as the latter have the potential to gather the most sticky compounds and put them within reach of sampling by a spacecraft. Our list of species included formaldehyde, methanol, acetic acid, formic acid, ethanol, butanol, benzene and hexanal.Results: We found that simple hydrocarbons have a very short residence time on <span class="hlt">ice</span>, and are expected to stay in gas phase. Oxygen-bearing organic compounds, though, stick to the <span class="hlt">ice</span> and will be concentrated on the walls and <span class="hlt">ice</span> grains, with the exception of formaldehyde. With the species listed above originally in equal abundance in gas phase, we found the <span class="hlt">ice</span> surface to hold mostly formic acid, acetic acid and butanol, with a small amount of ethanol and hexanal. The high number of collisions in the closed space of a 1 meter wide vent allows for a gas/adsorbed equilibration within a second. Way forward: The possible impact of ammonia, detected in the plumes, is unknown. Ammonia can accumulate on the <span class="hlt">ice</span> surface and influence adsorption of other species, and potentially create a liquid layer by depressing the freezing point of water. The impact of these</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014JPhCS.507c2024K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014JPhCS.507c2024K"><span>Partial Discharge Characteristics in <span class="hlt">Composite</span> <span class="hlt">Insulation</span> Systems with PPLP for HTS Cable</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kikuchi, Y.; Yamashita, K.; Kumada, A.; Hidaka, K.; Tatamidani, K.; Masuda, T.</p> <p>2014-05-01</p> <p>The electrical <span class="hlt">insulation</span> system of high-temperature superconducting (HTS) cable consists of liquid nitrogen (N2(l)) and polypropylene laminated <span class="hlt">paper</span> (PPLP). Partial discharge (PD) may occur in butt gaps of the <span class="hlt">insulation</span> layers and its characteristics imply the <span class="hlt">insulation</span> performance of HTS cables. N2(l) cooling system is installed in the power system and N2(l) will flow through the cables during the system operation. Filling the HTS cable with N2(l) in order to perform pre-shipment inspection is time-consuming and costly for cable manufacturers. Therefore, they are trying to find a cost effective method for pre-shipment inspections. One alternative is to use high pressure gaseous nitrogen (N2(g)) instead of N2(l). This article investigates PD characteristics such as PD inception electric field (PDIE) and PD extinction electric field (PDEE) in butt gaps of HTS cables in 0.1 to 0.3 MPa and 0.1 MPa to 1.0 MPa N2(g) environments. For assessing the surface/volume effects, PD characteristics are measured with changing the size of butt gaps. It turns out that PDIE and PDEE in N2(g) are linearly correlated with those in N2(l) at any gas pressure in our testing, and PDIE in 1.0 MPa N2(g) is almost 30% of that in 0.2 MPa It suggests that PD characteristics in N2(l) can be extrapolated from those in N2(g).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/2021204','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/2021204"><span>Perioperative thermal <span class="hlt">insulation</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Sessler, D I; McGuire, J; Sessler, A M</p> <p>1991-05-01</p> <p>To determine the efficacy of passive <span class="hlt">insulators</span> advocated for prevention of cutaneous heat loss, we determined heat loss in unanesthetized volunteers covered by one of the following: a cloth "split sheet" surgical drape; a Convertors disposable-<span class="hlt">paper</span> split sheet; a Thermadrape disposable laparotomy sheet; an unheated Bair Hugger patient-warming blanket; 1.5-mil-thick plastic hamper bags; and a prewarmed, cotton hospital blanket. Cutaneous heat loss was measured using 10 area-weighted thermal flux transducers while volunteers were exposed to a 20.6 degrees C environment for 1 h. Heat loss decreased significantly from 100 +/- 3 W during the control periods to 69 +/- 6 W (average of all covers) after 1 h of treatment. Heat losses from volunteers <span class="hlt">insulated</span> by the Thermadrape (61 +/- 6 W) and Bair Hugger covers (64 +/- 5 W) were significantly less than losses from those <span class="hlt">insulated</span> by plastic bags (77 +/- 11 W). The <span class="hlt">paper</span> drape (67 +/- 7 W) provided slightly, but not significantly, better <span class="hlt">insulation</span> than the cloth drape (70 +/- 4 W). Coverage by prewarmed cotton blankets initially resulted in the least heat loss (58 +/- 8 W), but after 40 min, resulted in heat loss significantly greater than that for the Thermadrape (71 +/- 7 W). Regional heat loss was roughly proportional to surface area, and the distribution of regional heat loss remained similar with all covers. These data suggest that cost and convenience should be major factors when choosing among passive perioperative <span class="hlt">insulating</span> covers. It is likely that the amount of skin surface covered is more important than the choice of skin region covered or the choice of <span class="hlt">insulating</span> material.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012PhDT........52R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012PhDT........52R"><span>Force Criterion Prediction of Damage for Carbon/Epoxy <span class="hlt">Composite</span> Panels Impacted by High Velocity <span class="hlt">Ice</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rhymer, Jennifer D.</p> <p></p> <p>The use of advanced fiber-reinforced polymer matrix <span class="hlt">composites</span> in load-bearing aircraft structures is increasing, as evident by the various <span class="hlt">composites</span>-intensive transport aircraft presently under development. A major impact source of concern for these structures is hail <span class="hlt">ice</span>, which affects design and skin-sizing (skin thickness determination) at various locations of the aircraft. Impacts onto <span class="hlt">composite</span> structures often cause internal damage that is not visually detectable due to the high strength and resiliency of the <span class="hlt">composite</span> material (unlike impacts onto metallic structures). This internal damage and its effect on the performance of the structure are of great concern to the aircraft industry. The prediction of damage in <span class="hlt">composite</span> structures due to SHI impact has been accomplished via experimental work, explicit dynamic nonlinear finite element analysis (FEA) and the definition of design oriented relationships. Experiments established the critical threshold and corresponding analysis provided contact force results not readily measurable in high velocity SHI impact experiments. The design oriented relationships summarize the FEA results and experimental database into contact force estimation curves that can be easily applied for damage prediction. Failure thresholds were established for the experimental conditions (panel thickness ranging from 1.56 to 4.66 mm and <span class="hlt">ice</span> diameters from 38.1 to 61.0 mm). Additionally, the observations made by high-speed video during the impact event, and ultrasonic C-scan post-impact, showed how the <span class="hlt">ice</span> failed during impact and the overall shape and location of the panel damage. Through analysis, the critical force, the force level where damage occurs above but not below, of a SHI impact onto the panel was found to be dependent only on the target structure. However, the peak force generated during impact was dependent on both the projectile and target. Design-oriented curves were generated allowing the prediction of the allowable</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016MS%26E..139a2042P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016MS%26E..139a2042P"><span>Interlaminar interaction in <span class="hlt">paper</span> thermoplastic laminate <span class="hlt">composites</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Prambauer, M.; Paulik, C.; Burgstaller, C.</p> <p>2016-07-01</p> <p>Bio-based <span class="hlt">composites</span> are a research topic since several decades, which aims for sustainable and durable materials. In the scope of this research, many different sources for biobased reinforcements have been investigated. Typical issues associated with the use of such are property variations due to cultivation area and climate, besides the influences of the type, pretreatment and fibre geometry. Another issue can be the availability of such natural fibres. Due to these reasons, we started using <span class="hlt">paper</span> sheets as reinforcements in laminate <span class="hlt">composites</span> with thermoplastic materials. In preliminary studies with polypropylene <span class="hlt">composites</span>, we found good mechanical properties, even higher than could be expected by estimating the <span class="hlt">composite</span> properties from the constituents by applying simple rule of mixtures type models. We suspect, besides some effect of <span class="hlt">paper</span> compaction, interlaminar effects to be the reason for this. Therefore, the aim of this work is to investigate the effects of the interfacial interaction on the different <span class="hlt">paper</span> laminate properties due to different matrix polymers. For this work, we used polypropylene, polyamide 6 and 12 as well as polystyrene. <span class="hlt">Composites</span> were produced via compression moulding and samples for mechanical testing and density evaluation were cut from the moulded plates. The results from mechanical tests show, that there is a reinforcing effect, regardless of matrix polymer used. Simple rule of mixtures evaluations show, that the different matrices exhibit different degrees of interaction, based on their chemical structure. In addition, also influences due to processing were found.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19950025344','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19950025344"><span>A water blown urethane <span class="hlt">insulation</span> for use in cryogenic environments</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Blevins, Elana; Sharpe, Jon</p> <p>1995-01-01</p> <p>Thermal Protection Systems (TPS) of NASA's Space Shuttle External Tank include polyurethane and polyisocyanurate modified polyurethane foam <span class="hlt">insulations</span>. These <span class="hlt">insulations</span>, currently foamed with CFC 11 blowing agent, serve to maintain cryogenic propellant quality, maintain the external tank structural temperature limits, and minimize the formation of <span class="hlt">ice</span> and frost that could potentially damage the ceramic <span class="hlt">insulation</span> on the space shuttle orbiter. During flight the external tank <span class="hlt">insulations</span> are exposed to mechanical, thermal and acoustical stresses. TPS must pass cryogenic flexure and substrate adhesion tests at -253 C, aerothermal and radiant heating tests at fluxes up to approximately 14 kilowatts per square meter, and thermal conductivity tests at cryogenic and elevated temperatures. Due to environmental concerns, the polyurethane <span class="hlt">insulation</span> industry and the External Tank Project are tasked with replacing CFC 11. The flight qualification of foam <span class="hlt">insulations</span> employing HCFC 141b as a foaming agent is currently in progress; HCFC 141b blown <span class="hlt">insulations</span> are scheduled for production implementation in 1995. Realizing that the second generation HCFC blowing agents are an interim solution, the evaluation of third generation blowing agents with zero ozone depletion potential is underway. NASA's TPS Materials Research Laboratory is evaluating third generation blowing agents in cryogenic <span class="hlt">insulations</span> for the External Tank; one option being investigated is the use of water as a foaming agent. A dimensionally stable <span class="hlt">insulation</span> with low friability, good adhesion to cryogenic substrates, and acceptable thermal conductivity has been developed with low viscosity materials that are easily processed in molding applications. The development criteria, statistical experimental approach, and resulting foam properties will be presented.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li class="active"><span>8</span></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_8 --> <div id="page_9" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li class="active"><span>9</span></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="161"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23722071','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23722071"><span><span class="hlt">Insulating</span> epoxy/barite and polyester/barite <span class="hlt">composites</span> for radiation attenuation.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>El-Sarraf, M A; El-Sayed Abdo, A</p> <p>2013-09-01</p> <p>A trial has been made to create <span class="hlt">insulating</span> Epoxy/Barite (EP/Brt) (ρ=2.85 g cm(-3)) and Crosslinked Unsaturated Polyester/Barite (CUP/Brt) (ρ=3.25 g cm(-3)) <span class="hlt">composites</span> with radiation attenuation and shielding capabilities. Experimental work regarding mechanical and physical properties was performed to study the <span class="hlt">composites</span> integrity for practical applications. The properties were found to be reasonable. Radiation attenuation properties have been carried out using emitted collimated beam from a fission (252)Cf (100 µg) neutron source, and the neutron-gamma spectrometer with stilbene scintillator. The pulse shape discriminating (P.S.D) technique based on the zero cross-over method was used to discriminate between neutron and gamma-ray pulses. Thermal neutron fluxes, measured using the BF3 detector and thermal neutron detection system, were used to plot the attenuation relations. The fast neutron macroscopic effective removal cross-section ΣR, gamma ray total attenuation coefficient µ and thermal neutron macroscopic cross-section Σ have been evaluated. Theoretical calculations have been achieved using MCNP-4C2 code to calculate ΣR, µ and Σ. Also, MERCSF-N program was used to calculate macroscopic effective removal cross-section ΣR. Measured and calculated results have been compared and were found to be in reasonable agreement. Copyright © 2013 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JAdD....730001M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JAdD....730001M"><span>Electrical <span class="hlt">insulating</span> liquid: A review</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mahanta, Deba Kumar; Laskar, Shakuntala</p> <p></p> <p><span class="hlt">Insulating</span> liquid plays an important role for the life span of the transformer. Petroleum-based mineral oil has become dominant <span class="hlt">insulating</span> liquid of transformer for more than a century for its excellent dielectric and cooling properties. However, the usage of petroleum-based mineral oil, derived from a nonrenewable energy source, has affected the environment for its nonbiodegradability property. Therefore, researchers direct their attention to renewable and biodegradable alternatives. Palm fatty acid ester, coconut oil, sunflower oil, etc. are considered as alternatives to replace mineral oil as transformer <span class="hlt">insulation</span> liquid. This <span class="hlt">paper</span> gives an extensive review of different liquid <span class="hlt">insulating</span> materials used in a transformer. Characterization of different liquids as an <span class="hlt">insulating</span> material has been discussed. An attempt has been made to classify different <span class="hlt">insulating</span> liquids-based on different properties.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JIEID..98..297H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JIEID..98..297H"><span>Prospect of Thermal <span class="hlt">Insulation</span> by Silica Aerogel: A Brief Review</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hasan, Mohammed Adnan; Sangashetty, Rashmi; Esther, A. Carmel Mary; Patil, Sharanabasappa B.; Sherikar, Baburao N.; Dey, Arjun</p> <p>2017-10-01</p> <p>Silica aerogel is a unique ultra light weight nano porous material which offers superior thermal <span class="hlt">insulation</span> property as compared to the conventional thermal <span class="hlt">insulating</span> materials. It can be applied not only for ground and aerospace applications but also in low and high temperatures and pressure regimes. Aerogel granules and monolith are synthesized by the sol-gel route while aerogel based <span class="hlt">composites</span> are fabricated by the reinforcement of fibers, particle and opacifiers. Due to the characteristic brittleness (i.e., poor mechanical properties) of monolith or bulk aerogel, it is restricted in several applications. To improve the mechanical integrity and flexibility, usually different fibers are reinforced with aerogel and hence it can be used as flexible thermal <span class="hlt">insulation</span> blankets. Further, to achieve effective thermal <span class="hlt">insulation</span> behaviour particularly at high temperature, often opacifiers are doped with silica aerogel. In the present brief review, the prospects of bulk aerogel and aerogel based <span class="hlt">composites</span> are discussed for the application of thermal <span class="hlt">insulation</span> and thermal stability.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19840015597','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19840015597"><span>Advanced leading edge thermal-structure concept. Direct bond reusable surface <span class="hlt">insulation</span> to a <span class="hlt">composite</span> structure</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Riccitiello, S. R.; Figueroa, H.; Coe, C. F.; Kuo, C. P.</p> <p>1984-01-01</p> <p>An advanced leading-edge concept was analyzed using the space shuttle leading edge system as a reference model. The comparison indicates that a direct-bond system utilizing a high temperature (2700 F) fibrous refractory <span class="hlt">composite</span> <span class="hlt">insulation</span> tile bonded to a high temperature (PI/graphite) <span class="hlt">composite</span> structure can result in a weight savings of up to 800 lb. The concern that tile damage or loss during ascent would result in adverse entry aerodynamics if a leading edge tile system were used is addressed. It was found from experiment that missing tiles (as many as 22) on the leading edge would not significantly affect the basic force-and-moment aerodynamic coefficients. Additionally, this concept affords a degree of redundancy to a thermal protection system in that the base structure (being a <span class="hlt">composite</span> material) ablates and neither melts nor burns through when subjected to entry heating in the event tiles are actually lost or damaged during ascent.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1998PhDT.........8T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1998PhDT.........8T"><span>CO-<span class="hlt">ices</span> in embedded Young Stellar Objects</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Teixeira, Teresa Cláeira V. S.</p> <p>1998-09-01</p> <p>Stars are born in dense cores within molecular clouds, enshrouded in large cocoons of gas and dust which completely obscure the forming star. The large degree of obscuration towards the young stars is due to the presence of solid dust grains in their circumstellar envelopes, which efficiently absorb the radiation from the star at visual and ultraviolet wavelengths, reradiating that energy at far-infrared and submillimeter wavelengths. The <span class="hlt">composition</span> and structure of the dust grains is not well known, but current studies point to grains having a refractory core and acquiring <span class="hlt">ice</span> mantles in the cool, shielded conditions of molecular clouds. Such <span class="hlt">ice</span> mantles are the subject of this thesis. Infrared spectroscopy is an important tool in the study of the complex <span class="hlt">ice</span> mantles on interstellar grains. A variety of absorption features at these wavelengths, which have been identified as the vibrational transitions of the molecules in the <span class="hlt">ices</span>, can provide important information on the <span class="hlt">composition</span>, structure and evolution of the grains. The work reported in this thesis consists of an observational study of the <span class="hlt">composition</span> of the <span class="hlt">ice</span> mantles acquired by the dust grains in molecular clouds (with particular emphasis on the CO-<span class="hlt">ices</span> in the material surrounding embedded Young Stellar Objects in nearby molecular clouds), what can be learned from that about the physical conditions in the regions where the <span class="hlt">ice</span> mantles exist, and what may affect their survival and evolution. In this work, spectra of the 4.67 micron solid CO absorption feature are presented, mostly towards embedded objects in Taurus. The thesis starts with a brief overview of technical aspects of spectroscopic observations at thermal infrared wavelengths, where the CO stretch absorption feature is located. The observations and data reduction procedures are then reported and discussed in detail. The likely <span class="hlt">composition</span> of the CO-bearing <span class="hlt">ices</span> is analysed by fitting the observations with laboratory data. The statistical</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=64765&Lab=NERL&keyword=jury&actType=&TIMSType=+&TIMSSubTypeID=&DEID=&epaNumber=&ntisID=&archiveStatus=Both&ombCat=Any&dateBeginCreated=&dateEndCreated=&dateBeginPublishedPresented=&dateEndPublishedPresented=&dateBeginUpdated=&dateEndUpdated=&dateBeginCompleted=&dateEndCompleted=&personID=&role=Any&journalID=&publisherID=&sortBy=revisionDate&count=50','EPA-EIMS'); return false;" href="https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=64765&Lab=NERL&keyword=jury&actType=&TIMSType=+&TIMSSubTypeID=&DEID=&epaNumber=&ntisID=&archiveStatus=Both&ombCat=Any&dateBeginCreated=&dateEndCreated=&dateBeginPublishedPresented=&dateEndPublishedPresented=&dateBeginUpdated=&dateEndUpdated=&dateBeginCompleted=&dateEndCompleted=&personID=&role=Any&journalID=&publisherID=&sortBy=revisionDate&count=50"><span>ION <span class="hlt">COMPOSITION</span> ELUCIDATION (<span class="hlt">ICE</span>): AN INVESTIGATIVE TOOL FOR CHARACTERIZATION AND IDENTIFICATION OF COMPOUNDS OF REGULATORY IMPORTANCE</span></a></p> <p><a target="_blank" href="http://oaspub.epa.gov/eims/query.page">EPA Science Inventory</a></p> <p></p> <p></p> <p>Ion <span class="hlt">Composition</span> Elucidation (<span class="hlt">ICE</span>) often leads to identification of compounds and provides high quality evidence for tracking compounds to their sources. Mass spectra for most organic compounds are not found in mass spectral libraries used to tentatively identify analytes. In addi...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1986PhDT........63M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1986PhDT........63M"><span>Resistivity and Resistivity Fluctuations of Thin Film Platinum-Aluminum Oxide Granular Metal-<span class="hlt">Insulator</span> <span class="hlt">Composites</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mantese, Joseph Vito</p> <p></p> <p>Thin film metal-<span class="hlt">insulator</span> <span class="hlt">composites</span> were used to study how the resistivity and fluctuations in the resistivity were altered by changes in conduction mechanism so as to understand the source of the fluctuations and to better understand the conduction processes themselves. Metal-<span class="hlt">insulator</span> <span class="hlt">composites</span> were prepared by co -evaporation of platinum and aluminum oxide in a high vacuum system to create a series of films which had a range of metal volume fill fractions, p, from 23% to 100%. The samples were patterned using standard photolithographic techniques to form sample geometries of typical dimensions, length (TURN) 40(mu)m, width (TURN) 2(mu)m and thickness (TURN) 1500(ANGSTROM). The resistivity, (rho), and power spectral density of the resistivity fluctuations, S(,(rho))(f), were measured as a function of p and temperature, T. (rho)(p,T) was found to be a rapidly increasing function of decreasing p, rising monotonically by more than 7 orders of magnitude as p was decreased from 100% to 23%. For p (GREATERTHEQ) 59% the resistivity decreased linearly with decreasing temperature until limited by impurity scattering. The resistivities for the low metal fill fraction materials (p (LESSTHEQ) 50%) increased as the temperature was reduced as expected of thermally assisted tunneling conduction in metal-<span class="hlt">insulator</span> <span class="hlt">composites</span>. The transition from metallic conduction to thermally assisted tunneling occurred at a critical value, p(,c), between 59% and 50% Pt. For all samples at all p and T, S(,(rho))(f)(PROPORTIONAL)1/f('(alpha)) (1/f noise) with 0.8 (LESSTHEQ) (alpha) (LESSTHEQ) .1.2 and f the frequency in Hertz. No systematic dependence upon either p or T was found. The normalized noise intensity fS(,(rho))(f)/(rho)('2) (,1) (,Hz) was found to increase monotonically by 5 orders of magnitude with decreasing p then saturate at p(,c) where the conduction mechanism changed from metallic conduction to thermally assisted tunneling. Effective medium theory was used to analyze the role</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018AIPC.1971d0021D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018AIPC.1971d0021D"><span><span class="hlt">Insulation</span> detection of electric vehicle batteries</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dai, Qiqi; Zhu, Zhongwen; Huang, Denggao; Du, Mingxing; Wei, Kexin</p> <p>2018-06-01</p> <p>In this <span class="hlt">paper</span>, an electric vehicle <span class="hlt">insulation</span> detection method with single side switching fixed resistance is designed, and the hardware and software design of the system are given. The experiment proves that the <span class="hlt">insulation</span> detection system can detect the <span class="hlt">insulation</span> resistance in a wide range of resistance values, and accurately report the fault level. This system can effectively monitor the <span class="hlt">insulation</span> fault between the car body and the high voltage line and avoid the passengers from being injured.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/20361995','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/20361995"><span>Plant proteins as binders in cellulosic <span class="hlt">paper</span> <span class="hlt">composites</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Fahmy, Yehia; El-Wakil, Nahla A; El-Gendy, Ahmed A; Abou-Zeid, Ragab E; Youssef, M A</p> <p>2010-07-01</p> <p>Plant proteins are used - for the first time - in this work as bulk binders for cellulosic fibers in <span class="hlt">paper</span> <span class="hlt">composites</span>. Soy bean protein and wheat gluten were denatured by two methods, namely by: urea+NaOH and by urea+NaOH+acrylamide. Addition of increased amounts of the denatured proteins resulted in a significant increase in all <span class="hlt">paper</span> strength properties. Soy protein led, in addition, to a remarkable enhancement in opacity. The use of proteins increased kaolin retention in the <span class="hlt">paper</span> <span class="hlt">composites</span>, while keeping the <span class="hlt">paper</span> strength higher than the blank protein-free <span class="hlt">paper</span>. The results show that plant proteins are favorable than synthetic adhesives; because they are biodegradable and do not cause troubles in <span class="hlt">paper</span> recycling i.e. they are environmentally friendly. (c) 2010 Elsevier B.V. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015JKPS...67.1783H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015JKPS...67.1783H"><span>DC breakdown characteristics of silicone polymer <span class="hlt">composites</span> for HVDC <span class="hlt">insulator</span> applications</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Han, Byung-Jo; Seo, In-Jin; Seong, Jae-Kyu; Hwang, Young-Ho; Yang, Hai-Won</p> <p>2015-11-01</p> <p>Critical components for HVDC transmission systems are polymer <span class="hlt">insulators</span>, which have stricter requirements that are more difficult to achieve compared to those of HVAC <span class="hlt">insulators</span>. In this study, we investigated the optimal design of HVDC polymer <span class="hlt">insulators</span> by using a DC electric field analysis and experiments. The physical properties of the polymer specimens were analyzed to develop an optimal HVDC polymer material, and four polymer specimens were prepared for DC breakdown experiments. Single and reverse polarity breakdown tests were conducted to analyze the effect of temperature on the breakdown strength of the polymer. In addition, electric fields were analyzed via simulations, in which a small-scale polymer <span class="hlt">insulator</span> model was applied to prevent dielectric breakdown due to electric field concentration, with four DC operating conditions taken into consideration. The experimental results show that the electrical breakdown strength and the electric field distribution exhibit significant differences in relation to different DC polarity transition procedures.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28335980','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28335980"><span><span class="hlt">Paper</span>-polymer <span class="hlt">composite</span> devices with minimal fluorescence background.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wang, Chang-Ming; Chen, Chong-You; Liao, Wei-Ssu</p> <p>2017-04-22</p> <p>Polymer film incorporated <span class="hlt">paper</span>-based devices show advantages in simplicity and rugged backing. However, their applications are restricted by the high fluorescence background interference of conventional laminating pouches. Herein, we report a straightforward approach for minimal fluorescence background device fabrication, in which filter <span class="hlt">paper</span> was shaped and laminated in between two biaxially oriented polypropylene (OPP) and polyvinyl butyral (PVB) <span class="hlt">composite</span> films. This <span class="hlt">composite</span> film provides mechanical strength for enhanced device durability, protection from environmental contamination, and prevents reagent degradation. This approach was tested by the determination of copper ions with a fluorescent probe, while the detection of glucose was used to illustrate the improved device durability. Our results show that lamination by the polymer <span class="hlt">composite</span> lengthens device lifetime, while allowing for fluorescence detection methods combination with greatly reduced fluorescent background widely present in commercially available lamination pouches. By the combination of rapid device prototyping with low cost materials, we believe that this <span class="hlt">composite</span> design would further expand the potential of <span class="hlt">paper</span>-based devices. Copyright © 2017 Elsevier B.V. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29771682','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29771682"><span>Graphene nanoplatelet <span class="hlt">composite</span> '<span class="hlt">paper</span>' as an electrostatic actuator.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Yu, Zeyang; Drzal, Lawrence T</p> <p>2018-08-03</p> <p>Graphene nanoplatelets (GnP) can be made into a thin '<span class="hlt">paper</span>' through vacuum filtration of GnP suspension. Electrodes were fabricated from the compressed GnP <span class="hlt">paper</span> and then by coating the surface with epoxy. The electrostatic actuator was constructed from two parallel-aligned <span class="hlt">composite</span> <span class="hlt">papers</span> fixed at the anode and a cathode connected to ground. The two <span class="hlt">composite</span> <span class="hlt">papers</span> would then separate when a voltage was applied. The GnP <span class="hlt">paper</span> was also modified to increase surface area by introducing porosity or adding ∼10 wt% C750 (GnP with diameter less than 1 μm); or changing the relative permittivity by adding barium titanate particles; or combining these two effects by adding CNCs. Overall the output work could be significantly improved to over 400%.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19930081073','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19930081073"><span>The Prevention of the <span class="hlt">Ice</span> Hazard on Airplanes</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Geer, William C; Scott, Merit</p> <p>1930-01-01</p> <p>A review of various methods to prevent <span class="hlt">ice</span> formation and adhesion to aircraft surfaces is given. It was concluded that the adhesion of <span class="hlt">ice</span> to a surface may be reduced somewhat by the application of certain waxes and varnishes. In the experiments described, the varnishes containing calcium stearate and calcium oleate gave the best results. In wind tunnel tests, the adhesion was further reduced by the application of these waxes and varnishes to a thin, heat <span class="hlt">insulating</span> layer of rubber. The adhesion of <span class="hlt">ice</span> is greatly reduced when the surface consists of a vehicle which carries an oil in sufficient quantity so that the surface of the vehicle is self lubricating. <span class="hlt">Ice</span> may be removed from wings, struts, wires and other parts of an airplane during flight by the inflation of properly constructed pneumatic rubber members, providing that these members have been previously treated with a suitable low adhesion oil.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017CEEng..13...20T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017CEEng..13...20T"><span>Determination of the Airborne Sound <span class="hlt">Insulation</span> of a Straw Bale Partition Wall</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Teslík, Jiří; Fabian, Radek; Hrubá, Barbora</p> <p>2017-06-01</p> <p>This <span class="hlt">paper</span> describes the results of a scientific project focused on determining of the Airborne Sound <span class="hlt">Insulation</span> of a peripheral non-load bearing wall made of straw bales expressed by Weighted Sound Reduction Index. Weighted Sound Reduction Index was determined by measuring in the certified acoustic laboratory at the Faculty of Mechanical Engineering at Brno University of Technology. The measured structure of the straw wall was modified in combinations with various materials, so the results include a wide range of possible <span class="hlt">compositions</span> of the wall. The key modification was application of plaster on both sides of the straw bale wall. This construction as is frequently done in actual straw houses. The additional measurements were performed on the straw wall with several variants of additional wall of slab materials. The airborne sound <span class="hlt">insulation</span> value has been also measured in separate stages of the construction. Thus it is possible to compare and determinate the effect of the single layers on the airborne sound <span class="hlt">insulation</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018AcAau.145..293L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018AcAau.145..293L"><span>Erosion characteristics of ethylene propylene diene monomer <span class="hlt">composite</span> <span class="hlt">insulation</span> by high-temperature dense particles</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Li, Jiang; Guo, Meng-fei; Lv, Xiang; Liu, Yang; Xi, Kun; Guan, Yi-wen</p> <p>2018-04-01</p> <p>In this study, a dense particles erosion test motor which can simulate the erosion state of a solid rocket motor under high acceleration was developed. Subsequently, erosion experiments were carried out for the ethylene propylene diene monomer <span class="hlt">composite</span> <span class="hlt">insulation</span> and the microstructure of the char layer analysed. A turning point effect was found from the influence of the particle impact velocity on the ablation rate, and three erosion modes were determined according to the micro-morphology of the char layer. A reasonable explanation for the different structures of the char layer in the three modes was presented based on the formation mechanism of the compact/loose structure of the char layer.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1999SSRv...90..219A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1999SSRv...90..219A"><span>Evolution of Interstellar <span class="hlt">Ices</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Allamandola, Louis J.; Bernstein, Max P.; Sandford, Scott A.; Walker, Robert L.</p> <p>1999-10-01</p> <p>Infrared observations, combined with realistic laboratory simulations, have revolutionized our understanding of interstellar <span class="hlt">ice</span> and dust, the building blocks of comets. <span class="hlt">Ices</span> in molecular clouds are dominated by the very simple molecules H2O, CH3OH, NH3, CO, CO2, and probably H2CO and H2. More complex species including nitriles, ketones, and esters are also present, but at lower concentrations. The evidence for these, as well as the abundant, carbon-rich, interstellar, polycyclic aromatic hydrocarbons (PAHs) is reviewed. Other possible contributors to the interstellar/pre-cometary <span class="hlt">ice</span> <span class="hlt">composition</span> include accretion of gas-phase molecules and in situ photochemical processing. By virtue of their low abundance, accretion of simple gas-phase species is shown to be the least important of the processes considered in determining <span class="hlt">ice</span> <span class="hlt">composition</span>. On the other hand, photochemical processing does play an important role in driving dust evolution and the <span class="hlt">composition</span> of minor species. Ultraviolet photolysis of realistic laboratory analogs readily produces H2, H2CO, CO2, CO, CH4, HCO, and the moderately complex organic molecules: CH3CH2OH (ethanol), HC(=O)NH2 (formamide), CH3C(=O)NH2 (acetamide), R-CN (nitriles), and hexamethylenetetramine (HMT, C6H12N4), as well as more complex species including amides, ketones, and polyoxymethylenes (POMs). Inclusion of PAHs in the <span class="hlt">ices</span> produces many species similar to those found in meteorites including aromatic alcohols, quinones and ethers. Photon assisted PAH-<span class="hlt">ice</span> deuterium exchange also occurs. All of these species are readily formed and are therefore likely cometary constituents.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014JGRD..11914045O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014JGRD..11914045O"><span>Chemical <span class="hlt">compositions</span> of sulfate and chloride salts over the last termination reconstructed from the Dome Fuji <span class="hlt">ice</span> core, inland Antarctica</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Oyabu, Ikumi; Iizuka, Yoshinori; Uemura, Ryu; Miyake, Takayuki; Hirabayashi, Motohiro; Motoyama, Hideaki; Sakurai, Toshimitsu; Suzuki, Toshitaka; Hondoh, Takeo</p> <p>2014-12-01</p> <p>The flux and chemical <span class="hlt">composition</span> of aerosols impact the climate. Antarctic <span class="hlt">ice</span> cores preserve the record of past atmospheric aerosols, providing useful information about past atmospheric environments. However, few studies have directly measured the chemical <span class="hlt">composition</span> of aerosol particles preserved in <span class="hlt">ice</span> cores. Here we present the chemical <span class="hlt">compositions</span> of sulfate and chloride salts from aerosol particles in the Dome Fuji <span class="hlt">ice</span> core. The analysis method involves <span class="hlt">ice</span> sublimation, and the period covers the last termination, 25.0-11.0 thousand years before present (kyr B.P.), with a 350 year resolution. The major components of the soluble particles are CaSO4, Na2SO4, and NaCl. The dominant sulfate salt changes at 16.8 kyr B.P. from CaSO4, a glacial type, to Na2SO4, an interglacial type. The sulfate salt flux (CaSO4 plus Na2SO4) inversely correlates with δ18O in Dome Fuji over millennial timescales. This correlation is consistent with the idea that sulfate salt aerosols contributed to the last deglacial warming of inland Antarctica by reducing the aerosol indirect effect. Between 16.3 and 11.0 kyr B.P., the presence of NaCl suggests that winter atmospheric aerosols are preserved. A high NaCl/Na2SO4 fraction between 12.3 and 11.0 kyr B.P. indicates that the contribution from the transport of winter atmospheric aerosols increased during this period.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018E%26ES..102a2014S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018E%26ES..102a2014S"><span>Nutritional <span class="hlt">composition</span>, glycemic index, glycemic load, and organoleptical quality of glucomannan-enriched soy milk <span class="hlt">ice</span> cream</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sa'adah, S.; Candra, O. M.; Nugrahani, G.; Pramono, A.; Afifah, D. N.</p> <p>2018-01-01</p> <p>Over the past decades, the number of childhood obesity cases has increased significantly, which led to an increase in the number of adults suffering from degenerative diseases such as diabetes mellitus (DM). Glucomannan-Enriched Soy Milk <span class="hlt">Ice</span> Cream (GSMIC) may prevent obesity in children. The aim of the study was to test the level of carbohydrates, protein, fat, dietary fiber, glycemic index, glycemic load, and organoleptic quality of GSMIC. This experiment used a completely randomized design to test three formulations of glucomannan flour and soy milk (0.5%, 1.5%, and 2.5%). The products were tested for nutritional <span class="hlt">composition</span>, and evaluated on glycemic index, glycemic load, and organoleptic quality. GSMIC 2.5% had higher levels of dietary fiber and high carbohydrate, protein, and fat content compared to <span class="hlt">ice</span> cream (3.99%, 30.7%, 1.50%, 1.33%, respectively). The glycemic index of <span class="hlt">ice</span> cream and 2.5% GSMIC were 75.83 (75%) and 51.48 (51%), respectively, while the glycemic load of <span class="hlt">ice</span> cream and 2.5% GSMIC were 9.04 and 11.61, respectively. Based on the organoleptic analysis, formulation preferred by the panellists was 2.5% glucomannan flour. Glucomannan flour affected the level of carbohydrates, protein, fat, dietary fiber, glycemic index, glycemic load, and organoleptic quality in soy milk <span class="hlt">ice</span> cream.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5097149','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5097149"><span>Production and evaluation of mineral and nutrient contents, chemical <span class="hlt">composition</span>, and sensory properties of <span class="hlt">ice</span> creams fortified with laboratory-prepared peach fibre</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Yangılar, Filiz</p> <p>2016-01-01</p> <p>Background In the coming years, a nutraceutical food may provide both physical and mental benefits that are commonly attributed to the active components of the food. Objective In this study, we determined the nutrient and mineral contents, sensory properties, and physical and chemical characteristics of <span class="hlt">ice</span> creams manufactured using peach fibre at different concentrations (1 and 2%). Method A total of five experimental groups were formed: two types (from peach peel and pulp) of flour, two fibre concentrations (1 and 2%), and a control group without fibres. Results Flour obtained from peach pulp and peel was found to have a significant (p<0.05) effect on the chemical <span class="hlt">composition</span> and elemental <span class="hlt">composition</span> of <span class="hlt">ice</span> cream samples, especially the rates of Ca, K, Mg, and P, which increased in the samples depending on the content of peach fibre. Sensory ratings and acceptability of <span class="hlt">ice</span> creams decreased significantly with increasing peach peel fibre, whereas <span class="hlt">ice</span> creams made with C (control) and B1 (<span class="hlt">ice</span> creams made from 1% peach pulp fibre) was the highest scored by the panellists. Conclusions Peach fibre concentrates might be used as a good source of nutraceutical ingredients. PMID:27814781</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..1814695S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..1814695S"><span>N-<span class="hlt">ICE</span>2015: Multi-disciplinary study of the young sea <span class="hlt">ice</span> system north of Svalbard from winter to summer.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Steen, Harald; Granskog, Mats; Assmy, Philipp; Duarte, Pedro; Hudson, Stephen; Gerland, Sebastian; Spreen, Gunnar; Smedsrud, Lars H.</p> <p>2016-04-01</p> <p>The Arctic Ocean is shifting to a new regime with a thinner and smaller sea-<span class="hlt">ice</span> area cover. Until now, winter sea <span class="hlt">ice</span> extent has changed less than during summer, as the heat loss to the atmosphere during autumn and winter is large enough form an <span class="hlt">ice</span> cover in most regions. The <span class="hlt">insulating</span> snow cover also heavily influences the winter <span class="hlt">ice</span> growth. Consequently, the older, thicker multi-year sea <span class="hlt">ice</span> has been replace by a younger and thinner sea. These large changes in the sea <span class="hlt">ice</span> cover may have dramatic consequences for ecosystems, energy fluxes and ultimately atmospheric circulation and the Northern Hemisphere climate. To study the effects of the changing Arctic the Norwegian Polar Institute, together with national and international partners, launched from January 11 to June 24, 2015 the Norwegian Young Sea <span class="hlt">ICE</span> cruise 2015 (N-<span class="hlt">ICE</span>2015). N-<span class="hlt">ICE</span>2015 was a multi-disciplinary cruise aimed at simultaneously studying the effect of the Arctic Ocean changes in the sea <span class="hlt">ice</span>, the atmosphere, in radiation, in ecosystems. as well as water chemistry. R/V Lance was frozen into the drift <span class="hlt">ice</span> north of Svalbard at about N83 E25 and drifted passively southwards with the <span class="hlt">ice</span> until she was broken loose. When she was loose, R/V Lance was brought back north to a similar starting position. While fast in the <span class="hlt">ice</span>, she served as a living and working platform for 100 scientist and engineers from 11 countries. One aim of N-<span class="hlt">ICE</span>2015 is to present a comprehensive data-set on the first year <span class="hlt">ice</span> dominated system available for the scientific community describing the state and changes of the Arctic sea <span class="hlt">ice</span> system from freezing to melt. Analyzing the data is progressing and some first results will be presented.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li class="active"><span>9</span></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_9 --> <div id="page_10" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li class="active"><span>10</span></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="181"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70037558','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70037558"><span>On the nature of the dirty <span class="hlt">ice</span> at the bottom of the GISP2 <span class="hlt">ice</span> core</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Bender, Michael L.; Burgess, Edward; Alley, Richard B.; Barnett, Bruce; Clow, Gary D.</p> <p>2010-01-01</p> <p>We present data on the triple Ar isotope <span class="hlt">composition</span> in trapped gas from clean, stratigraphically disturbed <span class="hlt">ice</span> between 2800 and 3040m depth in the GISP2 <span class="hlt">ice</span> core, and from basal dirty <span class="hlt">ice</span> from 3040 to 3053m depth. We also present data for the abundance and isotopic <span class="hlt">composition</span> of O2 and N2, and abundance of Ar, in the basal dirty <span class="hlt">ice</span>. The Ar/N2 ratio of dirty basal <span class="hlt">ice</span>, the heavy isotope enrichment (reflecting gravitational fractionation), and the total gas content all indicate that the gases in basal dirty <span class="hlt">ice</span> originate from the assimilation of clean <span class="hlt">ice</span> of the overlying glacier, which comprises most of the <span class="hlt">ice</span> in the dirty bottom layer. O2 is partly to completely depleted in basal <span class="hlt">ice</span>, reflecting active metabolism. The gravitationally corrected ratio of 40Ar/38Ar, which decreases with age in the global atmosphere, is compatible with an age of 100-250ka for clean disturbed <span class="hlt">ice</span>. In basal <span class="hlt">ice</span>, 40Ar is present in excess due to injection of radiogenic 40Ar produced in the underlying continental crust. The weak depth gradient of 40Ar in the dirty basal <span class="hlt">ice</span>, and the distribution of dirt, indicate mixing within the basal <span class="hlt">ice</span>, while various published lines of evidence indicate mixing within the overlying clean, disturbed <span class="hlt">ice</span>. Excess CH4, which reaches thousands of ppm in basal dirty <span class="hlt">ice</span> at GRIP, is virtually absent in overlying clean disturbed <span class="hlt">ice</span>, demonstrating that mixing of dirty basal <span class="hlt">ice</span> into the overlying clean <span class="hlt">ice</span>, if it occurs at all, is very slow. Order-of-magnitude estimates indicate that the mixing rate of clean <span class="hlt">ice</span> into dirty <span class="hlt">ice</span> is sufficient to maintain a steady thickness of dirty <span class="hlt">ice</span> against thinning from the mean <span class="hlt">ice</span> flow. The dirty <span class="hlt">ice</span> appears to consist of two or more basal components in addition to clean glacial <span class="hlt">ice</span>. A small amount of soil or permafrost, plus preglacial snow, lake or ground <span class="hlt">ice</span> could explain the observations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19730002820','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19730002820"><span>Development of advanced materials <span class="hlt">composites</span> for use as <span class="hlt">insulations</span> for LH2 tanks</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Lemons, C. R.; Watts, C. R.; Salmassy, O. K.</p> <p>1972-01-01</p> <p>A study of internal <span class="hlt">insulation</span> materials and fabrication processes for space shuttle LH2 tanks is reported. Emphasis was placed on an <span class="hlt">insulation</span> system capable of reentry and multiple reuse in the Shuttle environment. Results are given on the optimization and manufacturing process scale-up of a 3D fiberreinforced foam <span class="hlt">insulation</span>, BX-251-3D, derived from the Saturn S-4B internal <span class="hlt">insulation</span>. It is shown that BX-251-3D can be satisfactorily installed in large-scale tanks under conditions that will permit a significant cost saving over the existing S-4B technology.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015JGRC..120..647F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015JGRC..120..647F"><span>The refreezing of melt ponds on Arctic sea <span class="hlt">ice</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Flocco, Daniela; Feltham, Daniel L.; Bailey, Eleanor; Schroeder, David</p> <p>2015-02-01</p> <p>The presence of melt ponds on the surface of Arctic sea <span class="hlt">ice</span> significantly reduces its albedo, inducing a positive feedback leading to sea <span class="hlt">ice</span> thinning. While the role of melt ponds in enhancing the summer melt of sea <span class="hlt">ice</span> is well known, their impact on suppressing winter freezing of sea <span class="hlt">ice</span> has, hitherto, received less attention. Melt ponds freeze by forming an <span class="hlt">ice</span> lid at the upper surface, which <span class="hlt">insulates</span> them from the atmosphere and traps pond water between the underlying sea <span class="hlt">ice</span> and the <span class="hlt">ice</span> lid. The pond water is a store of latent heat, which is released during refreezing. Until a pond freezes completely, there can be minimal <span class="hlt">ice</span> growth at the base of the underlying sea <span class="hlt">ice</span>. In this work, we present a model of the refreezing of a melt pond that includes the heat and salt balances in the <span class="hlt">ice</span> lid, trapped pond, and underlying sea <span class="hlt">ice</span>. The model uses a two-stream radiation model to account for radiative scattering at phase boundaries. Simulations and related sensitivity studies suggest that trapped pond water may survive for over a month. We focus on the role that pond salinity has on delaying the refreezing process and retarding basal sea <span class="hlt">ice</span> growth. We estimate that for a typical sea <span class="hlt">ice</span> pond coverage in autumn, excluding the impact of trapped ponds in models overestimates <span class="hlt">ice</span> growth by up to 265 million km3, an overestimate of 26%.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011TCD.....5.3627B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011TCD.....5.3627B"><span>Stable isotope and gas properties of two <span class="hlt">ice</span> wedges from Cape Mamontov Klyk, Laptev Sea, Northern Siberia</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Boereboom, T.; Samyn, D.; Meyer, H.; Tison, J.-L.</p> <p>2011-12-01</p> <p>This <span class="hlt">paper</span> presents and discusses the texture, fabric and gas properties (contents of total gas, O2, N2, CO2, and CH4) of two <span class="hlt">ice</span> wedges from Cape Mamontov Klyk, Laptev Sea, Northern Siberia. The two <span class="hlt">ice</span> wedges display contrasting structures: one being of relatively "clean" <span class="hlt">ice</span> and the other showing clean <span class="hlt">ice</span> at its centre as well as debris-rich <span class="hlt">ice</span> on its sides (referred to as <span class="hlt">ice</span>-sand wedge). A comparison of gas properties, crystal size, fabrics and stable isotope data (δ18O and δD) allows discriminating between three different facies of <span class="hlt">ice</span> with specific paleoenvironmental signatures, suggesting different climatic conditions and rates of biological activity. More specifically, total gas content and <span class="hlt">composition</span> reveal variable intensities of meltwater infiltration and show the impact of biological processes with contrasting contributions from anaerobic and aerobic conditions. Stable isotope data are shown to be valid for discussing changes in paleoenvironmental conditions and/or decipher different sources for the snow feeding into the <span class="hlt">ice</span> wedges with time. Our data also give support to the previous assumption that the <span class="hlt">composite</span> <span class="hlt">ice</span> wedge was formed in Pleistocene and the <span class="hlt">ice</span> wedge in Holocene times. This study sheds more light on the conditions of <span class="hlt">ice</span> wedge growth under changing environmental conditions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19840005422','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19840005422"><span>Numerical simulation of two-dimensional heat transfer in <span class="hlt">composite</span> bodies with application to de-<span class="hlt">icing</span> of aircraft components. Ph.D. Thesis. Final Report</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Chao, D. F. K.</p> <p>1983-01-01</p> <p>Transient, numerical simulations of the de-<span class="hlt">icing</span> of <span class="hlt">composite</span> aircraft components by electrothermal heating were performed for a two dimensional rectangular geometry. The implicit Crank-Nicolson formulation was used to insure stability of the finite-difference heat conduction equations and the phase change in the <span class="hlt">ice</span> layer was simulated using the Enthalpy method. The Gauss-Seidel point iterative method was used to solve the system of difference equations. Numerical solutions illustrating de-icer performance for various <span class="hlt">composite</span> aircraft structures and environmental conditions are presented. Comparisons are made with previous studies. The simulation can also be used to solve a variety of other heat conduction problems involving <span class="hlt">composite</span> bodies.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20030015862','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20030015862"><span>Multipurpose Thermal <span class="hlt">Insulation</span> Test Apparatus</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Fesmire, James E. (Inventor); Augustynowicz, Stanislaw D. (Inventor)</p> <p>2002-01-01</p> <p>A multi-purpose thermal <span class="hlt">insulation</span> test apparatus is used for testing <span class="hlt">insulation</span> materials, or other components. The test apparatus is a fluid boil-off calorimeter system for calibrated measurement of the apparent thermal conductivity (k-value) of a specimen material at a fixed vacuum level. The apparatus includes an inner vessel for receiving a fluid with a normal boiling point below ambient temperature, such as liquid nitrogen, enclosed within a vacuum chamber. A cold mass assembly, including the inner vessel and thermal guards, is suspended from the top of the vacuum chamber. Handling tools attach to the cold mass assembly for convenient manipulation of the assembly and for the installation or wrapping of <span class="hlt">insulation</span> test materials. Liquid nitrogen is typically supplied to the inner vessel using a fill tube with funnel. A single port through the top of the vacuum chamber facilitates both filling and venting. Aerogel <span class="hlt">composite</span> stacks with reflective films are fastened to the top and the bottom of the inner vessel as thermal guards. The comparative k-value of the <span class="hlt">insulation</span> material is determined by measuring the boil-off flow rate of gas, the temperature differential across the <span class="hlt">insulation</span> thickness, and the dimensions (length and diameters) of the test specimen.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19850000489&hterms=temperature+resistance&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Dtemperature%2Bresistance','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19850000489&hterms=temperature+resistance&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Dtemperature%2Bresistance"><span><span class="hlt">Insulation</span> Blankets for High-Temperature Use</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Goldstein, H.; Leiser, D.; Sawko, P. M.; Larson, H. K.; Estrella, C.; Smith, M.; Pitoniak, F. J.</p> <p>1986-01-01</p> <p><span class="hlt">Insulating</span> blanket resists temperatures up to 1,500 degrees F (815 degrees C). Useful where high-temperature resistance, flexibility, and ease of installation are important - for example, <span class="hlt">insulation</span> for odd-shaped furnaces and high-temperature ducts, curtains for furnace openings and fire control, and conveyor belts in hot processes. Blanket is quilted <span class="hlt">composite</span> consisting of two face sheets: outer one of silica, inner one of silica or other glass cloth with center filling of pure silica glass felt sewn together with silica glass threads.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20030068097','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20030068097"><span>Quantification of <span class="hlt">Ice</span> Accretions for <span class="hlt">Icing</span> Scaling Evaluations</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Ruff, Gary A.; Anderson, David N.</p> <p>2003-01-01</p> <p>The comparison of <span class="hlt">ice</span> accretion characteristics is an integral part of aircraft <span class="hlt">icing</span> research. It is often necessary to compare an <span class="hlt">ice</span> accretion obtained from a flight test or numerical simulation to one produced in an <span class="hlt">icing</span> wind tunnel or for validation of an <span class="hlt">icing</span> scaling method. Traditionally, this has been accomplished by overlaying two-dimensional tracings of <span class="hlt">ice</span> accretion shapes. This <span class="hlt">paper</span> addresses the basic question of how to compare <span class="hlt">ice</span> accretions using more quantitative methods. For simplicity, geometric characteristics of the <span class="hlt">ice</span> accretions are used for the comparison. One method evaluated is a direct comparison of the percent differences of the geometric measurements. The second method inputs these measurements into a fuzzy inference system to obtain a single measure of the goodness of the comparison. The procedures are demonstrated by comparing <span class="hlt">ice</span> shapes obtained in the <span class="hlt">Icing</span> Research Tunnel at NASA Glenn Research Center during recent <span class="hlt">icing</span> scaling tests. The results demonstrate that this type of analysis is useful in quantifying the similarity of <span class="hlt">ice</span> accretion shapes and that the procedures should be further developed by expanding the analysis to additional <span class="hlt">icing</span> data sets.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018E%26ES..121c2027Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018E%26ES..121c2027Y"><span>Biodegradation performance of environmentally-friendly <span class="hlt">insulating</span> oil</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yang, Jun; He, Yan; Cai, Shengwei; Chen, Cheng; Wen, Gang; Wang, Feipeng; Fan, Fan; Wan, Chunxiang; Wu, Liya; Liu, Ruitong</p> <p>2018-02-01</p> <p>In this <span class="hlt">paper</span>, biodegradation performance of rapeseed <span class="hlt">insulating</span> oil (RDB) and FR3 <span class="hlt">insulating</span> oil (FR3) was studied by means of ready biodegradation method which was performed with Organization for Economic Co-operation and Development (OECD) 301B. For comparison, the biodegradation behaviour of 25# mineral <span class="hlt">insulating</span> oil was also characterized with the same method. The testing results shown that the biodegradation degree of rapeseed <span class="hlt">insulating</span> oil, FR3 <span class="hlt">insulating</span> oil and 25# mineral <span class="hlt">insulating</span> oil was 95.8%, 98.9% and 38.4% respectively. Following the “new chemical risk assessment guidelines” (HJ/T 154 - 2004), which illustrates the methods used to identify and assess the process safety hazards inherent. The guidelines can draw that the two vegetable <span class="hlt">insulating</span> oils, i.e. rapeseed <span class="hlt">insulating</span> oil and FR3 <span class="hlt">insulating</span> oil are easily biodegradable. Therefore, the both can be classified as environmentally-friendly <span class="hlt">insulating</span> oil. As expected, 25# mineral <span class="hlt">insulating</span> oil is hardly biodegradable. The main reason is that 25# mineral <span class="hlt">insulating</span> oil consists of isoalkanes, cyclanes and a few arenes, which has few unsaturated bonds. Biodegradation of rapeseed <span class="hlt">insulating</span> oil and FR3 <span class="hlt">insulating</span> oil also remain some difference. Biodegradation mechanism of vegetable <span class="hlt">insulating</span> oil was revealed from the perspective of hydrolysis kinetics.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19890034403&hterms=1535&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3D1535','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19890034403&hterms=1535&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3D1535"><span>The isotopic <span class="hlt">composition</span> of methane in polar <span class="hlt">ice</span> cores</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Craig, H.; Chou, C. C.; Welhan, J. A.; Stevens, C. M.; Engelkemeir, A.</p> <p>1988-01-01</p> <p>Air bubbles in polar <span class="hlt">ice</span> cores indicate that about 300 years ago the atmospheric mixing ratio of methane began to increase rapidly. Today the mixing ratio is about 1.7 parts per million by volume, and, having doubled once in the past several hundred years, it will double again in the next 60 years if current rates continue. Carbon isotope ratios in methane up to 350 years in age have been measured with as little as 25 kilograms of polar <span class="hlt">ice</span> recovered in 4-meter-long <span class="hlt">ice</span>-core segments. The data show that: (1) in situ microbiology or chemistry has not altered the <span class="hlt">ice</span>-core methane concentrations, and (2) that the carbon-13 to carbon-12 ratio of atmospheric CH4 in <span class="hlt">ice</span> from 100 years and 300 years ago was about 2 per mil lower than at present. Atmospheric methane has a rich spectrum of isotopic sources: the <span class="hlt">ice</span>-core data indicate that anthropogenic burning of the earth's biomass is the principal cause of the recent C-13H4 enrichment, although other factors may also contribute.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24838633','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24838633"><span>Nanostructured graphene <span class="hlt">composite</span> <span class="hlt">papers</span> for highly flexible and foldable supercapacitors.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Liu, Lili; Niu, Zhiqiang; Zhang, Li; Zhou, Weiya; Chen, Xiaodong; Xie, Sishen</p> <p>2014-07-23</p> <p>Reduced graphene oxide (rGO) and polyaniline (PANI) assemble onto the surface of cellulose fibers (CFs) and into the pores of CF <span class="hlt">paper</span>, to form a hierarchical nanostructured PANI-rGO/CF <span class="hlt">composite</span> <span class="hlt">paper</span>. Based on these <span class="hlt">composite</span> <span class="hlt">papers</span>, flexible and foldable all-solid-state supercapacitors are achieved. © 2014 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.P33A2867S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.P33A2867S"><span>Surfaces of Ganymede and Callisto: H2O-<span class="hlt">ice</span> particle sizes and <span class="hlt">composition</span> of non-<span class="hlt">ice</span> materials</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Stephan, K.; Hoffmann, H.; Hibbitts, C.; Wagner, R. J.; Jaumann, R.</p> <p>2017-12-01</p> <p>Band depth ratios (BDRs) of the major H2O-<span class="hlt">ice</span> absorptions in the NIMS spectra of the Galilean satellites Ganymede and Callisto have been found to be mainly unaffected by the abundance of the dark non-<span class="hlt">ice</span> material(s) and can be leveraged to provide semi-quantitative indicators of variations in the H2O-<span class="hlt">ice</span> particle sizes across their surfaces. Interestingly, the derived H2O-<span class="hlt">ice</span> particle sizes vary continuously with geographic latitude on both satellites. H2O-<span class="hlt">ice</span> particles on Callisto appear slightly larger at low and mid latitude than observed on Ganymede, whereas the BDR values converge toward the poles indicating similarly small H2O-<span class="hlt">ice</span> particle sizes for both satellites. This smooth latitudinal trend on both satellites may be related to their surface temperatures and the possible thermal migration of water vapor to higher latitudes and grain welding at lower latitudes. It is not expected that the observed relationship between the BDRs and H2O-<span class="hlt">ice</span> particle sizes occurs for mixtures with every non-<span class="hlt">ice</span> material expected to exist on planetary surfaces. Therefore, <span class="hlt">ice</span> mixtures with a variety of considered non-<span class="hlt">ice</span> materials such as carbon-rich materials, phyllosilicates and salts have been investigated and the validity of this relationship tested depending on different H2O-<span class="hlt">ice</span> abundances and particle sizes. The relationship seems to be valid for most materials if the amount of the non-<span class="hlt">ice</span> material in the mixture does not exceed a few percent or the non-<span class="hlt">ice</span> component is not hydrated, i.e. does not itself possess water-related bands near 1.4 and 1.9 microns. Best results across the nearly full range of percentage could be achieved for carbon-rich material, iron sulfides, and hydroxylated phyllosilicates, which are expected to be the major constituent of carbonaceous chondrites. In contrast, significant amounts of hydrated material, as identified on Europa, significantly changes the BDRs and cannot fully explain the global trend.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017E3SWC..1901044T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017E3SWC..1901044T"><span>Comparative analysis of cellulose pressboard and aramid <span class="hlt">paper</span> used in air <span class="hlt">insulation</span> systems of high-voltage devices</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Turba, Tomasz; Frącz, Paweł</p> <p>2017-10-01</p> <p>The <span class="hlt">paper</span> presents results of a comparative analysis of parameters of two kinds of solid dielectrics used in air <span class="hlt">insulation</span> systems to prevent occurring partial discharges. The research works regarded materials made of: cellulose pressboard and aramid <span class="hlt">paper</span>. All measurements were performed under laboratory conditions by changing the value of partial discharges generation voltage until breakdown occurred in the inhomogeneous environment that was simulated using needle-plate (made of copper) electrode system. The main contribution which resulted from studies is a statement that potential use of aramid <span class="hlt">paper</span> as a dielectric can extend the life of a high voltage electric device as compared to standard cellulose pressboard usage due to higher electric resistances to breakdown or detection of corona voltage. Results shown that the aramid <span class="hlt">paper</span> has greater electric resistance to breakdown in comparison to cellulose with no difference between both on detecting corona of partial discharge.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1992STIN...9316605B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1992STIN...9316605B"><span>ASRM case <span class="hlt">insulation</span> design and development</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bell, Matthew S.; Tam, William F. S.</p> <p>1992-10-01</p> <p>This <span class="hlt">paper</span> describes the achievements made on the Advanced Solid Rocket Motor (ASRM) case <span class="hlt">insulation</span> design and development program. The ASRM case <span class="hlt">insulation</span> system described herein protects the metal case and joints from direct radiation and hot gas impingement. Critical failure of solid rocket systems is often traceable to failure of the <span class="hlt">insulation</span> design. The wide ranging accomplishments included the development of a nonasbestos <span class="hlt">insulation</span> material for ASRM that replaced the existing Redesigned Solid Rocket Motor (RSRM) asbestos-filled nitrile butadiene rubber (NBR) along with a performance gain of 300 pounds, and improved reliability of all the <span class="hlt">insulation</span> joint designs, i.e., segmented case joint, case-to-nozzle and case-to-igniter joint. The <span class="hlt">insulation</span> process development program included the internal stripwinding process. This process advancement allowed Aerojet to match to exceed the capability of other propulsion companies.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19930007416','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19930007416"><span>ASRM case <span class="hlt">insulation</span> design and development</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Bell, Matthew S.; Tam, William F. S.</p> <p>1992-01-01</p> <p>This <span class="hlt">paper</span> describes the achievements made on the Advanced Solid Rocket Motor (ASRM) case <span class="hlt">insulation</span> design and development program. The ASRM case <span class="hlt">insulation</span> system described herein protects the metal case and joints from direct radiation and hot gas impingement. Critical failure of solid rocket systems is often traceable to failure of the <span class="hlt">insulation</span> design. The wide ranging accomplishments included the development of a nonasbestos <span class="hlt">insulation</span> material for ASRM that replaced the existing Redesigned Solid Rocket Motor (RSRM) asbestos-filled nitrile butadiene rubber (NBR) along with a performance gain of 300 pounds, and improved reliability of all the <span class="hlt">insulation</span> joint designs, i.e., segmented case joint, case-to-nozzle and case-to-igniter joint. The <span class="hlt">insulation</span> process development program included the internal stripwinding process. This process advancement allowed Aerojet to match to exceed the capability of other propulsion companies.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017MS%26E..245b2089B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017MS%26E..245b2089B"><span>Effect of Autoclaved Aerated Concrete Modification with High-Impact Polystyrene on Sound <span class="hlt">Insulation</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Brelak, Sylwia; Dachowski, Ryszard</p> <p>2017-10-01</p> <p>Autoclaved aerated concrete is one of the most commonly used building materials. Its advantages include low density, high thermal <span class="hlt">insulation</span> capacity and high fire resistance. It has a relatively high compressive strength, though not high enough to be able to compete with other building materials in this respect. One of the directions leading to the improvement of physical and mechanical properties of autoclaved aerated concrete is the modification of its <span class="hlt">composition</span>. A noticeable effect of pulverized high-impact polystyrene (improved compressive strength and water absorption) was relevant for the decision to continue the study of its effects. This <span class="hlt">paper</span> discusses the effect of high-impact polystyrene on sound <span class="hlt">insulation</span> in AAC products. The tests demonstrated a positive influence of the modifier on AAC sound <span class="hlt">insulation</span> enhancement. Results from the tests performed on HIPS-modified AAC products were showed and compared with the properties of conventional products. The effect of the polymer on the microstructure of the products obtained was described briefly.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20130012683','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20130012683"><span>Sprayable Aerogel Bead <span class="hlt">Compositions</span> With High Shear Flow Resistance and High Thermal <span class="hlt">Insulation</span> Value</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Ou, Danny; Trifu, Roxana; Caggiano, Gregory</p> <p>2013-01-01</p> <p>A sprayable aerogel <span class="hlt">insulation</span> has been developed that has good mechanical integrity and lower thermal conductivity than incumbent polyurethane spray-on foam <span class="hlt">insulation</span>, at similar or lower areal densities, to prevent <span class="hlt">insulation</span> cracking and debonding in an effort to eliminate the generation of inflight debris. This new, lightweight aerogel under bead form can be used as <span class="hlt">insulation</span> in various thermal management systems that require low mass and volume, such as cryogenic storage tanks, pipelines, space platforms, and launch vehicles.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..16.3801S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..16.3801S"><span>In-situ single particle <span class="hlt">composition</span> analysis of free tropospheric <span class="hlt">ice</span> nuclei and <span class="hlt">ice</span> residues in mixed-phase clouds during INUIT-JFJ 2013</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schmidt, Susan; Schneider, Johannes; Thomas, Klimach; Stephan, Mertes; Ludwig, Schenk; Udo, Kästner; Frank, Stratmann; Joachim, Curtius; Piotr, Kupiszewski; Ernest, Weingartner; Emanuel, Hammer; Paul, Vochezer; Martin, Schnaiter; Stephan, Borrmann</p> <p>2014-05-01</p> <p>In the framework of the DFG (deutsche Forschungsgemeinschaft)-funded research unit INUIT (<span class="hlt">Ice</span> Nuclei research UnIT) a field campaign at the High Alpine Research Station Jungfraujoch (JFJ, Swiss Alps, Sphinx Laboratory, 3580 m asl; 7°59'2''E, 46°32'53''N) took place in January/February 2013 (INUIT-JFJ 2013). The goal of the measurements was to investigate the chemical <span class="hlt">composition</span> of <span class="hlt">ice</span> particle residues (IPR) in ambient air as well as the background aerosol particles. Previous investigations conducted at the JFJ showed that particles consisting of mineral components dominate the <span class="hlt">ice</span> particle residue number (Kamphus et al., 2008) but also particles consisting of black carbon were found to be enriched in IPR (Mertes et al., 2007; Cozic et al., 2008). Cziczo et al. find out that lead as well is a good <span class="hlt">ice</span> nucleus and was measured in IPR at previous measurements at the JFJ. During INUIT-JFJ 2013, the IPR were sampled out of mixed-phase clouds by an <span class="hlt">Ice</span>-CVI (<span class="hlt">Ice</span> Counterflow Virtual Impactor, Mertes et al., 2007) and an ISI (<span class="hlt">Ice</span> Selective Inlet, Kupiszewski et al., 2013) and analyzed by the single particle mass spectrometer ALABAMA (Aircraft-based Laser Ablation Aerosol Mass Spectrometer; Brands et al., 2011). Additionally, the ALABAMA was connected to a total aerosol-inlet to investigate the chemical <span class="hlt">composition</span> of background aerosol particles. During 217 hours of background aerosol measurements we analyzed more than 27000 aerosol particles, which consisted mainly of pure organic components or organics mixed with ammonium, metals or mineral components. During six cloud events with approximately 63 h measurement time we detected 162 IPR sampled by the <span class="hlt">Ice</span>-CVI. The main part of these IPR were also composed of organic material mixed with other chemical compounds. Additionally, we found particles which consisted of mineral components (approximately 23 %). Sampling mixed-phase cloud through the ISI we measured during four cloud events 34 <span class="hlt">ice</span> residues in approximately 30 h</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..16.1690J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..16.1690J"><span>Antarctic Climate Variability: Covariance of Ozone and Sea <span class="hlt">Ice</span> in Atmosphere - Ocean Coupled Model Simulations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jrrar, Amna; Abraham, N. Luke; Pyle, John A.; Holland, David</p> <p>2014-05-01</p> <p>Changes in sea <span class="hlt">ice</span> significantly modulate climate change because of its high reflective and <span class="hlt">insulating</span> nature. While Arctic Sea <span class="hlt">Ice</span> Extent (SIE) shows a negative trend. Antarctic SIE shows a weak but positive trend, estimated at 0.127 x 106 km2 per decade. The trend results from large regional cancellations, more <span class="hlt">ice</span> in the Weddell and the Ross seas, and less <span class="hlt">ice</span> in the Amundsen - Bellingshausen seas. A number of studies had demonstrated that stratospheric ozone depletion has had a major impact on the atmospheric circulation, causing a positive trend in the Southern Annular Mode (SAM), which has been linked to the observed positive trend in autumn sea <span class="hlt">ice</span> in the Ross Sea. However, other modelling studies show that models forced with prescribed ozone hole simulate decreased sea <span class="hlt">ice</span> in all regions comparative to a control run. A recent study has also shown that stratospheric ozone recovery will mitigate Antarctic sea <span class="hlt">ice</span> loss. To verify this assumed relationship, it is important first to investigate the covariance between ozone's natural (dynamical) variability and Antarctic sea <span class="hlt">ice</span> distribution in pre-industrial climate, to estimate the trend due to natural variability. We investigate the relationship between anomalous Antarctic ozone years and the subsequent changes in Antarctic sea <span class="hlt">ice</span> distribution in a multidecadal control simulation using the AO-UMUKCA model. The model has a horizontal resolution of 3.75 X 2.5 degrees in longitude and latitude; and 60 hybrid height levels in the vertical, from the surface up to a height of 84 km. The ocean component is the NEMO ocean model on the ORCA2 tripolar grid, and the sea <span class="hlt">ice</span> model is CICE. We evaluate the model's performance in terms of sea <span class="hlt">ice</span> distribution, and we calculate sea <span class="hlt">ice</span> extent trends for <span class="hlt">composites</span> of anomalously low versus anomalously high SH polar ozone column. We apply EOF analysis to the seasonal anomalies of sea <span class="hlt">ice</span> concentration, MSLP, and Z 500, and identify the leading climate modes controlling the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1372443-skyrme-insulators-insulators-brink-superconductivity','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1372443-skyrme-insulators-insulators-brink-superconductivity"><span>Skyrme <span class="hlt">insulators</span>: <span class="hlt">insulators</span> at the brink of superconductivity</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Ertem, Onur; Chang, Po -Yao; Coleman, Piers; ...</p> <p>2017-08-04</p> <p>Current theories of superfluidity are based on the idea of a coherent quantum state with topologically protected, quantized circulation. When this topological protection is absent, as in the case of 3He-A, the coherent quantum state no longer supports persistent superflow. In this <span class="hlt">paper</span>, we argue that the loss of topological protection in a superconductor gives rise to an <span class="hlt">insulating</span> ground state. Specifically, we introduce the concept of a Skyrme <span class="hlt">insulator</span> to describe the coherent dielectric state that results from the topological failure of superflow carried by a complex vector order parameter. Here, we apply this idea to the case ofmore » SmB6, arguing that the observation of a diamagnetic Fermi surface within an <span class="hlt">insulating</span> bulk can be understood as a realization of this state. Our theory enables us to understand the linear specific heat of SmB6 in terms of a neutral Majorana Fermi sea and leads us to predict that in low fields of order a Gauss, SmB6 will develop a Meissner effect.« less</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li class="active"><span>10</span></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_10 --> <div id="page_11" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li class="active"><span>11</span></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="201"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20060047484&hterms=vacuum+insulation&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3Dvacuum%2Binsulation','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20060047484&hterms=vacuum+insulation&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3Dvacuum%2Binsulation"><span>Structural Continuum Modeling of Space Shuttle External Tank Foam <span class="hlt">Insulation</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Steeve, Brian; Ayala, Sam; Purlee, T. Eric; Shaw, Phillip</p> <p>2006-01-01</p> <p>The Space Shuttle External Tank is covered with rigid polymeric closed-cell foam <span class="hlt">insulation</span> to prevent <span class="hlt">ice</span> formation, protect the metallic tank from aerodynamic heating, and control the breakup of the tank during re-entry. The cryogenic state of the tank, as well as the ascent into a vacuum environment, places this foam under significant stress. Because the loss of the foam during ascent poses a critical risk to the shuttle orbiter, there is much interest in understanding the stress state in the foam <span class="hlt">insulation</span> and how it may contribute to fracture and debris loss. Several foam applications on the external tank have been analyzed using finite element methods. This presentation describes the approach used to model the foam material behavior and compares analytical results to experiments.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015IJNLM..75...77L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015IJNLM..75...77L"><span>Theory of <span class="hlt">ice</span>-skating</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Le Berre, Martine; Pomeau, Yves</p> <p>2015-10-01</p> <p>Almost frictionless skating on <span class="hlt">ice</span> relies on a thin layer of melted water <span class="hlt">insulating</span> mechanically the blade of the skate from <span class="hlt">ice</span>. Using the basic equations of fluid mechanics and Stefan law, we derive a set of two coupled equations for the thickness of the film and the length of contact, a length scale which cannot be taken as its value at rest. The analytical study of these equations allows to define a small a-dimensional parameter depending on the longitudinal coordinate which can be neglected everywhere except close to the contact points at the front and the end of the blade, where a boundary layer solution is given. This solution provides without any calculation the order of magnitude of the film thickness, and its dependence with respect to external parameters like the velocity and mass of the skater and the radius of profile and bite angle of the blade, in good agreement with the numerical study. Moreover this solution also shows that a lubricating water layer of macroscopic thickness always exists for standard values of <span class="hlt">ice</span> skating data, contrary to what happens in the case of cavitation of droplets due to thermal heating (Leidenfrost effect).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014cosp...40E1038G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014cosp...40E1038G"><span>Cosmic Ray Studies with <span class="hlt">Ice</span>Cube</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gonzalez, Javier</p> <p></p> <p>In this contribution we will give an overview of the cosmic ray studies conducted within the <span class="hlt">Ice</span>Cube collaboration. The <span class="hlt">Ice</span>Cube detector in the geographical south pole can be used to measure various characteristics of the extensive air showers induced by high energy cosmic rays. With <span class="hlt">Ice</span>Top, the surface component of the detector, we detect the electromagnetic and muon components of the air showers, while with the deep detector we detect the high energy muons. We have measured the energy spectrum of cosmic ray primaries in the range between 1.58PeV and 1.26 EeV. A combined analysis of the high energy muon bundles in the <span class="hlt">ice</span> and the air shower footprint in <span class="hlt">Ice</span>Top provides a measure of primary <span class="hlt">composition</span>. We will also discuss how the sensitivity to low energy muons in the air showers has the potential to produce additional measures of primary <span class="hlt">composition</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C33C1211G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C33C1211G"><span>Is snow-<span class="hlt">ice</span> now a major contributor to sea <span class="hlt">ice</span> mass balance in the western Transpolar Drift region?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Graham, R. M.; Merkouriadi, I.; Cheng, B.; Rösel, A.; Granskog, M. A.</p> <p>2017-12-01</p> <p>During the Norwegian young sea <span class="hlt">ICE</span> (N-<span class="hlt">ICE</span>2015) campaign, which took place in the first half of 2015 north of Svalbard, a deep winter snow pack (50 cm) on sea <span class="hlt">ice</span> was observed, that was 50% thicker than earlier climatological studies suggested for this region. Moreover, a significant fraction of snow contributed to the total <span class="hlt">ice</span> mass in second-year <span class="hlt">ice</span> (SYI) (9% on average). Interestingly, very little snow (3% snow by mass) was present in first-year <span class="hlt">ice</span> (FYI). The combination of sea <span class="hlt">ice</span> thinning and increased precipitation north of Svalbard is expected to promote the formation of snow-<span class="hlt">ice</span>. Here we use the 1-D snow/<span class="hlt">ice</span> thermodynamic model HIGHTSI forced with reanalysis data, to show that for the case study of N-<span class="hlt">ICE</span>2015, snow-<span class="hlt">ice</span> would even form over SYI with an initial thickness of 2 m. In current conditions north of Svalbard, snow-<span class="hlt">ice</span> is ubiquitous and contributes to the thickness growth up to 30%. This contribution is important, especially in the absence of any bottom thermodynamic growth due to the thick <span class="hlt">insulating</span> snow cover. Growth of FYI north of Svalbard is mainly controlled by the timing of growth onset relative to snow precipitation events and cold spells. These usually short-lived conditions are largely determined by the frequency of storms entering the Arctic from the Atlantic Ocean. In our case, a later freeze onset was favorable for FYI growth due to less snow accumulation in early autumn. This limited snow-<span class="hlt">ice</span> formation but promoted bottom thermodynamic growth. We surmise these findings are related to a regional phenomenon in the Atlantic sector of the Arctic, with frequent storm events which bring increasing amounts of precipitation in autumn and winter, and also affect the duration of cold temperatures required for <span class="hlt">ice</span> growth in winter. We discuss the implications for the importance of snow-<span class="hlt">ice</span> in the future Arctic, formerly believed to be non-existent in the central Arctic due to thick perennial <span class="hlt">ice</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20160013723','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20160013723"><span>A Synthesis of the Basal Thermal State of the Greenland <span class="hlt">Ice</span> Sheet</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Macgregor, J. A.; Fahnestock, M. A.; Catania, G. A.; Aschwanden, A.; Clow, G. D.; Colgan, W. T.; Gogineni, S. P.; Morlighem, M.; Nowicki, S. M. J.; Paden, J. D.; <a style="text-decoration: none; " href="javascript:void(0); " onClick="displayelement('author_20160013723'); toggleEditAbsImage('author_20160013723_show'); toggleEditAbsImage('author_20160013723_hide'); "> <img style="display:inline; width:12px; height:12px; " src="images/arrow-up.gif" width="12" height="12" border="0" alt="hide" id="author_20160013723_show"> <img style="width:12px; height:12px; display:none; " src="images/arrow-down.gif" width="12" height="12" border="0" alt="hide" id="author_20160013723_hide"></p> <p>2016-01-01</p> <p>Greenland's thick <span class="hlt">ice</span> sheet <span class="hlt">insulates</span> the bedrock below from the cold temperatures at the surface, so the bottom of the <span class="hlt">ice</span> is often tens of degrees warmer than at the top, because the <span class="hlt">ice</span> bottom is slowly warmed by heat coming from the Earth's depths. Knowing whether Greenland's <span class="hlt">ice</span> lies on wet, slippery ground or is anchored to dry, frozen bedrock is essential for predicting how this <span class="hlt">ice</span> will flow in the future. But scientists have very few direct observations of the thermal conditions beneath the <span class="hlt">ice</span> sheet, obtained through fewer than two dozen boreholes that have reached the bottom. Our study synthesizes several independent methods to infer the Greenland <span class="hlt">Ice</span> Sheet's basal thermal state -whether the bottom of the <span class="hlt">ice</span> is melted or not-leading to the first map that identifies frozen and thawed areas across the whole <span class="hlt">ice</span> sheet. This map will guide targets for future investigations of the Greenland <span class="hlt">Ice</span> Sheet toward the most vulnerable and poorly understood regions, ultimately improving our understanding of its dynamics and contribution to future sea-level rise. It is of particular relevance to ongoing Operation <span class="hlt">Ice</span>Bridge activities and future large-scale airborne missions over Greenland.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22494862-insulator-charging-limits-direct-current-across-tunneling-metal-insulator-semiconductor-junctions','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22494862-insulator-charging-limits-direct-current-across-tunneling-metal-insulator-semiconductor-junctions"><span><span class="hlt">Insulator</span> charging limits direct current across tunneling metal-<span class="hlt">insulator</span>-semiconductor junctions</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Vilan, Ayelet</p> <p></p> <p>Molecular electronics studies how the molecular nature affects the probability of charge carriers to tunnel through the molecules. Nevertheless, transport is also critically affected by the contacts to the molecules, an aspect that is often overlooked. Specifically, the limited ability of non-metallic contacts to maintain the required charge balance across the fairly <span class="hlt">insulating</span> molecule often have dramatic effects. This <span class="hlt">paper</span> shows that in the case of lead/organic monolayer-silicon junctions, a charge balance is responsible for an unusual current scaling, with the junction diameter (perimeter), rather than its area. This is attributed to the balance between the 2D charging at themore » metal/<span class="hlt">insulator</span> interface and the 3D charging of the semiconductor space-charge region. A derivative method is developed to quantify transport across tunneling metal-<span class="hlt">insulator</span>-semiconductor junctions; this enables separating the tunneling barrier from the space-charge barrier for a given current-voltage curve, without complementary measurements. The <span class="hlt">paper</span> provides practical tools to analyze specific molecular junctions compatible with existing silicon technology, and demonstrates the importance of contacts' physics in modeling charge transport across molecular junctions.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ApPhA.124..142F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ApPhA.124..142F"><span>Anti-<span class="hlt">icing</span>/frosting and self-cleaning performance of superhydrophobic aluminum alloys</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Feng, Libang; Yan, Zhongna; Shi, Xueting; Sultonzoda, Firdavs</p> <p>2018-02-01</p> <p><span class="hlt">Ice</span> formation and frost deposition on cryogenic equipment and systems can result in serious problems and huge economic loss. Hence, it is quite necessary to develop new materials to prevent <span class="hlt">icing</span> and frosting on cold surfaces in engineering fields. Here, a superhydrophobic aluminum alloy with enhanced anti-frosting, anti-<span class="hlt">icing</span>, and self-cleaning performance has been developed by a facile one-step method. The anti-frosting/<span class="hlt">icing</span> performance of superhydrophobic aluminum alloys is confirmed by frosting/<span class="hlt">icing</span> time delay, consolidating and freezing temperature reduction, and lower amount of frost/<span class="hlt">ice</span> adhesion. Meanwhile, the excellent self-cleaning performance is authenticated by the fact that simulated pollution particles can be cleaned out by rolling water droplets completely. Finally, based on the classical nucleation theory, anti-<span class="hlt">icing</span> and anti-frosting mechanisms of the superhydrophobic aluminum alloys are deduced. Results show that grounded on "air cushion" and "heat <span class="hlt">insulation</span>" effect, a larger nucleation barrier and a lower crystal growth rate can be observed, which, hence, inhibit <span class="hlt">ice</span> formation and frost deposition. It can be concluded that preparing superhydrophobic surfaces would be an effective strategy for improving anti-<span class="hlt">icing</span>, anti-frosting, and self-cleaning performance of aluminum alloys.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22311104-estimation-dc-transport-dynamics-strongly-correlated-la-pr-ca-mno-sub-film-using-insulator-metal-composite-model-terahertz-conductivity','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22311104-estimation-dc-transport-dynamics-strongly-correlated-la-pr-ca-mno-sub-film-using-insulator-metal-composite-model-terahertz-conductivity"><span>Estimation of dc transport dynamics in strongly correlated (La,Pr,Ca)MnO{sub 3} film using an <span class="hlt">insulator</span>-metal <span class="hlt">composite</span> model for terahertz conductivity</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Nguyen, T. V. A.; Graduate School of Engineering Science, Osaka University, 1-3 Machikaneyama, Toyonaka, Osaka 560-8531; Hattori, A. N.</p> <p>2014-07-14</p> <p>Temperature-dependent conductivities at dc and terahertz (THz) frequency region (σ{sub THz}(ω,T)) were obtained for a strongly correlated (La{sub 0.275}Pr{sub 0.35}Ca{sub 0.375})MnO{sub 3} (LPCMO) film using THz time domain spectroscopy. A <span class="hlt">composite</span> model that describes σ{sub THz}(ω,T) for LPCMO through the <span class="hlt">insulator</span>-metal transition (IMT) was established by incorporating Austin-Mott model characterizing the hopping of localized electrons and Drude model explaining the behavior of free electrons. This model enables us to reliably investigate the dc transport dynamics from THz conductivity measurement, i.e., simultaneously evaluate the dc conductivity and the competing <span class="hlt">composition</span> of metal and <span class="hlt">insulator</span> phases through the IMT, reflecting the changesmore » in microscopic conductivity of these phases.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015GeoRL..42.5442L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015GeoRL..42.5442L"><span>Observed platelet <span class="hlt">ice</span> distributions in Antarctic sea <span class="hlt">ice</span>: An index for ocean-<span class="hlt">ice</span> shelf heat flux</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Langhorne, P. J.; Hughes, K. G.; Gough, A. J.; Smith, I. J.; Williams, M. J. M.; Robinson, N. J.; Stevens, C. L.; Rack, W.; Price, D.; Leonard, G. H.; Mahoney, A. R.; Haas, C.; Haskell, T. G.</p> <p>2015-07-01</p> <p>Antarctic sea <span class="hlt">ice</span> that has been affected by supercooled <span class="hlt">Ice</span> Shelf Water (ISW) has a unique crystallographic structure and is called platelet <span class="hlt">ice</span>. In this <span class="hlt">paper</span> we synthesize platelet <span class="hlt">ice</span> observations to construct a continent-wide map of the winter presence of ISW at the ocean surface. The observations demonstrate that, in some regions of coastal Antarctica, supercooled ISW drives a negative oceanic heat flux of -30 Wm-2 that persists for several months during winter, significantly affecting sea <span class="hlt">ice</span> thickness. In other regions, particularly where the thinning of <span class="hlt">ice</span> shelves is believed to be greatest, platelet <span class="hlt">ice</span> is not observed. Our new data set includes the longest <span class="hlt">ice</span>-ocean record for Antarctica, which dates back to 1902 near the McMurdo <span class="hlt">Ice</span> Shelf. These historical data indicate that, over the past 100 years, any change in the volume of very cold surface outflow from this <span class="hlt">ice</span> shelf is less than the uncertainties in the measurements.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140011454','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140011454"><span>Hydrogen-Bonding Surfaces for <span class="hlt">Ice</span> Mitigation</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Smith, Joseph G., Jr.; Wohl, Christopher J.; Kreeger, Richard E.; Hadley, Kevin R.; McDougall, Nicholas</p> <p>2014-01-01</p> <p><span class="hlt">Ice</span> formation on aircraft, either on the ground or in-flight, is a major safety issue. While ground <span class="hlt">icing</span> events occur predominantly during the winter months, in-flight <span class="hlt">icing</span> can happen anytime during the year. The latter is more problematic since it could result in increased drag and loss of lift. Under a Phase I ARMD NARI Seedling Activity, coated aluminum surfaces possessing hydrogen-bonding groups were under investigation for mitigating <span class="hlt">ice</span> formation. Hydroxyl and methyl terminated dimethylethoxysilanes were prepared via known chemistries and characterized by spectroscopic methods. These materials were subsequently used to coat aluminum surfaces. Surface <span class="hlt">compositions</span> were based on pure hydroxyl and methyl terminated species as well as mixtures of the two. Coated surfaces were characterized by contact angle goniometry. Receding water contact angle data suggested several potential surfaces that may exhibit reduced <span class="hlt">ice</span> adhesion. Qualitative <span class="hlt">icing</span> experiments performed under representative environmental temperatures using supercooled distilled water delivered via spray coating were inconclusive. Molecular modeling studies suggested that chain mobility affected the interface between <span class="hlt">ice</span> and the surface more than terminal group chemical <span class="hlt">composition</span>. Chain mobility resulted from the creation of "pockets" of increased free volume for longer chains to occupy.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20080004577','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20080004577"><span>Environmentally friendly anti-<span class="hlt">icing</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Zuk, John (Inventor); Haslim, Leonard A. (Inventor); Lockyer, Robert T. (Inventor)</p> <p>1998-01-01</p> <p>The present invention describes an aqueous, non-electrolytic, non-toxic, biodegradable, continuous single phase liquid anti-<span class="hlt">icing</span> or deicing <span class="hlt">composition</span> for use on the surfaces of, for example, aircraft, airport pavements, roadways, walkways, bridges, entrances, structures, canals, locks, components, vessels, nautical components, railroad switches, and motor vehicles. The anti-<span class="hlt">icing</span> or deicing <span class="hlt">composition</span> comprises: (a) water; (b) a non-toxic freezing point depressant selected from the group consisting of monohydric alcohols having from 2 to 6 carbon atoms, polyhydric alcohols having from 3 to 12 carbon atoms, monomethyl or ethyl ethers of polyhydric alcohols having from 3 to 12 atoms or mixtures thereof, wherein the freezing point depressant present is between about 14 to 60 percent by weight; (c) a thickener which is present in between about 0.01 and 10 percent by weight; and (d) optionally a corrosion inhibitor which is present in between about 0.01 and 0.1 percent by weight of the total <span class="hlt">composition</span>. In one embodiment, the deicing <span class="hlt">composition</span> further includes (e) a monohydric primary aliphatic unbranched alcohol as a means of forming a thin layer of the <span class="hlt">composition</span> on the surface of the structure to be given <span class="hlt">ice</span> protection, and/or as means of forming a homogenized foam with xanthan thickener; which alcohol is selected from the group consisting of alcohols having between 8 to 24 carbon atoms, preferably, 1-dodecanol. <span class="hlt">Compositions</span> of water, propylene glycol, and/or propanol and xanthan are preferred.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19870013913','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19870013913"><span>Mechanical and thermal properties of planetologically important <span class="hlt">ices</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Croft, Steven K.</p> <p>1987-01-01</p> <p>Two squences of <span class="hlt">ice</span> <span class="hlt">composition</span> were proposed for the icy satellites: a dense nebula model and a solar nebula model. Careful modeling of the structure, <span class="hlt">composition</span>, and thermal history of satellites composed of these various <span class="hlt">ices</span> requires quantitative information on the density, compressibility, thermal expansion, heat capacity, and thermal conductivity. Equations of state were fitted to the density data of the molecular <span class="hlt">ices</span>. The unusual thermal and mechanical properties of the molecular and binary <span class="hlt">ices</span> suggest a larger range of phenomena than previously anticipated, sufficiently complex perhaps to account for many of the unusual geologic phenomena found on the icy satellites.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4066517','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4066517"><span>Antarctic sea <span class="hlt">ice</span> control on ocean circulation in present and glacial climates</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Ferrari, Raffaele; Jansen, Malte F.; Adkins, Jess F.; Burke, Andrea; Stewart, Andrew L.; Thompson, Andrew F.</p> <p>2014-01-01</p> <p>In the modern climate, the ocean below 2 km is mainly filled by waters sinking into the abyss around Antarctica and in the North Atlantic. Paleoproxies indicate that waters of North Atlantic origin were instead absent below 2 km at the Last Glacial Maximum, resulting in an expansion of the volume occupied by Antarctic origin waters. In this study we show that this rearrangement of deep water masses is dynamically linked to the expansion of summer sea <span class="hlt">ice</span> around Antarctica. A simple theory further suggests that these deep waters only came to the surface under sea <span class="hlt">ice</span>, which <span class="hlt">insulated</span> them from atmospheric forcing, and were weakly mixed with overlying waters, thus being able to store carbon for long times. This unappreciated link between the expansion of sea <span class="hlt">ice</span> and the appearance of a voluminous and <span class="hlt">insulated</span> water mass may help quantify the ocean’s role in regulating atmospheric carbon dioxide on glacial–interglacial timescales. Previous studies pointed to many independent changes in ocean physics to account for the observed swings in atmospheric carbon dioxide. Here it is shown that many of these changes are dynamically linked and therefore must co-occur. PMID:24889624</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24889624','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24889624"><span>Antarctic sea <span class="hlt">ice</span> control on ocean circulation in present and glacial climates.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Ferrari, Raffaele; Jansen, Malte F; Adkins, Jess F; Burke, Andrea; Stewart, Andrew L; Thompson, Andrew F</p> <p>2014-06-17</p> <p>In the modern climate, the ocean below 2 km is mainly filled by waters sinking into the abyss around Antarctica and in the North Atlantic. Paleoproxies indicate that waters of North Atlantic origin were instead absent below 2 km at the Last Glacial Maximum, resulting in an expansion of the volume occupied by Antarctic origin waters. In this study we show that this rearrangement of deep water masses is dynamically linked to the expansion of summer sea <span class="hlt">ice</span> around Antarctica. A simple theory further suggests that these deep waters only came to the surface under sea <span class="hlt">ice</span>, which <span class="hlt">insulated</span> them from atmospheric forcing, and were weakly mixed with overlying waters, thus being able to store carbon for long times. This unappreciated link between the expansion of sea <span class="hlt">ice</span> and the appearance of a voluminous and <span class="hlt">insulated</span> water mass may help quantify the ocean's role in regulating atmospheric carbon dioxide on glacial-interglacial timescales. Previous studies pointed to many independent changes in ocean physics to account for the observed swings in atmospheric carbon dioxide. Here it is shown that many of these changes are dynamically linked and therefore must co-occur.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20130012573','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20130012573"><span>Thermal Performance Testing of Cryogenic <span class="hlt">Insulation</span> Systems</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Fesmire, James E.; Augustynowicz, Stan D.; Scholtens, Brekke E.</p> <p>2007-01-01</p> <p>Efficient methods for characterizing thermal performance of materials under cryogenic and vacuum conditions have been developed. These methods provide thermal conductivity data on materials under actual-use conditions and are complementary to established methods. The actual-use environment of full temperature difference in combination with vacuum-pressure is essential for understanding <span class="hlt">insulation</span> system performance. Test articles include solids, foams, powders, layered blankets, <span class="hlt">composite</span> panels, and other materials. Test methodology and apparatus design for several <span class="hlt">insulation</span> test cryostats are discussed. The measurement principle is liquid nitrogen boil-off calorimetry. Heat flux capability ranges from approximately 0.5 to 500 watts per square meter; corresponding apparent thermal conductivity values range from below 0.01 up to about 60 mW/m- K. Example data for different <span class="hlt">insulation</span> materials are also presented. Upon further standardization work, these patented <span class="hlt">insulation</span> test cryostats can be available to industry for a wide range of practical applications.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20110023761','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20110023761"><span>An Overview of NASA Engine <span class="hlt">Ice</span>-Crystal <span class="hlt">Icing</span> Research</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Addy, Harold E., Jr.; Veres, Joseph P.</p> <p>2011-01-01</p> <p><span class="hlt">Ice</span> accretions that have formed inside gas turbine engines as a result of flight in clouds of high concentrations of <span class="hlt">ice</span> crystals in the atmosphere have recently been identified as an aviation safety hazard. NASA s Aviation Safety Program (AvSP) has made plans to conduct research in this area to address the hazard. This <span class="hlt">paper</span> gives an overview of NASA s engine <span class="hlt">ice</span>-crystal <span class="hlt">icing</span> research project plans. Included are the rationale, approach, and details of various aspects of NASA s research.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1079099','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1079099"><span>Project Overcoat - An Exploration of Exterior <span class="hlt">Insulation</span> Strategies for 1-1/2-Story Roof Applications in Cold Climates</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Ojczyk, Cindy; Mosiman, Garrett; Huelman, Pat</p> <p></p> <p>The development of an alternative method to interior-applied <span class="hlt">insulation</span> strategies or exterior applied 'band-aids' such as heat tapes and <span class="hlt">ice</span> belts may help reduce energy needs of millions of 1-1/2 story homes while reducing the risk of <span class="hlt">ice</span> dam formation. A potential strategy for energy improvement of the roof is borrowed from new construction best practices: Here an 'overcoat' of a continuous air, moisture, and thermal barrier is applied on the outside of the roof structure for improved overall performance. The continuous <span class="hlt">insulation</span> of this approach facilitates a reduction in thermal bridging which could further reduce energy consumption and bringmore » existing homes closer to meeting the Building America goals for energy reduction. Research favors an exterior approach to deep energy retrofits and <span class="hlt">ice</span> dam prevention in existing homes. The greatest amount of research focuses on whole house deep energy retrofits leaving a void in roof-only applications. The research is also void of data supporting the hygrothermal performance, durability, constructability, and cost of roof-only exterior overcoat strategies. Yet, contractors interviewed for this report indicate an understanding that exterior approaches are most promising for mitigating <span class="hlt">ice</span> dams and energy loss and are able to sell these strategies to homeowners.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20130012675','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20130012675"><span>Polymer-Reinforced, Non-Brittle, Lightweight Cryogenic <span class="hlt">Insulation</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Hess, David M.</p> <p>2013-01-01</p> <p>The primary application for cryogenic <span class="hlt">insulating</span> foams will be fuel tank applications for fueling systems. It is crucial for this <span class="hlt">insulation</span> to be incorporated into systems that survive vacuum and terrestrial environments. It is hypothesized that by forming an open-cell silica-reinforced polymer structure, the foam structures will exhibit the necessary strength to maintain shape. This will, in turn, maintain the <span class="hlt">insulating</span> capabilities of the foam <span class="hlt">insulation</span>. Besides mechanical stability in the form of crush resistance, it is important for these <span class="hlt">insulating</span> materials to exhibit water penetration resistance. Hydrocarbon-terminated foam surfaces were implemented to impart hydrophobic functionality that apparently limits moisture penetration through the foam. During the freezing process, water accumulates on the surfaces of the foams. However, when hydrocarbon-terminated surfaces are present, water apparently beads and forms crystals, leading to less apparent accumulation. The object of this work is to develop inexpensive structural cryogenic <span class="hlt">insulation</span> foam that has increased impact resistance for launch and ground-based cryogenic systems. Two parallel approaches will be pursued: a silica-polymer co-foaming technique and a post foam coating technique. <span class="hlt">Insulation</span> characteristics, flexibility, and water uptake can be fine-tuned through the manipulation of the polyurethane foam scaffold. Silicate coatings for polyurethane foams and aerogel-impregnated polyurethane foams have been developed and tested. A highly porous aerogel-like material may be fabricated using a co-foam and coated foam techniques, and can <span class="hlt">insulate</span> at liquid temperatures using the <span class="hlt">composite</span> foam</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012TRACE..21..285O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012TRACE..21..285O"><span>Dynamic-Type <span class="hlt">Ice</span> Thermal Storage Systems</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ohira, Akiyoshi</p> <p></p> <p>This <span class="hlt">paper</span> deals with reviews for research and development of a dynamic-type <span class="hlt">ice</span> thermal storage system. This system has three main features. First, the <span class="hlt">ice</span> thermal storage tank and the <span class="hlt">ice</span> generator are separate. Second, <span class="hlt">ice</span> is transported to the tank from the <span class="hlt">ice</span> generator by water or air. Third, the <span class="hlt">ice</span> making and melting processes are operated at the same time. Outlet water temperature from the dynamic-type <span class="hlt">ice</span> thermal storage tank remains low for a longer time. In this <span class="hlt">paper</span>, dynamic-Type <span class="hlt">ice</span> thermal storage systems are divided into three parts: the <span class="hlt">ice</span> making part, the <span class="hlt">ice</span> transport part, and the cold energy release part. Each part is reviewed separately.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016mecs.conf...66Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016mecs.conf...66Z"><span>Study on Thermal and Mechanical Properties of EPDM <span class="hlt">Insulation</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhang, Zhong-Shui; Xu, Jin-Sheng; Chen, Xiong; Jiang, Jing</p> <p></p> <p>As the most common <span class="hlt">insulation</span> material of solid rocket motors, thermal and mechanical properties of ethylene propylene diene monomer (EPDM) <span class="hlt">composite</span> are inspected in the study. Referring to the results of thermogravimetric analysis (TGA), <span class="hlt">composition</span> and morphology of EPDM <span class="hlt">composite</span> in different thermal degradation degree are investigated by scanning electron microscope (SEM) to inspect the mechanism of thermal <span class="hlt">insulation</span>. Mechanical properties of EPDM <span class="hlt">composite</span> in the state of pyrolysis are investigated by uniaxial tensile tests. At the state of initial pyrolysis, <span class="hlt">composite</span> belongs to the category of hyperelastic-viscoelastic material. The tendency of tensile strength increased and elongation decreased with increasing of heating temperature. <span class="hlt">Composite</span> behaves as the linear rule at the state of late pyrolysis, which belongs to the category of bittle. The elasticity modulus of curves are almost the same while the heating temperature ranges from 200°C to 300°C, and then gradually go down. The tensile strength of pyrolytic material reach the highest at the heating temperature of 300°C, and the virgin material has the largest elongation.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li class="active"><span>11</span></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_11 --> <div id="page_12" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li class="active"><span>12</span></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="221"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28011294','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28011294"><span>Sea-<span class="hlt">ice</span> eukaryotes of the Gulf of Finland, Baltic Sea, and evidence for herbivory on weakly shade-adapted <span class="hlt">ice</span> algae.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Majaneva, Markus; Blomster, Jaanika; Müller, Susann; Autio, Riitta; Majaneva, Sanna; Hyytiäinen, Kirsi; Nagai, Satoshi; Rintala, Janne-Markus</p> <p>2017-02-01</p> <p>To determine community <span class="hlt">composition</span> and physiological status of early spring sea-<span class="hlt">ice</span> organisms, we collected sea-<span class="hlt">ice</span>, slush and under-<span class="hlt">ice</span> water samples from the Baltic Sea. We combined light microscopy, HPLC pigment analysis and pyrosequencing, and related the biomass and physiological status of sea-<span class="hlt">ice</span> algae with the protistan community <span class="hlt">composition</span> in a new way in the area. In terms of biomass, centric diatoms including a distinct Melosira arctica bloom in the upper intermediate section of the fast <span class="hlt">ice</span>, dinoflagellates, euglenoids and the cyanobacterium Aphanizomenon sp. predominated in the sea-<span class="hlt">ice</span> sections and unidentified flagellates in the slush. Based on pigment analyses, the <span class="hlt">ice</span>-algal communities showed no adjusted photosynthetic pigment pools throughout the sea <span class="hlt">ice</span>, and the bottom-<span class="hlt">ice</span> communities were not shade-adapted. The sea <span class="hlt">ice</span> included more characteristic phototrophic taxa (49%) than did slush (18%) and under-<span class="hlt">ice</span> water (37%). Cercozoans and ciliates were the richest taxon groups, and the differences among the communities arose mainly from the various phagotrophic protistan taxa inhabiting the communities. The presence of pheophytin a coincided with an elevated ciliate biomass and read abundance in the drift <span class="hlt">ice</span> and with a high Eurytemora affinis read abundance in the pack <span class="hlt">ice</span>, indicating that ciliates and Eurytemora affinis were grazing on algae. Copyright © 2016 Elsevier GmbH. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19970009603','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19970009603"><span>Polarimetric Signatures of Sea <span class="hlt">Ice</span>. Part 1; Theoretical Model</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Nghiem, S. V.; Kwok, R.; Yueh, S. H.; Drinkwater, M. R.</p> <p>1995-01-01</p> <p>Physical, structural, and electromagnetic properties and interrelating processes in sea <span class="hlt">ice</span> are used to develop a <span class="hlt">composite</span> model for polarimetric backscattering signatures of sea <span class="hlt">ice</span>. Physical properties of sea <span class="hlt">ice</span> constituents such as <span class="hlt">ice</span>, brine, air, and salt are presented in terms of their effects on electromagnetic wave interactions. Sea <span class="hlt">ice</span> structure and geometry of scatterers are related to wave propagation, attenuation, and scattering. Temperature and salinity, which are determining factors for the thermodynamic phase distribution in sea <span class="hlt">ice</span>, are consistently used to derive both effective permittivities and polarimetric scattering coefficients. Polarimetric signatures of sea <span class="hlt">ice</span> depend on crystal sizes and brine volumes, which are affected by <span class="hlt">ice</span> growth rates. Desalination by brine expulsion, drainage, or other mechanisms modifies wave penetration and scattering. Sea <span class="hlt">ice</span> signatures are further complicated by surface conditions such as rough interfaces, hummocks, snow cover, brine skim, or slush layer. Based on the same set of geophysical parameters characterizing sea <span class="hlt">ice</span>, a <span class="hlt">composite</span> model is developed to calculate effective permittivities and backscattering covariance matrices at microwave frequencies for interpretation of sea <span class="hlt">ice</span> polarimetric signatures.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/20623577','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/20623577"><span>Thin-film <span class="hlt">composite</span> materials as a dielectric layer for flexible metal-<span class="hlt">insulator</span>-metal capacitors.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Tiwari, Jitendra N; Meena, Jagan Singh; Wu, Chung-Shu; Tiwari, Rajanish N; Chu, Min-Ching; Chang, Feng-Chih; Ko, Fu-Hsiang</p> <p>2010-09-24</p> <p>A new organic-organic nanoscale <span class="hlt">composite</span> thin-film (NCTF) dielectric has been synthesized by solution deposition of 1-bromoadamantane and triblock copolymer (Pluronic P123, BASF, EO20-PO70-EO20), in which the precursor solution has been achieved with organic additives. We have used a sol-gel process to make a metal-<span class="hlt">insulator</span>-metal capacitor (MIM) comprising a nanoscale (10 nm-thick) thin-film on a flexible polyimide (PI) substrate at room temperature. Scanning electron microscope and atomic force microscope revealed that the deposited NCTFs were crack-free, uniform, highly resistant to moisture absorption, and well adhered on the Au-Cr/PI. The electrical properties of 1-bromoadamantane-P123 NCTF were characterized by dielectric constant, capacitance, and leakage current measurements. The 1-bromoadamantane-P123 NCTF on the PI substrate showed a low leakage current density of 5.5 x 10(-11) A cm(-2) and good capacitance of 2.4 fF at 1 MHz. In addition, the calculated dielectric constant of 1-bromoadamantane-P123 NCTF was 1.9, making them suitable candidates for use in future flexible electronic devices as a stable intermetal dielectric. The electrical <span class="hlt">insulating</span> properties of 1-bromoadamantane-P123 NCTF have been improved due to the optimized dipole moments of the van der Waals interactions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..17.5048K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..17.5048K"><span>Single-particle characterization of <span class="hlt">ice</span>-nucleating particles and <span class="hlt">ice</span> particles residuals sampled by three different techniques</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kandler, Konrad; Worringen, Annette; Benker, Nathalie; Dirsch, Thomas; Mertes, Stephan; Schenk, Ludwig; Kästner, Udo; Frank, Fabian; Nillius, Björn; Bundke, Ulrich; Rose, Diana; Curtius, Joachim; Kupiszewski, Piotr; Weingartner, Ernest; Vochezer, Paul; Schneider, Johannes; Schmidt, Susan; Weinbruch, Stephan; Ebert, Martin</p> <p>2015-04-01</p> <p>During January/February 2013, at the High Alpine Research Station Jungfraujoch a measurement campaign was carried out, which was centered on atmospheric <span class="hlt">ice</span>-nucleating particles (INP) and <span class="hlt">ice</span> particle residuals (IPR). Three different techniques for separation of INP and IPR from the non-<span class="hlt">ice</span>-active particles are compared. The <span class="hlt">Ice</span> Selective Inlet (ISI) and the <span class="hlt">Ice</span> Counterflow Virtual Impactor (<span class="hlt">Ice</span>-CVI) sample <span class="hlt">ice</span> particles from mixed phase clouds and allow for the analysis of the residuals. The combination of the Fast <span class="hlt">Ice</span> Nucleus Chamber (FINCH) and the <span class="hlt">Ice</span> Nuclei Pumped Counterflow Virtual Impactor (IN-PCVI) provides <span class="hlt">ice</span>-activating conditions to aerosol particles and extracts the activated INP for analysis. Collected particles were analyzed by scanning electron microscopy and energy-dispersive X-ray microanalysis to determine size, chemical <span class="hlt">composition</span> and mixing state. All INP/IPR-separating techniques had considerable abundances (median 20 - 70 %) of instrumental contamination artifacts (ISI: Si-O spheres, probably calibration aerosol; <span class="hlt">Ice</span>-CVI: Al-O particles; FINCH+IN-PCVI: steel particles). Also, potential sampling artifacts (e.g., pure soluble material) occurred with a median abundance of < 20 %. While these could be explained as IPR by <span class="hlt">ice</span> break-up, for INP their IN-ability pathway is less clear. After removal of the contamination artifacts, silicates and Ca-rich particles, carbonaceous material and metal oxides were the major INP/IPR particle types separated by all three techniques. Soot was a minor contributor. Lead was detected in less than 10 % of the particles, of which the majority were internal mixtures with other particle types. Sea-salt and sulfates were identified by all three methods as INP/IPR. Most samples showed a maximum of the INP/IPR size distribution at 400 nm geometric diameter. In a few cases, a second super-micron maximum was identified. Soot/carbonaceous material and metal oxides were present mainly in the submicron range. ISI and FINCH</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20130011366','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20130011366"><span>Aerogel Blanket <span class="hlt">Insulation</span> Materials for Cryogenic Applications</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Coffman, B. E.; Fesmire, J. E.; White, S.; Gould, G.; Augustynowicz, S.</p> <p>2009-01-01</p> <p>Aerogel blanket materials for use in thermal <span class="hlt">insulation</span> systems are now commercially available and implemented by industry. Prototype aerogel blanket materials were presented at the Cryogenic Engineering Conference in 1997 and by 2004 had progressed to full commercial production by Aspen Aerogels. Today, this new technology material is providing superior energy efficiencies and enabling new design approaches for more cost effective cryogenic systems. Aerogel processing technology and methods are continuing to improve, offering a tailor-able array of product formulations for many different thermal and environmental requirements. Many different varieties and combinations of aerogel blankets have been characterized using <span class="hlt">insulation</span> test cryostats at the Cryogenics Test Laboratory of NASA Kennedy Space Center. Detailed thermal conductivity data for a select group of materials are presented for engineering use. Heat transfer evaluations for the entire vacuum pressure range, including ambient conditions, are given. Examples of current cryogenic applications of aerogel blanket <span class="hlt">insulation</span> are also given. KEYWORDS: Cryogenic tanks, thermal <span class="hlt">insulation</span>, <span class="hlt">composite</span> materials, aerogel, thermal conductivity, liquid nitrogen boil-off</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19710000458','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19710000458"><span>Hot-blade stripper for polyester <span class="hlt">insulation</span> on FCC</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Angele, W.; Chambers, C. M.</p> <p>1971-01-01</p> <p>Stripper incorporates a blade which is electrically heated to a controlled temperature. Heated blade softens and strips <span class="hlt">insulation</span> from cable while <span class="hlt">paper</span> ribbon removes <span class="hlt">insulation</span> material and keeps blade clean for next operation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015MS%26E...71a2004A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015MS%26E...71a2004A"><span>Thermal <span class="hlt">insulation</span> of pipelines by foamed glass-ceramic</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Apkaryan, A. S.; Kudyakov, A. I.</p> <p>2015-01-01</p> <p>Based on broken glass, clay and organic additives granular <span class="hlt">insulating</span> glass crystalline material and technology of its receipt are developed. The regularities of the effect of <span class="hlt">composition</span> and firing temperature on the properties of the granules are specified. The resulting granular thermally <span class="hlt">insulating</span> material is produced with a bulk density of 260-280 kg/m3 pellet strength - 1.74 MPa, thermal conductivity - 0.075 W/m °C, water absorption - 2.6 % by weight. The effect of the basic physical characteristics of the components of the charge on the process of pore formation is studied. According to the research results, basic parameters affecting the sustainability of the swelling glass are specified. Rational charge <span class="hlt">composition</span>, thermal and gas synthesis mode are chosen so that the partial pressure of gases is below the surface tension of the melt. This enables the formation of granules with small closed pores and vitrified surface. The article is the result of studies on the application of materials for pipe <span class="hlt">insulation</span> of heating mains with foamed glass ceramics.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/6867697','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/biblio/6867697"><span>Laminated <span class="hlt">insulators</span> having heat dissipation means</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Niemann, R.C.; Mataya, K.F.; Gonczy, J.D.</p> <p>1980-04-24</p> <p>A laminated body is provided with heat dissipation capabilities. The <span class="hlt">insulator</span> body is formed by dielectric layers interleaved with heat conductive layers, and bonded by an adhesive to form a <span class="hlt">composite</span> structure. The heat conductive layers include provision for connection to an external thermal circuit.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ApPhL.110x3505M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ApPhL.110x3505M"><span>Origin of positive fixed charge at <span class="hlt">insulator</span>/AlGaN interfaces and its control by AlGaN <span class="hlt">composition</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Matys, M.; Stoklas, R.; Blaho, M.; Adamowicz, B.</p> <p>2017-06-01</p> <p>The key feature for the precise tuning of Vth in GaN-based metal-<span class="hlt">insulator</span>-semiconductor (MIS) high electron mobility transistors is the control of the positive fixed charge (Qf) at the <span class="hlt">insulator</span>/III-N interfaces, whose amount is often comparable to the negative surface polarization charge ( Qp o l -). In order to clarify the origin of Qf, we carried out a comprehensive capacitance-voltage (C-V) characterization of SiO2/AlxGa1-xN/GaN and SiN/AlxGa1-xN/GaN structures with Al <span class="hlt">composition</span> (x) varying from 0.15 to 0.4. For both types of structures, we observed a significant Vth shift in C-V curves towards the positive gate voltage with increasing x. On the contrary, the Schottky gate structures exhibited Vth shift towards the more negative biases. From the numerical simulations of C-V curves using the Poisson's equation supported by the analytical calculations of Vth, we showed that the Vth shift in the examined MIS structures is due to a significant decrease in the positive Qf with rising x. Finally, we examined this result with respect to various hypotheses developed in the literature to explain the origin of the positive Qf at <span class="hlt">insulator</span>/III-N interfaces.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5503389','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5503389"><span>Fabrication of Cellulose Nanofiber/AlOOH Aerogel for Flame Retardant and Thermal <span class="hlt">Insulation</span></span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Fan, Bitao; Chen, Shujun; Yao, Qiufang; Sun, Qingfeng; Jin, Chunde</p> <p>2017-01-01</p> <p>Cellulose nanofiber/AlOOH aerogel for flame retardant and thermal <span class="hlt">insulation</span> was successfully prepared through a hydrothermal method. Their flame retardant and thermal <span class="hlt">insulation</span> properties were investigated. The morphology image of the cellulose nanofiber/AlOOH exhibited spherical AlOOH with an average diameter of 0.5 μm that was wrapped by cellulose nanofiber or adhered to them. Cellulose nanofiber/AlOOH <span class="hlt">composite</span> aerogels exhibited excellent flame retardant and thermal <span class="hlt">insulation</span> properties through the flammability test, which indicated that the as-prepared <span class="hlt">composite</span> aerogels would have a promising future in the application of some important areas such as protection of lightweight construction materials. PMID:28772670</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PhRvL.119v7204B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PhRvL.119v7204B"><span>Quantum Spin <span class="hlt">Ice</span> under a [111] Magnetic Field: From Pyrochlore to Kagome</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bojesen, Troels Arnfred; Onoda, Shigeki</p> <p>2017-12-01</p> <p>Quantum spin <span class="hlt">ice</span>, modeled for magnetic rare-earth pyrochlores, has attracted great interest for hosting a U(1) quantum spin liquid, which involves spin-<span class="hlt">ice</span> monopoles as gapped deconfined spinons, as well as gapless excitations analogous to photons. However, the global phase diagram under a [111] magnetic field remains open. Here we uncover by means of unbiased quantum Monte Carlo simulations that a supersolid of monopoles, showing both a superfluidity and a partial ionization, intervenes the kagome spin <span class="hlt">ice</span> and a fully ionized monopole <span class="hlt">insulator</span>, in contrast to classical spin <span class="hlt">ice</span> where a direct discontinuous phase transition takes place. We also show that on cooling, kagome spin <span class="hlt">ice</span> evolves towards a valence-bond solid similar to what appears in the associated kagome lattice model [S. V. Isakov et al., Phys. Rev. Lett. 97, 147202 (2006), 10.1103/PhysRevLett.97.147202]. Possible relevance to experiments is discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AIPC.1866d0006B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AIPC.1866d0006B"><span>The influence of partial replacement of hemp shives by expanded perlite on physical properties of hemp-lime <span class="hlt">composite</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Brzyski, Przemysław; Widomski, Marcin</p> <p>2017-07-01</p> <p>The use of waste plants in building materials production is consistent with the principles of sustainable development, including waste management, CO2 balance, biodegradability of the material e.g. after building demolition. The porous structure of plant materials determines their usability as the <span class="hlt">insulation</span> materials. An example of plant applicable in the construction industry is the industrial hemp. The shives are produced from the wooden core of the hemp stem as lightweight <span class="hlt">insulating</span> filler in the <span class="hlt">composite</span> based on lime binder. The discussed hemp-lime <span class="hlt">composite</span>, due to the presence of lightweight, porous organic aggregates exhibits satisfactory thermal <span class="hlt">insulation</span> properties and is used as filling and <span class="hlt">insulation</span> of walls (as well as roofs and floors) in buildings of the wooden frame construction. The irregular shape of shives and their low density causes nonhomogenous compaction of <span class="hlt">composite</span> and the formation of voids between the randomly arranged shives. In this <span class="hlt">paper</span> the series of hemp-lime <span class="hlt">composites</span> were tested. Apart from hemp shives, an additional aggregate - expanded perlite was used as a fine, lightweight, thermal <span class="hlt">insulating</span> filler. Application of the additional aggregate was aimed to fill the voids between hemp shives and to investigate its influence on the physical properties of <span class="hlt">composite</span>: apparent density, total porosity, water absorption and thermal conductivity.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014ACPD...1423027W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014ACPD...1423027W"><span>Single-particle characterization of <span class="hlt">ice</span>-nucleating particles and <span class="hlt">ice</span> particle residuals sampled by three different techniques</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Worringen, A.; Kandler, K.; Benker, N.; Dirsch, T.; Weinbruch, S.; Mertes, S.; Schenk, L.; Kästner, U.; Frank, F.; Nillius, B.; Bundke, U.; Rose, D.; Curtius, J.; Kupiszewski, P.; Weingartner, E.; Schneider, J.; Schmidt, S.; Ebert, M.</p> <p>2014-09-01</p> <p>In the present work, three different techniques are used to separate <span class="hlt">ice</span>-nucleating particles (INP) and <span class="hlt">ice</span> particle residuals (IPR) from non-<span class="hlt">ice</span>-active particles: the <span class="hlt">Ice</span> Selective Inlet (ISI) and the <span class="hlt">Ice</span> Counterflow Virtual Impactor (<span class="hlt">Ice</span>-CVI), which sample <span class="hlt">ice</span> particles from mixed phase clouds and allow for the analysis of the residuals, as well as the combination of the Fast <span class="hlt">Ice</span> Nucleus Chamber (FINCH) and the <span class="hlt">Ice</span> Nuclei Pumped Virtual Impactor (IN-PCVI), which provides <span class="hlt">ice</span>-activating conditions to aerosol particles and extracts the activated ones for analysis. The collected particles were analyzed by scanning electron microscopy and energy-dispersive X-ray microanalysis to determine their size, chemical <span class="hlt">composition</span> and mixing state. Samples were taken during January/February 2013 at the High Alpine Research Station Jungfraujoch. All INP/IPR-separating techniques had considerable abundances (median 20-70%) of contamination artifacts (ISI: Si-O spheres, probably calibration aerosol; <span class="hlt">Ice</span>-CVI: Al-O particles; FINCH + IN-PCVI: steel particles). Also, potential measurement artifacts (soluble material) occurred (median abundance < 20%). After removal of the contamination particles, silicates and Ca-rich particles, carbonaceous material and metal oxides were the major INP/IPR particle types separated by all three techniques. Minor types include soot and Pb-bearing particles. Sea-salt and sulfates were identified by all three methods as INP/IPR. Lead was identified in less than 10% of the INP/IPR. It was mainly present as an internal mixture with other particle types, but also external lead-rich particles were found. Most samples showed a maximum of the INP/IPR size distribution at 400 nm geometric diameter. In a few cases, a second super-micron maximum was identified. Soot/carbonaceous material and metal oxides were present mainly in the submicron range. ISI and FINCH yielded silicates and Ca-rich particles mainly with diameters above 1 μm, while the <span class="hlt">Ice</span>-CVI also</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.1689H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.1689H"><span>Chemical and physical characterization of fertile soil-derived <span class="hlt">ice</span> residuals from the Fifth International <span class="hlt">Ice</span> Nucleation workshop in November 2014 (FIN-1)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hiranuma, Naruki; Möhler, Ottmar; Kulkarni, Gourihar; Laskin, Alexander; Zelenyuk, Alla</p> <p>2017-04-01</p> <p>The climate impact of <span class="hlt">ice</span>-nucleating particles (INPs) derived from fertile soils on global scale has been recently accented by their diversity and efficient freezing ability. However, their representation in atmospheric models is limited in part due to our incomplete knowledge of fertile soil <span class="hlt">composition</span>, abundance and associated sensitivity to heterogeneous <span class="hlt">ice</span> nucleation. To fill given knowledge gap, we have investigated a unique/rich set of <span class="hlt">ice</span> crystal residual samples derived from a variety of fertile soil samples obtained through our participation in the Fifth International <span class="hlt">Ice</span> Nucleation workshop (FIN-1). FIN-1 was held at the Aerosol Interaction and Dynamics in the Atmosphere (AIDA) facility at Karlsruhe Institute of Technology (KIT), which is the world's foremost facility for studying <span class="hlt">ice</span> clouds in a controlled setting, in November 2014 to comprehensively study the heterogeneous <span class="hlt">ice</span> formation in the atmosphere with collaboration among 10 international groups that were funded through European consortium, NSF and USDOE agencies. Here, we will present the nanoscale surface morphology and elemental/molecular <span class="hlt">composition</span> of <span class="hlt">ice</span> crystal residuals as well as that of total aerosol samples from the FIN-1 activity to identify and classify any specific mineral and organic inclusions that may have promoted nucleation of <span class="hlt">ice</span>. Comparing total aerosols to residuals will shed light on the <span class="hlt">composition</span> and abundance of certain particle types in INPs. Acknowledgements: The valuable contributions of the INUIT (<span class="hlt">Ice</span> Nuclei Research Unit) collaborators, the FIN organizers, their institutions and the FIN-1 Workshop science team are gratefully acknowledged.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26572417','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26572417"><span>Effect of precipitated calcium carbonate--Cellulose nanofibrils <span class="hlt">composite</span> filler on <span class="hlt">paper</span> properties.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>He, Ming; Cho, Byoung-Uk; Won, Jong Myoung</p> <p>2016-01-20</p> <p>A new concept of <span class="hlt">composite</span> filler was developed by using cellulose nanofibrils (CNF), precipitated calcium carbonate (PCC) and cationic starch (C-starch). In this study, cellulose nanofibrils were utilized in two different ways: a PCC-CNF <span class="hlt">composite</span> filler and a papermaking additive in sheet forming. The aim was to elucidate their effects on flocculation, filler retention and the strength and optical properties of handsheets. The highest filler retention was obtained by using the PCC-CNF <span class="hlt">composite</span> filler in <span class="hlt">paper</span> sheets. The <span class="hlt">paper</span> filled with the <span class="hlt">composite</span> fillers had much higher bursting and tensile strengths than conventional PCC loading. It was also found that the <span class="hlt">paper</span> prepared with PCC-CNF <span class="hlt">composite</span> fillers became denser with increasing the filler content of <span class="hlt">paper</span>. Copyright © 2015 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24994469','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24994469"><span>Recycling disposable cups into <span class="hlt">paper</span> plastic <span class="hlt">composites</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Mitchell, Jonathan; Vandeperre, Luc; Dvorak, Rob; Kosior, Ed; Tarverdi, Karnik; Cheeseman, Christopher</p> <p>2014-11-01</p> <p>The majority of disposable cups are made from <span class="hlt">paper</span> plastic laminates (PPL) which consist of high quality cellulose fibre with a thin internal polyethylene coating. There are limited recycling options for PPLs and this has contributed to disposable cups becoming a high profile, problematic waste. In this work disposable cups have been shredded to form PPL flakes and these have been used to reinforce polypropylene to form novel <span class="hlt">paper</span> plastic <span class="hlt">composites</span> (PPCs). The PPL flakes and polypropylene were mixed, extruded, pelletised and injection moulded at low temperatures to prevent degradation of the cellulose fibres. The level of PPL flake addition and the use of a maleated polyolefin coupling agent to enhance interfacial adhesion have been investigated. Samples have been characterised using tensile testing, dynamic mechanical analysis (DMA) and thermogravimetric analysis. Use of a coupling agent allows <span class="hlt">composites</span> containing 40 wt.% of PPL flakes to increase tensile strength of PP by 50% to 30 MPa. The Young modulus also increases from 1 to 2.5 GPa and the work to fracture increases by a factor of 5. The work demonstrates that PPL disposable cups have potential to be beneficially reused as reinforcement in novel polypropylene <span class="hlt">composites</span>. Copyright © 2014 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1998RvMP...70.1039I','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1998RvMP...70.1039I"><span>Metal-<span class="hlt">insulator</span> transitions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Imada, Masatoshi; Fujimori, Atsushi; Tokura, Yoshinori</p> <p>1998-10-01</p> <p>Metal-<span class="hlt">insulator</span> transitions are accompanied by huge resistivity changes, even over tens of orders of magnitude, and are widely observed in condensed-matter systems. This article presents the observations and current understanding of the metal-<span class="hlt">insulator</span> transition with a pedagogical introduction to the subject. Especially important are the transitions driven by correlation effects associated with the electron-electron interaction. The <span class="hlt">insulating</span> phase caused by the correlation effects is categorized as the Mott <span class="hlt">Insulator</span>. Near the transition point the metallic state shows fluctuations and orderings in the spin, charge, and orbital degrees of freedom. The properties of these metals are frequently quite different from those of ordinary metals, as measured by transport, optical, and magnetic probes. The review first describes theoretical approaches to the unusual metallic states and to the metal-<span class="hlt">insulator</span> transition. The Fermi-liquid theory treats the correlations that can be adiabatically connected with the noninteracting picture. Strong-coupling models that do not require Fermi-liquid behavior have also been developed. Much work has also been done on the scaling theory of the transition. A central issue for this review is the evaluation of these approaches in simple theoretical systems such as the Hubbard model and t-J models. Another key issue is strong competition among various orderings as in the interplay of spin and orbital fluctuations. Experimentally, the unusual properties of the metallic state near the <span class="hlt">insulating</span> transition have been most extensively studied in d-electron systems. In particular, there is revived interest in transition-metal oxides, motivated by the epoch-making findings of high-temperature superconductivity in cuprates and colossal magnetoresistance in manganites. The article reviews the rich phenomena of anomalous metallicity, taking as examples Ti, V, Cr, Mn, Fe, Co, Ni, Cu, and Ru compounds. The diverse phenomena include strong spin and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007cren.book..120T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007cren.book..120T"><span><span class="hlt">Insulation</span> Progress since the Mid-1950s</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Timmerhaus, K. D.</p> <p></p> <p>Storage vessel and cryostat design for modern cryogenic systems has become rather routine as the result of the wide use of and application of cryogenic fluids. Such vessels for these fluids range in size from 1 L flasks used in the laboratory for liquid nitrogen to the more than 200,000 m3 double-walled tanks used for temporary storage of liquefied natural gas before being transported overseas to their final destination. These storage vessels for cryogenic fluids range in type from low-performance containers <span class="hlt">insulated</span> with rigid foam or fibrous <span class="hlt">insulation</span> to high-performance containers <span class="hlt">insulated</span> with evacuated multilayer <span class="hlt">insulations</span>. The overriding factors in the type of container selected normally are of economics and safety. This <span class="hlt">paper</span> will consider various <span class="hlt">insulation</span> concepts used in such cryogenic storage systems and will review the progress that has been made over the past 50 years in these <span class="hlt">insulation</span> systems.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007AGUFM.C41A0044S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007AGUFM.C41A0044S"><span>Studies of contemporary glacier basal <span class="hlt">ice</span> cryostructures to identify buried basal <span class="hlt">ice</span> in the permafrost: an example from the Matanuska Glacier, Alaska.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Stephani, E.; Fortier, D.; Kanevskiy, M.; Dillon, M.; Shur, Y.</p> <p>2007-12-01</p> <p>In the permafrost, massive <span class="hlt">ice</span> bodies occur as buried glacier <span class="hlt">ice</span>, aufeis <span class="hlt">ice</span>, recrystalized snow, massive segregated <span class="hlt">ice</span>, injection <span class="hlt">ice</span>, <span class="hlt">ice</span> wedges or <span class="hlt">ice</span> formed in underground cavities ("pool <span class="hlt">ice</span>", "thermokarst-cave <span class="hlt">ice</span>"). The origin of massive <span class="hlt">ice</span> bodies in the permafrost bears considerable implications for the reconstructions of paleoenvironments and paleoclimates. Our work aims to help the permafrost scientists working on massive icy sediments to distinguish buried basal glacier <span class="hlt">ice</span> from other types of buried <span class="hlt">ice</span>. To do so, the properties and structure of contemporary basal <span class="hlt">ice</span> must be well known. Field investigations at the Matanuska Glacier (Chugach range, South-central Alaska), consisted in descriptions and sampling of natural basal <span class="hlt">ice</span> exposures. We have used the basal <span class="hlt">ice</span> facies classification of Lawson (1979) which is simple, easy to use in the field and provides a good framework for the description of basal <span class="hlt">ice</span> exposures. Cores were extracted and brought back to the laboratory for water and grain-size analyses. The sediments forming the cryostructure were mostly polymodal, poorly sorted gravelly silt to gravelly fine sand, with mud contents generally over 50%. These data will be used to calibrate three-dimensional (3D) models produced from micro-tomographic scans of basal <span class="hlt">ice</span> which will produce quantitative estimates of volumetric <span class="hlt">ice</span> and sediments contents of basal <span class="hlt">ice</span> cryostructures. Ultimately, visual qualitative and quantitative characterization of the basal <span class="hlt">ice</span> components of 3D models together with field observations and laboratory analysis will allow for a new micro-facies and cryostructures classification of the basal <span class="hlt">ice</span>. Our work will also have applications in glaciology, glacial geology, geomorphology, Quaternary and paleo-climatological studies based on inferences made from the structure of basal glacier <span class="hlt">ice</span>. This <span class="hlt">paper</span> presents the internal <span class="hlt">composition</span> of the basal <span class="hlt">ice</span> facies in terms of cryostructures assemblages (Fortier et al.: 2007) and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22253455-novel-two-step-laser-ablation-ionization-mass-spectrometry-laims-actor-spectator-ice-layers-probing-chemical-composition-sub-ice-beneath-sub-ice-layer','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22253455-novel-two-step-laser-ablation-ionization-mass-spectrometry-laims-actor-spectator-ice-layers-probing-chemical-composition-sub-ice-beneath-sub-ice-layer"><span>Novel two-step laser ablation and ionization mass spectrometry (2S-LAIMS) of actor-spectator <span class="hlt">ice</span> layers: Probing chemical <span class="hlt">composition</span> of D{sub 2}O <span class="hlt">ice</span> beneath a H{sub 2}O <span class="hlt">ice</span> layer</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Yang, Rui, E-mail: ryang73@ustc.edu; Gudipati, Murthy S., E-mail: gudipati@jpl.nasa.gov</p> <p>2014-03-14</p> <p>ablation and ionization. This new technique can thus be potentially employed to undertake in situ analysis of materials imbedded in diverse media, such as cryogenic <span class="hlt">ices</span>, biological samples, tissues, minerals, etc., by covered with an IR-absorbing laser ablation medium and study the chemical <span class="hlt">composition</span> and reaction pathways of the analyte in its natural surroundings.« less</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li class="active"><span>12</span></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_12 --> <div id="page_13" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li class="active"><span>13</span></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="241"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.P24A..06S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.P24A..06S"><span>Asynchronously Coupled Models of <span class="hlt">Ice</span> Loss from Airless Planetary Bodies</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schorghofer, N.</p> <p>2016-12-01</p> <p><span class="hlt">Ice</span> is found near the surface of dwarf planet Ceres, in some main belt asteroids, and perhaps in NEOs that will be explored or even mined in future. The simple but important question of how fast <span class="hlt">ice</span> is lost from airless bodies can present computational challenges. The thermal cycle on the surface repeats on much shorter time-scales than <span class="hlt">ice</span> retreats; one process acts on the time-scale of hours, the other over billions of years. This multi-scale situation is addressed with asynchronous coupling, where models with different time steps are woven together. The sharp contrast at the retreating <span class="hlt">ice</span> table is dealt with with explicit interface tracking. For Ceres, which is covered with a thermally <span class="hlt">insulating</span> dust mantle, desiccation rates are orders of magnitude slower than had been calculated with simpler models. More model challenges remain: The role of impact devolatization and the time-scale for complete desiccation of an asteroid. I will also share my experience with code distribution using GitHub and Zenodo.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1013857','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/servlets/purl/1013857"><span>Process for making ceramic <span class="hlt">insulation</span></span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Akash, Akash [Salt Lake City, UT; Balakrishnan, G Nair [Sandy, UT</p> <p>2009-12-08</p> <p>A method is provided for producing <span class="hlt">insulation</span> materials and <span class="hlt">insulation</span> for high temperature applications using novel castable and powder-based ceramics. The ceramic components produced using the proposed process offers (i) a fine porosity (from nano-to micro scale); (ii) a superior strength-to-weight ratio; and (iii) flexibility in designing multilayered features offering multifunctionality which will increase the service lifetime of <span class="hlt">insulation</span> and refractory components used in the solid oxide fuel cell, direct carbon fuel cell, furnace, metal melting, glass, chemical, <span class="hlt">paper</span>/pulp, automobile, industrial heating, coal, and power generation industries. Further, the ceramic components made using this method may have net-shape and/or net-size advantages with minimum post machining requirements.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4435194','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4435194"><span>Development of a Capacitive <span class="hlt">Ice</span> Sensor to Measure <span class="hlt">Ice</span> Growth in Real Time</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Zhi, Xiang; Cho, Hyo Chang; Wang, Bo; Ahn, Cheol Hee; Moon, Hyeong Soon; Go, Jeung Sang</p> <p>2015-01-01</p> <p>This <span class="hlt">paper</span> presents the development of the capacitive sensor to measure the growth of <span class="hlt">ice</span> on a fuel pipe surface in real time. The <span class="hlt">ice</span> sensor consists of pairs of electrodes to detect the change in capacitance and a thermocouple temperature sensor to examine the <span class="hlt">ice</span> formation situation. In addition, an environmental chamber was specially designed to control the humidity and temperature to simulate the <span class="hlt">ice</span> formation conditions. From the humidity, a water film is formed on the <span class="hlt">ice</span> sensor, which results in an increase in capacitance. <span class="hlt">Ice</span> nucleation occurs, followed by the rapid formation of frost <span class="hlt">ice</span> that decreases the capacitance suddenly. The capacitance is saturated. The developed <span class="hlt">ice</span> sensor explains the <span class="hlt">ice</span> growth providing information about the <span class="hlt">icing</span> temperature in real time. PMID:25808770</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25808770','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25808770"><span>Development of a capacitive <span class="hlt">ice</span> sensor to measure <span class="hlt">ice</span> growth in real time.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Zhi, Xiang; Cho, Hyo Chang; Wang, Bo; Ahn, Cheol Hee; Moon, Hyeong Soon; Go, Jeung Sang</p> <p>2015-03-19</p> <p>This <span class="hlt">paper</span> presents the development of the capacitive sensor to measure the growth of <span class="hlt">ice</span> on a fuel pipe surface in real time. The <span class="hlt">ice</span> sensor consists of pairs of electrodes to detect the change in capacitance and a thermocouple temperature sensor to examine the <span class="hlt">ice</span> formation situation. In addition, an environmental chamber was specially designed to control the humidity and temperature to simulate the <span class="hlt">ice</span> formation conditions. From the humidity, a water film is formed on the <span class="hlt">ice</span> sensor, which results in an increase in capacitance. <span class="hlt">Ice</span> nucleation occurs, followed by the rapid formation of frost <span class="hlt">ice</span> that decreases the capacitance suddenly. The capacitance is saturated. The developed <span class="hlt">ice</span> sensor explains the <span class="hlt">ice</span> growth providing information about the <span class="hlt">icing</span> temperature in real time.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25679117','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25679117"><span>Nonvolatile memory thin-film transistors using biodegradable chicken albumen gate <span class="hlt">insulator</span> and oxide semiconductor channel on eco-friendly <span class="hlt">paper</span> substrate.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Kim, So-Jung; Jeon, Da-Bin; Park, Jung-Ho; Ryu, Min-Ki; Yang, Jong-Heon; Hwang, Chi-Sun; Kim, Gi-Heon; Yoon, Sung-Min</p> <p>2015-03-04</p> <p>Nonvolatile memory thin-film transistors (TFTs) fabricated on <span class="hlt">paper</span> substrates were proposed as one of the eco-friendly electronic devices. The gate stack was composed of chicken albumen gate <span class="hlt">insulator</span> and In-Ga-Zn-O semiconducting channel layers. All the fabrication processes were performed below 120 °C. To improve the process compatibility of the synthethic <span class="hlt">paper</span> substrate, an Al2O3 thin film was introduced as adhesion and barrier layers by atomic layer deposition. The dielectric properties of biomaterial albumen gate <span class="hlt">insulator</span> were also enhanced by the preparation of Al2O3 capping layer. The nonvolatile bistabilities were realized by the switching phenomena of residual polarization within the albumen thin film. The fabricated device exhibited a counterclockwise hysteresis with a memory window of 11.8 V, high on/off ratio of approximately 1.1 × 10(6), and high saturation mobility (μsat) of 11.5 cm(2)/(V s). Furthermore, these device characteristics were not markedly degraded even after the delamination and under the bending situration. When the curvature radius was set as 5.3 cm, the ION/IOFF ratio and μsat were obtained to be 5.9 × 10(6) and 7.9 cm(2)/(V s), respectively.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015ACP....15.4161W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015ACP....15.4161W"><span>Single-particle characterization of <span class="hlt">ice</span>-nucleating particles and <span class="hlt">ice</span> particle residuals sampled by three different techniques</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Worringen, A.; Kandler, K.; Benker, N.; Dirsch, T.; Mertes, S.; Schenk, L.; Kästner, U.; Frank, F.; Nillius, B.; Bundke, U.; Rose, D.; Curtius, J.; Kupiszewski, P.; Weingartner, E.; Vochezer, P.; Schneider, J.; Schmidt, S.; Weinbruch, S.; Ebert, M.</p> <p>2015-04-01</p> <p>In the present work, three different techniques to separate <span class="hlt">ice</span>-nucleating particles (INPs) as well as <span class="hlt">ice</span> particle residuals (IPRs) from non-<span class="hlt">ice</span>-active particles are compared. The <span class="hlt">Ice</span> Selective Inlet (ISI) and the <span class="hlt">Ice</span> Counterflow Virtual Impactor (<span class="hlt">Ice</span>-CVI) sample <span class="hlt">ice</span> particles from mixed-phase clouds and allow after evaporation in the instrument for the analysis of the residuals. The Fast <span class="hlt">Ice</span> Nucleus Chamber (FINCH) coupled with the <span class="hlt">Ice</span> Nuclei Pumped Counterflow Virtual Impactor (IN-PCVI) provides <span class="hlt">ice</span>-activating conditions to aerosol particles and extracts the activated particles for analysis. The instruments were run during a joint field campaign which took place in January and February 2013 at the High Alpine Research Station Jungfraujoch (Switzerland). INPs and IPRs were analyzed offline by scanning electron microscopy and energy-dispersive X-ray microanalysis to determine their size, chemical <span class="hlt">composition</span> and mixing state. Online analysis of the size and chemical <span class="hlt">composition</span> of INP activated in FINCH was performed by laser ablation mass spectrometry. With all three INP/IPR separation techniques high abundances (median 20-70%) of instrumental contamination artifacts were observed (ISI: Si-O spheres, probably calibration aerosol; <span class="hlt">Ice</span>-CVI: Al-O particles; FINCH + IN-PCVI: steel particles). After removal of the instrumental contamination particles, silicates, Ca-rich particles, carbonaceous material and metal oxides were the major INP/IPR particle types obtained by all three techniques. In addition, considerable amounts (median abundance mostly a few percent) of soluble material (e.g., sea salt, sulfates) were observed. As these soluble particles are often not expected to act as INP/IPR, we consider them as potential measurement artifacts. Minor types of INP/IPR include soot and Pb-bearing particles. The Pb-bearing particles are mainly present as an internal mixture with other particle types. Most samples showed a maximum of the INP/IPR size distribution at 200</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1176563','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/servlets/purl/1176563"><span>High temperature structural <span class="hlt">insulating</span> material</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Chen, Wayne Y.</p> <p>1987-01-06</p> <p>A high temperature structural <span class="hlt">insulating</span> material useful as a liner for cylinders of high temperature engines through the favorable combination of high service temperature (above about 800.degree. C.), low thermal conductivity (below about 0.2 W/m.degree. C.), and high compressive strength (above about 250 psi). The <span class="hlt">insulating</span> material is produced by selecting hollow ceramic beads with a softening temperature above about 800.degree. C., a diameter within the range of 20-200 .mu.m, and a wall thickness in the range of about 2-4 .mu.m; compacting the beads and a compatible silicate binder <span class="hlt">composition</span> under pressure and sintering conditions to provide the desired structural form with the structure having a closed-cell, compact array of bonded beads.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/875190','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/servlets/purl/875190"><span>High temperature structural <span class="hlt">insulating</span> material</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Chen, Wayne Y.</p> <p>1987-01-01</p> <p>A high temperature structural <span class="hlt">insulating</span> material useful as a liner for cylinders of high temperature engines through the favorable combination of high service temperature (above about 800.degree. C.), low thermal conductivity (below about 0.2 W/m.degree. C.), and high compressive strength (above about 250 psi). The <span class="hlt">insulating</span> material is produced by selecting hollow ceramic beads with a softening temperature above about 800.degree. C., a diameter within the range of 20-200 .mu.m, and a wall thickness in the range of about 2-4 .mu.m; compacting the beads and a compatible silicate binder <span class="hlt">composition</span> under pressure and sintering conditions to provide the desired structural form with the structure having a closed-cell, compact array of bonded beads.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/6173514','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/biblio/6173514"><span>High temperature structural <span class="hlt">insulating</span> material</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Chen, W.Y.</p> <p>1984-07-27</p> <p>A high temperature structural <span class="hlt">insulating</span> material useful as a liner for cylinders of high temperature engines through the favorable combination of high service temperature (above about 800/sup 0/C), low thermal conductivity (below about 0.2 W/m/sup 0/C), and high compressive strength (above about 250 psi). The <span class="hlt">insulating</span> material is produced by selecting hollow ceramic beads with a softening temperature above about 800/sup 0/C, a diameter within the range of 20-200 ..mu..m, and a wall thickness in the range of about 2 to 4 ..mu..m; compacting the beads and a compatible silicate binder <span class="hlt">composition</span> under pressure and sintering conditions to provide the desired structural form with the structure having a closed-cell, compact array of bonded beads.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20030022773','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20030022773"><span>Snow and <span class="hlt">Ice</span> Products from the Moderate Resolution Imaging Spectroradiometer</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Hall, Dorothy K.; Salomonson, Vincent V.; Riggs, George A.; Klein, Andrew G.</p> <p>2003-01-01</p> <p>Snow and sea <span class="hlt">ice</span> products, derived from the Moderate Resolution Imaging Spectroradiometer (MODIS) instrument, flown on the Terra and Aqua satellites, are or will be available through the National Snow and <span class="hlt">Ice</span> Data Center Distributed Active Archive Center (DAAC). The algorithms that produce the products are automated, thus providing a consistent global data set that is suitable for climate studies. The suite of MODIS snow products begins with a 500-m resolution, 2330-km swath snow-cover map that is then projected onto a sinusoidal grid to produce daily and 8-day <span class="hlt">composite</span> tile products. The sequence proceeds to daily and 8-day <span class="hlt">composite</span> climate-modeling grid (CMG) products at 0.05 resolution. A daily snow albedo product will be available in early 2003 as a beta test product. The sequence of sea <span class="hlt">ice</span> products begins with a swath product at 1-km resolution that provides sea <span class="hlt">ice</span> extent and <span class="hlt">ice</span>-surface temperature (IST). The sea <span class="hlt">ice</span> swath products are then mapped onto the Lambert azimuthal equal area or EASE-Grid projection to create a daily and 8-day <span class="hlt">composite</span> sea <span class="hlt">ice</span> tile product, also at 1 -km resolution. Climate-Modeling Grid (CMG) sea <span class="hlt">ice</span> products in the EASE-Grid projection at 4-km resolution are planned for early 2003.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018AIPC.1944b0028G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018AIPC.1944b0028G"><span>Compressive behavior of energy-saving fired facing brick <span class="hlt">composite</span> wall</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Guo, Kai; Wu, Cai</p> <p>2018-03-01</p> <p>The energy-saving fired facing brick <span class="hlt">composite</span> wall has a broad development prospects due to its merits of thermal <span class="hlt">insulation</span>, energy conservation, beautiful, and natural. The construction and characteristics of this wall are introduced and analyzed in this <span class="hlt">paper</span>. Experimental studies of samples are also conducted to investigate its compressive performance. The results show that the energy-saving fired facing brick <span class="hlt">composite</span> wall has high compressive capacity. It has considerable application prospect, the study in this <span class="hlt">paper</span> provides foundation to further studies.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.P43C2889P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.P43C2889P"><span>Variability in radar returns from Martian debris-covered glaciers attributed to surface debris layer roughness and <span class="hlt">composition</span>: implications for the regional distribution of massive subsurface <span class="hlt">ice</span> and near-surface pore-filling <span class="hlt">ice</span>.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Petersen, E.; Holt, J. W.; Levy, J. S.; Lalich, D.</p> <p>2017-12-01</p> <p>Lobate debris aprons, lineated valley fill, and concentric crater fill are a class of Martian landform thought to be glaciers blanketed by a lithic debris layer. They are found in the mid latitudes (roughly 30-50°N and S) where surface <span class="hlt">ice</span> is presently unstable. Shallow Radar (SHARAD) sounder observations are in many cases able to resolve the basal contact between the glacier and underlying bedrock, showing that the bulk <span class="hlt">composition</span> of these features is water <span class="hlt">ice</span> with < 20% lithic debris; they are thus often referred to as debris-covered glaciers (DCG). The basal contact of candidate glaciers is not always present in SHARAD radargrams, and variable reflection power between glacier sites suggests that non-detections may be due to a reduction of echo power below the noise floor. A likely candidate for signal loss is the variable roughness of different glacial surface textures. We test this mechanism of signal reduction via analysis of SHARAD reflections augmented by surface roughness analyses generated from HiRISE stereo DEMs. This method provides a means of constraining the electrical properties of the surface debris. We show that measured surface roughness is sufficient to explain basal reflection signal loss for five glacier sites in the region of Deuteronilus/Protonilus Mensae (R2 = 0.90), with the dielectric constant for the surface debris layer constrained to 4.9 ± 0.3. Assuming debris formed of basalt rock, this value is consistent with a porous debris layer containing up to 64% <span class="hlt">ice</span>, or an <span class="hlt">ice</span>-free debris layer with porosity of 28-34%. From this work, we conclude that (1) weak or non-existent basal reflections at these sites are due to roughness-induced radar signal loss and not due to differing properties of the basal interface, (2) all DCG candidates in this study exhibit similar bulk <span class="hlt">compositions</span> of relatively pure water <span class="hlt">ice</span>, and (3) the surface debris layer is formed of porous lithic debris which may contain a significant fraction of pore <span class="hlt">ice</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19870009722&hterms=spectrophotometry&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3Dspectrophotometry','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19870009722&hterms=spectrophotometry&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3Dspectrophotometry"><span>Ultraviolet spectrophotometry of comet Giacobini-Zinner during the <span class="hlt">ICE</span> encounter. [International Cometary Explorer (<span class="hlt">ICE</span>)</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Ahearn, Michael F.; Mcfadden, Lucy A.; Feldman, Paul D.; Boehnhardt, Hermann; Rahe, Juergen; Festou, Michael; Brandt, John C.; Maran, Stephen P.; Niedner, Malcom B.; Smith, Andrew M.</p> <p>1986-01-01</p> <p>The IUE spectrophotometry of Comet P/Giacobini-Zinner was acquired in support of the International Cometary Explorer (<span class="hlt">ICE</span>) mission. The abundances (or upper limits) of UV-active species were calculated. During the <span class="hlt">ICE</span> encounter the H2O production rate was 3 times 10 to the 28th power/sec, + or - 50%, consistent with values derived from the <span class="hlt">ICE</span> experiments. Comparison of the abundance of CO2(+) ions with the total electron density measured by the plasma electron experiment on <span class="hlt">ICE</span> indicates a deficiency of ions relative to electrons indicating a population of ions not detected by remote sensing. The absence of detectable Mg(+) rules out this species as a possible ion of M/Q = 24 detected by the Ion <span class="hlt">Composition</span> Instrument, part of the <span class="hlt">ICE</span> complement of instruments.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C41E..01H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C41E..01H"><span><span class="hlt">Ice</span> shelf structure and stability: Larsen C <span class="hlt">Ice</span> Shelf, Antarctica</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hubbard, B. P.; Ashmore, D.; Bevan, S. L.; Booth, A. D.; Holland, P.; Jansen, D.; Kuipers Munneke, P.; Kulessa, B.; Luckman, A. J.; Sevestre, H.; O'Leary, M.</p> <p>2017-12-01</p> <p>We report on recent empirical investigations of the internal structure and stability (or otherwise) of Larsen C <span class="hlt">Ice</span> Shelf (LCIS), Antarctica, focusing on research carried out for the MIDAS research project between 2014 and 2017. Borehole- and surface geophysics-based fieldwork carried out in austral springs 2014 and 2015 revealed that ephemeral surface ponds, preferentially located within the major inlets within the northern sector of the <span class="hlt">ice</span> shelf, result in the formation of several tens of metres of (relatively dense) subsurface <span class="hlt">ice</span> within what would otherwise have been a progressively densifying snow and firn column. Five boreholes were drilled throughout the sector and logged by optical televiewer, showing this refrozen <span class="hlt">ice</span> to be extensive and of variable <span class="hlt">composition</span> depending on its process of formation. Mapping the depth-distribution of the resulting <span class="hlt">ice</span> types and associating each with a simple flow-line model of <span class="hlt">ice</span> motion and accumulation indicates that this area of LCIS has experienced substantial melting for some centuries but that surface ponding has only occurred in recent decades, possibly restricted to the past 20 years. We also present near-surface temperature data that reveal surprising temporal patterns in foehn wind activity and intensity. Finally, we report on the geometrical extension and widening of a rift that was responsible for calving a 5,800 km^2 iceberg from the LCIS in July 2017. The nature of rift propagation through `suture' <span class="hlt">ice</span> bands, widely considered to be composed of marine <span class="hlt">ice</span>, is contrasted with that of its propagation through meteoric <span class="hlt">ice</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/21538461-epitaxy-strain-composition-effects-metal-insulator-transition-characteristics-smnio-sub-thin-films','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/21538461-epitaxy-strain-composition-effects-metal-insulator-transition-characteristics-smnio-sub-thin-films"><span>Epitaxy, strain, and <span class="hlt">composition</span> effects on metal-<span class="hlt">insulator</span> transition characteristics of SmNiO{sub 3} thin films</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Aydogdu, Gulgun H.; Ha, Sieu D.; Viswanath, B.</p> <p></p> <p>SmNiO{sub 3} (SNO) thin films were deposited on LaAlO{sub 3} (LAO), SrTiO{sub 3}, SrLaAlO{sub 4}, Si, and Al{sub 2}O{sub 3} (sapphire) substrates by RF magnetron sputtering and studies were conducted to understand how film structure and <span class="hlt">composition</span> influence the <span class="hlt">insulator</span>-metal transition properties. It is observed that the compressive strain induces the <span class="hlt">insulator</span> to metal transition (MIT), while tensile strain suppresses it. In the case of non-epitaxial films, semiconducting behavior is obtained on sapphire over a broad temperature range, while on heavily-doped Si substrate; an MIT is seen in out-of-plane resistance measurement. In addition, thickness dependence on the resistance behavior andmore » nickel oxidation state has been examined for epitaxial SNO films on LAO substrates. Fine control of the MIT by modifications to the mismatch strain and thickness provides insights to enhance the performance and the functionality of these films for emerging electron devices.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2000E%26PSL.181..529S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2000E%26PSL.181..529S"><span><span class="hlt">Ice</span> formation in subglacial Lake Vostok, Central Antarctica</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Souchez, R.; Petit, J. R.; Tison, J.-L.; Jouzel, J.; Verbeke, V.</p> <p>2000-09-01</p> <p>The investigation of chemical and isotopic properties in the lake <span class="hlt">ice</span> from the Vostok <span class="hlt">ice</span> core gives clues to the mechanisms involved in <span class="hlt">ice</span> formation within the lake. A small lake water salinity can be reasonably deduced from the chemical data. Possible implications for the water circulation of Lake Vostok are developed. The characteristics of the isotopic <span class="hlt">composition</span> of the lake <span class="hlt">ice</span> indicate that <span class="hlt">ice</span> formation in Lake Vostok occurred by frazil <span class="hlt">ice</span> crystal generation due to supercooling as a consequence of rising waters and a possible contrast in water salinity. Subsequent consolidation of the developed loose <span class="hlt">ice</span> crystals results in the accretion of <span class="hlt">ice</span> to the ceiling of the lake.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20010048416&hterms=hydrometer&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dhydrometer','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20010048416&hterms=hydrometer&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dhydrometer"><span><span class="hlt">Ice</span> Nucleation in Deep Convection</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Jensen, Eric; Ackerman, Andrew; Stevens, David; Gore, Warren J. (Technical Monitor)</p> <p>2001-01-01</p> <p>The processes controlling production of <span class="hlt">ice</span> crystals in deep, rapidly ascending convective columns are poorly understood due to the difficulties involved with either modeling or in situ sampling of these violent clouds. A large number of <span class="hlt">ice</span> crystals are no doubt generated when droplets freeze at about -40 C. However, at higher levels, these crystals are likely depleted due to precipitation and detrainment. As the <span class="hlt">ice</span> surface area decreases, the relative humidity can increase well above <span class="hlt">ice</span> saturation, resulting in bursts of <span class="hlt">ice</span> nucleation. We will present simulations of these processes using a large-eddy simulation model with detailed microphysics. Size bins are included for aerosols, liquid droplets, <span class="hlt">ice</span> crystals, and mixed-phase (<span class="hlt">ice</span>/liquid) hydrometers. Microphysical processes simulated include droplet activation, freezing, melting, homogeneous freezing of sulfate aerosols, and heterogeneous <span class="hlt">ice</span> nucleation. We are focusing on the importance of <span class="hlt">ice</span> nucleation events in the upper part of the cloud at temperatures below -40 C. We will show that the ultimate evolution of the cloud in this region (and the anvil produced by the convection) is sensitive to these <span class="hlt">ice</span> nucleation events, and hence to the <span class="hlt">composition</span> of upper tropospheric aerosols that get entrained into the convective column.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20110024021','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20110024021"><span>Thin Thermal-<span class="hlt">Insulation</span> Blankets for Very High Temperatures</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Choi, Michael K.</p> <p>2003-01-01</p> <p>Thermal-<span class="hlt">insulation</span> blankets of a proposed type would be exceptionally thin and would endure temperatures up to 2,100 C. These blankets were originally intended to protect components of the NASA Solar Probe spacecraft against radiant heating at its planned closest approach to the Sun (a distance of 4 solar radii). These blankets could also be used on Earth to provide thermal protection in special applications (especially in vacuum chambers) for which conventional thermal-<span class="hlt">insulation</span> blankets would be too thick or would not perform adequately. A blanket according to the proposal (see figure) would be made of molybdenum, titanium nitride, and carbon- carbon <span class="hlt">composite</span> mesh, which melt at temperatures of 2,610, 2,930, and 2,130 C, respectively. The emittance of molybdenum is 0.24, while that of titanium nitride is 0.03. Carbon-carbon <span class="hlt">composite</span> mesh is a thermal <span class="hlt">insulator</span>. Typically, the blanket would include 0.25-mil (.0.00635-mm)-thick hot-side and cold-side cover layers of molybdenum. Titanium nitride would be vapor-deposited on both surfaces of each cover layer. Between the cover layers there would be 10 inner layers of 0.15-mil (.0.0038-mm)-thick molybdenum with vapor-deposited titanium nitride on both sides of each layer. The thickness of each titanium nitride coat would be about 1,000 A. The cover and inner layers would be interspersed with 0.25-mil (0.00635-mm)-thick layers of carbon-carbon <span class="hlt">composite</span> mesh. The blanket would have total thickness of 4.75 mils (approximately equal to 0.121 mm) and an areal mass density of 0.7 kilograms per square meter. One could, of course, increase the thermal- <span class="hlt">insulation</span> capability of the blanket by increasing number of inner layers (thereby unavoidably increasing the total thickness and mass density).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20150003183','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20150003183"><span><span class="hlt">Insulation</span> Test Cryostat with Lift Mechanism</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Dokos, Adam G. (Inventor); Fesmire, James E. (Inventor)</p> <p>2014-01-01</p> <p>A multi-purpose, cylindrical thermal <span class="hlt">insulation</span> test apparatus is used for testing <span class="hlt">insulation</span> materials and systems of materials using a liquid boil-off calorimeter system for absolute measurement of the effective thermal conductivity (k-value) and heat flux of a specimen material at a fixed environmental condition (cold-side temperature, warm-side temperature, vacuum pressure level, and residual gas <span class="hlt">composition</span>). The apparatus includes an inner vessel for receiving a liquid with a normal boiling point below ambient temperature, such as liquid nitrogen, enclosed within a vacuum chamber. A cold mass assembly, including the upper and lower guard chambers and a middle test vessel, is suspended from a lid of the vacuum canister. Each of the three chambers is filled and vented through a single feedthrough. All fluid and instrumentation feedthroughs are mounted and suspended from a top domed lid to allow easy removal of the cold mass. A lift mechanism allows manipulation of the cold mass assembly and <span class="hlt">insulation</span> test article.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20160014452','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20160014452"><span><span class="hlt">Insulation</span> Test Cryostat with Lift Mechanism</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Fesmire, James E. (Inventor); Dokos, Adam G. (Inventor)</p> <p>2016-01-01</p> <p>A multi-purpose, cylindrical thermal <span class="hlt">insulation</span> test apparatus is used for testing <span class="hlt">insulation</span> materials and systems of materials using a liquid boil-off calorimeter system for absolute measurement of the effective thermal conductivity (k-value) and heat flux of a specimen material at a fixed environmental condition (cold-side temperature, warm-side temperature, vacuum pressure level, and residual gas <span class="hlt">composition</span>). An inner vessel receives liquid with a normal boiling point below ambient temperature, such as liquid nitrogen, enclosed within a vacuum chamber. A cold mass assembly, including upper and lower guard chambers and middle test vessel, is suspended from a lid of the vacuum canister. Each of the three chambers is filled and vented through a single feedthrough. All fluid and instrumentation feedthroughs are mounted and suspended from a top domed lid allowing easy removal of the cold mass. A lift mechanism allows manipulation of the cold mass assembly and <span class="hlt">insulation</span> test article.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li class="active"><span>13</span></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_13 --> <div id="page_14" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li class="active"><span>14</span></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="261"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26879259','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26879259"><span>Metastable Nitric Acid Trihydrate in <span class="hlt">Ice</span> Clouds.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Weiss, Fabian; Kubel, Frank; Gálvez, Óscar; Hoelzel, Markus; Parker, Stewart F; Baloh, Philipp; Iannarelli, Riccardo; Rossi, Michel J; Grothe, Hinrich</p> <p>2016-03-01</p> <p>The <span class="hlt">composition</span> of high-altitude <span class="hlt">ice</span> clouds is still a matter of intense discussion. The constituents in question are <span class="hlt">ice</span> and nitric acid hydrates, but the exact phase <span class="hlt">composition</span> of clouds and its formation mechanisms are still unknown. In this work, conclusive evidence for a long-predicted phase, alpha-nitric acid trihydrate (alpha-NAT), is presented. This phase was characterized by a combination of X-ray and neutron diffraction experiments, allowing a convincing structure solution. Furthermore, vibrational spectra (infrared and inelastic neutron scattering) were recorded and compared with theoretical calculations. A strong interaction between water <span class="hlt">ice</span> and alpha-NAT was found, which explains the experimental spectra and the phase-transition kinetics. On the basis of these results, we propose a new three-step mechanism for NAT formation in high-altitude <span class="hlt">ice</span> clouds. © 2016 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19900024509&hterms=europa+ice&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Deuropa%2Bice','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19900024509&hterms=europa+ice&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Deuropa%2Bice"><span>Thermal state of an <span class="hlt">ice</span> shell on Europa</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Ojakangas, Gregory W.; Stevenson, David J.</p> <p>1989-01-01</p> <p>The thickness of the <span class="hlt">ice</span> shell presently hypothesized for Europa, which is decoupled from a silicate core by a liquid water layer, is calculated as a function of colatitude and longitude under suitable assumptions for two plausible <span class="hlt">ice</span> rheology behaviors: that of Maxwell type, and that of generalized flow-law rheology. Due to the dissipation rate's pronounced temperature dependence, virtually all tidal dissipation is found to concentrate in the lowest few kilometers of the shell. While for some parameter choices an <span class="hlt">insulating</span> regolith that raises the near-surface temperature by more than a few tens of degrees C may stabilize the shell against polar wander, a modest regolith may enhance the probability of such wander's occurrence through the reduction of the shell's retarding friction.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19750022192','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19750022192"><span>Thermal/acoustical aircraft <span class="hlt">insulation</span> material</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Struzik, E. A.; Kunz, R.; Lin, R.</p> <p>1975-01-01</p> <p>Attempts made to improve the acoustical properties of low density Fiberfrax foam, an aircraft <span class="hlt">insulation</span> material, are reported. Characterizations were also made of the physical and thermal properties. Two methods, optimization of fiber blend <span class="hlt">composition</span> and modification of the foam fabrication process, were examined as possible means of improving foam acoustics. Flame impingement tests were also made; results show performance was satisfactory.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1005031','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1005031"><span><span class="hlt">Ice</span>T users' guide and reference.</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Moreland, Kenneth D.</p> <p>2011-01-01</p> <p>The Image <span class="hlt">Composition</span> Engine for Tiles (<span class="hlt">Ice</span>T) is a high-performance sort-last parallel rendering library. In addition to providing accelerated rendering for a standard display, <span class="hlt">Ice</span>T provides the unique ability to generate images for tiled displays. The overall resolution of the display may be several times larger than any viewport that may be rendered by a single machine. This document is an overview of the user interface to <span class="hlt">Ice</span>T.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/438705-progress-gas-insulated-transformers','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/438705-progress-gas-insulated-transformers"><span>Progress of gas-<span class="hlt">insulated</span> transformers</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Togawa, Y.; Ikeda, M.; Toda, K.</p> <p></p> <p>The world`s first transformer was manufactured at Ganz in Hungary in 1885. Two years later in 1887 patents applications were made for about oil immersed transformers in the US. Since then, oil immersed types have predominated for medium- and large-capacity transformers, which are now giving way to gas <span class="hlt">insulated</span> transformers in some areas. Behind such trends are plans to construct substations inside buildings or underground, because of the difficulty in acquiring land for substations in large cities where power demand is concentrated. Requirements are protection against accidents, compactness and overall economy. Total gas <span class="hlt">insulated</span> substations combining GIS units and gasmore » <span class="hlt">insulated</span> transformers these needs. Demand for gas <span class="hlt">insulated</span> transformers has been increasing rapidly, particularly in Japan and Hong Kong. First, relatively small-capacity models below 20--30 MVA were put into practical use and today 275 kV, 300 MVa models are in use and 500kV, 1,500 MVA models are coming into use. Engineering is progressing very rapidly in these areas. This <span class="hlt">paper</span> describes the design techniques and important maintenance techniques for the latest gas <span class="hlt">insulated</span> transformers from 5,000 kVA to 300 MVA.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20110006939','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20110006939"><span>Cryogenic Vacuum <span class="hlt">Insulation</span> for Vessels and Piping</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Kogan, A.; Fesmire, J.; Johnson, W.; Minnick, J.</p> <p>2010-01-01</p> <p>Cryogenic vacuum <span class="hlt">insulation</span> systems, with proper materials selection and execution, can offer the highest levels of thermal performance. Three areas of consideration are vital to achieve the optimum result: materials, representative test conditions, and engineering approach for the particular application. Deficiency in one of these three areas can prevent optimum performance and lead to severe inefficiency. Materials of interest include micro-fiberglass, multilayer <span class="hlt">insulation</span>, and <span class="hlt">composite</span> arrangements. Cylindrical liquid nitrogen boil-off calorimetry methods were used. The need for standard thermal conductivity data is addressed through baseline testing. Engineering analysis and design factors such as layer thickness, density, and practicality are also considered.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19950010001','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19950010001"><span>Computational Simulation of the Formation and Material Behavior of <span class="hlt">Ice</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Tong, Michael T.; Singhal, Surendra N.; Chamis, Christos C.</p> <p>1994-01-01</p> <p>Computational methods are described for simulating the formation and the material behavior of <span class="hlt">ice</span> in prevailing transient environments. The methodology developed at the NASA Lewis Research Center was adopted. A three dimensional finite-element heat transfer analyzer was used to predict the thickness of <span class="hlt">ice</span> formed under prevailing environmental conditions. A multi-factor interaction model for simulating the material behavior of time-variant <span class="hlt">ice</span> layers is presented. The model, used in conjunction with laminated <span class="hlt">composite</span> mechanics, updates the material properties of an <span class="hlt">ice</span> block as its thickness increases with time. A sample case of <span class="hlt">ice</span> formation in a body of water was used to demonstrate the methodology. The results showed that the formation and the material behavior of <span class="hlt">ice</span> can be computationally simulated using the available <span class="hlt">composites</span> technology.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19910036901&hterms=aerospace+high+temperature+insulation&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Daerospace%2Bhigh%2Btemperature%2Binsulation','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19910036901&hterms=aerospace+high+temperature+insulation&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Daerospace%2Bhigh%2Btemperature%2Binsulation"><span>Reusable cryogenic foam <span class="hlt">insulation</span> for advanced aerospace vehicles</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Mcauliffe, Patrick S.; Taylor, Allan H.; Sparks, Larry L.; Dube, William P.</p> <p>1991-01-01</p> <p>Future high-speed aircraft and aerospace vehicles using cryogenic propellants will require an advanced reusable <span class="hlt">insulation</span> system for the propellant tank structure. This cryogenic <span class="hlt">insulation</span> system must be lightweight, structurally and thermally efficient, and capable of multiple reuse without cracking or degraded performance. This <span class="hlt">paper</span> presents recent progress in the development of a reusable cryogenic foam <span class="hlt">insulation</span> system having a maximum service temperature of 400 F. The system consists of preshaped, precut blocks of rigid polymethacrylimide foam <span class="hlt">insulation</span>, wrapped with a high-temperature Kapton and aluminum foil vapor barrier which is adhesively bonded to the propellant tank wall.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/6831720','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/biblio/6831720"><span>Method for forming fibrous silicon carbide <span class="hlt">insulating</span> material</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Wei, G.C.</p> <p>1983-10-12</p> <p>A method whereby silicon carbide-bonded SiC fiber <span class="hlt">composites</span> are prepared from carbon-bonded C fiber <span class="hlt">composites</span> is disclosed. Carbon-bonded C fiber <span class="hlt">composite</span> material is treated with gaseous silicon monoxide generated from the reaction of a mixture of colloidal silica and carbon black at an elevated temperature in an argon atmosphere. The carbon in the carbon bond and fiber is thus chemically converted to SiC resulting in a silicon carbide-bonded SiC fiber <span class="hlt">composite</span> that can be used for fabricating dense, high-strength high-toughness SiC <span class="hlt">composites</span> or as thermal <span class="hlt">insulating</span> materials in oxidizing environments.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/865241','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/servlets/purl/865241"><span>Method for forming fibrous silicon carbide <span class="hlt">insulating</span> material</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Wei, George C.</p> <p>1984-01-01</p> <p>A method whereby silicon carbide-bonded SiC fiber <span class="hlt">composites</span> are prepared from carbon-bonded C fiber <span class="hlt">composites</span> is disclosed. Carbon-bonded C fiber <span class="hlt">composite</span> material is treated with gaseous silicon monoxide generated from the reaction of a mixture of colloidal silica and carbon black at an elevated temperature in an argon atmosphere. The carbon in the carbon bond and fiber is thus chemically converted to SiC resulting in a silicon carbide-bonded SiC fiber <span class="hlt">composite</span> that can be used for fabricating dense, high-strength high-toughness SiC <span class="hlt">composites</span> or as thermal <span class="hlt">insulating</span> materials in oxidizing environments.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016PhDT........79B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016PhDT........79B"><span>Interactions of arctic clouds, radiation, and sea <span class="hlt">ice</span> in present-day and future climates</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Burt, Melissa Ann</p> <p></p> <p>The Arctic climate system involves complex interactions among the atmosphere, land surface, and the sea-<span class="hlt">ice</span>-covered Arctic Ocean. Observed changes in the Arctic have emerged and projected climate trends are of significant concern. Surface warming over the last few decades is nearly double that of the entire Earth. Reduced sea-<span class="hlt">ice</span> extent and volume, changes to ecosystems, and melting permafrost are some examples of noticeable changes in the region. This work is aimed at improving our understanding of how Arctic clouds interact with, and influence, the surface budget, how clouds influence the distribution of sea <span class="hlt">ice</span>, and the role of downwelling longwave radiation (DLR) in climate change. In the first half of this study, we explore the roles of sea-<span class="hlt">ice</span> thickness and downwelling longwave radiation in Arctic amplification. As the Arctic sea <span class="hlt">ice</span> thins and ultimately disappears in a warming climate, its <span class="hlt">insulating</span> power decreases. This causes the surface air temperature to approach the temperature of the relatively warm ocean water below the <span class="hlt">ice</span>. The resulting increases in air temperature, water vapor and cloudiness lead to an increase in the surface downwelling longwave radiation, which enables a further thinning of the <span class="hlt">ice</span>. This positive <span class="hlt">ice-insulation</span> feedback operates mainly in the autumn and winter. A climate-change simulation with the Community Earth System Model shows that, averaged over the year, the increase in Arctic DLR is three times stronger than the increase in Arctic absorbed solar radiation at the surface. The warming of the surface air over the Arctic Ocean during fall and winter creates a strong thermal contrast with the colder surrounding continents. Sea-level pressure falls over the Arctic Ocean and the high-latitude circulation reorganizes into a shallow "winter monsoon." The resulting increase in surface wind speed promotes stronger surface evaporation and higher humidity over portions of the Arctic Ocean, thus reinforcing the <span class="hlt">ice-insulation</span> feedback</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20130012459','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20130012459"><span>Thermal Performance Testing of Order Dependancy of Aerogels Multilayered <span class="hlt">Insulation</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Johnson, Wesley L.; Fesmire, James E.; Demko, J. A.</p> <p>2009-01-01</p> <p>Robust multilayer <span class="hlt">insulation</span> systems have long been a goal of many research projects. Such <span class="hlt">insulation</span> systems must provide some degree of structural support and also mechanical integrity during loss of vacuum scenarios while continuing to provide <span class="hlt">insulative</span> value to the vessel. Aerogel <span class="hlt">composite</span> blankets can be the best <span class="hlt">insulation</span> materials in ambient pressure environments; in high vacuum, the thermal performance of aerogel improves by about one order of magnitude. Standard multilayer <span class="hlt">insulation</span> (MU) is typically 50% worse at ambient pressure and at soft vacuum, but as much as two or three orders of magnitude better at high vacuum. Different combinations of aerogel and multilayer <span class="hlt">insulation</span> systems have been tested at Cryogenics Test Laboratory of NASA Kennedy Space Center. Analysis performed at Oak Ridge National Laboratory showed an importance to the relative location of the MU and aerogel blankets. Apparent thermal conductivity testing under cryogenic-vacuum conditions was performed to verify the analytical conclusion. Tests results are shown to be in agreement with the analysis which indicated that the best performance is obtained with aerogel layers located in the middle of the blanket <span class="hlt">insulation</span> system.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016DSRII.125..191D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016DSRII.125..191D"><span>A shape and <span class="hlt">compositional</span> analysis of <span class="hlt">ice</span>-rafted debris in cores from IODP Expedition 323 in the Bering Sea</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dadd, Kelsie; Foley, Kristen</p> <p>2016-03-01</p> <p>Sediment cores recovered during IODP Expedition 323 in the Bering Sea, northern Pacific, contained numerous <span class="hlt">ice</span>-rafted debris (IRD) clasts up to 85 mm in length. The physical properties (including roundness and sphericity) of 136 clasts from the working half of the cores, a subsample of the total clast number, were analysed and their <span class="hlt">composition</span> determined using standard petrographic techniques. After removal of pumice and possible fall-in derived material from the clast population, a total of 86 clasts from the original collection were considered to be IRD. While roundness and sphericity vary greatly in the clast population, the IRD are predominately discoid in shape with oblate/prolate indices typically between -5 and 5. There are four time periods over the approximately 4.5 Ma sample interval, 0.36-0.67 Ma, 0.82-1.06 Ma 1.54-1.77 Ma and >3.28 Ma, where there are no IRD in the sample set for sites of the Bering slope, suggesting that these times may have been <span class="hlt">ice</span>-free. Most clasts show some rounding and are likely to have spent time on beaches with wave action. Wave action on beaches suggests periods of no <span class="hlt">ice</span> or only seasonal sea-<span class="hlt">ice</span>. The low roundness values of other clasts, however, suggest they underwent little working and, therefore, the presence of glaciers or more permanent sea-<span class="hlt">ice</span> at times in those locations. The abundance of rounded and unfaceted clasts as IRD suggests a lack of large <span class="hlt">ice</span> sheets in the area during cool periods. Clast <span class="hlt">composition</span> of the IRD is divided into four broad groups, basalt and andesite, granite and metamorphic, sedimentary, and felsic volcanic. The granite and metamorphic and more mature sedimentary lithologies are most likely derived from the Alaskan continental margin, while the extrusive igneous clasts could be derived from a variety of volcanic sources surrounding the Bering Sea, both emergent now or emergent at times of lower sea level. There is only a poor correlation with IRD abundance and marine isotope stages (MIS) for</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018BGeo...15.3331N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018BGeo...15.3331N"><span>CO2 flux over young and snow-covered Arctic pack <span class="hlt">ice</span> in winter and spring</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nomura, Daiki; Granskog, Mats A.; Fransson, Agneta; Chierici, Melissa; Silyakova, Anna; Ohshima, Kay I.; Cohen, Lana; Delille, Bruno; Hudson, Stephen R.; Dieckmann, Gerhard S.</p> <p>2018-06-01</p> <p>Rare CO2 flux measurements from Arctic pack <span class="hlt">ice</span> show that two types of <span class="hlt">ice</span> contribute to the release of CO2 from the <span class="hlt">ice</span> to the atmosphere during winter and spring: young, thin <span class="hlt">ice</span> with a thin layer of snow and older (several weeks), thicker <span class="hlt">ice</span> with thick snow cover. Young, thin sea <span class="hlt">ice</span> is characterized by high salinity and high porosity, and snow-covered thick <span class="hlt">ice</span> remains relatively warm ( > -7.5 °C) due to the <span class="hlt">insulating</span> snow cover despite air temperatures as low as -40 °C. Therefore, brine volume fractions of these two <span class="hlt">ice</span> types are high enough to provide favorable conditions for gas exchange between sea <span class="hlt">ice</span> and the atmosphere even in mid-winter. Although the potential CO2 flux from sea <span class="hlt">ice</span> decreased due to the presence of the snow, the snow surface is still a CO2 source to the atmosphere for low snow density and thin snow conditions. We found that young sea <span class="hlt">ice</span> that is formed in leads without snow cover produces CO2 fluxes an order of magnitude higher than those in snow-covered older <span class="hlt">ice</span> (+1.0 ± 0.6 mmol C m-2 day-1 for young <span class="hlt">ice</span> and +0.2 ± 0.2 mmol C m-2 day-1 for older <span class="hlt">ice</span>).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-PIA19712.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-PIA19712.html"><span>Pluto: The <span class="hlt">Ice</span> Plot Thickens</span></a></p> <p><a target="_blank" href="https://images.nasa.gov/">NASA Image and Video Library</a></p> <p></p> <p>2015-07-15</p> <p>The latest spectra from New Horizons Ralph instrument reveal an abundance of methane <span class="hlt">ice</span>, but with striking differences from place to place across the frozen surface of Pluto. In the north polar cap, methane <span class="hlt">ice</span> is diluted in a thick, transparent slab of nitrogen <span class="hlt">ice</span> resulting in strong absorption of infrared light. In one of the visually dark equatorial patches, the methane <span class="hlt">ice</span> has shallower infrared absorptions indicative of a very different texture. An Earthly example of different textures of a frozen substance: a fluffy bank of clean snow is bright white, but compacted polar <span class="hlt">ice</span> looks blue. New Horizons' surface <span class="hlt">composition</span> team has begun the intricate process of analyzing Ralph data to determine the detailed <span class="hlt">compositions</span> of the distinct regions on Pluto. This is the first detailed image of Pluto from the Linear Etalon Imaging Spectral Array, part of the Ralph instrument on New Horizons. The observations were made at three wavelengths of infrared light, which are invisible to the human eye. In this picture, blue corresponds to light of wavelengths 1.62 to 1.70 micrometers, a channel covering a medium-strong absorption band of methane <span class="hlt">ice</span>, green (1.97 to 2.05 micrometers) represents a channel where methane <span class="hlt">ice</span> does not absorb light, and red (2.30 to 2.33 micrometers) is a channel where the light is very heavily absorbed by methane <span class="hlt">ice</span>. The two areas outlined on Pluto show where Ralph observations obtained the spectral traces at the right. Note that the methane absorptions (notable dips) in the spectrum from the northern region are much deeper than the dips in the spectrum from the dark patch. The Ralph data were obtained by New Horizons on July 12, 2015. http://photojournal.jpl.nasa.gov/catalog/PIA19712</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008IJTPE.128..690O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008IJTPE.128..690O"><span>Study on <span class="hlt">Insulation</span> Diagnosis of Power Lines in Apartment Houses</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Okamoto, Tatsuki; Taki, Shoji; Fukui, Toshiaki; Soga, Akiya; Ezure, Shoichiro; Asano, Jun-Ichi; Uto, Yukio</p> <p></p> <p><span class="hlt">Insulation</span> diagnosis is vital issue for safety of urban lives despite of the difficulty of power interruption even for the diagnosis. Recently, live-line <span class="hlt">insulation</span> diagnosis becomes more important and realistic to maintain good <span class="hlt">insulation</span> conditions of power lines in apartment houses in wide range of residential sizes. This <span class="hlt">paper</span> describes new trend of <span class="hlt">insulation</span> diagnosis of power lines of apartment houses based on clip-on current measurement method with a lot of live-line measurement data and also describes the applicability of new live-line <span class="hlt">insulation</span> diagnostic method.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20100022136&hterms=Space+Liquid&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3DSpace%2BLiquid','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20100022136&hterms=Space+Liquid&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3DSpace%2BLiquid"><span>Space Shuttle Main Engine Liquid Air <span class="hlt">Insulation</span> Redesign Lessons Learned</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Gaddy, Darrell; Carroll, Paul; Head, Kenneth; Fasheh, John; Stuart, Jessica</p> <p>2010-01-01</p> <p>The Space Shuttle Main Engine Liquid Air <span class="hlt">Insulation</span> redesign was required to prevent the reoccurance of the STS-111 High Pressure Speed Sensor In-Flight Anomaly. The STS-111 In-Flight Anomaly Failure Investigation Team's initial redesign of the High Pressure Fuel Turbopump Pump End Ball Bearing Liquid Air <span class="hlt">Insulation</span> failed the certification test by producing Liquid Air. The certification test failure indicated not only the High Pressure Fuel Turbopump Liquid Air <span class="hlt">Insulation</span>, but all other Space Shuttle Main Engine Liquid Air <span class="hlt">Insulation</span>. This <span class="hlt">paper</span> will document the original Space Shuttle Main Engine Liquid Air STS-111 In-Flight Anomaly investigation, the heritage Space Shuttle Main Engine <span class="hlt">Insulation</span> certification testing faults, the techniques and instrumentation used to accurately test the Liquid Air <span class="hlt">Insulation</span> systems on the Stennis Space Center SSME test stand, the analysis techniques used to identify the Liquid Air <span class="hlt">Insulation</span> problem areas and the analytical verification of the redesign before entering certification testing, Trade study down selected to three potential design solutions, the results of the development testing which down selected the final Liquid Air Redesign are also documented within this <span class="hlt">paper</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA601202','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA601202"><span>Seasonal <span class="hlt">Ice</span> Zone Reconnaissance Surveys Coordination</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2013-09-30</p> <p>of SIZRS are covered in separate reports. Our long-term goal is to track and understand the interplay among the <span class="hlt">ice</span>, atmosphere, and ocean...OMB control number. 1. REPORT DATE 30 SEP 2013 2. REPORT TYPE 3. DATES COVERED 00-00-2013 to 00-00-2013 4. TITLE AND SUBTITLE Seasonal <span class="hlt">Ice</span> Zone...sensing resources include MODIS visible and IR imagery, NSIDC <span class="hlt">ice</span> extent charts based on a <span class="hlt">composite</span> of passive microwave products (http://nsidc.org</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20030014602&hterms=tile&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dtile','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20030014602&hterms=tile&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dtile"><span>Reusable Surface <span class="hlt">Insulation</span> Tile Thermal Protection Materials: Past, Present and the Future</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Leiser, Daniel B.; Stewart, David A.; Venkatapathy, Ethiras (Technical Monitor)</p> <p>2002-01-01</p> <p>Silica (LI-900) Reusable Surface <span class="hlt">Insulation</span> (RSI) tile have been used on the majority of the Shuttle since its initial flight. Its overall performance with Reaction Cured Glass (RCG) coating applied will be reviewed. Improvements in <span class="hlt">insulations</span>, Fibrous Refractory <span class="hlt">Composite</span> <span class="hlt">Insulation</span> (FRCI-12) and Alumina Enhanced Thermal Barrier (AETB-8) and coatings/surface treatments such as Toughened Uni-Piece Fibrous <span class="hlt">Insulation</span> (TUFI) have been developed and successfully applied. The performance of these enhancements on the Shuttle Orbiters over the past few years along with the next version of tile materials, High Efficiency Tantalum-based Ceramic (HETC) with even broader applicability will also be discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1176549','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/servlets/purl/1176549"><span>Heat <span class="hlt">insulating</span> system for a fast reactor shield slab</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Kotora Jr., James; Groh, Edward F.; Kann, William J.; Burelbach, James P.</p> <p>1986-04-01</p> <p>Improved thermal <span class="hlt">insulation</span> for a nuclear reactor deck comprising many helical coil springs disposed in generally parallel, side-by-side laterally overlapping or interfitted relationship to one another so as to define a three-dimensional <span class="hlt">composite</span> having both metal and voids between the metal, and enclosure means for holding the <span class="hlt">composite</span> to the underside of the deck.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li class="active"><span>14</span></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_14 --> <div id="page_15" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li class="active"><span>15</span></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="281"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/875214','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/servlets/purl/875214"><span>Heat <span class="hlt">insulating</span> system for a fast reactor shield slab</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Kotora, Jr., James; Groh, Edward F.; Kann, William J.; Burelbach, James P.</p> <p>1986-01-01</p> <p>Improved thermal <span class="hlt">insulation</span> for a nuclear reactor deck comprising many helical coil springs disposed in generally parallel, side-by-side laterally overlapping or interfitted relationship to one another so as to define a three-dimensional <span class="hlt">composite</span> having both metal and voids between the metal, and enclosure means for holding the <span class="hlt">composite</span> to the underside of the deck.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/6130289','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/biblio/6130289"><span>Heat <span class="hlt">insulating</span> system for a fast reactor shield slab</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Kotora, J. Jr.; Groh, E.F.; Kann, W.J.; Burelbach, J.P.</p> <p>1984-04-10</p> <p>Improved thermal <span class="hlt">insulation</span> for a nuclear reactor deck comprises many helical coil springs disposed in generally parallel, side-by-side laterally overlapping or interfitted relationship to one another so as to define a three-dimensional <span class="hlt">composite</span> having both metal and voids between the metal, and enclosure means for holding the <span class="hlt">composite</span> to the underside of the deck.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.A34E..01W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.A34E..01W"><span>A detailed study of <span class="hlt">ice</span> nucleation by feldspar minerals</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Whale, T. F.; Murray, B. J.; Wilson, T. W.; Carpenter, M. A.; Harrison, A.; Holden, M. A.; Vergara Temprado, J.; Morris, J.; O'Sullivan, D.</p> <p>2015-12-01</p> <p>Immersion mode heterogeneous <span class="hlt">ice</span> nucleation plays a crucial role in controlling the <span class="hlt">composition</span> of mixed phase clouds, which contain both supercooled liquid water and <span class="hlt">ice</span> particles. The amount of <span class="hlt">ice</span> in mixed phase clouds can affect cloud particle size, lifetime and extent and so affects radiative properties and precipitation. Feldspar minerals are probably the most important minerals for <span class="hlt">ice</span> nucleation in mixed phase clouds because they nucleate <span class="hlt">ice</span> more efficiently than other components of atmospheric mineral dust (Atkinson et al. 2013). The feldspar class of minerals is complex, containing numerous chemical <span class="hlt">compositions</span>, several crystal polymorphs and wide variations in microscopic structure. Here we present the results of a study into <span class="hlt">ice</span> nucleation by a wide range of different feldspars. We found that, in general, alkali feldspars nucleate <span class="hlt">ice</span> more efficiently than plagioclase feldspars. However, we also found that particular alkali feldspars nucleate <span class="hlt">ice</span> relatively inefficiently, suggesting that chemical <span class="hlt">composition</span> is not the only important factor that dictates the <span class="hlt">ice</span> nucleation efficiency of feldspar minerals. <span class="hlt">Ice</span> nucleation by feldspar is described well by the singular model and is probably site specific in nature. The alkali feldspars that do not nucleate <span class="hlt">ice</span> efficiently possess relatively homogenous structure on the micrometre scale suggesting that the important sites for nucleation are related to surface topography. <span class="hlt">Ice</span> nucleation active site densities for the majority of tested alkali feldspars are similar to those found by Atkinson et al (2013), meaning that the validity of global aerosol modelling conducted in that study is not affected. Additionally, we have found that <span class="hlt">ice</span> nucleation by feldspars is strongly influenced, both positively and negatively, by the solute content of droplets. Most other nucleants we have tested are unaffected by solutes. This provides insight into the mechanism of <span class="hlt">ice</span> nucleation by feldspars and could be of importance</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5951378','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5951378"><span>Ageing Study of Palm Oil and Coconut Oil in the Presence of <span class="hlt">Insulation</span> <span class="hlt">Paper</span> for Transformers Application</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Mohamad, Nur Aqilah; Azis, Norhafiz; Jasni, Jasronita; Yunus, Robiah; Yaakub, Zaini</p> <p>2018-01-01</p> <p>This <span class="hlt">paper</span> presents a sealed ageing study of palm oil (PO) and coconut oil (CO) in the presence of <span class="hlt">insulation</span> <span class="hlt">paper</span>. The type of PO under study is refined, bleached, and deodorized palm oil (RBDPO) olein. Three different variations of RBDPO and one sample of CO are aged at temperatures of 90 °C, 110 °C, and 130 °C. The properties of RBDPO and CO as well as <span class="hlt">paper</span> under ageing are then analysed through dielectric and physicochemical measurements. It is found that the effect of ageing is not significant on the alternating current (AC) breakdown voltages and relative permittivities of RBDPO and CO. There is a slight increment trend of the resistivity for CO, while for all of the RBDPO, the resistivity slightly decreases as the ageing progresses. Only CO shows an apparent reduction of the dielectric dissipation factor. Throughout the ageing time, the acidities of all of the RBDPO and CO remain at low level, while the moisture in oils decreases. The tensile index (TI) of the <span class="hlt">papers</span> for all of the RBDPO and CO retain more than 50% of the TI. A significant increment of the <span class="hlt">paper</span> ageing rates of all of the RBDPO and CO is observed at an ageing temperature of 130 °C. PMID:29601520</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29601520','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29601520"><span>Ageing Study of Palm Oil and Coconut Oil in the Presence of <span class="hlt">Insulation</span> <span class="hlt">Paper</span> for Transformers Application.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Mohamad, Nur Aqilah; Azis, Norhafiz; Jasni, Jasronita; Ab Kadir, Mohd Zainal Abidin; Yunus, Robiah; Yaakub, Zaini</p> <p>2018-03-30</p> <p>This <span class="hlt">paper</span> presents a sealed ageing study of palm oil (PO) and coconut oil (CO) in the presence of <span class="hlt">insulation</span> <span class="hlt">paper</span>. The type of PO under study is refined, bleached, and deodorized palm oil (RBDPO) olein. Three different variations of RBDPO and one sample of CO are aged at temperatures of 90 °C, 110 °C, and 130 °C. The properties of RBDPO and CO as well as <span class="hlt">paper</span> under ageing are then analysed through dielectric and physicochemical measurements. It is found that the effect of ageing is not significant on the alternating current (AC) breakdown voltages and relative permittivities of RBDPO and CO. There is a slight increment trend of the resistivity for CO, while for all of the RBDPO, the resistivity slightly decreases as the ageing progresses. Only CO shows an apparent reduction of the dielectric dissipation factor. Throughout the ageing time, the acidities of all of the RBDPO and CO remain at low level, while the moisture in oils decreases. The tensile index (TI) of the <span class="hlt">papers</span> for all of the RBDPO and CO retain more than 50% of the TI. A significant increment of the <span class="hlt">paper</span> ageing rates of all of the RBDPO and CO is observed at an ageing temperature of 130 °C.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.P43E..03P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.P43E..03P"><span>On Organic Material in E Ring <span class="hlt">Ice</span> Grains</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Postberg, F.; Khawaja, N.; Reviol, R.; Nölle, L.; Klenner, F.; Hsu, H. W.; Horanyi, M.</p> <p>2015-12-01</p> <p>Pure water <span class="hlt">ice</span> dominates the <span class="hlt">composition</span> of the micron and sub-micron sized dust particles in Saturn's E-ring, a ring constantly replenished by active <span class="hlt">ice</span> jets of the moon Enceladus [1]. Details about the <span class="hlt">composition</span> of this tenuous, optically thin ring can only be constrained by in situ measurements. The Cosmic Dust Analyzer (CDA) onboard Cassini investigates the <span class="hlt">composition</span> of these grains by cationic time-of-flight mass spectra of individual <span class="hlt">ice</span> grains hitting the instruments target surface. From these spectra three <span class="hlt">compositional</span> types of E ring <span class="hlt">ice</span> grains have been identified previously [2,3]: Type-1: Almost pure water, Type-2: Enriched in organics, and Type-3: Enriched in salt. Unlike Type-1 and 3, organic-enriched Type-2 spectra have not yet been investigated in depth. Here we report the first detailed <span class="hlt">compositional</span> analysis of this type. The spectra analysis is supported by a large-scale laboratory ground campaign yielding a library of analogue spectra for organic material embedded in a water <span class="hlt">ice</span> matrix. In contrast to Type 1 and 3, Type-2 spectra display a great <span class="hlt">compositional</span> diversity, which indicates varying contributions of several organic species. So far we have identified characteristic fragment patterns of at least three classes of organic compounds: aromatic species, amines, and carbonyl group species. Work is in progress to quantify concentrations of the identified species and to assign yet un-specified organic mass lines in Type 2 spectra. Due to the dynamical evolution of the orbital elements of E ring grains a large fraction collides with the icy moons embedded in the E ring. Therefore, the organic components identified by CDA can accumulate on the surfaces of these bodies over time. Ref: :[1]Kempf et al., Icarus-206, 2010. [2]Postberg et al., Nature-459, 2009. [3]Postberg et al., Icarus-193, 2008.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20160006877','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20160006877"><span>The Effect of Surface Chemical Functionality Upon <span class="hlt">Ice</span> Adhesion</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Smith, Joseph G., Jr.; Wohl, Christopher J.; Doss, Jereme; Spence, Destiny; Kreeger, Richard E.; Palacios, Jose; Knuth, Taylor; Hadley, Kevin R.; McDougal, Nicholas D.</p> <p>2015-01-01</p> <p>In nature, anti-freeze proteins present in fish utilize specific organic functionalities to disrupt <span class="hlt">ice</span> crystal formation and propagation. Based on these structures, surfaces with controlled chemical functionality and chain length were evaluated both experimentally and computationally to assess the effect of both parameters in mitigating <span class="hlt">ice</span> formation. Linear aliphatic dimethylethoxysilanes terminated with methyl or hydroxyl groups were prepared, characterized, and used to coat aluminum. The effect upon <span class="hlt">icing</span> using a microdroplet freezing apparatus and the Adverse Environment Rotor Test Stand found hydroxyl-terminated materials exhibited a greater propensity for <span class="hlt">ice</span> formation and adhesion. Molecular dynamics simulations of a silica substrate bearing functionalized species of similar <span class="hlt">composition</span> were brought into contact with a pre-equilibrated <span class="hlt">ice</span> crystal. Several parameters including chain mobility were monitored to ascertain the size of a quasi-liquid layer. The studies suggested that chain mobility affected the interface between <span class="hlt">ice</span> and the surface more than terminal group chemical <span class="hlt">composition</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017MS%26E..209a2093D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017MS%26E..209a2093D"><span>Designing Predictive Diagnose Method for <span class="hlt">Insulation</span> Resistance Degradation of the Electrical Power Cables from Neutral <span class="hlt">Insulated</span> Power Networks</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dobra, R.; Pasculescu, D.; Risteiu, M.; Buica, G.; Jevremović, V.</p> <p>2017-06-01</p> <p>This <span class="hlt">paper</span> describe some possibilities to minimize voltages switching-off risks from the mining power networks, in case of <span class="hlt">insulated</span> resistance faults by using a predictive diagnose method. The cables from the neutral <span class="hlt">insulated</span> power networks (underground mining) are designed to provide a flexible electrical connection between portable or mobile equipment and a point of supply, including main feeder cable for continuous miners, pump cable, and power supply cable. An electronic protection for <span class="hlt">insulated</span> resistance of mining power cables can be made using this predictive strategy. The main role of electronic relays for <span class="hlt">insulation</span> resistance degradation of the electrical power cables, from neutral <span class="hlt">insulated</span> power networks, is to provide a permanent measurement of the <span class="hlt">insulated</span> resistance between phases and ground, in order to switch-off voltage when the resistance value is below a standard value. The automat system of protection is able to signalize the failure and the human operator will be early informed about the switch-off power and will have time to take proper measures to fix the failure. This logic for fast and automat switch-off voltage without aprioristic announcement is suitable for the electrical installations, realizing so a protection against fires and explosion. It is presented an algorithm and an anticipative relay for <span class="hlt">insulated</span> resistance control from three-phase low voltage installations with <span class="hlt">insulated</span> neutral connection.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/6354215-advances-ice-mechanics','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/6354215-advances-ice-mechanics"><span>Advances in <span class="hlt">ice</span> mechanics - 1987</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Chung, J.S.; Hallam, S.D.; Maatanen, M.</p> <p>1987-01-01</p> <p>This book presents the <span class="hlt">papers</span> given at a symposium on the interaction of icebergs with offshore platforms. Topics considered at the symposium included advances in <span class="hlt">ice</span> mechanics in the United Kingdom, <span class="hlt">ice</span> mechanics in Finland, recent advances in <span class="hlt">ice</span> mechanics in Canada, advances in sea <span class="hlt">ice</span> mechanics in the USA, foundations, monitoring, hazards, risk assessment, and deformation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20080005121','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20080005121"><span>Microsphere <span class="hlt">insulation</span> systems</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Allen, Mark S. (Inventor); Willen, Gary S. (Inventor); Mohling, Robert A. (Inventor)</p> <p>2005-01-01</p> <p>A new <span class="hlt">insulation</span> system is provided that contains microspheres. This <span class="hlt">insulation</span> system can be used to provide <span class="hlt">insulated</span> panels and clamshells, and to <span class="hlt">insulate</span> annular spaces around objects used to transfer, store, or transport cryogens and other temperature-sensitive materials. This <span class="hlt">insulation</span> system provides better performance with reduced maintenance than current <span class="hlt">insulation</span> systems.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24579057','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24579057"><span>Bacterial <span class="hlt">ice</span> crystal controlling proteins.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Lorv, Janet S H; Rose, David R; Glick, Bernard R</p> <p>2014-01-01</p> <p>Across the world, many <span class="hlt">ice</span> active bacteria utilize <span class="hlt">ice</span> crystal controlling proteins for aid in freezing tolerance at subzero temperatures. <span class="hlt">Ice</span> crystal controlling proteins include both antifreeze and <span class="hlt">ice</span> nucleation proteins. Antifreeze proteins minimize freezing damage by inhibiting growth of large <span class="hlt">ice</span> crystals, while <span class="hlt">ice</span> nucleation proteins induce formation of embryonic <span class="hlt">ice</span> crystals. Although both protein classes have differing functions, these proteins use the same <span class="hlt">ice</span> binding mechanisms. Rather than direct binding, it is probable that these protein classes create an <span class="hlt">ice</span> surface prior to <span class="hlt">ice</span> crystal surface adsorption. Function is differentiated by molecular size of the protein. This <span class="hlt">paper</span> reviews the similar and different aspects of bacterial antifreeze and <span class="hlt">ice</span> nucleation proteins, the role of these proteins in freezing tolerance, prevalence of these proteins in psychrophiles, and current mechanisms of protein-<span class="hlt">ice</span> interactions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.A43F0302B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.A43F0302B"><span>Development of a balloon-borne device for analysis of high-altitude <span class="hlt">ice</span> and aerosol particulates: <span class="hlt">Ice</span> Cryo Encapsulator by Balloon (<span class="hlt">ICE</span>-Ball)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Boaggio, K.; Bandamede, M.; Bancroft, L.; Hurler, K.; Magee, N. B.</p> <p>2016-12-01</p> <p>We report on details of continuing instrument development and deployment of a novel balloon-borne device for capturing and characterizing atmospheric <span class="hlt">ice</span> and aerosol particles, the <span class="hlt">Ice</span> Cryo Encapsulator by Balloon (<span class="hlt">ICE</span>-Ball). The device is designed to capture and preserve cirrus <span class="hlt">ice</span> particles, maintaining them at cold equilibrium temperatures, so that high-altitude particles can recovered, transferred intact, and then imaged under SEM at an unprecedented resolution (approximately 3 nm maximum resolution). In addition to cirrus <span class="hlt">ice</span> particles, high altitude aerosol particles are also captured, imaged, and analyzed for geometry, chemical <span class="hlt">composition</span>, and activity as <span class="hlt">ice</span> nucleating particles. Prototype versions of <span class="hlt">ICE</span>-Ball have successfully captured and preserved high altitude <span class="hlt">ice</span> particles and aerosols, then returned them for recovery and SEM imaging and analysis. New improvements include 1) ability to capture particles from multiple narrowly-defined altitudes on a single payload, 2) high quality measurements of coincident temperature, humidity, and high-resolution video at capture altitude, 3) ability to capture particles during both ascent and descent, 4) better characterization of particle collection volume and collection efficiency, and 5) improved isolation and characterization of capture-cell cryo environment. This presentation provides detailed capability specifications for anyone interested in using measurements, collaborating on continued instrument development, or including this instrument in ongoing or future field campaigns.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19740002610','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19740002610"><span>Reliability and effective thermal conductivity of three metallic-ceramic <span class="hlt">composite</span> <span class="hlt">insulating</span> coatings on cooled hydrogen-oxygen rockets</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Price, H. G., Jr.; Schacht, R. L.; Quentmeyer, R. J.</p> <p>1973-01-01</p> <p>An experimental investigation of the structural integrity and effective thermal conductivity of three metallic-ceramic <span class="hlt">composite</span> coatings was conducted. These coatings were plasma sprayed onto the combustion side of water-cooled, 12.7-centimeter throat diameter, hydrogen-oxygen rocket thrust chambers operating at 2.07 to 4.14 meganewtons per square meter chamber pressure. The metallic-ceramic <span class="hlt">composites</span> functioned for six to 17 cycles and for as long as 213 seconds of rocket operations and could have probably provided their <span class="hlt">insulating</span> properties for many additional cycles. The effective thermal conductivity of all the coatings was in the range of 0.7472 to 4.483 w/(m)(K), which makes the coatings a very effective thermal barrier. Photomicrographic studies of cross-sectioned coolant tubes seem to indicate that the effective thermal conductivity of the coatings is controlled by contact resistance between the particles, as a result of the spraying process, and not the thermal conductivity of the bulk materials.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C33B1185F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C33B1185F"><span>The role of feedbacks in Antarctic sea <span class="hlt">ice</span> change</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Feltham, D. L.; Frew, R. C.; Holland, P.</p> <p>2017-12-01</p> <p>The changes in Antarctic sea <span class="hlt">ice</span> over the last thirty years have a strong seasonal dependence, and the way these changes grow in spring and decay in autumn suggests that feedbacks are strongly involved. The changes may ultimately be caused by atmospheric warming, the winds, snowfall changes, etc., but we cannot understand these forcings without first untangling the feedbacks. A highly simplified coupled sea <span class="hlt">ice</span> -mixed layer model has been developed to investigate the importance of feedbacks on the evolution of sea <span class="hlt">ice</span> in two contrasting regions in the Southern Ocean; the Amundsen Sea where sea <span class="hlt">ice</span> extent has been decreasing, and the Weddell Sea where it has been expanding. The change in mixed layer depth in response to changes in the atmosphere to ocean energy flux is implicit in a strong negative feedback on <span class="hlt">ice</span> cover changes in the Amundsen Sea, with atmospheric cooling leading to a deeper mixed layer resulting in greater entrainment of warm Circumpolar Deep Water, causing increased basal melting of sea <span class="hlt">ice</span>. This strong negative feedback produces counter intuitive responses to changes in forcings in the Amundsen Sea. This feedback is absent in the Weddell due to the complete destratification and strong water column cooling that occurs each winter in simulations. The impact of other feedbacks, including the albedo feedback, changes in <span class="hlt">insulation</span> due to <span class="hlt">ice</span> thickness and changes in the freezing temperature of the mixed layer, were found to be of secondary importance compared to changes in the mixed layer depth.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JHyDy..30..336W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JHyDy..30..336W"><span>Revisit submergence of <span class="hlt">ice</span> blocks in front of <span class="hlt">ice</span> cover—an experimental study</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wang, Jun; Wu, Yi-fan; Sui, Jueyi</p> <p>2018-04-01</p> <p>The present <span class="hlt">paper</span> studies the stabilities of <span class="hlt">ice</span> blocks in front of an <span class="hlt">ice</span> cover based on experiments carried out in laboratory by using four types of <span class="hlt">ice</span> blocks with different dimensions. The forces acting on the <span class="hlt">ice</span> blocks in front of the <span class="hlt">ice</span> cover are analyzed. The critical criteria for the entrainment of <span class="hlt">ice</span> blocks in front of the <span class="hlt">ice</span> cover are established by considering the drag force caused by the flowing water, the collision force, and the hydraulic pressure force. Formula for determining whether or not an <span class="hlt">ice</span> block will be entrained under the <span class="hlt">ice</span> cover is derived. All three dimensions of the <span class="hlt">ice</span> block are considered in the proposed formula. The velocities calculated by using the developed formula are compared with those of calculated by other formulas proposed by other researchers, as well as the measured flow velocities for the entrainment of <span class="hlt">ice</span> blocks in laboratory. The fitting values obtained by using the derived formula agree well with the experimental results.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5455717','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5455717"><span>Seismic Experimental Study on New-Type <span class="hlt">Composite</span> Exterior Wallboard with Integrated Structural Function and <span class="hlt">Insulation</span></span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Ma, Shaochun; Jiang, Nan</p> <p>2015-01-01</p> <p>In order to evaluate the seismic performance of new-type <span class="hlt">composite</span> exterior wallboard, a total of six exterior and interior wallboards were incorporated in the experiment of seismic performance. Seismic performance such as the stress process, damage mode, hysteresis and skeleton curve, load-carrying and ductility coefficient, damping and energy dissipation, stiffness degradation as well as material strain of the exterior wallboards were analyzed with emphasis and compared with interior wallboards. Results of the experiment and analysis showed that both interior and exterior wallboards exhibited outstanding seismic performance. Due to the existence of <span class="hlt">insulation</span> layer and externally bonded single gypsum board, the capacity of elastoplastic deformation and seismic energy dissipation of the exterior wallboards was improved and each seismic performance indicator of the exterior wallboards outperformed the interior wallboards.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1990STIN...9119981B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1990STIN...9119981B"><span>Thermal <span class="hlt">insulation</span> of a cryogenic tank for a space telescope using a pretensioned suspension of Fiber Reinforced <span class="hlt">Composite</span> (FRC)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bongers, Bernd; Haider, Otmar; Tauber, Wolfgang</p> <p>1990-09-01</p> <p>For the thermal <span class="hlt">insulation</span> of cryogenic tanks in satellite applications Fiber Reinforced <span class="hlt">Composite</span> (FRC) materials are preferable because of their low thermal conductivity and high tensile strength compared to metallic materials. At the Infrared Space Observatory (ISO) satellite the main Liquid Helium (LHe) tank is suspended by one spatial framework and eight pretensioned chain strands at each side. Frameworks and chain strands are acting as a thermal barrier and therefore made of FRC. To meet the various and, in parts contractive requirements, sophisticated design approaches are chosen for the structural parts.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29072120','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29072120"><span>LCA of an <span class="hlt">ice</span> cream cup of polyethylene coated <span class="hlt">paper</span>: how does the choice of the end-of-life affect the results?</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Buccino, Carla; Ferrara, Carmen; Malvano, Carmela; De Feo, Giovanni</p> <p>2017-11-07</p> <p>This study presents an evaluation of the environmental performance of an <span class="hlt">ice</span> cream cup made of polyethylene (PE)/<span class="hlt">paper</span> laminate using a life cycle assessment approach 'from cradle to grave'. Two opposite alternative disposal scenarios, as well as their intermediate combinations, were considered: 100% incineration and 100% landfilling. The environmental impacts were calculated using the EPD 2013 evaluation method since the study was developed in an Environmental Product Declaration perspective as well as the method ReCiPe 2008 H at the endpoint level. PE/<span class="hlt">paper</span> laminate production was the most impactful process since it provided the highest contribution to total impacts in four of six impact categories considered. <span class="hlt">Ice</span> cream cup production was the second impactful process. The 100% incineration scenario provided negligible contribution to life cycle total impact for all impact categories; while considering the landfilling scenario, the percentage contributions to the total impact provided by the end-of-life phase increased considerably, until to be comparable to the contributions provided by the production processes of the PE/<span class="hlt">paper</span> laminate and the <span class="hlt">ice</span> cream cup. The obtained results highlighted that different disposal scenarios can affect significantly the conclusions of a study. At the endpoint level, incineration was more environmentally sound than landfilling for all the ReCiPe damage categories.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20030025277&hterms=statistics&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3Dstatistics','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20030025277&hterms=statistics&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3Dstatistics"><span>Space/Time Statistics of Polar <span class="hlt">Ice</span> Motion</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Emery, William J.; Fowler, Charles; Maslanik, James A.</p> <p>2003-01-01</p> <p><span class="hlt">Ice</span> motions have been computed from passive microwave imagery (SMMR and SSM/I) on a daily basis for both Polar Regions. In the Arctic these daily motions have been merged with daily motions from AVHRR imagery and the Arctic buoy program. In the Antarctic motion only from the AVHRR were available for merging with the passive microwave vectors. Long-term means, monthly means and weekly means have all been computed from the resulting 22-year time series of polar <span class="hlt">ice</span> motion. <span class="hlt">Papers</span> are in preparation that present the long term (22 year) means, their variability and show animations of the monthly means over this time period for both Polar Regions. These <span class="hlt">papers</span> will have links to "enhanced objects" that allow the reader to view the animations as part of the <span class="hlt">paper</span>. The first <span class="hlt">paper</span> presents the <span class="hlt">ice</span> motion results from each of the Polar Regions. The second <span class="hlt">paper</span> looks only at <span class="hlt">ice</span> motion in the Arctic in order to develop a time series of <span class="hlt">ice</span> age in the Arctic. Starting with the first full SMMR year in 1979 we keep track of each individual "<span class="hlt">ice</span> element" (resolution of the sensor) and track it in the subsequent monthly time series. After a year we "age" each "particle" and we thus can keep track of the age of the <span class="hlt">ice</span> starting in 1979. We keep track of <span class="hlt">ice</span> age classes between one and five years and thus we can see the evolution of the <span class="hlt">ice</span> as it ages after the initial 5-year period. This calculation shows how we are losing the older <span class="hlt">ice</span> through Fram Strait at a rather alarming rate particularly in the past 15 years. This loss of older <span class="hlt">ice</span> has resulted in an overall decrease in the thickest, oldest <span class="hlt">ice</span>, which is now limited to a region just north of the Canadian Archipelago with tongues extending out across the pole towards the Siberian Shelf. This loss of old <span class="hlt">ice</span> is consistent with the effects of global warming which provides the heat needed to melt, move and disperse this oldest <span class="hlt">ice</span> through Fram Strait. This is the first step in a progression that may eventually open the Arctic</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016PhRvB..94k5104Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016PhRvB..94k5104Y"><span><span class="hlt">Composite</span> particle theory of three-dimensional gapped fermionic phases: Fractional topological <span class="hlt">insulators</span> and charge-loop excitation symmetry</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ye, Peng; Hughes, Taylor L.; Maciejko, Joseph; Fradkin, Eduardo</p> <p>2016-09-01</p> <p>Topological phases of matter are usually realized in deconfined phases of gauge theories. In this context, confined phases with strongly fluctuating gauge fields seem to be irrelevant to the physics of topological phases. For example, the low-energy theory of the two-dimensional (2D) toric code model (i.e., the deconfined phase of Z2 gauge theory) is a U(1 )×U(1 ) Chern-Simons theory in which gauge charges (i.e., e and m particles) are deconfined and the gauge fields are gapped, while the confined phase is topologically trivial. In this <span class="hlt">paper</span>, we point out a route to constructing exotic three-dimensional (3D) gapped fermionic phases in a confining phase of a gauge theory. Starting from a parton construction with strongly fluctuating compact U(1 )×U(1 ) gauge fields, we construct gapped phases of interacting fermions by condensing two linearly independent bosonic <span class="hlt">composite</span> particles consisting of partons and U(1 )×U(1 ) magnetic monopoles. This can be regarded as a 3D generalization of the 2D Bais-Slingerland condensation mechanism. Charge fractionalization results from a Debye-Hückel-type screening cloud formed by the condensed <span class="hlt">composite</span> particles. Within our general framework, we explore two aspects of symmetry-enriched 3D Abelian topological phases. First, we construct a new fermionic state of matter with time-reversal symmetry and Θ ≠π , the fractional topological <span class="hlt">insulator</span>. Second, we generalize the notion of anyonic symmetry of 2D Abelian topological phases to the charge-loop excitation symmetry (Charles ) of 3D Abelian topological phases. We show that line twist defects, which realize Charles transformations, exhibit non-Abelian fusion properties.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li class="active"><span>15</span></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_15 --> <div id="page_16" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li class="active"><span>16</span></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="301"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014PrAeS..64....1G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014PrAeS..64....1G"><span>Lightning strike protection of <span class="hlt">composites</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gagné, Martin; Therriault, Daniel</p> <p>2014-01-01</p> <p>Aircraft structures are being redesigned to use fiber-reinforced <span class="hlt">composites</span> mainly due to their high specific stiffness and strength. One of the main drawbacks from changing from electrically conductive metals to <span class="hlt">insulating</span> or semi-conducting <span class="hlt">composites</span> is the higher vulnerability of the aircraft to lightning strike damage. The current protection approach consists of bonding a metal mesh to the surface of the <span class="hlt">composite</span> structure, but this weight increase negatively impact the fuel efficiency. This review <span class="hlt">paper</span> presents an overview of the lightning strike problematic, the regulations, the lightning damage to <span class="hlt">composite</span>, the current protection solutions and other material or technology alternatives. Advanced materials such as polymer-based nanocomposites and carbon nanotube buckypapers are promising candidates for lightweight lightning strike protection technology.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-GSFC_20171208_Archive_e000258.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-GSFC_20171208_Archive_e000258.html"><span>NASA: First Map Of Thawed Areas Under Greenland <span class="hlt">Ice</span> Sheet</span></a></p> <p><a target="_blank" href="https://images.nasa.gov/">NASA Image and Video Library</a></p> <p></p> <p>2017-12-08</p> <p>NASA researchers have helped produce the first map showing what parts of the bottom of the massive Greenland <span class="hlt">Ice</span> Sheet are thawed – key information in better predicting how the <span class="hlt">ice</span> sheet will react to a warming climate. Greenland’s thick <span class="hlt">ice</span> sheet <span class="hlt">insulates</span> the bedrock below from the cold temperatures at the surface, so the bottom of the <span class="hlt">ice</span> is often tens of degrees warmer than at the top, because the <span class="hlt">ice</span> bottom is slowly warmed by heat coming from the Earth’s depths. Knowing whether Greenland’s <span class="hlt">ice</span> lies on wet, slippery ground or is anchored to dry, frozen bedrock is essential for predicting how this <span class="hlt">ice</span> will flow in the future, But scientists have very few direct observations of the thermal conditions beneath the <span class="hlt">ice</span> sheet, obtained through fewer than two dozen boreholes that have reached the bottom. Now, a new study synthesizes several methods to infer the Greenland <span class="hlt">Ice</span> Sheet’s basal thermal state –whether the bottom of the <span class="hlt">ice</span> is melted or not– leading to the first map that identifies frozen and thawed areas across the whole <span class="hlt">ice</span> sheet. Map caption: This first-of-a-kind map, showing which parts of the bottom of the Greenland <span class="hlt">Ice</span> Sheet are likely thawed (red), frozen (blue) or still uncertain (gray), will help scientists better predict how the <span class="hlt">ice</span> will flow in a warming climate. Credit: NASA Earth Observatory/Jesse Allen Read more: go.nasa.gov/2avKgl2 NASA image use policy. NASA Goddard Space Flight Center enables NASA’s mission through four scientific endeavors: Earth Science, Heliophysics, Solar System Exploration, and Astrophysics. Goddard plays a leading role in NASA’s accomplishments by contributing compelling scientific knowledge to advance the Agency’s mission. Follow us on Twitter Like us on Facebook Find us on Instagram</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4813916','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4813916"><span>Estimating Clothing Thermal <span class="hlt">Insulation</span> Using an Infrared Camera</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Lee, Jeong-Hoon; Kim, Young-Keun; Kim, Kyung-Soo; Kim, Soohyun</p> <p>2016-01-01</p> <p>In this <span class="hlt">paper</span>, a novel algorithm for estimating clothing <span class="hlt">insulation</span> is proposed to assess thermal comfort, based on the non-contact and real-time measurements of the face and clothing temperatures by an infrared camera. The proposed method can accurately measure the clothing <span class="hlt">insulation</span> of various garments under different clothing fit and sitting postures. The proposed estimation method is investigated to be effective to measure its clothing <span class="hlt">insulation</span> significantly in different seasonal clothing conditions using a paired t-test in 99% confidence interval. Temperatures simulated with the proposed estimated <span class="hlt">insulation</span> value show closer to the values of actual temperature than those with individual clothing <span class="hlt">insulation</span> values. Upper clothing’s temperature is more accurate within 3% error and lower clothing’s temperature is more accurate by 3.7%~6.2% error in indoor working scenarios. The proposed algorithm can reflect the effect of air layer which makes <span class="hlt">insulation</span> different in the calculation to estimate clothing <span class="hlt">insulation</span> using the temperature of the face and clothing. In future, the proposed method is expected to be applied to evaluate the customized passenger comfort effectively. PMID:27005625</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26808844','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26808844"><span>Off-<span class="hlt">Ice</span> Anaerobic Power Does Not Predict On-<span class="hlt">Ice</span> Repeated Shift Performance in Hockey.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Peterson, Ben J; Fitzgerald, John S; Dietz, Calvin C; Ziegler, Kevin S; Baker, Sarah E; Snyder, Eric M</p> <p>2016-09-01</p> <p>Peterson, BJ, Fitzgerald, JS, Dietz, CC, Ziegler, KS, Baker, SE, and Snyder, EM. Off-<span class="hlt">ice</span> anaerobic power does not predict on-<span class="hlt">ice</span> repeated shift performance in hockey. J Strength Cond Res 30(9): 2375-2381, 2016-Anaerobic power is a significant predictor of acceleration and top speed in team sport athletes. Historically, these findings have been applied to <span class="hlt">ice</span> hockey although recent research has brought their validity for this sport into question. As <span class="hlt">ice</span> hockey emphasizes the ability to repeatedly produce power, single bout anaerobic power tests should be examined to determine their ability to predict on-<span class="hlt">ice</span> performance. We tested whether conventional off-<span class="hlt">ice</span> anaerobic power tests could predict on-<span class="hlt">ice</span> acceleration, top speed, and repeated shift performance. Forty-five hockey players, aged 18-24 years, completed anthropometric, off-<span class="hlt">ice</span>, and on-<span class="hlt">ice</span> tests. Anthropometric and off-<span class="hlt">ice</span> testing included height, weight, body <span class="hlt">composition</span>, vertical jump, and Wingate tests. On-<span class="hlt">ice</span> testing consisted of acceleration, top speed, and repeated shift fatigue tests. Vertical jump (VJ) (r = -0.42; r = -0.58), Wingate relative peak power (WRPP) (r = -0.32; r = -0.43), and relative mean power (WRMP) (r = -0.34; r = -0.48) were significantly correlated (p ≤ 0.05) to on-<span class="hlt">ice</span> acceleration and top speed, respectively. Conversely, none of the off-<span class="hlt">ice</span> tests correlated with on-<span class="hlt">ice</span> repeated shift performance, as measured by first gate, second gate, or total course fatigue; VJ (r = 0.06; r = 0.13; r = 0.09), WRPP (r = 0.06; r = 0.14; r = 0.10), or WRMP (r = -0.10; r = -0.01; r = -0.01). Although conventional off-<span class="hlt">ice</span> anaerobic power tests predict single bout on-<span class="hlt">ice</span> acceleration and top speed, they neither predict the repeated shift ability of the player, nor are good markers for performance in <span class="hlt">ice</span> hockey.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3918373','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3918373"><span>Bacterial <span class="hlt">Ice</span> Crystal Controlling Proteins</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Lorv, Janet S. H.; Rose, David R.; Glick, Bernard R.</p> <p>2014-01-01</p> <p>Across the world, many <span class="hlt">ice</span> active bacteria utilize <span class="hlt">ice</span> crystal controlling proteins for aid in freezing tolerance at subzero temperatures. <span class="hlt">Ice</span> crystal controlling proteins include both antifreeze and <span class="hlt">ice</span> nucleation proteins. Antifreeze proteins minimize freezing damage by inhibiting growth of large <span class="hlt">ice</span> crystals, while <span class="hlt">ice</span> nucleation proteins induce formation of embryonic <span class="hlt">ice</span> crystals. Although both protein classes have differing functions, these proteins use the same <span class="hlt">ice</span> binding mechanisms. Rather than direct binding, it is probable that these protein classes create an <span class="hlt">ice</span> surface prior to <span class="hlt">ice</span> crystal surface adsorption. Function is differentiated by molecular size of the protein. This <span class="hlt">paper</span> reviews the similar and different aspects of bacterial antifreeze and <span class="hlt">ice</span> nucleation proteins, the role of these proteins in freezing tolerance, prevalence of these proteins in psychrophiles, and current mechanisms of protein-<span class="hlt">ice</span> interactions. PMID:24579057</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3081589','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3081589"><span><span class="hlt">ICE</span> SLURRY APPLICATIONS</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Kauffeld, M.; WANG, M. J.; Goldstein, V.; Kasza, K. E.</p> <p>2011-01-01</p> <p>The role of secondary refrigerants is expected to grow as the focus on the reduction of greenhouse gas emissions increases. The effectiveness of secondary refrigerants can be improved when phase changing media are introduced in place of single phase media. Operating at temperatures below the freezing point of water, <span class="hlt">ice</span> slurry facilitates several efficiency improvements such as reductions in pumping energy consumption as well as lowering the required temperature difference in heat exchangers due to the beneficial thermo-physical properties of <span class="hlt">ice</span> slurry. Research has shown that <span class="hlt">ice</span> slurry can be engineered to have ideal <span class="hlt">ice</span> particle characteristics so that it can be easily stored in tanks without agglomeration and then be extractable for pumping at very high <span class="hlt">ice</span> fraction without plugging. In addition <span class="hlt">ice</span> slurry can be used in many direct contact food and medical protective cooling applications. This <span class="hlt">paper</span> provides an overview of the latest developments in <span class="hlt">ice</span> slurry technology. PMID:21528014</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008AIPC..985.1475M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008AIPC..985.1475M"><span>The Performance of Gas Filled Multilayer <span class="hlt">Insulation</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mills, G. L.; Zeller, C. M.</p> <p>2008-03-01</p> <p>The NASA Exploration Program is currently planning to use liquid oxygen, methane and hydrogen for propulsion in future spacecraft for the human exploration of the Moon and Mars. This will require the efficient long term, on-orbit storage of these cryogens. Multilayer <span class="hlt">insulation</span> (MLI) will be critical to achieving the required thermal performance since it has much lower heat transfer than any other <span class="hlt">insulation</span> when used in a vacuum. However, the size and mass constraints of these propulsion systems will not allow a structural shell to be used to provide vacuum for the MLI during ground hold and launch. One approach is to purge the MLI during ground hold with an inert gas which is then vented during launch ascent and on-orbit. In this <span class="hlt">paper</span>, we report on experimental tests and modeling that we have done on MLI used to <span class="hlt">insulate</span> a cryogenic tank. These include measurements of the heat transfer of gas filled <span class="hlt">insulation</span>, evacuated <span class="hlt">insulation</span> and during the transition in between.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2005AGUFM.V12B..01G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2005AGUFM.V12B..01G"><span><span class="hlt">Ice</span> Thickness, Melting Rates and Styles of Activity in <span class="hlt">Ice</span>-Volcano Interaction</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gudmundsson, M. T.</p> <p>2005-12-01</p> <p>In most cases when eruptions occur within glaciers they lead to rapid <span class="hlt">ice</span> melting, jokulhlaups and/or lahars. Many parameters influence the style of activity and its impact on the environment. These include <span class="hlt">ice</span> thickness (size of glacier), bedrock geometry, magma flow rate and magma <span class="hlt">composition</span>. The eruptions that have been observed can roughly be divided into: (1) eruptions under several hundred meters thick <span class="hlt">ice</span> on a relatively flat bedrock, (2) eruptions on flat or sloping bed through relatively thin <span class="hlt">ice</span>, and (3) volcanism where effects are limitied to confinement of lava flows or melting of <span class="hlt">ice</span> by pyroclastic flows or surges. This last category (<span class="hlt">ice</span>-contact volcanism) need not cause much <span class="hlt">ice</span> melting. Many of the deposits formed by Pleistocene volcanism in Iceland, British Columbia and Antarctica belong to the first category. An important difference between this type of activity and submarine activity (where pressure is hydrostatic) is that pressure at vents may in many cases be much lower than glaciostatic due to partial support of <span class="hlt">ice</span> cover over vents by the surrounding glacier. Reduced pressure favours explosive activity. Thus the effusive/explosive transition may occur several hundred metres underneath the <span class="hlt">ice</span> surface. Explosive fragmentation of magma leads to much higher rates of heat transfer than does effusive eruption of pillow lavas, and hence much higher melting rates. This effect of reduced pressure at vents will be less pronounced in a large <span class="hlt">ice</span> sheet than in a smaller glacier or <span class="hlt">ice</span> cap, since the hydraulic gradient that drives water away from an eruption site will be lower in the large glacier. This may have implications for form and type of eruption deposits and their relationship with <span class="hlt">ice</span> thickness and glacier size.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20090022235','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20090022235"><span>Using Aerogel-Based <span class="hlt">Insulation</span> Material To Prevent Foam Loss on the Liquid-Hydrogen Intertank</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>2008-01-01</p> <p>Uninsulated areas on cryogenic propellant tanks and feedlines cause moisture in the air to condense or <span class="hlt">ice</span> to form. Flange joints, bracket supports, expansion bellows, and other cavities are uninsulated by design. These areas cannot be sealed because conventional thermal <span class="hlt">insulation</span> materials would restrict mechanical articulations. Aerogel-based thermal <span class="hlt">insulation</span> systems are able to seal critical locations such as the liquid-oxygen (LO2) feedline bellows. A new thermal <span class="hlt">insulation</span> system was also necessary between the intertank wall, flange, and the liquid-hydrogen (LH2) tank dome, where there is a cavity (or crevice) with an exposed 20-K surface. When nitrogen gas is used for purging within the intertank volume, it condenses on this cold surface. Some solid nitrogen may also form on the colder side of the crevice. Voids or discontinuities within the foam can pressurize and cause areas of foam to weaken and break off, reducing thermal efficiency and creating potentially dangerous debris. To prevent this foam loss, we developed a thermal <span class="hlt">insulation</span> system using bulk-fill aerogel material and demonstrated it with a one-tenth-scale model of the LH2 intertank flange area</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29392850','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29392850"><span>Construction of 3D Skeleton for Polymer <span class="hlt">Composites</span> Achieving a High Thermal Conductivity.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Yao, Yimin; Sun, Jiajia; Zeng, Xiaoliang; Sun, Rong; Xu, Jian-Bin; Wong, Ching-Ping</p> <p>2018-03-01</p> <p>Owing to the growing heat removal issue in modern electronic devices, electrically <span class="hlt">insulating</span> polymer <span class="hlt">composites</span> with high thermal conductivity have drawn much attention during the past decade. However, the conventional method to improve through-plane thermal conductivity of these polymer <span class="hlt">composites</span> usually yields an undesired value (below 3.0 Wm -1 K -1 ). Here, construction of a 3D phonon skeleton is reported composed of stacked boron nitride (BN) platelets reinforced with reduced graphene oxide (rGO) for epoxy <span class="hlt">composites</span> by the combination of <span class="hlt">ice</span>-templated and infiltrating methods. At a low filler loading of 13.16 vol%, the resulting 3D BN-rGO/epoxy <span class="hlt">composites</span> exhibit an ultrahigh through-plane thermal conductivity of 5.05 Wm -1 K -1 as the best thermal-conduction performance reported so far for BN sheet-based <span class="hlt">composites</span>. Theoretical models qualitatively demonstrate that this enhancement results from the formation of phonon-matching 3D BN-rGO networks, leading to high rates of phonon transport. The strong potential application for thermal management has been demonstrated by the surface temperature variations of the <span class="hlt">composites</span> with time during heating and cooling. © 2018 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.C43B0741F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C43B0741F"><span>The effect of under-<span class="hlt">ice</span> melt ponds on their surroundings in the Arctic</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Feltham, D. L.; Smith, N.; Flocco, D.</p> <p>2016-12-01</p> <p>In the summer months, melt water from the surface of the Arctic sea <span class="hlt">ice</span> can percolate down through the <span class="hlt">ice</span> and flow out of its base. This water is relatively warm and fresh compared to the ocean water beneath it, and so it floats between the <span class="hlt">ice</span> and the oceanic mixed layer, forming pools of melt water called under-<span class="hlt">ice</span> melt ponds. Sheets of <span class="hlt">ice</span>, known as false bottoms, can subsequently form via double diffusion processes at the under-<span class="hlt">ice</span> melt pond interface with the ocean, trapping the pond against the <span class="hlt">ice</span> and completely isolating it from the ocean below. This has an <span class="hlt">insulating</span> effect on the parent sea <span class="hlt">ice</span> above the trapped pond, altering its rate of basal ablation. A one-dimensional, thermodynamic model of Arctic sea <span class="hlt">ice</span> has been adapted to study the evolution of under-<span class="hlt">ice</span> melt ponds and false bottoms over time. Comparing simulations of sea <span class="hlt">ice</span> evolution with and without an under-<span class="hlt">ice</span> melt pond provides a measure of how an under-<span class="hlt">ice</span> melt pond affects the mass balance of the sea <span class="hlt">ice</span> above it. Sensitivity studies testing the response of the model to a range of uncertain parameters have been performed, revealing some interesting implications of under-<span class="hlt">ice</span> ponds during their life cycle. By changing the rate of basal ablation of the parent sea <span class="hlt">ice</span>, and so the flux of fresh water and salt into the ocean, under-<span class="hlt">ice</span> melt ponds affect the properties of the mixed layer beneath the sea <span class="hlt">ice</span>. Our model of under-<span class="hlt">ice</span> melt pond refreezing has been coupled to a simple oceanic mixed layer model to determine the effect on mixed layer depth, salinity and temperature.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22280540-using-fiberglass-volumes-vpi-superconductive-magnetic-systems-insulation','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22280540-using-fiberglass-volumes-vpi-superconductive-magnetic-systems-insulation"><span>Using fiberglass volumes for VPI of superconductive magnetic systems’ <span class="hlt">insulation</span></span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Andreev, I. S.; Bezrukov, A. A.; Pischugin, A. B.</p> <p>2014-01-29</p> <p>The <span class="hlt">paper</span> describes the method of manufacturing fiberglass molds for vacuum pressure impregnation (VPI) of high-voltage <span class="hlt">insulation</span> of superconductive magnetic systems (SMS) with epoxidian hot-setting compounds. The basic advantages of using such vacuum volumes are improved quality of <span class="hlt">insulation</span> impregnation in complex-shaped areas, and considerable cost-saving of preparing VPI of large-sized components due to dispensing with the stage of fabricating a metal impregnating volume. Such fiberglass vacuum molds were used for VPI of high-voltage <span class="hlt">insulation</span> samples of an ITER reactor’s PF1 poloidal coil. Electric <span class="hlt">insulation</span> of these samples has successfully undergone a wide range of high-voltage and mechanical tests atmore » room and cryogenic temperatures. Some results of the tests are also given in this <span class="hlt">paper</span>.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PhFl...30b7101J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PhFl...30b7101J"><span>Mixed <span class="hlt">ice</span> accretion on aircraft wings</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Janjua, Zaid A.; Turnbull, Barbara; Hibberd, Stephen; Choi, Kwing-So</p> <p>2018-02-01</p> <p><span class="hlt">Ice</span> accretion is a problematic natural phenomenon that affects a wide range of engineering applications including power cables, radio masts, and wind turbines. Accretion on aircraft wings occurs when supercooled water droplets freeze instantaneously on impact to form rime <span class="hlt">ice</span> or runback as water along the wing to form glaze <span class="hlt">ice</span>. Most models to date have ignored the accretion of mixed <span class="hlt">ice</span>, which is a combination of rime and glaze. A parameter we term the "freezing fraction" is defined as the fraction of a supercooled droplet that freezes on impact with the top surface of the accretion <span class="hlt">ice</span> to explore the concept of mixed <span class="hlt">ice</span> accretion. Additionally we consider different "packing densities" of rime <span class="hlt">ice</span>, mimicking the different bulk rime densities observed in nature. <span class="hlt">Ice</span> accretion is considered in four stages: rime, primary mixed, secondary mixed, and glaze <span class="hlt">ice</span>. Predictions match with existing models and experimental data in the limiting rime and glaze cases. The mixed <span class="hlt">ice</span> formulation however provides additional insight into the <span class="hlt">composition</span> of the overall <span class="hlt">ice</span> structure, which ultimately influences adhesion and <span class="hlt">ice</span> thickness, and shows that for similar atmospheric parameter ranges, this simple mixed <span class="hlt">ice</span> description leads to very different accretion rates. A simple one-dimensional energy balance was solved to show how this freezing fraction parameter increases with decrease in atmospheric temperature, with lower freezing fraction promoting glaze <span class="hlt">ice</span> accretion.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008AIPC..985.1367P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008AIPC..985.1367P"><span>Synthesis of the Multilayer Cryogenic <span class="hlt">Insulation</span> Modelling and Measurements</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Polinski, J.; Chorowski, M.; Choudhury, A.; Datta, T. S.</p> <p>2008-03-01</p> <p>A thermodynamic approach towards <span class="hlt">insulation</span> systems in cryogenic engineering is proposed. A mathematical model of the heat transfer through multilayer <span class="hlt">insulation</span> (MLI) has been developed and experimentally verified. The model comprises both physical and engineering parameters determining the MLI performance and enables a complex optimization of the <span class="hlt">insulation</span> system including the choice of the <span class="hlt">insulation</span> location in a vacuum space. The model takes into account an interstitial (interlayer) gas pressure variation with the MLI number of layers and layers density. The <span class="hlt">paper</span> presents the discussion of MLI performance in different conditions and provides comparison of computation results with experimental reference and measured data.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015Icar..261...14F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015Icar..261...14F"><span>Kinetics of hydrogen/deuterium exchanges in cometary <span class="hlt">ices</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Faure, Mathilde; Quirico, Eric; Faure, Alexandre; Schmitt, Bernard; Theulé, Patrice; Marboeuf, Ulysse</p> <p>2015-11-01</p> <p>The D/H <span class="hlt">composition</span> of volatile molecules composing cometary <span class="hlt">ices</span> brings key constraints on the origin of comets, on the extent of their presolar heritage, as well as on the origin of atmospheres and hydrospheres of terrestrial planets. Nevertheless, the D/H <span class="hlt">composition</span> may have been modified to various extents in the nucleus when a comet approaches the Sun and experiences deep physical and chemical modifications in its subsurface. We question here the evolution of the D/H ratio of organic species by proton exchanges with water <span class="hlt">ice</span>. We experimentally studied the kinetics of D/H exchanges on the <span class="hlt">ice</span> mixtures H2O:CD3OD, H2O:CD3ND2 and D2O:HCN. Our results show that fast exchanges occur on the -OH and -NH2 chemical groups, which are processed through hydrogen bonds exchanges with water and by the molecular mobility triggered by structural changes, such as glass transition or crystallization. D/H exchanges kinetic is best described by a second-order kinetic law with activation energies of 4300 ± 900 K and 3300 ± 100 K for H2O:CD3OD and H2O:CD3ND2 <span class="hlt">ice</span> mixtures, respectively. The corresponding pre-exponential factors ln(A(s-1)) are 25 ± 7 and 20 ± 1, respectively. No exchange was observed in the case of HCN trapped in D2O <span class="hlt">ice</span>. These results strongly suggest that upon thermal heating (1) -OH and -NH2 chemical groups of any organic molecules loose their primordial D/H <span class="hlt">composition</span> and equilibrate with water <span class="hlt">ice</span>, (2) HCN does not experience proton transfer and keeps a primordial D/H <span class="hlt">composition</span> and (3) C-H chemical groups are not isotopically modified.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AIPC.1839b0089X','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AIPC.1839b0089X"><span>Road <span class="hlt">icing</span> forecasting and detecting system</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Xu, Hongke; Zheng, Jinnan; Li, Peiqi; Wang, Qiucai</p> <p>2017-05-01</p> <p>Regard for the facts that the low accuracy and low real-time of the artificial observation to determine the road <span class="hlt">icing</span> condition, and it is difficult to forecast <span class="hlt">icing</span> situation, according to the main factors influencing the road-<span class="hlt">icing</span>, and the electrical characteristics reflected by the pavement <span class="hlt">ice</span> layer, this <span class="hlt">paper</span> presents an innovative system, that is, <span class="hlt">ice</span>-forecasting of the highway's dangerous section. The system bases on road surface water salinity measurements and pavement temperature measurement to calculate the freezing point of water and temperature change trend, and then predicts the occurrence time of road <span class="hlt">icing</span>; using capacitance measurements to verdict the road surface is frozen or not; This <span class="hlt">paper</span> expounds the method of using single chip microcomputer as the core of the control system and described the business process of the system.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20170005511','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20170005511"><span>Relationship of Cure Temperature to Mechanical, Physical, and Dielectric Performance of PDMS Glass <span class="hlt">Composite</span> for Electric Motor <span class="hlt">Insulation</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Miller, Sandi G.; Becker, Kathleen; Williams, Tiffany S.; Scheiman, Daniel A.; McCorkle, Linda S.; Heimann, Paula J.; Ring, Andrew; Woodworth, Andrew</p> <p>2017-01-01</p> <p>Achieving NASAs aggressive fuel burn and emission reduction for N-plus-3 aircraft will require hybrid electric propulsion system in which electric motors driven by either power generated from turbine or energy storage system will power the fan for propulsion. Motors designed for hybrid electric aircraft are expected to operate at medium to high voltages over long durations in a high altitude service environment. Such conditions have driven research toward the development of wire <span class="hlt">insulation</span> with improved mechanical strength, thermal stability and increased breakdown voltage. The silicone class of materials has been considered for electric wire <span class="hlt">insulation</span> due to its inherent thermal stability, dielectric strength and mechanical integrity. This <span class="hlt">paper</span> evaluates the dependence of these properties on the cure conditions of a polydimethyl-siloxane (PDMS) elastomer; where both cure temperature and base-to-catalyst ratio were varied. The PDMS elastomer was evaluated as a bulk material and an impregnation matrix within a lightweight glass veil support. The E-glass support was selected for mechanical stiffness and dielectric strength. This work has shown a correlation between cure conditions and material physical properties. Tensile strength increased with cure temperature whereas breakdown voltage tended to be independent of process variations. The results will be used to direct material formulation based on specific <span class="hlt">insulation</span> requirements.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010EGUGA..12.8925N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010EGUGA..12.8925N"><span>Chemistry of microparticles trapped in last glacial period <span class="hlt">ice</span> of EPICA-DML deep <span class="hlt">ice</span> core</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nedelcu, Aneta F.; Faria, Sérgio H.; Kipfstuhl, Sepp; Kuhs, Werner F.</p> <p>2010-05-01</p> <p>The EDML <span class="hlt">ice</span> core, drilled within the framework of the European project for <span class="hlt">Ice</span> Coring in Antarctica, (EPICA), in the interior of Dronning Maud Land, DML, Antarctica (at 75°S, 0°E), is the first deep <span class="hlt">ice</span> core in the Atlantic sector of the Southern Ocean region that provides higher-resolution atmosphere and climate records for the last glacial period, when compared with other <span class="hlt">ice</span> cores retrieved from the East Antarctic plateau [1]. The chemical impurities embedded in the <span class="hlt">ice</span> matrix of an <span class="hlt">ice</span> sheet are basic proxies for climate reconstruction, and their concentration and <span class="hlt">composition</span> usually determine the occurrence of distinct (cloudy or clear) strata in the <span class="hlt">ice</span> sheet structure. The easiest observable impurities in polar <span class="hlt">ice</span> are air bubbles. But a considerable amount of the impurities trapped inside <span class="hlt">ice</span> layers are observed as microscopic deposits of solid (soluble or insoluble) particles, not bigger than a few micra in size, called microinclusions. Layers of <span class="hlt">ice</span> with a high content of (micro)inclusions are in general called cloudy bands and are considered to have been formed from the precipitations deposited during colder periods. Roughly, we expect that the colder the climate during the time the snow accumulated, the cloudier the <span class="hlt">ice</span> stratum that forms afterwards [2]. Mainly by means of in-situ micro-Raman spectroscopy, it has been shown that in Antarctic glacial <span class="hlt">ice</span> the soluble microinclusions occur mostly as sulphate and nitrate salts [3], while in Arctic <span class="hlt">ice</span> more commonly as carbonate salts [4]. These findings could be explained in terms of different aerosol <span class="hlt">compositions</span> determined by the specific regional environments and climatic conditions [5]. Regarding the insoluble particles that might exist in natural <span class="hlt">ice</span>, with higher frequency in <span class="hlt">ice</span> layers formed during glacial type stages, the general findings classify them in the (alumino)silicate mineralogical class [6]. Microinclusions existent in solid samples taken from clear and cloudy <span class="hlt">ice</span> layers, corresponding</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20020041914','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20020041914"><span>Optimal Design of Functionally Graded Metallic Foam <span class="hlt">Insulations</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Haftka, Raphael T.; Sankar, Bhavani; Venkataraman, Satchi; Zhu, Huadong</p> <p>2002-01-01</p> <p> simple nonlinear differential equation. Preliminary results of this work were presented at the American Society of <span class="hlt">Composites</span> meeting, and the final version was submitted for publication in the AIAA Journal. In addition to minimizing the transmitted heat, we investigated the optimum design for minimum weight given an acceptable level of heat transmission through the <span class="hlt">insulation</span>. The optimality criterion developed was different from that obtained for minimizing beat transfer coefficient. For minimum mass design, we had to find for a given temperature the optimum density, which minimized the logarithmic derivative of the <span class="hlt">insulation</span> thermal conductivity with respect to its density. The logarithmic derivative is defined as the ratio of relative change in the dependent response (thermal conductivity) to the relative change in the independent variable (density). The results have been documented as a conference <span class="hlt">paper</span> that will be presented at the upcoming AIAA.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22680091-sterile-neutrinos-flavor-ratios-icecube','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22680091-sterile-neutrinos-flavor-ratios-icecube"><span>Sterile neutrinos and flavor ratios in <span class="hlt">Ice</span>Cube</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Brdar, Vedran; Kopp, Joachim; Wang, Xiao-Ping, E-mail: vbrdar@uni-mainz.de, E-mail: jkopp@uni-mainz.de, E-mail: xiaowang@uni-mainz.de</p> <p>2017-01-01</p> <p>The flavor <span class="hlt">composition</span> of astrophysical neutrinos observed in neutrino telescopes is a powerful discriminator between different astrophysical neutrino production mechanisms and can also teach us about the particle physics properties of neutrinos. In this <span class="hlt">paper</span>, we investigate how the possible existence of light sterile neutrinos can affect these flavor ratios. We consider two scenarios: (i) neutrino production in conventional astrophysical sources, followed by partial oscillation into sterile states; (ii) neutrinos from dark matter decay with a primary flavor <span class="hlt">composition</span> enhanced in tau neutrinos or sterile neutrinos. Throughout the <span class="hlt">paper</span>, we constrain the sterile neutrino mixing parameters from a full globalmore » fit to short and long baseline data. We present our results in the form of flavor triangles and, for scenario (ii), as exclusion limits on the dark matter mass and lifetime, derived from a fit to <span class="hlt">Ice</span>Cube high energy starting events and through-going muons. We argue that identifying a possible flux of neutrinos from dark matter decay may require analyzing the flavor <span class="hlt">composition</span> as a function of neutrino energy.« less</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li class="active"><span>16</span></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_16 --> <div id="page_17" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li class="active"><span>17</span></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="321"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19860015289','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19860015289"><span>Evaluation of capillary reinforced <span class="hlt">composites</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Cahill, J. E.; Halase, J. F.; South, W. K.; Stoffer, L. J.</p> <p>1985-01-01</p> <p>Anti-<span class="hlt">icing</span> of the inlet of jet engines is generally performed with high pressure heated air that is directed forward from the compressor through a series of pipes to various manifolds located near the structures to be anti-<span class="hlt">iced</span>. From these manifolds, the air is directed to all flowpath surfaces that may be susceptible to <span class="hlt">ice</span> formation. There the anti-<span class="hlt">icing</span> function may be performed by either heat conduction or film heating. Unfortunately, the prospect of utilizing lighweight, high strength <span class="hlt">composites</span> for inlet structures of jet engines has been frustrated by the low transverse thermal conductivity of such materials. It was the objective of this program to develop an advanced materials and design concept for anti-<span class="hlt">icing</span> <span class="hlt">composite</span> structures. The concept that was evaluated used capillary glass tubes embedded on the surface of a <span class="hlt">composite</span> structure with heated air ducted through the tubes. An analytical computer program was developed to predict the anti-<span class="hlt">icing</span> performance of such tubes and a test program was conducted to demonstrate actual performance of this system. Test data and analytical code results were in excellent agreement. Both indicate feasibility of using capillary tubes for surface heating as a means for <span class="hlt">composite</span> engine structures to combat <span class="hlt">ice</span> accumulation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20110023905','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20110023905"><span>Improved Thermal-<span class="hlt">Insulation</span> Systems for Low Temperatures</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Fesmire, James E.; Augustynowicz, Stanislaw D.</p> <p>2003-01-01</p> <p>Improved thermal-<span class="hlt">insulation</span> materials and structures and the techniques for manufacturing them are undergoing development for use in low-temperature applications. Examples of low-temperature equipment for which these thermal <span class="hlt">insulation</span> systems could provide improved energy efficiency include storage tanks for cryogens, superconducting electric-power-transmission equipment, containers for transport of food and other perishable commodities, and cold boxes for low-temperature industrial processes. These systems could also be used to <span class="hlt">insulate</span> piping used to transfer cryogens and other fluids, such as liquefied natural gas, refrigerants, chilled water, crude oil, or low-pressure steam. The present thermal-<span class="hlt">insulation</span> systems are layer <span class="hlt">composites</span> based partly on the older class of thermal-<span class="hlt">insulation</span> systems denoted generally as multilayer <span class="hlt">insulation</span> (MLI). A typical MLI structure includes an evacuated jacket, within which many layers of radiation shields are stacked or wrapped close together. Low-thermal-conductivity spacers are typically placed between the reflection layers to keep them from touching. MLI can work very well when a high vacuum level (less than 10(exp-4) torr) is maintained and utmost care is taken during installation, but its thermal performance deteriorates sharply as the pressure in the evacuated space rises into the soft vacuum range [pressures greater than 0.1 torr (greater than 13 Pa)]. In addition, the thermal performance of MLI is extremely sensitive to mechanical compression and edge effects and can easily decrease from one to two orders of magnitude from its ideal value even when the MLI is kept under high vacuum condition. The present thermal-<span class="hlt">insulation</span> systems are designed to perform well under soft vacuum level, in particular the range of 1 to 10 torr. They are also designed with larger interlayer spacings to reduce vulnerability to compression (and consequent heat leak) caused by installation and use. The superiority of these systems is the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20120003167','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20120003167"><span>Pressure Dependence of <span class="hlt">Insulator-Insulator</span> Contact Charging</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Hogue, Michael D.</p> <p>2005-01-01</p> <p>The mechanism of <span class="hlt">insulator-insulator</span> triboelectric (contact) charging is being studied by the Electrostatics and Surface Physics Laboratory at KSC. The hypothesis that surface ion exchange is the primary mechanism is being tested experimentally. A two-phase model based on a small partial pressure of singly charged ions in an ambient ideal gas in equilibrium with a submonolayer adsorbed film will provide predictions about charging as a function Of ion mass, pressure, temperature, and surface adsorption energy. Interactions between ions will be considered in terms of coulombic and screened potential energies. This work is yielding better understanding of the triboelectrification of <span class="hlt">insulators</span>, which is an important problem in. space exploration technology. The work is also relevant to important industrial processes such as xerography and the application of paints and coatings. Determining a better understanding of the fundamental mechanism of <span class="hlt">insulator-insulator</span> triboelectrification will hopefully lead to better means of eliminating or at least mitigating its hazards and enhancing its useful applications.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20130013431','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20130013431"><span>On the <span class="hlt">Ice</span> Nucleation Spectrum</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Barahona, D.</p> <p>2012-01-01</p> <p>This work presents a novel formulation of the <span class="hlt">ice</span> nucleation spectrum, i.e. the function relating the <span class="hlt">ice</span> crystal concentration to cloud formation conditions and aerosol properties. The new formulation is physically-based and explicitly accounts for the dependency of the <span class="hlt">ice</span> crystal concentration on temperature, supersaturation, cooling rate, and particle size, surface area and <span class="hlt">composition</span>. This is achieved by introducing the concepts of <span class="hlt">ice</span> nucleation coefficient (the number of <span class="hlt">ice</span> germs present in a particle) and nucleation probability dispersion function (the distribution of <span class="hlt">ice</span> nucleation coefficients within the aerosol population). The new formulation is used to generate <span class="hlt">ice</span> nucleation parameterizations for the homogeneous freezing of cloud droplets and the heterogeneous deposition <span class="hlt">ice</span> nucleation on dust and soot <span class="hlt">ice</span> nuclei. For homogeneous freezing, it was found that by increasing the dispersion in the droplet volume distribution the fraction of supercooled droplets in the population increases. For heterogeneous <span class="hlt">ice</span> nucleation the new formulation consistently describes singular and stochastic behavior within a single framework. Using a fundamentally stochastic approach, both cooling rate independence and constancy of the <span class="hlt">ice</span> nucleation fraction over time, features typically associated with singular behavior, were reproduced. Analysis of the temporal dependency of the <span class="hlt">ice</span> nucleation spectrum suggested that experimental methods that measure the <span class="hlt">ice</span> nucleation fraction over few seconds would tend to underestimate the <span class="hlt">ice</span> nuclei concentration. It is shown that inferring the aerosol heterogeneous <span class="hlt">ice</span> nucleation properties from measurements of the onset supersaturation and temperature may carry significant error as the variability in <span class="hlt">ice</span> nucleation properties within the aerosol population is not accounted for. This work provides a simple and rigorous <span class="hlt">ice</span> nucleation framework where theoretical predictions, laboratory measurements and field campaign data can be</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19950011769','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19950011769"><span>Outgassing of solid material into vacuum thermal <span class="hlt">insulation</span> spaces</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Wang, Pao-Lien</p> <p>1994-01-01</p> <p>Many cryogenic storage tanks use vacuum between inner and outer tank for thermal <span class="hlt">insulation</span>. These cryogenic tanks also use a radiation shield barrier in the vacuum space to prevent radiation heat transfer. This shield is usually constructed by using multiple wraps of aluminized mylar and glass <span class="hlt">paper</span> as inserts. For obtaining maximum thermal performance, a good vacuum level must be maintained with the <span class="hlt">insulation</span> system. It has been found that over a period of time solid <span class="hlt">insulation</span> materials will vaporize into the vacuum space and the vacuum will degrade. In order to determine the degradation of vacuum, the rate of outgassing of the <span class="hlt">insulation</span> materials must be determined. Outgassing rate of several <span class="hlt">insulation</span> materials obtained from literature search were listed in tabular form.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19770064004&hterms=asma&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dasma','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19770064004&hterms=asma&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dasma"><span>Rain erosion considerations for launch vehicle <span class="hlt">insulation</span> systems</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Daniels, D. J.; Sieker, W. D.</p> <p>1977-01-01</p> <p>In recent years the Delta launch vehicle has incorporated the capability to be launched through rain. This capability was developed to eliminate a design constraint which could result in a costly launch delay. This <span class="hlt">paper</span> presents the methodology developed to implement rain erosion protection for the <span class="hlt">insulated</span> exterior vehicle surfaces. The effect of the interaction between <span class="hlt">insulation</span> material rain erosion resistance, rainstorm models, surface geometry and trajectory variations is examined. It is concluded that rain erosion can significantly impact the performance of launch vehicle <span class="hlt">insulation</span> systems and should be considered in their design.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012JaJAP..51iMG03J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012JaJAP..51iMG03J"><span>Conductivity Variation Observed by Polarization and Depolarization Current Measurements of High-Voltage Equipment <span class="hlt">Insulation</span> System</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jamail, Nor Akmal Mohd; Piah, Mohamed Afendi Mohamed; Muhamad, Nor Asiah</p> <p>2012-09-01</p> <p>Nondestructive and time domain dielectric measurement techniques such as polarization and depolarization current (PDC) measurements have recently been widely used as a potential tool for determining high-voltage <span class="hlt">insulation</span> conditions by analyzing the <span class="hlt">insulation</span> conductivity. The variation in the conductivity of an <span class="hlt">insulator</span> was found to depend on several parameters: the difference between the polarization and depolarization currents, geometric capacitance, and the relative permittivity of the <span class="hlt">insulation</span> material. In this <span class="hlt">paper</span> the conductivities of different types of oil-<span class="hlt">paper</span> <span class="hlt">insulation</span> material are presented. The <span class="hlt">insulation</span> conductivities of several types of electrical apparatus were simulated using MATLAB. Conductivity <span class="hlt">insulation</span> was found to be high at high polarizations and at the lowest depolarization current. It was also found to increase with increasing relative permittivity as well as with decreasing geometric capacitance of the <span class="hlt">insulating</span> material.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018MS%26E..374a2008B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018MS%26E..374a2008B"><span>The Influence of Mechanical Parameters on Dielectric Characteristics of Rigid Electrical <span class="hlt">Insulating</span> Materials</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Buică, G.; Antonov, A. E.; Beiu, C.; Dobra, R.; Risteiu, M.</p> <p>2018-06-01</p> <p>Rigid electrical <span class="hlt">insulating</span> materials are used in the manufacture of work equipment with electric safety function, being mainly intended for use in the energy sector. The <span class="hlt">paper</span> presents the results of the research on the identification of the technical and safety requirements for rigid electrical <span class="hlt">insulating</span> materials that are part of the electrical <span class="hlt">insulating</span> work equipment. The <span class="hlt">paper</span> aims to show the behaviour of rigid electrical <span class="hlt">insulating</span> materials under the influence of mechanical risk factors, in order to check the functionality and to ensure the safety function for the entire life time. There were tested rigid electrical <span class="hlt">insulating</span> equipment designed to be used as safety means in electrical power stations and overhead power lines.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015PhPl...22d2113Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015PhPl...22d2113Z"><span>Mechanism and influencing factors on critical pulse width of oil-immersed polymer <span class="hlt">insulators</span> under short pulses</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhao, Liang; Su, Jian Cang; Li, Rui; Zeng, Bo; Cheng, Jie; Zheng, Lei; Yu, Bin Xiong; Wu, Xiao Long; Zhang, Xi Bo; Pan, Ya Feng</p> <p>2015-04-01</p> <p>The critical pulse width (τc) is a pulse width at which the surface flashover threshold (Ef) is equal to the bulk breakdown threshold (EBD) for liquid-polymer <span class="hlt">composite</span> <span class="hlt">insulation</span> systems, which is discovered by Zhao et al. [Annual Report Conference on Electrical <span class="hlt">Insulation</span> and Dielectric Phenomena (IEEE Dielectrics and Electrical <span class="hlt">Insulation</span> Society, Shenzhen, China, 2013), Vol. 2, pp. 854-857]. In this <span class="hlt">paper</span>, the mechanism of τc is interpreted in perspective of the threshold and the time delay (td) of surface flashover and bulk breakdown, respectively. It is found that two changes appear as the pulse width decreases which are responsible for the existence of τc: (1) EBD is lower than Ef; (2) td of bulk breakdown is shorter than td of surface flashover. In addition, factors which have influences on τc are investigated, such as the dielectric type, the <span class="hlt">insulation</span> length, the dielectric thickness, the dielectrics configuration, the pulse number, and the liquid purity. These influences of factors are generalized as three types if τc is expected to increase: (1) factors causing EBD to decrease, such as increasing the pulse number or employing a dielectric of lower EBD; (2) factors causing Ef to increase, such as complicating the <span class="hlt">insulator</span>'s configuration or increasing the liquid purity; (3) factors causing EBD and Ef to increase together, but Ef increases faster than EBD, such as decreasing the dielectric thickness or the <span class="hlt">insulation</span> length. With the data in references, all the three cases are verified experimentally. In the end, a general method based on τc for solid <span class="hlt">insulation</span> design is presented and the significance of τc on solid <span class="hlt">insulation</span> design and on solid demolition are discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29761564','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29761564"><span>Laser-Induced Molybdenum Carbide-Graphene <span class="hlt">Composites</span> for 3D Foldable <span class="hlt">Paper</span> Electronics.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Zang, Xining; Shen, Caiwei; Chu, Yao; Li, Buxuan; Wei, Minsong; Zhong, Junwen; Sanghadasa, Mohan; Lin, Liwei</p> <p>2018-05-15</p> <p>Versatile and low-cost manufacturing processes/materials are essential for the development of <span class="hlt">paper</span> electronics. Here, a direct-write laser patterning process is developed to make conductive molybdenum carbide-graphene (MCG) <span class="hlt">composites</span> directly on <span class="hlt">paper</span> substrates. The hierarchically porous MCG structures are converted from fibrous <span class="hlt">paper</span> soaked with the gelatin-mediated inks containing molybdenum ions. The resulting Mo 3 C 2 and graphene <span class="hlt">composites</span> are mechanically stable and electrochemically active for various potential applications, such as electrochemical ion detectors and gas sensors, energy harvesters, and supercapacitors. Experimentally, the electrical conductivity of the <span class="hlt">composite</span> is resilient to mechanical deformation with less than 5% degradation after 750 cycles of 180° repeated folding tests. As such, the direct laser conversion of MCGs on <span class="hlt">papers</span> can be applicable for <span class="hlt">paper</span>-based electronics, including the 3D origami folding structures. © 2018 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1980nbs..reptR....K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1980nbs..reptR....K"><span>Breakdown between bare electrodes with an oil-<span class="hlt">paper</span> interface</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kelley, E. F.; Hebner, R. E., Jr.</p> <p>1980-06-01</p> <p>Measurements of the location of electrical breakdown in a <span class="hlt">composite</span> <span class="hlt">insulating</span> system were made. For these measurements a <span class="hlt">paper</span> sample was mounted so that it connected the two electrodes. Electrode structures ranging from plane-plane to sphere-sphere were used. The electrode <span class="hlt">paper</span> system was tested in oil in an attempt to determine the properties of an oil <span class="hlt">paper</span> interface. The data indicated that in a carefully prepared system the breakdown will not necessarily occur at the interface. In addition, it was found that the breakdown voltages were not significantly lower for those breakdowns which occurred at the interface than for those which did not. It was noted that if the <span class="hlt">paper</span> interface was not dried or if many gaseous voids were left in or on the <span class="hlt">paper</span>, the breakdown will regularly occur at the interface and at a lower voltage.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70169889','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70169889"><span>Tracking millennial-scale Holocene glacial advance and retreat using osmium isotopes: Insights from the Greenland <span class="hlt">ice</span> sheet</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Rooney, Alan D.; Selby, David; Llyod, Jeremy M.; Roberts, David H.; Luckge, Andreas; Sageman, Bradley B.; Prouty, Nancy G.</p> <p>2016-01-01</p> <p>High-resolution Os isotope stratigraphy can aid in reconstructing Pleistocene <span class="hlt">ice</span> sheet fluctuation and elucidating the role of local and regional weathering fluxes on the marine Os residence time. This <span class="hlt">paper</span> presents new Os isotope data from ocean cores adjacent to the West Greenland <span class="hlt">ice</span> sheet that have excellent chronological controls. Cores MSM-520 and DA00-06 represent distal to proximal sites adjacent to two West Greenland <span class="hlt">ice</span> streams. Core MSM-520 has a steadily decreasing Os signal over the last 10 kyr (187Os/188Os = 1.35–0.81). In contrast, Os isotopes from core DA00-06 (proximal to the calving front of Jakobshavn Isbræ) highlight four stages of <span class="hlt">ice</span> stream retreat and advance over the past 10 kyr (187Os/188Os = 2.31; 1.68; 2.09; 1.47). Our high-resolution chemostratigraphic records provide vital benchmarks for <span class="hlt">ice</span>-sheet modelers as we attempt to better constrain the future response of major <span class="hlt">ice</span> sheets to climate change. Variations in Os isotope <span class="hlt">composition</span> from sediment and macro-algae (seaweed) sourced from regional and global settings serve to emphasize the overwhelming effect weathering sources have on seawater Os isotope <span class="hlt">composition</span>. Further, these findings demonstrate that the residence time of Os is shorter than previous estimates of ∼104 yr.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20080013293','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20080013293"><span>Airfoil <span class="hlt">Ice</span>-Accretion Aerodynamics Simulation</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Bragg, Michael B.; Broeren, Andy P.; Addy, Harold E.; Potapczuk, Mark G.; Guffond, Didier; Montreuil, E.</p> <p>2007-01-01</p> <p>NASA Glenn Research Center, ONERA, and the University of Illinois are conducting a major research program whose goal is to improve our understanding of the aerodynamic scaling of <span class="hlt">ice</span> accretions on airfoils. The program when it is completed will result in validated scaled simulation methods that produce the essential aerodynamic features of the full-scale <span class="hlt">iced</span>-airfoil. This research will provide some of the first, high-fidelity, full-scale, <span class="hlt">iced</span>-airfoil aerodynamic data. An initial study classified <span class="hlt">ice</span> accretions based on their aerodynamics into four types: roughness, streamwise <span class="hlt">ice</span>, horn <span class="hlt">ice</span>, and spanwise-ridge <span class="hlt">ice</span>. Subscale testing using a NACA 23012 airfoil was performed in the NASA IRT and University of Illinois wind tunnel to better understand the aerodynamics of these <span class="hlt">ice</span> types and to test various levels of <span class="hlt">ice</span> simulation fidelity. These studies are briefly reviewed here and have been presented in more detail in other <span class="hlt">papers</span>. Based on these results, full-scale testing at the ONERA F1 tunnel using cast <span class="hlt">ice</span> shapes obtained from molds taken in the IRT will provide full-scale <span class="hlt">iced</span> airfoil data from full-scale <span class="hlt">ice</span> accretions. Using these data as a baseline, the final step is to validate the simulation methods in scale in the Illinois wind tunnel. Computational <span class="hlt">ice</span> accretion methods including LEWICE and ONICE have been used to guide the experiments and are briefly described and results shown. When full-scale and simulation aerodynamic results are available, these data will be used to further develop computational tools. Thus the purpose of the <span class="hlt">paper</span> is to present an overview of the program and key results to date.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19670000016','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19670000016"><span>Dispersion of borax in plastic is excellent fire-retardant heat <span class="hlt">insulator</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Evans, H.; Hughes, J.; Schmitz, F.</p> <p>1967-01-01</p> <p>A mix of borax powder and a chlorinated anhydrous polyester resin yields a plastic <span class="hlt">composition</span> that is fire-retardant, yields a minimum of toxic gases when heated, and exhibits high thermal <span class="hlt">insulating</span> properties. This <span class="hlt">composition</span> can be used as a coating or can be converted into laminated or cast shapes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20010048683&hterms=NETWORK+DISTRIBUTION+ENERGY&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3DNETWORK%2BOf%2BDISTRIBUTION%2BENERGY','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20010048683&hterms=NETWORK+DISTRIBUTION+ENERGY&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3DNETWORK%2BOf%2BDISTRIBUTION%2BENERGY"><span>A Network Model for the Effective Thermal Conductivity of Rigid Fibrous Refractory <span class="hlt">Insulations</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Marschall, Jochen; Cooper, D. M. (Technical Monitor)</p> <p>1995-01-01</p> <p>A procedure is described for computing the effective thermal conductivity of a rigid fibrous refractory <span class="hlt">insulation</span>. The <span class="hlt">insulation</span> is modeled as a 3-dimensional Cartesian network of thermal conductance. The values and volume distributions of the conductance are assigned to reflect the physical properties of the <span class="hlt">insulation</span>, its constituent fibers, and any permeating gas. The effective thermal conductivity is computed by considering the simultaneous energy transport by solid conduction, gas conduction and radiation through a cubic volume of model <span class="hlt">insulation</span>; thus the coupling between heat transfer modes is retained (within the simplifications inherent to the model), rather than suppressed by treating these heat transfer modes as independent. The model takes into account <span class="hlt">insulation</span> <span class="hlt">composition</span>, density and fiber anisotropy, as well as the geometric and material properties of the constituent fibers. A relatively good agreement, between calculated and experimentally derived thermal conductivity values, is obtained for a variety of rigid fibrous <span class="hlt">insulations</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PhPl...25e2708L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PhPl...25e2708L"><span>Dynamical analysis of surface-<span class="hlt">insulated</span> planar wire array Z-pinches</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Li, Yang; Sheng, Liang; Hei, Dongwei; Li, Xingwen; Zhang, Jinhai; Li, Mo; Qiu, Aici</p> <p>2018-05-01</p> <p>The ablation and implosion dynamics of planar wire array Z-pinches with and without surface <span class="hlt">insulation</span> are compared and discussed in this <span class="hlt">paper</span>. This <span class="hlt">paper</span> first presents a phenomenological model named the ablation and cascade snowplow implosion (ACSI) model, which accounts for the ablation and implosion phases of a planar wire array Z-pinch in a single simulation. The comparison between experimental data and simulation results shows that the ACSI model could give a fairly good description about the dynamical characteristics of planar wire array Z-pinches. Surface <span class="hlt">insulation</span> introduces notable differences in the ablation phase of planar wire array Z-pinches. The ablation phase is divided into two stages: <span class="hlt">insulation</span> layer ablation and tungsten wire ablation. The two-stage ablation process of <span class="hlt">insulated</span> wires is simulated in the ACSI model by updating the formulas describing the ablation process.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19950012870','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19950012870"><span><span class="hlt">Ice</span> Accretion with Varying Surface Tension</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Bilanin, Alan J.; Anderson, David N.</p> <p>1995-01-01</p> <p>During an <span class="hlt">icing</span> encounter of an aircraft in flight, super-cooled water droplets impinging on an airfoil may splash before freezing. This <span class="hlt">paper</span> reports tests performed to determine if this effect is significant and uses the results to develop an improved scaling method for use in <span class="hlt">icing</span> test facilities. Simple laboratory tests showed that drops splash on impact at the Reynolds and Weber numbers typical of <span class="hlt">icing</span> encounters. Further confirmation of droplet splash came from <span class="hlt">icing</span> tests performed in the NaSA Lewis <span class="hlt">Icing</span> Research Tunnel (IRT) with a surfactant added to the spray water to reduce the surface tension. The resulting <span class="hlt">ice</span> shapes were significantly different from those formed when no surfactant was added to the water. These results suggested that the droplet Weber number must be kept constant to properly scale <span class="hlt">icing</span> test conditions. Finally, the <span class="hlt">paper</span> presents a Weber-number-based scaling method and reports results from scaling tests in the IRT in which model size was reduced up to a factor of 3. Scale and reference <span class="hlt">ice</span> shapes are shown which confirm the effectiveness of this new scaling method.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://rosap.ntl.bts.gov/view/dot/25671','DOTNTL'); return false;" href="https://rosap.ntl.bts.gov/view/dot/25671"><span>Design and construction guidelines for thermally <span class="hlt">insulated</span> concrete pavements.</span></a></p> <p><a target="_blank" href="http://ntlsearch.bts.gov/tris/index.do">DOT National Transportation Integrated Search</a></p> <p></p> <p>2013-01-01</p> <p>The report describes the construction and design of <span class="hlt">composite</span> pavements as a viable design strategy to use an : asphalt concrete (AC) wearing course as the <span class="hlt">insulating</span> material and a Portland cement concrete (PCC) structural : layer as the load-carryi...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20010037604','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20010037604"><span>Satellite Remote Sensing: Passive-Microwave Measurements of Sea <span class="hlt">Ice</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Parkinson, Claire L.; Zukor, Dorothy J. (Technical Monitor)</p> <p>2001-01-01</p> <p>Satellite passive-microwave measurements of sea <span class="hlt">ice</span> have provided global or near-global sea <span class="hlt">ice</span> data for most of the period since the launch of the Nimbus 5 satellite in December 1972, and have done so with horizontal resolutions on the order of 25-50 km and a frequency of every few days. These data have been used to calculate sea <span class="hlt">ice</span> concentrations (percent areal coverages), sea <span class="hlt">ice</span> extents, the length of the sea <span class="hlt">ice</span> season, sea <span class="hlt">ice</span> temperatures, and sea <span class="hlt">ice</span> velocities, and to determine the timing of the seasonal onset of melt as well as aspects of the <span class="hlt">ice</span>-type <span class="hlt">composition</span> of the sea <span class="hlt">ice</span> cover. In each case, the calculations are based on the microwave emission characteristics of sea <span class="hlt">ice</span> and the important contrasts between the microwave emissions of sea <span class="hlt">ice</span> and those of the surrounding liquid-water medium.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19840030725&hterms=heat+insulation&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dheat%2Binsulation','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19840030725&hterms=heat+insulation&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dheat%2Binsulation"><span>Producibility of fibrous refractory <span class="hlt">composite</span> <span class="hlt">insulation</span>, FRCI 40-20. [for reusable heat shielding</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Strauss, E. L.; Johnson, C. W.; Graese, R. W.; Campbell, R. L.</p> <p>1983-01-01</p> <p>Fibrous Refractory <span class="hlt">Composite</span> <span class="hlt">Insulation</span> (FRCI) is a NASA-developed, second generation, reusable heat-shield material that comprises a mixture of aluminoborosilicate fibers, silica fibers, and silicon carbide. Under NASA contract, a program was conducted to demonstrate the capability for manufacturing FRCI 40-20 billets. A detailed fabrication procedure was written and validated by testing specimens from the first two billets. The material conformed to NASA requirements for density, tensile strength, modulus of rupture, thermal expansion, cristobalite content, and uniformity. Twenty-four billets were prepared to provide 20 deliverable articles. Production billets were checked for density, modulus of rupture, cristobalite content, and uniformity. Billet density ranged from 309.48 to 332.22 kg/cu m (19.32 to 20.74 lb/cu ft) and modulus of rupture from 4690 to 10,140 kPa (680 to 1470 psi). Cristobalite content was less than 1 percent. A Weibull analysis of modulus-of-rupture data indicated a 1.5 percent probability for failure below the specified strength of 4480 kPa (650 psi).</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li class="active"><span>17</span></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_17 --> <div id="page_18" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li class="active"><span>18</span></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="341"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5492567','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5492567"><span>On Line Service <span class="hlt">Composition</span> in the Integrated Clinical Environment for eHealth and Medical Systems</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>García-Valls, Marisol; Touahria, Imad Eddine</p> <p>2017-01-01</p> <p>Medical and eHealth systems are progressively realized in the context of standardized architectures that support safety and ease the integration of the heterogeneous (and often proprietary) medical devices and sensors. The Integrated Clinical Environment (<span class="hlt">ICE</span>) architecture appeared recently with the goal of becoming a common framework for defining the structure of the medical applications as concerns the safe integration of medical devices and sensors. <span class="hlt">ICE</span> is simply a high level architecture that defines the functional blocks that should be part of a medical system to support interoperability. As a result, the underlying communication backbone is broadly undefined as concerns the enabling software technology (including the middleware) and associated algorithms that meet the <span class="hlt">ICE</span> requirements of the flexible integration of medical devices and services. Supporting the on line <span class="hlt">composition</span> of services in a medical system is also not part of <span class="hlt">ICE</span>; however, supporting this behavior would enable flexible orchestration of functions (e.g., addition and/or removal of services and medical equipment) on the fly. iLandis one of the few software technologies that supports on line service <span class="hlt">composition</span> and reconfiguration, ensuring time-bounded transitions across different service orchestrations; it supports the design, deployment and on line reconfiguration of applications, which this <span class="hlt">paper</span> applies to service-based eHealth domains. This <span class="hlt">paper</span> designs the integration between <span class="hlt">ICE</span> architecture and iLand middleware to enhance the capabilities of <span class="hlt">ICE</span> with on line service <span class="hlt">composition</span> and the time-bounded reconfiguration of medical systems based on distributed services. A prototype implementation of a service-based eHealth system for the remote monitoring of patients is described; it validates the enhanced capacity of <span class="hlt">ICE</span> to support dynamic reconfiguration of the application services. Results show that the temporal cost of the on line reconfiguration of the eHealth application is bounded</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28594371','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28594371"><span>On Line Service <span class="hlt">Composition</span> in the Integrated Clinical Environment for eHealth and Medical Systems.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>García-Valls, Marisol; Touahria, Imad Eddine</p> <p>2017-06-08</p> <p>Medical and eHealth systems are progressively realized in the context of standardized architectures that support safety and ease the integration of the heterogeneous (and often proprietary) medical devices and sensors. The Integrated Clinical Environment (<span class="hlt">ICE</span>) architecture appeared recently with the goal of becoming a common framework for defining the structure of the medical applications as concerns the safe integration of medical devices and sensors. <span class="hlt">ICE</span> is simply a high level architecture that defines the functional blocks that should be part of a medical system to support interoperability. As a result, the underlying communication backbone is broadly undefined as concerns the enabling software technology (including the middleware) and associated algorithms that meet the <span class="hlt">ICE</span> requirements of the flexible integration of medical devices and services. Supporting the on line <span class="hlt">composition</span> of services in a medical system is also not part of <span class="hlt">ICE</span>; however, supporting this behavior would enable flexible orchestration of functions (e.g., addition and/or removal of services and medical equipment) on the fly. iLandis one of the few software technologies that supports on line service <span class="hlt">composition</span> and reconfiguration, ensuring time-bounded transitions across different service orchestrations; it supports the design, deployment and on line reconfiguration of applications, which this <span class="hlt">paper</span> applies to service-based eHealth domains. This <span class="hlt">paper</span> designs the integration between <span class="hlt">ICE</span> architecture and iLand middleware to enhance the capabilities of <span class="hlt">ICE</span> with on line service <span class="hlt">composition</span> and the time-bounded reconfiguration of medical systems based on distributed services. A prototype implementation of a service-based eHealth system for the remote monitoring of patients is described; it validates the enhanced capacity of <span class="hlt">ICE</span> to support dynamic reconfiguration of the application services. Results show that the temporal cost of the on line reconfiguration of the eHealth application is bounded</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22207625','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22207625"><span>High pressure <span class="hlt">ices</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Hermann, Andreas; Ashcroft, N W; Hoffmann, Roald</p> <p>2012-01-17</p> <p>H(2)O will be more resistant to metallization than previously thought. From computational evolutionary structure searches, we find a sequence of new stable and meta-stable structures for the ground state of <span class="hlt">ice</span> in the 1-5 TPa (10 to 50 Mbar) regime, in the static approximation. The previously proposed Pbcm structure is superseded by a Pmc2(1) phase at p = 930 GPa, followed by a predicted transition to a P2(1) crystal structure at p = 1.3 TPa. This phase, featuring higher coordination at O and H, is stable over a wide pressure range, reaching 4.8 TPa. We analyze carefully the geometrical changes in the calculated structures, especially the buckling at the H in O-H-O motifs. All structures are <span class="hlt">insulating</span>--chemistry burns a deep and (with pressure increase) lasting hole in the density of states near the highest occupied electronic levels of what might be component metallic lattices. Metallization of <span class="hlt">ice</span> in our calculations occurs only near 4.8 TPa, where the metallic C2/m phase becomes most stable. In this regime, zero-point energies much larger than typical enthalpy differences suggest possible melting of the H sublattice, or even the entire crystal.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..1816263P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..1816263P"><span>Soot Aerosol Particles as Cloud Condensation Nuclei: from <span class="hlt">Ice</span> Nucleation Activity to <span class="hlt">Ice</span> Crystal Morphology</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pirim, Claire; Ikhenazene, Raouf; Ortega, Isamel Kenneth; Carpentier, Yvain; Focsa, Cristian; Chazallon, Bertrand; Ouf, François-Xavier</p> <p>2016-04-01</p> <p>Emissions of solid-state particles (soot) from engine exhausts due to incomplete fuel combustion is considered to influence <span class="hlt">ice</span> and liquid water cloud droplet activation [1]. The activity of these aerosols would originate from their ability to be important centers of <span class="hlt">ice</span>-particle nucleation, as they would promote <span class="hlt">ice</span> formation above water homogeneous freezing point. Soot particles are reported to be generally worse <span class="hlt">ice</span> nuclei than mineral dust because they activate nucleation at higher <span class="hlt">ice</span>-supersaturations for deposition nucleation and at lower temperatures for immersion freezing than ratios usually expected for homogeneous nucleation [2]. In fact, there are still numerous opened questions as to whether and how soot's physico-chemical properties (structure, morphology and chemical <span class="hlt">composition</span>) can influence their nucleation ability. Therefore, systematic investigations of soot aerosol nucleation activity via one specific nucleation mode, here deposition nucleation, combined with thorough structural and <span class="hlt">compositional</span> analyzes are needed in order to establish any association between the particles' activity and their physico-chemical properties. In addition, since the morphology of the <span class="hlt">ice</span> crystals can influence their radiative properties [3], we investigated their morphology as they grow over both soot and pristine substrates at different temperatures and humidity ratios. In the present work, Combustion Aerosol STandart soot samples were produced from propane using various experimental conditions. Their nucleation activity was studied in deposition mode (from water vapor), and monitored using a temperature-controlled reactor in which the sample's relative humidity is precisely measured with a cryo-hygrometer. Formation of water/<span class="hlt">ice</span> onto the particles is followed both optically and spectroscopically, using a microscope coupled to a Raman spectrometer. Vibrational signatures of hydroxyls (O-H) emerge when the particle becomes hydrated and are used to characterize <span class="hlt">ice</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.P24C..02C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.P24C..02C"><span>The <span class="hlt">Compositions</span>, Particle Sizes, and Distributions of <span class="hlt">Ice</span> Aerosols in the Mars Mesosphere from 2009-2016 CRISM Visible-NearIR Limb Spectra</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Clancy, R. T.; Smith, M. D.; Wolff, M. J.; Toigo, A. D.; Seelos, K. D.; Murchie, S. L.</p> <p>2016-12-01</p> <p>Since 2009, the CRISM visible-nearIR imaging spectrometer onboard the Mars Reconnaissance Orbiter (MRO) has returned over 70 orbits of Mars limb image scans over the 0-130 km altitude range. Pole-to-pole latitudinal coverage is obtained from the near-polar, sun-synchronous (LT 3pm) MRO orbit for a limited set of surface longitudes centered on Tharsis, Valles Mariners, Meridioni, and Hellas regions. Seasonal coverage extends over the full seasonal range (Ls=0-360°), as accumulated over 2009-2016 (MY 29-33), supporting a range of aerosol and airglow studies (Smith et al., 2013; Clancy et al., 2012, 2013). The 0.4-4.0 μm wavelength range of these CRISM limb observations proves particularly suitable to characterizing aerosol <span class="hlt">composition</span> and particle sizes, particularly for the Mars mesosphere (z=50-100 km), which has only recently been observed with any dedication by MCS (Sefton-Nash et al, 2013) and CRISM limb measurements. Dust and H2O, CO2 <span class="hlt">ice</span> aerosols are clearly distinguished by their distinct scattering and absorption behaviors over the key 2-4 μm wavelength region, and their particle sizes are well determined by the 0.4-3 μm wavelength region. Several key attributes are determined for Mars mesospheric aerosols. Dust aerosols are largely undetected, and are apparently injected to such heights only during global dust storms (Clancy et al, 2010). <span class="hlt">Ice</span> clouds are generally common at 55-75 km altitudes, although in separate halves of the Mars year. CO2 and H2O <span class="hlt">ice</span> clouds are most prominent during the aphelion and perihelion portions of the Mars orbit, respectively. CO2 <span class="hlt">ice</span> clouds, which occur at low latitudes over specific surface longitudes, present distinct particle size populations ranging from 0.5 to 1.5 μm (Reff). Mesospheric H2O <span class="hlt">ice</span> clouds exhibit somewhat smaller particle sizes (Reff=0.3-1 μm) and extend over low to mid latitudes. This orbital dependence for mesospheric <span class="hlt">ice</span> aerosol <span class="hlt">composition</span> indicates extreme annual (orbital) variation in mesospheric</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.C33E..08N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C33E..08N"><span>Arctic Sea <span class="hlt">Ice</span> Classification and Mapping for Surface Albedo Parameterization in Sea <span class="hlt">Ice</span> Modeling</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nghiem, S. V.; Clemente-Colón, P.; Perovich, D. K.; Polashenski, C.; Simpson, W. R.; Rigor, I. G.; Woods, J. E.; Nguyen, D. T.; Neumann, G.</p> <p>2016-12-01</p> <p>A regime shift of Arctic sea <span class="hlt">ice</span> from predominantly perennial sea <span class="hlt">ice</span> (multi-year <span class="hlt">ice</span> or MYI) to seasonal sea <span class="hlt">ice</span> (first-year <span class="hlt">ice</span> or FYI) has occurred in recent decades. This shift has profoundly altered the proportional <span class="hlt">composition</span> of different sea <span class="hlt">ice</span> classes and the surface albedo distribution pertaining to each sea <span class="hlt">ice</span> class. Such changes impacts physical, chemical, and biological processes in the Arctic atmosphere-<span class="hlt">ice</span>-ocean system. The drastic changes upset the traditional geophysical representation of surface albedo of the Arctic sea <span class="hlt">ice</span> cover in current models. A critical science issue is that these profound changes must be rigorously and systematically observed and characterized to enable a transformative re-parameterization of key model inputs, such as <span class="hlt">ice</span> surface albedo, to <span class="hlt">ice</span>-ocean-atmosphere climate modeling in order to obtain re-analyses that accurately reproduce Arctic changes and also to improve sea <span class="hlt">ice</span> and weather forecast models. Addressing this challenge is a strategy identified by the National Research Council study on "Seasonal to Decadal Predictions of Arctic Sea <span class="hlt">Ice</span> - Challenges and Strategies" to replicate the new Arctic reality. We review results of albedo characteristics associated with different sea <span class="hlt">ice</span> classes such as FYI and MYI. Then we demonstrate the capability for sea <span class="hlt">ice</span> classification and mapping using algorithms developed by the Jet Propulsion Laboratory and by the U.S. National <span class="hlt">Ice</span> Center for use with multi-sourced satellite radar data at L, C, and Ku bands. Results obtained with independent algorithms for different radar frequencies consistently identify sea <span class="hlt">ice</span> classes and thereby cross-verify the sea <span class="hlt">ice</span> classification methods. Moreover, field observations obtained from buoy webcams and along an extensive trek across Elson Lagoon and a sector of the Beaufort Sea during the BRomine, Ozone, and Mercury EXperiment (BROMEX) in March 2012 are used to validate satellite products of sea <span class="hlt">ice</span> classes. This research enables the mapping</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20130012682','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20130012682"><span><span class="hlt">Composite</span> Aerogel Multifoil Protective Shielding</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Jones, Steven M.</p> <p>2013-01-01</p> <p>New technologies are needed to survive the temperatures, radiation, and hypervelocity particles that exploration spacecraft encounter. Multilayer <span class="hlt">insulations</span> (MLIs) have been used on many spacecraft as thermal <span class="hlt">insulation</span>. Other materials and <span class="hlt">composites</span> have been used as micrometeorite shielding or radiation shielding. However, no material <span class="hlt">composite</span> has been developed and employed as a combined thermal <span class="hlt">insulation</span>, micrometeorite, and radiation shielding. By replacing the scrims that have been used to separate the foil layers in MLIs with various aerogels, and by using a variety of different metal foils, the overall protective performance of MLIs can be greatly expanded to act as thermal <span class="hlt">insulation</span>, radiation shielding, and hypervelocity particle shielding. Aerogels are highly porous, low-density solids that are produced by the gelation of metal alkoxides and supercritical drying. Aerogels have been flown in NASA missions as a hypervelocity particle capture medium (Stardust) and as thermal <span class="hlt">insulation</span> (2003 MER). <span class="hlt">Composite</span> aerogel multifoil protective shielding would be used to provide thermal <span class="hlt">insulation</span>, while also shielding spacecraft or components from radiation and hypervelocity particle impacts. Multiple layers of foil separated by aerogel would act as a thermal barrier by preventing the transport of heat energy through the <span class="hlt">composite</span>. The silica aerogel would act as a convective and conductive thermal barrier, while the titania powder and metal foils would absorb and reflect the radiative heat. It would also capture small hypervelocity particles, such as micrometeorites, since it would be a stuffed, multi-shock Whipple shield. The metal foil layers would slow and break up the impacting particles, while the aerogel layers would convert the kinetic energy of the particles to thermal and mechanical energy and stop the particles.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24750909','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24750909"><span>Preparation of conductive <span class="hlt">paper</span> <span class="hlt">composites</span> based on natural cellulosic fibers for packaging applications.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Youssef, Ahmed M; El-Samahy, Magda Ali; Abdel Rehim, Mona H</p> <p>2012-08-01</p> <p>Conducting <span class="hlt">paper</span> based on natural cellulosic fibers and conductive polymers was prepared using unbleached bagasse and/or rice straw fibers (as cellulosic raw materials) and polyaniline (PANi) as conducting polymer. These <span class="hlt">composites</span> were synthesized by in situ emulsion polymerization using ammonium persulfate (APS) as oxidant in the presence of dodecylbenzene sulfonic acid (DBSA) as emulsifier. The prepared <span class="hlt">composites</span> were characterized using Fourier transform infrared (FTIR), thermal gravimetric analysis (TGA), differential scanning calorimeter (DSC), and their morphology was investigated using scanning electron microscope (SEM). Electrical conductivity measurements showed that the conductivity of the <span class="hlt">paper</span> sheets increases by increasing the ratio of PANi in the <span class="hlt">composite</span>. Mechanical properties of the <span class="hlt">paper</span> sheets were also investigated, the results revealed that the values of breaking length, burst factor, and tear factor are decreased with increasing ratio of added PANi, and this effect is more pronounced in bagasse-based <span class="hlt">composites</span>. The new conductive <span class="hlt">composites</span> can have potential use as anti-static packaging material or anti-bacterial <span class="hlt">paper</span> for packaging applications. Copyright © 2012 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.P54B..04C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.P54B..04C"><span>Radar Detection of Layering in <span class="hlt">Ice</span>: Experiments on a Constructed Layered <span class="hlt">Ice</span> Sheet</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Carter, L. M.; Koenig, L.; Courville, Z.; Ghent, R. R.; Koutnik, M. R.</p> <p>2016-12-01</p> <p>The polar caps and glaciers of both Earth and Mars display internal layering that preserves a record of past climate. These layers are apparent both in optical datasets (high resolution images, core samples) and in ground penetrating radar (GPR) data. On Mars, the SHARAD (Shallow Radar) radar on the Mars Reconnaissance Orbiter shows fine layering that changes spatially and with depth across the polar caps. This internal layering has been attributed to changes in fractional dust contamination due to obliquity-induced climate variations, but there are other processes that can lead to internal layers visible in radar data. In particular, terrestrial sounding of <span class="hlt">ice</span> sheets compared with core samples have revealed that <span class="hlt">ice</span> density and <span class="hlt">composition</span> differences account for the majority of the radar reflectors. The large cold rooms and <span class="hlt">ice</span> laboratory facility at the U.S. Army Cold Regions Research and Engineering Laboratory (CRREL) provide us a unique opportunity to construct experimental <span class="hlt">ice</span> sheets in a controlled setting and measure them with radar. In a CRREL laboratory, we constructed a layered <span class="hlt">ice</span> sheet that is 3-m deep with a various snow and <span class="hlt">ice</span> layers with known dust concentrations (using JSC Mars-1 basaltic simulant) and density differences. These <span class="hlt">ice</span> sheets were profiled using a commercial GPR, at frequencies of 200, 400 and 900 MHz, to determine how the radar profile changes due to systematic and known changes in snow and <span class="hlt">ice</span> layers, including layers with sub-wavelength spacing. We will report results from these experiments and implications for interpreting radar-detected layering in <span class="hlt">ice</span> on Earth and Mars.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015NatSR...5E7931W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015NatSR...5E7931W"><span>Intrinsic Topological <span class="hlt">Insulator</span> Bi1.5Sb0.5Te3-xSex Thin Crystals</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wang, Wei; Li, Li; Zou, Wenqin; He, Liang; Song, Fengqi; Zhang, Rong; Wu, Xiaoshan; Zhang, Fengming</p> <p>2015-01-01</p> <p>The quaternary topological <span class="hlt">insulator</span> (Bi,Sb)2(Te,Se)3 has demonstrated topological surface states with an <span class="hlt">insulating</span> bulk. Scientists have identified an optimized <span class="hlt">composition</span> of Bi1.5Sb0.5Te1.7Se1.3 with the highest resistivity reported. But the physics that drive to this <span class="hlt">composition</span> remains unclear. Here we report the crystal structure and the magneto-transport properties of Bi1.5Sb0.5Te3-xSex (BSTS) series. A correlation between the structure and the physical properties has been revealed. We found out that within the rhombohedral structure, the <span class="hlt">composition</span> with most Te substituting Se has the highest resistivity. On the other hand, segregation of other <span class="hlt">composition</span> phases will introduce much higher bulk concentration.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018TCry...12.1957A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018TCry...12.1957A"><span>Microtopographic control on the ground thermal regime in <span class="hlt">ice</span> wedge polygons</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Abolt, Charles J.; Young, Michael H.; Atchley, Adam L.; Harp, Dylan R.</p> <p>2018-06-01</p> <p>The goal of this research is to constrain the influence of <span class="hlt">ice</span> wedge polygon microtopography on near-surface ground temperatures. <span class="hlt">Ice</span> wedge polygon microtopography is prone to rapid deformation in a changing climate, and cracking in the <span class="hlt">ice</span> wedge depends on thermal conditions at the top of the permafrost; therefore, feedbacks between microtopography and ground temperature can shed light on the potential for future <span class="hlt">ice</span> wedge cracking in the Arctic. We first report on a year of sub-daily ground temperature observations at 5 depths and 9 locations throughout a cluster of low-centered polygons near Prudhoe Bay, Alaska, and demonstrate that the rims become the coldest zone of the polygon during winter, due to thinner snowpack. We then calibrate a polygon-scale numerical model of coupled thermal and hydrologic processes against this dataset, achieving an RMSE of less than 1.1 °C between observed and simulated ground temperature. Finally, we conduct a sensitivity analysis of the model by systematically manipulating the height of the rims and the depth of the troughs and tracking the effects on <span class="hlt">ice</span> wedge temperature. The results indicate that winter temperatures in the <span class="hlt">ice</span> wedge are sensitive to both rim height and trough depth, but more sensitive to rim height. Rims act as preferential outlets of subsurface heat; increasing rim size decreases winter temperatures in the <span class="hlt">ice</span> wedge. Deeper troughs lead to increased snow entrapment, promoting <span class="hlt">insulation</span> of the <span class="hlt">ice</span> wedge. The potential for <span class="hlt">ice</span> wedge cracking is therefore reduced if rims are destroyed or if troughs subside, due to warmer conditions in the <span class="hlt">ice</span> wedge. These findings can help explain the origins of secondary <span class="hlt">ice</span> wedges in modern and ancient polygons. The findings also imply that the potential for re-establishing rims in modern thermokarst-affected terrain will be limited by reduced cracking activity in the <span class="hlt">ice</span> wedges, even if regional air temperatures stabilize.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29016475','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29016475"><span>Relationship between Physiological Off-<span class="hlt">Ice</span> Testing, On-<span class="hlt">Ice</span> Skating, and Game Performance in Division I Women's <span class="hlt">Ice</span> Hockey Players.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Boland, Michelle; Miele, Emily M; Delude, Katie</p> <p>2017-10-07</p> <p>The purpose was to identify off-<span class="hlt">ice</span> testing variables that correlate to skating and game performance in Division I collegiate women <span class="hlt">ice</span> hockey players. Twenty female, forward and defensive players (19.95 ± 1.35 yr) were assessed for weight, height, percent fat mass (%FAT), bone mineral density, predicted one repetition maximum (RM) absolute and relative (REL%) bench press (BP) and hex bar deadlift (HDL), lower body explosive power, anaerobic power, countermovement vertical jump (CMJ), maximum inspiratory pressure (MIP), and on-<span class="hlt">ice</span> repeated skate sprint (RSS) performance. The on-<span class="hlt">ice</span> RSS test included 6 timed 85.6 m sprints with participants wearing full hockey equipment; fastest time (FT), average time (AT) and fatigue index (FI) for the first length skate (FLS; 10 m) and total length skate (TLS; 85.6 m) were used for analysis. Game performance was evaluated with game statistics: goals, assists, points, plus-minus, and shots on goal (SOG). Correlation coefficients were used to determine relationships. Percent fat mass was positively correlated (p < 0.05) with FLS-FI and TLS-AT; TLS-FT was negatively correlated with REL%HDL; BP-RM was negatively correlated with FLS-FT and FLS-AT; MIP positively correlated with assists, points, and SOG; FLS-AT negatively correlated with assists. Game performance in women <span class="hlt">ice</span> hockey players may be enhanced by greater MIP, repeat acceleration ability, and mode-specific training. Faster skating times were associated with lower %FAT. Skating performance in women <span class="hlt">ice</span> hockey players may be enhanced by improving body <span class="hlt">composition</span>, anaerobic power, and both lower and upper body strength in off-<span class="hlt">ice</span> training.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ChPhL..35e7301D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ChPhL..35e7301D"><span>Atomic-Ordering-Induced Quantum Phase Transition between Topological Crystalline <span class="hlt">Insulator</span> and Z 2 Topological <span class="hlt">Insulator</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Deng, Hui-Xiong; Song, Zhi-Gang; Li, Shu-Shen; Wei, Su-Huai; Luo, Jun-Wei</p> <p>2018-05-01</p> <p>Topological phase transition in a single material usually refers to transitions between a trivial band <span class="hlt">insulator</span> and a topological Dirac phase, but the transition may also occur between different classes of topological Dirac phases. However, it is a fundamental challenge to realize quantum transition between Z2 nontrivial topological <span class="hlt">insulator</span> (TI) and topological crystalline <span class="hlt">insulator</span> (TCI) in one material because Z2 TI and TCI are hardly both co-exist in a single material due to their contradictory requirement on the number of band inversions. The Z2 TIs must have an odd number of band inversions over all the time-reversal invariant momenta, whereas, the newly discovered TCIs, as a distinct class of the topological Dirac materials protected by the underlying crystalline symmetry, owns an even number of band inversions. Here, take PbSnTe2 alloy as an example, we show that at proper alloy <span class="hlt">composition</span> the atomic-ordering is an effective way to tune the symmetry of the alloy so that we can electrically switch between TCI phase and Z2 TI phase when the alloy is ordered from a random phase into a stable CuPt phase. Our results suggest that atomic-ordering provides a new platform to switch between different topological phases.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.A13A2051K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A13A2051K"><span>Immersion Freezing of Aluminas: The Effect of Crystallographic Properties on <span class="hlt">Ice</span> Nucleation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>King, M.; Chong, E.; Freedman, M. A.</p> <p>2017-12-01</p> <p>Atmospheric aerosol particles serve as the nuclei for heterogeneous <span class="hlt">ice</span> nucleation, a process that allows for <span class="hlt">ice</span> to form at higher temperatures and lower supersaturations with respect to <span class="hlt">ice</span>. This process is essential to the formation of <span class="hlt">ice</span> in cirrus clouds. Heterogeneous <span class="hlt">ice</span> nucleation is affected by many factors including the <span class="hlt">composition</span>, crystal structure, porosity, and surface area of the particles. However, these factors are not well understood and, as such, are difficult to account for in climate models. To test the effects of crystal structure on <span class="hlt">ice</span> nucleation, a system of transition aluminas (Al2O3) that differ only in their crystal structure, despite being <span class="hlt">compositionally</span> similar, were tested using immersion freezing. Particles were immersed in water and placed into a temperature controlled chamber. Freezing events were then recorded as the chamber was cooled to negative 30 °. Alpha-alumina, which is a member of the hexagonal crystal system, showed a significantly higher temperature at which all particles froze in comparison to other samples. This supports the hypothesis that, since a hexagonal crystal structure is the lowest energy state for <span class="hlt">ice</span>, hexagonal surface structures would best facilitate <span class="hlt">ice</span> nucleation. However, a similar sample of hexagonal chi-alumina did not show the same results. Further analysis of the samples will be done to characterize surface structures and <span class="hlt">composition</span>. These conflicting data sets raise interesting questions about the effect of other surface features, such as surface area and porosity, on <span class="hlt">ice</span> nucleation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017TCry...11.2033D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017TCry...11.2033D"><span><span class="hlt">Ice</span> bridges and ridges in the Maxwell-EB sea <span class="hlt">ice</span> rheology</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dansereau, Véronique; Weiss, Jérôme; Saramito, Pierre; Lattes, Philippe; Coche, Edmond</p> <p>2017-09-01</p> <p>This <span class="hlt">paper</span> presents a first implementation of a new rheological model for sea <span class="hlt">ice</span> on geophysical scales. This continuum model, called Maxwell elasto-brittle (Maxwell-EB), is based on a Maxwell constitutive law, a progressive damage mechanism that is coupled to both the elastic modulus and apparent viscosity of the <span class="hlt">ice</span> cover and a Mohr-Coulomb damage criterion that allows for pure (uniaxial and biaxial) tensile strength. The model is tested on the basis of its capability to reproduce the complex mechanical and dynamical behaviour of sea <span class="hlt">ice</span> drifting through a narrow passage. Idealized as well as realistic simulations of the flow of <span class="hlt">ice</span> through Nares Strait are presented. These demonstrate that the model reproduces the formation of stable <span class="hlt">ice</span> bridges as well as the stoppage of the flow, a phenomenon occurring within numerous channels of the Arctic. In agreement with observations, the model captures the propagation of damage along narrow arch-like kinematic features, the discontinuities in the velocity field across these features dividing the <span class="hlt">ice</span> cover into floes, the strong spatial localization of the thickest, ridged <span class="hlt">ice</span>, the presence of landfast <span class="hlt">ice</span> in bays and fjords and the opening of polynyas downstream of the strait. The model represents various dynamical behaviours linked to an overall weakening of the <span class="hlt">ice</span> cover and to the shorter lifespan of <span class="hlt">ice</span> bridges, with implications in terms of increased <span class="hlt">ice</span> export through narrow outflow pathways of the Arctic.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017MS%26E..279a2006L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017MS%26E..279a2006L"><span>Cryogenic electrical properties of irradiated cyanate ester/epoxy <span class="hlt">insulation</span> for fusion magnets</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Li, X.; Wu, Z. X.; Li, J.; Xu, D.; Liu, H. M.; Huang, R. J.; Li, L. F.</p> <p>2017-12-01</p> <p>The <span class="hlt">insulation</span> materials used in high field fusion magnets require excellent mechanical properties, high electrical breakdown strength, good thermal conductivity and high radiation tolerance. Previous investigations showed that cyanate ester/epoxy (CE/EP) <span class="hlt">insulation</span> material, a candidate <span class="hlt">insulation</span> for fusion magnets, can maintain good mechanical performance at cryogenic temperature after 10 MGy irradiation and has a much longer pot life than traditional epoxy <span class="hlt">insulation</span> material. In order to quantify the electrical properties of the CE/EP <span class="hlt">insulation</span> material at low temperature, a cryogenic electrical property testing system cooled by a G-M cryocooler was developed for this study. An <span class="hlt">insulation</span> material with 40% cyanate ester and 60% epoxy was subjected to 60Co γ-ray irradiation in air at ambient temperature with a dose rate of 300 Gy/min, and total doses of 1 MGy, 5 MGy and 10 MGy. The electrical breakdown strength of this CE/EP <span class="hlt">insulation</span> material was measured before and after irradiation. The results show that cryogenic temperature has a positive effect on the electrical breakdown strength of this <span class="hlt">composite</span>, while the influence of 60Co γ-ray irradiation is not obvious at 6.1 K.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AAS...22220202O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AAS...22220202O"><span>Interstellar <span class="hlt">Ice</span> Chemistry: From Water to Complex Organics</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Oberg, Karin I.; Fayolle, E.; Linnartz, H.; van Dishoeck, E.; Fillion, J.; Bertin, M.</p> <p>2013-06-01</p> <p>Molecular cloud cores, protostellar envelopes and protoplanetary disk midplanes are all characterized by freeze-out of atoms and molecules (other than H and H2) onto interstellar dust grains. On the grain surface, atom addition reactions, especially hydrogenation, are efficient and H2O forms readily from O, CH3OH from CO etc. The result is an icy mantle typically dominated by H2O, but also rich in CO2, CO, NH3, CH3OH and CH4. These <span class="hlt">ices</span> are further processed through interactions with radiation, electrons and energetic particles. Because of the efficiency of the freeze-out process, and the complex chemistry that succeeds it, these icy grain mantles constitute a major reservoir of volatiles during star formation and are also the source of much of the chemical evolution observed in star forming regions. Laboratory experiments allow us to explore how molecules and radicals desorb, dissociate, diffuse and react in <span class="hlt">ices</span> when exposed to different sources of energy. Changes in <span class="hlt">ice</span> <span class="hlt">composition</span> and structure is constrained using infrared spectroscopy and mass spectrometry. By comparing <span class="hlt">ice</span> desorption, segregation, and chemistry efficiencies under different experimental conditions, we can characterize the basic <span class="hlt">ice</span> processes, e.g. diffusion of different species, that underpin the observable changes in <span class="hlt">ice</span> <span class="hlt">composition</span> and structure. This information can then be used to predict the interstellar <span class="hlt">ice</span> chemical evolution. I will review some of the key laboratory discoveries on <span class="hlt">ice</span> chemistry during the past few years and how they have been used to predict and interpret astronomical observations of <span class="hlt">ice</span> bands and gas-phase molecules associated with <span class="hlt">ice</span> evaporation. These include measurements of thermal diffusion in and evaporation from <span class="hlt">ice</span> mixtures, non-thermal diffusion efficiencies (including the recent results on frequency resolved UV photodesorption), and the expected temperature dependencies of the complex <span class="hlt">ice</span> chemistry regulated by radical formation and diffusion. Based on these</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015PhDT.......260M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015PhDT.......260M"><span>Systematic Studies of Cosmic-Ray Anisotropy and Energy Spectrum with <span class="hlt">Ice</span>Cube and <span class="hlt">Ice</span>Top</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>McNally, Frank</p> <p></p> <p>Anisotropy in the cosmic-ray arrival direction distribution has been well documented over a large energy range, but its origin remains largely a mystery. In the TeV to PeV energy range, the galactic magnetic field thoroughly scatters cosmic rays, but anisotropy at the part-per-mille level and smaller persists, potentially carrying information about nearby cosmic-ray accelerators and the galactic magnetic field. The <span class="hlt">Ice</span>Cube Neutrino Observatory was the first detector to observe anisotropy at these energies in the Southern sky. This work uses 318 billion cosmic-ray induced muon events, collected between May 2009 and May 2015 from both the in-<span class="hlt">ice</span> component of <span class="hlt">Ice</span>Cube as well as the surface component, <span class="hlt">Ice</span>Top. The observed global anisotropy features large regions of relative excess and deficit, with amplitudes on the order of 10-3. While a decomposition of the arrival direction distribution into spherical harmonics shows that most of the power is contained in the low-multipole (ℓ ≤ 4) moments, higher-multipole components are found to be statistically significant down to an angular scale of less than 10°, approaching the angular resolution of the detector. Above 100TeV, a change in the topology of the arrival direction distribution is observed, and the anisotropy is characterized by a wide relative deficit whose amplitude increases with primary energy up to at least 5PeV, the highest energies currently accessible to <span class="hlt">Ice</span>Cube with sufficient event statistics. No time dependence of the large- and small-scale structures is observed in the six-year period covered by this analysis within statistical and systematic uncertainties. Analysis of the energy spectrum and <span class="hlt">composition</span> in the PeV energy range as a function of sky position is performed with <span class="hlt">Ice</span>Top data over a five-year period using a likelihood-based reconstruction. Both the energy spectrum and the <span class="hlt">composition</span> distribution are found to be consistent with a single source population over declination bands. This work</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5375860','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5375860"><span>Characterization of Textile-<span class="hlt">Insulated</span> Capacitive Biosensors</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Ng, Charn Loong; Reaz, Mamun Bin Ibne</p> <p>2017-01-01</p> <p>Capacitive biosensors are an emerging technology revolutionizing wearable sensing systems and personal healthcare devices. They are capable of continuously measuring bioelectrical signals from the human body while utilizing textiles as an <span class="hlt">insulator</span>. Different textile types have their own unique properties that alter skin-electrode capacitance and the performance of capacitive biosensors. This <span class="hlt">paper</span> aims to identify the best textile <span class="hlt">insulator</span> to be used with capacitive biosensors by analysing the characteristics of 6 types of common textile materials (cotton, linen, rayon, nylon, polyester, and PVC-textile) while evaluating their impact on the performance of a capacitive biosensor. A textile-<span class="hlt">insulated</span> capacitive (TEX-C) biosensor was developed and validated on 3 subjects. Experimental results revealed that higher skin-electrode capacitance of a TEX-C biosensor yields a lower noise floor and better signal quality. Natural fabric such as cotton and linen were the two best <span class="hlt">insulating</span> materials to integrate with a capacitive biosensor. They yielded the lowest noise floor of 2 mV and achieved consistent electromyography (EMG) signals measurements throughout the performance test. PMID:28287493</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012ESASP.691E..35N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012ESASP.691E..35N"><span>Parameter Identification Of Multilayer Thermal <span class="hlt">Insulation</span> By Inverse Problems</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nenarokomov, Aleksey V.; Alifanov, Oleg M.; Gonzalez, Vivaldo M.</p> <p>2012-07-01</p> <p>The purpose of this <span class="hlt">paper</span> is to introduce an iterative regularization method in the research of radiative and thermal properties of materials with further applications in the design of Thermal Control Systems (TCS) of spacecrafts. In this <span class="hlt">paper</span> the radiative and thermal properties (heat capacity, emissivity and thermal conductance) of a multilayered thermal-<span class="hlt">insulating</span> blanket (MLI), which is a screen-vacuum thermal <span class="hlt">insulation</span> as a part of the (TCS) for perspective spacecrafts, are estimated. Properties of the materials under study are determined in the result of temperature and heat flux measurement data processing based on the solution of the Inverse Heat Transfer Problem (IHTP) technique. Given are physical and mathematical models of heat transfer processes in a specimen of the multilayered thermal-<span class="hlt">insulating</span> blanket located in the experimental facility. A mathematical formulation of the IHTP, based on sensitivity function approach, is presented too. The practical testing was performed for specimen of the real MLI. This <span class="hlt">paper</span> consists of recent researches, which developed the approach suggested at [1].</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li class="active"><span>18</span></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_18 --> <div id="page_19" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li class="active"><span>19</span></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="361"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JAP...122k5105H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JAP...122k5105H"><span>Sharp improvement of flashover strength from <span class="hlt">composite</span> micro-textured surfaces</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Huo, Yankun; Liu, Wenyuan; Ke, Changfeng; Chang, Chao; Chen, Changhua</p> <p>2017-09-01</p> <p>A <span class="hlt">composite</span> micro-textured surface structure is proposed and demonstrated to enhance the surface flashover strength of polymer <span class="hlt">insulators</span> used in vacuum. The structure is fabricated in two stages, with periodic triangular grooves of approximately 210 μm in width formed in the first stage and micro-holes of approximately 2 μm coated on the inner surface of grooves in the second. The aim is to exploit the synergistic effects between the grooves and micro-holes to suppress the secondary electron yield to obtain a better flashover performance. To acquire <span class="hlt">insulators</span> with the <span class="hlt">composite</span> micro-textured surface, the CO2 laser processing technique is applied to treat the surface of the PMMA <span class="hlt">insulators</span>. The test results show that the flashover voltages of the <span class="hlt">insulators</span> with the two-stage fabricated structure increase by 150% compared with the untreated samples in the best state. Compared with the traditional macro-groove structures on <span class="hlt">insulators</span>, the proposed <span class="hlt">composite</span> micro-textured <span class="hlt">insulators</span> exhibit a better surface flashover performance.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20080040137&hterms=AES&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3DAES','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20080040137&hterms=AES&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3DAES"><span>Comparison of NASA Team2 and AES-York <span class="hlt">Ice</span> Concentration Algorithms Against Operational <span class="hlt">Ice</span> Charts From the Canadian <span class="hlt">Ice</span> Service</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Shokr, Mohammed; Markus, Thorsten</p> <p>2006-01-01</p> <p><span class="hlt">Ice</span> concentration retrieved from spaceborne passive-microwave observations is a prime input to operational sea-<span class="hlt">ice</span>-monitoring programs, numerical weather prediction models, and global climate models. Atmospheric Environment Service (AES)- York and the Enhanced National Aeronautics and Space Administration Team (NT2) are two algorithms that calculate <span class="hlt">ice</span> concentration from Special Sensor Microwave/Imager observations. This <span class="hlt">paper</span> furnishes a comparison between <span class="hlt">ice</span> concentrations (total, thin, and thick types) output from NT2 and AES-York algorithms against the corresponding estimates from the operational analysis of Radarsat images in the Canadian <span class="hlt">Ice</span> Service (CIS). A new data fusion technique, which incorporates the actual sensor's footprint, was developed to facilitate this study. Results have shown that the NT2 and AES-York algorithms underestimate total <span class="hlt">ice</span> concentration by 18.35% and 9.66% concentration counts on average, with 16.8% and 15.35% standard deviation, respectively. However, the retrieved concentrations of thin and thick <span class="hlt">ice</span> are in much more discrepancy with the operational CIS estimates when either one of these two types dominates the viewing area. This is more likely to occur when the total <span class="hlt">ice</span> concentration approaches 100%. If thin and thick <span class="hlt">ice</span> types coexist in comparable concentrations, the algorithms' estimates agree with CIS'S estimates. In terms of <span class="hlt">ice</span> concentration retrieval, thin <span class="hlt">ice</span> is more problematic than thick <span class="hlt">ice</span>. The concept of using a single tie point to represent a thin <span class="hlt">ice</span> surface is not realistic and provides the largest error source for retrieval accuracy. While AES-York provides total <span class="hlt">ice</span> concentration in slightly more agreement with CIS'S estimates, NT2 provides better agreement in retrieving thin and thick <span class="hlt">ice</span> concentrations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EPJWC.14501003D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EPJWC.14501003D"><span>Investigating cosmic rays and air shower physics with <span class="hlt">IceCube/Ice</span>Top</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dembinski, Hans</p> <p>2017-06-01</p> <p><span class="hlt">Ice</span>Cube is a cubic-kilometer detector in the deep <span class="hlt">ice</span> at South Pole. Its square-kilometer surface array, <span class="hlt">Ice</span>Top, is located at 2800 m altitude. <span class="hlt">Ice</span>Top is large and dense enough to cover the cosmic-ray energy spectrum from PeV to EeV energies with a remarkably small systematic uncertainty, thanks to being close to the shower maximum. The experiment offers new insights into hadronic physics of air showers by observing three components: the electromagnetic signal at the surface, GeV muons in the periphery of the showers, and TeV muons in the deep <span class="hlt">ice</span>. The cosmic-ray flux is measured with the surface signal. The mass <span class="hlt">composition</span> is extracted from the energy loss of TeV muons observed in the deep <span class="hlt">ice</span> in coincidence with signals at the surface. The muon lateral distribution is obtained from GeV muons identified in surface signals in the periphery of the shower. The energy spectrum of the most energetic TeV muons is also under study, as well as special events with laterally separated TeV muon tracks which originate from high-pT TeV muons. A combination of all these measurements opens the possibility to perform powerful new tests of hadronic interaction models used to simulate air showers. The latest results will be reviewed from this perspective.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1982Natur.298..830T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1982Natur.298..830T"><span>Space Shuttle <span class="hlt">ice</span> nuclei</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Turco, R. P.; Toon, O. B.; Whitten, R. C.; Cicerone, R. J.</p> <p>1982-08-01</p> <p>Estimates are made showing that, as a consequence of rocket activity in the earth's upper atmosphere in the Shuttle era, average <span class="hlt">ice</span> nuclei concentrations in the upper atmosphere could increase by a factor of two, and that an aluminum dust layer weighing up to 1000 tons might eventually form in the lower atmosphere. The concentrations of Space Shuttle <span class="hlt">ice</span> nuclei (SSIN) in the upper troposphere and lower stratosphere were estimated by taking into account the <span class="hlt">composition</span> of the particles, the extent of surface poisoning, and the size of the particles. Calculated stratospheric size distributions at 20 km with Space Shuttle particulate injection, calculated SSIN concentrations at 10 and 20 km altitude corresponding to different water vapor/<span class="hlt">ice</span> supersaturations, and predicted SSIN concentrations in the lower stratosphere and upper troposphere are shown.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4800274','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4800274"><span><span class="hlt">Insulated</span> Foamy Viral Vectors</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Browning, Diana L.; Collins, Casey P.; Hocum, Jonah D.; Leap, David J.; Rae, Dustin T.; Trobridge, Grant D.</p> <p>2016-01-01</p> <p>Retroviral vector-mediated gene therapy is promising, but genotoxicity has limited its use in the clinic. Genotoxicity is highly dependent on the retroviral vector used, and foamy viral (FV) vectors appear relatively safe. However, internal promoters may still potentially activate nearby genes. We developed <span class="hlt">insulated</span> FV vectors, using four previously described <span class="hlt">insulators</span>: a version of the well-studied chicken hypersensitivity site 4 <span class="hlt">insulator</span> (650cHS4), two synthetic CCCTC-binding factor (CTCF)-based <span class="hlt">insulators</span>, and an <span class="hlt">insulator</span> based on the CCAAT box-binding transcription factor/nuclear factor I (7xCTF/NF1). We directly compared these <span class="hlt">insulators</span> for enhancer-blocking activity, effect on FV vector titer, and fidelity of transfer to both proviral long terminal repeats. The synthetic CTCF-based <span class="hlt">insulators</span> had the strongest <span class="hlt">insulating</span> activity, but reduced titers significantly. The 7xCTF/NF1 <span class="hlt">insulator</span> did not reduce titers but had weak <span class="hlt">insulating</span> activity. The 650cHS4-<span class="hlt">insulated</span> FV vector was identified as the overall most promising vector. Uninsulated and 650cHS4-<span class="hlt">insulated</span> FV vectors were both significantly less genotoxic than gammaretroviral vectors. Integration sites were evaluated in cord blood CD34+ cells and the 650cHS4-<span class="hlt">insulated</span> FV vector had fewer hotspots compared with an uninsulated FV vector. These data suggest that <span class="hlt">insulated</span> FV vectors are promising for hematopoietic stem cell gene therapy. PMID:26715244</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25722036','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25722036"><span>The complete mitochondrial genome of the <span class="hlt">ice</span> pigeon (Columba livia breed <span class="hlt">ice</span>).</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Zhang, Rui-Hua; He, Wen-Xiao</p> <p>2015-02-01</p> <p>The <span class="hlt">ice</span> pigeon is a breed of fancy pigeon developed over many years of selective breeding. In the present work, we report the complete mitochondrial genome sequence of <span class="hlt">ice</span> pigeon for the first time. The total length of the mitogenome was 17,236 bp with the base <span class="hlt">composition</span> of 30.2% for A, 24.0% for T, 31.9% for C, and 13.9% for G and an A-T (54.2 %)-rich feature was detected. It harbored 13 protein-coding genes, 2 ribosomal RNA genes, 22 transfer RNA genes and 1 non-coding control region (D-loop region). The arrangement of all genes was identical to the typical mitochondrial genomes of pigeon. The complete mitochondrial genome sequence of <span class="hlt">ice</span> pigeon would serve as an important data set of the germplasm resources for further study.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20090034380&hterms=europa+glacier&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Deuropa%2Bglacier','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20090034380&hterms=europa+glacier&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Deuropa%2Bglacier"><span>Life in <span class="hlt">Ice</span>: Implications to Astrobiology</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Hoover, Richard B.</p> <p>2009-01-01</p> <p>During the 2008 Tawani International Expedition Schirmacher Oasis/Lake Untersee Antarctica Expedition, living and instantly motile bacteria were found in freshly thawed meltwater from <span class="hlt">ice</span> of the Schirmacher Oasis Lakes, the Anuchin Glacier <span class="hlt">ice</span> and samples of the that perennial <span class="hlt">ice</span> sheet above Lake Untersee. This phenomenon of living bacteria encased in <span class="hlt">ice</span> had previously been observed in the 32,000 year old <span class="hlt">ice</span> of the Fox Tunnel. The bacteria found in this <span class="hlt">ice</span> included the strain FTR1T which was isolated and published as valid new species (Carnobacterium pleistocenium) the first validly published living Pleistocene organism still alive today. Living bacteria were also extracted from ancient <span class="hlt">ice</span> cores from Vostok, Antarctica. The discovery that many strains of bacteria are able to survive and remain alive while frozen in <span class="hlt">ice</span> sheets for long periods of time may have direct relevance to Astrobiology. The abundance of viable bacteria in the <span class="hlt">ice</span> sheets of Antarctica suggests that the presence of live bacteria in <span class="hlt">ice</span> is common, rather than an isolated phenomenon. This <span class="hlt">paper</span> will discuss the results of recent studies at NSSTC of bacteria cryopreserved in <span class="hlt">ice</span>. This <span class="hlt">paper</span> advances the hypothesis that cryopreserved cells, and perhaps even viable bacterial cells, may exist today--frozen in the water-<span class="hlt">ice</span> of lunar craters, the Polar Caps or craters of Mars; or in the permafrost of Mars; <span class="hlt">ice</span> and rocks of comets or water bearing asteroids; or in the frozen crusts of the icy moons of Jupiter and Saturn. The existence of bacterial life in <span class="hlt">ice</span> suggests that it may not be necessary to drill through a thick <span class="hlt">ice</span> crust to reach liquid water seas deep beneath the icy crusts of Europa, Ganymede and Enceladus. The presence of viable bacteria in the <span class="hlt">ice</span> of the Earth s Polar Caps suggests that the possibility that cryo-panspermia (i.e., the trans-planetary transfer of microbial life by impact ejection/spallation of bacteria-rich polar <span class="hlt">ice</span> masses) deserves serious consideration and study as a</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70024786','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70024786"><span>Diffusion model validation and interpretation of stable isotopes in river and lake <span class="hlt">ice</span></span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Ferrick, M.G.; Calkins, D.J.; Perron, N.M.; Cragin, J.H.; Kendall, C.</p> <p>2002-01-01</p> <p>The stable isotope stratigraphy of river- and lake-<span class="hlt">ice</span> archives winter hydroclimatic conditions, and can potentially be used to identify changing water sources or to provide important insights into <span class="hlt">ice</span> formation processes and growth rates. However, accurate interpretations rely on known isotopic fractionation during <span class="hlt">ice</span> growth. A one-dimensional diffusion model of the liquid boundary layer adjacent to an advancing solid interface, originally developed to simulate solute rejection by growing crystals, has been used without verification to describe non-equilibrium fractionation during congelation <span class="hlt">ice</span> growth. Results are not in agreement, suggesting the presence of important uncertainties. In this <span class="hlt">paper</span> we seek validation of the diffusion model for this application using large-scale laboratory experiments with controlled freezing rates and frequent sampling. We obtained consistent, almost constant, isotopic boundary layer thicknesses over a representative range of <span class="hlt">ice</span> growth rates on both quiescent and well-mixed water. With the 18O boundary layer thickness from the laboratory, the model successfully quantified reduced river-<span class="hlt">ice</span> growth rates relative to those of a nearby lake. These results were more representative and easier to obtain than those of a conventional thermal <span class="hlt">ice</span>-growth model. This diffusion model validation and boundary layer thickness determination provide a powerful tool for interpreting the stable isotope stratigraphy of floating <span class="hlt">ice</span>. The laboratory experiment also replicated successive fractionation events in response to a freeze-thaw-refreeze cycle, providing a mechanism for apparent <span class="hlt">ice</span> fractionation that exceeds equilibrium. Analysis of the <span class="hlt">composition</span> of snow <span class="hlt">ice</span> and frazil <span class="hlt">ice</span> in river and lake cores indicated surprising similarities between these <span class="hlt">ice</span> forms. Published in 2002 by John Wiley & Sons, Ltd.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JEMat..46.4414S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JEMat..46.4414S"><span>Experimental Evaluation and Comparison of Thermal Conductivity of High-Voltage <span class="hlt">Insulation</span> Materials for Vacuum Electronic Devices</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Suresh, C.; Srikrishna, P.</p> <p>2017-07-01</p> <p>Vacuum electronic devices operate with very high voltage differences between their sub-assemblies which are separated by very small distances. These devices also emit large amounts of heat that needs to be dissipated. Hence, there exists a requirement for high-voltage <span class="hlt">insulators</span> with good thermal conductivity for voltage isolation and efficient heat dissipation. However, these voltage <span class="hlt">insulators</span> are generally poor conductors of heat. In the present work, an effort has been made to obtain good high-voltage <span class="hlt">insulation</span> materials with substantial improvement in their thermal conductivity. New mixtures of <span class="hlt">composites</span> were formed by blending varying percentages (by volumes) of aluminum nitride powders with that of neat room-temperature vulcanizing (RTV) silicone elastomer compound. In this work, a thermal conductivity test setup has been devised for the quantification of the thermal conductivity of the <span class="hlt">insulators</span>. The thermal conductivities and high-voltage isolation capabilities of various blended <span class="hlt">composites</span> were quantified and were compared with that of neat RTV to evaluate the relative improvement.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JPhCS.897a2007K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JPhCS.897a2007K"><span>Irradiation effect of the <span class="hlt">insulating</span> materials for fusion superconducting magnets at cryogenic temperature</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kobayashi, Koji; Akiyama, Yoko; Nishijima, Shigehiro</p> <p>2017-09-01</p> <p>In ITER, superconducting magnets should be used in such severe environment as high fluence of fast neutron, cryogenic temperature and large electromagnetic forces. <span class="hlt">Insulating</span> material is one of the most sensitive component to radiation. So radiation resistance on mechanical properties at cryogenic temperature are required for <span class="hlt">insulating</span> material. The purpose of this study is to evaluate irradiation effect of <span class="hlt">insulating</span> material at cryogenic temperature by gamma-ray irradiation. Firstly, glass fiber reinforced plastic (GFRP) and hybrid <span class="hlt">composite</span> were prepared. After irradiation at room temperature (RT) or liquid nitrogen temperature (LNT, 77 K), interlaminar shear strength (ILSS) and glass-transition temperature (Tg) measurement were conducted. It was shown that <span class="hlt">insulating</span> materials irradiated at room temperature were much degraded than those at cryogenic temperature.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1425052-dirac-electron-mediated-magnetic-proximity-effect-topological-insulator-magnetic-insulator-heterostructures','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1425052-dirac-electron-mediated-magnetic-proximity-effect-topological-insulator-magnetic-insulator-heterostructures"><span>Dirac-electron-mediated magnetic proximity effect in topological <span class="hlt">insulator</span>/magnetic <span class="hlt">insulator</span> heterostructures</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Li, Mingda; Song, Qichen; Zhao, Weiwei</p> <p></p> <p>The possible realization of dissipationless chiral edge current in a topological <span class="hlt">insulator</span>/magnetic <span class="hlt">insulator</span> heterostructure is based on the condition that the magnetic proximity exchange coupling at the interface is dominated by the Dirac surface states of the topological <span class="hlt">insulator</span>. We report a polarized neutron reflectometry observation of Dirac-electron-mediated magnetic proximity effect in a bulk-<span class="hlt">insulating</span> topological <span class="hlt">insulator</span> (Bi 0.2Sb 0.8) 2Te 3/magnetic <span class="hlt">insulator</span> EuS heterostructure. We are able to maximize the proximity-induced magnetism by applying an electrical back gate to tune the Fermi level of topological <span class="hlt">insulator</span> to be close to the Dirac point. A phenomenological model based on diamagnetic screeningmore » is developed to explain the suppressed proximity-induced magnetism at high carrier density. Our work paves the way to utilize the magnetic proximity effect at the topological <span class="hlt">insulator</span>/magnetic <span class="hlt">insulator</span> heterointerface for low-power spintronic applications.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1425052-dirac-electron-mediated-magnetic-proximity-effect-topological-insulator-magnetic-insulator-heterostructures','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1425052-dirac-electron-mediated-magnetic-proximity-effect-topological-insulator-magnetic-insulator-heterostructures"><span>Dirac-electron-mediated magnetic proximity effect in topological <span class="hlt">insulator</span>/magnetic <span class="hlt">insulator</span> heterostructures</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Li, Mingda; Song, Qichen; Zhao, Weiwei; ...</p> <p>2017-11-01</p> <p>The possible realization of dissipationless chiral edge current in a topological <span class="hlt">insulator</span>/magnetic <span class="hlt">insulator</span> heterostructure is based on the condition that the magnetic proximity exchange coupling at the interface is dominated by the Dirac surface states of the topological <span class="hlt">insulator</span>. We report a polarized neutron reflectometry observation of Dirac-electron-mediated magnetic proximity effect in a bulk-<span class="hlt">insulating</span> topological <span class="hlt">insulator</span> (Bi 0.2Sb 0.8) 2Te 3/magnetic <span class="hlt">insulator</span> EuS heterostructure. We are able to maximize the proximity-induced magnetism by applying an electrical back gate to tune the Fermi level of topological <span class="hlt">insulator</span> to be close to the Dirac point. A phenomenological model based on diamagnetic screeningmore » is developed to explain the suppressed proximity-induced magnetism at high carrier density. Our work paves the way to utilize the magnetic proximity effect at the topological <span class="hlt">insulator</span>/magnetic <span class="hlt">insulator</span> heterointerface for low-power spintronic applications.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..1614037S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..1614037S"><span>Comparing the <span class="hlt">ice</span> nucleation efficiencies of <span class="hlt">ice</span> nucleating substrates to natural mineral dusts</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Steinke, Isabelle; Funk, Roger; Höhler, Kristina; Haarig, Moritz; Hoffmann, Nadine; Hoose, Corinna; Kiselev, Alexei; Möhler, Ottmar; Leisner, Thomas</p> <p>2014-05-01</p> <p>Mineral dust particles in the atmosphere may act as efficient <span class="hlt">ice</span> nuclei over a wide range of temperature and relative humidity conditions. The <span class="hlt">ice</span> nucleation capability of dust particles mostly depends on the particle surface area and the associated physico-chemical surface properties. It has been observed that the surface-related <span class="hlt">ice</span> nucleation efficiency of different dust particles and mineral species can vary by several orders of magnitude. However, the relation between aerosol surface properties and observed <span class="hlt">ice</span> nucleation efficiency is still not completely understood due to the large variability of chemical <span class="hlt">compositions</span> and morphological features. In order to gain a better understanding of small scale freezing processes, we investigated the freezing of several hundreds of small droplets (V=0.4 nl) deposited on materials with reasonably well defined surfaces such as crystalline silicon wafers, graphite and freshly cleaved mica sheets under atmospherically relevant conditions. These substrates are intended to serve as simple model structures compared to the surface of natural aerosol particles. To learn more about the impact of particle morphology on <span class="hlt">ice</span> nucleation processes, we also investigated micro-structured silicon wafers with prescribed trenches. The <span class="hlt">ice</span> nucleation efficiencies deduced from these experiments are expressed as <span class="hlt">ice</span> nucleation active surface site density values. With this approach, the freezing properties of the above-described substrates could be compared to those of natural mineral dusts such as agricultural soil dusts, volcanic ash and fossil diatoms, which have been investigated in AIDA cloud chamber experiments. All tested <span class="hlt">ice</span> nucleating substrates were consistently less efficient at nucleating <span class="hlt">ice</span> than the natural mineral dusts. Crystalline silicon only had a negligible influence on the freezing of small droplets, leading to freezing near the homogeneous freezing temperature threshold. Applying surface structures to silicon led to a</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018E%26ES..113a2062J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018E%26ES..113a2062J"><span>The Development and Application of Simulative <span class="hlt">Insulation</span> Resistance Tester</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jia, Yan; Chai, Ziqi; Wang, Bo; Ma, Hao</p> <p>2018-02-01</p> <p>The <span class="hlt">insulation</span> state determines the performance and <span class="hlt">insulation</span> life of electrical equipment, so it has to be judged in a timely and accurate manner. <span class="hlt">Insulation</span> resistance test, as the simplest and most basic test of high voltage electric tests, can measure the <span class="hlt">insulation</span> resistance and absorption ratio which are effective criterion of part or whole damp or dirty, breakdown, severe overheating aging and other <span class="hlt">insulation</span> defects. It means that the electrical test personnel need to be familiar with the principle of <span class="hlt">insulation</span> resistance test, and able to operate the <span class="hlt">insulation</span> resistance tester correctly. At present, like the <span class="hlt">insulation</span> resistance test, most of electrical tests are trained by physical devices with the real high voltage. Although this allows the students to truly experience the test process and notes on security, it also has certain limitations in terms of safety and test efficiency, especially for a large number of new staves needing induction training every year. This <span class="hlt">paper</span> presents a new kind of electrical test training system based on the simulative device of dielectric loss measurement and simulative electrical testing devices. It can not only overcome the defects of current training methods, but also provide other advantages in economical efficiency and scalability. That makes it possible for the system to be allied in widespread.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010EGUGA..12..761D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010EGUGA..12..761D"><span>Compression experiments on artificial, alpine and marine <span class="hlt">ice</span>: implications for <span class="hlt">ice</span>-shelf/continental interactions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dierckx, Marie; Goossens, Thomas; Samyn, Denis; Tison, Jean-Louis</p> <p>2010-05-01</p> <p>Antarctic <span class="hlt">ice</span> shelves are important components of continental <span class="hlt">ice</span> dynamics, in that they control grounded <span class="hlt">ice</span> flow towards the ocean. As such, Antarctic <span class="hlt">ice</span> shelves are a key parameter to the stability of the Antarctic <span class="hlt">ice</span> sheet in the context of global change. Marine <span class="hlt">ice</span>, formed by sea water accretion beneath some <span class="hlt">ice</span> shelves, displays distinct physical (grain textures, bubble content, ...) and chemical (salinity, isotopic <span class="hlt">composition</span>, ...) characteristics as compared to glacier <span class="hlt">ice</span> and sea <span class="hlt">ice</span>. The aim is to refine Glen's flow relation (generally used for <span class="hlt">ice</span> behaviour in deformation) under various parameters (temperature, salinity, debris, grain size ...) to improve deformation laws used in dynamic <span class="hlt">ice</span> shelf models, which would then give more accurate and / or realistic predictions on <span class="hlt">ice</span> shelf stability. To better understand the mechanical properties of natural <span class="hlt">ice</span>, deformation experiments were performed on <span class="hlt">ice</span> samples in laboratory, using a pneumatic compression device. To do so, we developed a custom built compression rig operated by pneumatic drives. It has been designed for performing uniaxial compression tests at constant load and under unconfined conditions. The operating pressure ranges from about 0.5 to 10 Bars. This allows modifying the experimental conditions to match the conditions found at the grounding zone (in the 1 Bar range). To maintain the <span class="hlt">ice</span> at low temperature, the samples are immersed in a Silicone oil bath connected to an external refrigeration system. During the experiments, the vertical displacement of the piston and the applied force is measured by sensors which are connected to a digital acquisition system. We started our experiments with artificial <span class="hlt">ice</span> and went on with continental <span class="hlt">ice</span> samples from glaciers in the Alps. The first results allowed us to acquire realistic mechanical data for natural <span class="hlt">ice</span>. <span class="hlt">Ice</span> viscosity was calculated for different types of artificial <span class="hlt">ice</span>, using Glen's flow law, and showed the importance of impurities</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=Mare&pg=5&id=ED160671','ERIC'); return false;" href="https://eric.ed.gov/?q=Mare&pg=5&id=ED160671"><span>Social Background <span class="hlt">Composition</span> and Educational Growth. Discussion <span class="hlt">Papers</span> No. 471-77.</span></a></p> <p><a target="_blank" href="http://www.eric.ed.gov/ERICWebPortal/search/extended.jsp?_pageLabel=advanced">ERIC Educational Resources Information Center</a></p> <p>Mare, Robert D.</p> <p></p> <p>This <span class="hlt">paper</span> examines the impact of intercohort changes in social background <span class="hlt">composition</span> on changes in grade progression rates at selected schooling levels. It is argued that the relative and absolute effects of background <span class="hlt">composition</span> on grade progression rates should decline over levels of schooling. Empirical support for these arguments is…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29692405','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29692405"><span>Arctic sea <span class="hlt">ice</span> is an important temporal sink and means of transport for microplastic.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Peeken, Ilka; Primpke, Sebastian; Beyer, Birte; Gütermann, Julia; Katlein, Christian; Krumpen, Thomas; Bergmann, Melanie; Hehemann, Laura; Gerdts, Gunnar</p> <p>2018-04-24</p> <p>Microplastics (MP) are recognized as a growing environmental hazard and have been identified as far as the remote Polar Regions, with particularly high concentrations of microplastics in sea <span class="hlt">ice</span>. Little is known regarding the horizontal variability of MP within sea <span class="hlt">ice</span> and how the underlying water body affects MP <span class="hlt">composition</span> during sea <span class="hlt">ice</span> growth. Here we show that sea <span class="hlt">ice</span> MP has no uniform polymer <span class="hlt">composition</span> and that, depending on the growth region and drift paths of the sea <span class="hlt">ice</span>, unique MP patterns can be observed in different sea <span class="hlt">ice</span> horizons. Thus even in remote regions such as the Arctic Ocean, certain MP indicate the presence of localized sources. Increasing exploitation of Arctic resources will likely lead to a higher MP load in the Arctic sea <span class="hlt">ice</span> and will enhance the release of MP in the areas of strong seasonal sea <span class="hlt">ice</span> melt and the outflow gateways.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29704449','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29704449"><span>Contribution of sea <span class="hlt">ice</span> microbial production to Antarctic benthic communities is driven by sea <span class="hlt">ice</span> dynamics and <span class="hlt">composition</span> of functional guilds.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wing, Stephen R; Leichter, James J; Wing, Lucy C; Stokes, Dale; Genovese, Sal J; McMullin, Rebecca M; Shatova, Olya A</p> <p>2018-04-28</p> <p>Organic matter produced by the sea <span class="hlt">ice</span> microbial community (SIMCo) is an important link between sea <span class="hlt">ice</span> dynamics and secondary production in near-shore food webs of Antarctica. Sea <span class="hlt">ice</span> conditions in McMurdo Sound were quantified from time series of MODIS satellite images for Sept. 1 through Feb. 28 of 2007-2015. A predictable sea <span class="hlt">ice</span> persistence gradient along the length of the Sound and evidence for a distinct change in sea <span class="hlt">ice</span> dynamics in 2011 were observed. We used stable isotope analysis (δ 13 C and δ 15 N) of SIMCo, suspended particulate organic matter (SPOM) and shallow water (10-20 m) macroinvertebrates to reveal patterns in trophic structure of, and incorporation of organic matter from SIMCo into, benthic communities at eight sites distributed along the sea <span class="hlt">ice</span> persistence gradient. Mass-balance analysis revealed distinct trophic architecture among communities and large fluxes of SIMCo into the near-shore food web, with the estimates ranging from 2 to 84% of organic matter derived from SIMCo for individual species. Analysis of patterns in density, and biomass of macroinvertebrate communities among sites allowed us to model net incorporation of organic matter from SIMCo, in terms of biomass per unit area (g/m 2 ), into benthic communities. Here, organic matter derived from SIMCo supported 39 to 71 per cent of total biomass. Furthermore, for six species, we observed declines in contribution of SIMCo between years with persistent sea <span class="hlt">ice</span> (2008-2009) and years with extensive sea <span class="hlt">ice</span> breakout (2012-2015). Our data demonstrate the vital role of SIMCo in ecosystem function in Antarctica and strong linkages between sea <span class="hlt">ice</span> dynamics and near-shore secondary productivity. These results have important implications for our understanding of how benthic communities will respond to changes in sea <span class="hlt">ice</span> dynamics associated with climate change and highlight the important role of shallow water macroinvertebrate communities as sentinels of change for the Antarctic marine</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19800042192&hterms=melting+ice+caps&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dmelting%2Bice%2Bcaps','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19800042192&hterms=melting+ice+caps&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dmelting%2Bice%2Bcaps"><span>Volcano-<span class="hlt">ice</span> interactions on Mars</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Allen, C. C.</p> <p>1979-01-01</p> <p>Central volcanic eruptions beneath terrestrial glaciers have built steep-sided, flat-topped mountains composed of pillow lava, glassy tuff, capping flows, and cones of basalt. Subglacial fissure eruptions produced ridges of similar <span class="hlt">composition</span>. In some places the products from a number of subglacial vents have combined to form widespread deposits. The morphologies of these subglacial volcanoes are distinctive enough to allow their recognition at the resolutions characteristic of Viking orbiter imagery. Analogs to terrestrial subglacial volcanoes have been identified on the northern plains and near the south polar cap of Mars. The polar feature provides probable evidence of volcanic eruptions beneath polar <span class="hlt">ice</span>. A mixed unit of rock and <span class="hlt">ice</span> is postulated to have overlain portions of the northern plains, with eruptions into this ground <span class="hlt">ice</span> having produced mountains and ridges analogous to those in Iceland. Subsequent breakdown of this unit due to <span class="hlt">ice</span> melting revealed the volcanic features. Estimated heights of these landforms indicate that the <span class="hlt">ice</span>-rich unit once ranged from approximately 100 to 1200 m thick.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19980227786','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19980227786"><span>Temperature Histories in Ceramic-<span class="hlt">Insulated</span> Heat-Sink Nozzle</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Ciepluch, Carl C.</p> <p>1960-01-01</p> <p>Temperature histories were calculated for a <span class="hlt">composite</span> nozzle wall by a simplified numerical integration calculation procedure. These calculations indicated that there is a unique ratio of <span class="hlt">insulation</span> and metal heat-sink thickness that will minimize total wall thickness for a given operating condition and required running time. The optimum <span class="hlt">insulation</span> and metal thickness will vary throughout the nozzle as a result of the variation in heat-transfer rate. The use of low chamber pressure results in a significant increase in the maximum running time of a given weight nozzle. Experimentally measured wall temperatures were lower than those calculated. This was due in part to the assumption of one-dimensional or slab heat flow in the calculation procedure.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li class="active"><span>19</span></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_19 --> <div id="page_20" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li class="active"><span>20</span></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="381"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20130010710','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20130010710"><span>Cryogenic Moisture Uptake in Foam <span class="hlt">Insulation</span> for Space Launch Vehicles</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Fesmire, James E.; ScholtensCoffman, Brekke E.; Sass, Jared P.; Williams, Martha K.; Smith, Trent M.; Meneghelli, Barrry J.</p> <p>2008-01-01</p> <p>Rigid polyurethane foams and rigid polyisocyanurate foams (spray-on foam <span class="hlt">insulation</span>), like those flown on Shuttle, Delta IV, and will be flown on Ares-I and Ares-V, can gain an extraordinary amount of water when under cryogenic conditions for several hours. These foams, when exposed for eight hours to launch pad environments on one side and cryogenic temperature on the other, increase their weight from 35 to 80 percent depending on the duration of weathering or aging. This effect translates into several thousand pounds of additional weight for space vehicles at lift-off. A new cryogenic moisture uptake apparatus was designed to determine the amount of water/<span class="hlt">ice</span> taken into the specimen under actual-use propellant loading conditions. This experimental study included the measurement of the amount of moisture uptake within different foam materials. Results of testing using both aged specimens and weathered specimens are presented. To better understand cryogenic foam <span class="hlt">insulation</span> performance, cryogenic moisture testing is shown to be essential. The implications for future launch vehicle thermal protection system design and flight performance are discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018AIPC.1941b0048W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018AIPC.1941b0048W"><span>Design analysis of ceramic and polymer 150 kV <span class="hlt">insulators</span> for tropical condition using quickfield software</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Walukow, Stephy B.; Manjang, Salama; Zainuddin, Zahir; Samman, Faizal Arya</p> <p>2018-03-01</p> <p>This research is to analyze design of ceramic and polymer 150 kV <span class="hlt">insulators</span> for the tropical area. The use of an <span class="hlt">insulator</span> certainly requires an electric field. The leakage current and breakdown voltage this happens the contaminant on the surface of the <span class="hlt">insulator</span>. This type of contaminant can be rain, dust, salt air, extreme weather (much in tropical climates), industrial pollutants and cracks on the surface resulting in collisions. The method used in this research is magnetic field and electric field isolator using Quicfield software. To get the test results variation ranges 20 kV, 70 kV and 150 kV. Side effects of magnetic and electric fields around the <span class="hlt">insulator</span>. The simulation results show the accumulated contaminants on the surface. Planning should be done in <span class="hlt">insulator</span> <span class="hlt">insulator</span> on unstable <span class="hlt">insulator</span>. Thus, the approach using this commercially available software can be applied to. Therefore, the development of further simulations on the different types of <span class="hlt">composite</span> <span class="hlt">insulators</span> used on.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19920013862','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19920013862"><span>NASA's aircraft <span class="hlt">icing</span> technology program</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Reinmann, John J.</p> <p>1991-01-01</p> <p>NASA' Aircraft <span class="hlt">Icing</span> Technology program is aimed at developing innovative technologies for safe and efficient flight into forecasted <span class="hlt">icing</span>. The program addresses the needs of all aircraft classes and supports both commercial and military applications. The program is guided by three key strategic objectives: (1) numerically simulate an aircraft's response to an in-flight <span class="hlt">icing</span> encounter, (2) provide improved experimental <span class="hlt">icing</span> simulation facilities and testing techniques, and (3) offer innovative approaches to <span class="hlt">ice</span> protection. Our research focuses on topics that directly support stated industry needs, and we work closely with industry to assure a rapid and smooth transfer of technology. This <span class="hlt">paper</span> presents selected results that illustrate progress towards the three strategic objectives, and it provides a comprehensive list of references on the NASA <span class="hlt">icing</span> program.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20170008732','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20170008732"><span>An Integrated Approach to Swept Wing <span class="hlt">Icing</span> Simulation</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Potapczuk, Mark G.; Broeren, Andy P.</p> <p>2017-01-01</p> <p>This <span class="hlt">paper</span> describes the various elements of a simulation approach used to develop a database of <span class="hlt">ice</span> shape geometries and the resulting aerodynamic performance data for a representative commercial transport wing model exposed to a variety of <span class="hlt">icing</span> conditions. This effort included testing in the NASA <span class="hlt">Icing</span> Research Tunnel, the Wichita State University Walter H. Beech Wind Tunnel, and the ONERA F1 Subsonic Wind Tunnel as well as the use of <span class="hlt">ice</span> accretion codes, an inviscid design code, and computational fluid dynamics codes. Additionally, methods for capturing full three-dimensional <span class="hlt">ice</span> shape geometries, geometry interpolation along the span of the wing, and creation of artificial <span class="hlt">ice</span> shapes based upon that geometric data were developed for this effort. The <span class="hlt">icing</span> conditions used for this effort were representative of actual <span class="hlt">ice</span> shape encounter scenarios and run the gamut from <span class="hlt">ice</span> roughness to full three-dimensional scalloped <span class="hlt">ice</span> shapes. The effort is still underway so this <span class="hlt">paper</span> is a status report of work accomplished to date and a description of the remaining elements of the effort.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018TCry...12.1745C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018TCry...12.1745C"><span>Archival processes of the water stable isotope signal in East Antarctic <span class="hlt">ice</span> cores</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Casado, Mathieu; Landais, Amaelle; Picard, Ghislain; Münch, Thomas; Laepple, Thomas; Stenni, Barbara; Dreossi, Giuliano; Ekaykin, Alexey; Arnaud, Laurent; Genthon, Christophe; Touzeau, Alexandra; Masson-Delmotte, Valerie; Jouzel, Jean</p> <p>2018-05-01</p> <p>The oldest <span class="hlt">ice</span> core records are obtained from the East Antarctic Plateau. Water isotopes are key proxies to reconstructing past climatic conditions over the <span class="hlt">ice</span> sheet and at the evaporation source. The accuracy of climate reconstructions depends on knowledge of all processes affecting water vapour, precipitation and snow isotopic <span class="hlt">compositions</span>. Fractionation processes are well understood and can be integrated in trajectory-based Rayleigh distillation and isotope-enabled climate models. However, a quantitative understanding of processes potentially altering snow isotopic <span class="hlt">composition</span> after deposition is still missing. In low-accumulation sites, such as those found in East Antarctica, these poorly constrained processes are likely to play a significant role and limit the interpretability of an <span class="hlt">ice</span> core's isotopic <span class="hlt">composition</span>. By combining observations of isotopic <span class="hlt">composition</span> in vapour, precipitation, surface snow and buried snow from Dome C, a deep <span class="hlt">ice</span> core site on the East Antarctic Plateau, we found indications of a seasonal impact of metamorphism on the surface snow isotopic signal when compared to the initial precipitation. Particularly in summer, exchanges of water molecules between vapour and snow are driven by the diurnal sublimation-condensation cycles. Overall, we observe in between precipitation events modification of the surface snow isotopic <span class="hlt">composition</span>. Using high-resolution water isotopic <span class="hlt">composition</span> profiles from snow pits at five Antarctic sites with different accumulation rates, we identified common patterns which cannot be attributed to the seasonal variability of precipitation. These differences in the precipitation, surface snow and buried snow isotopic <span class="hlt">composition</span> provide evidence of post-deposition processes affecting <span class="hlt">ice</span> core records in low-accumulation areas.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFM.P23B1936D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFM.P23B1936D"><span>Hydrocarbon <span class="hlt">ices</span> in extra-red TNOs and Centaurs</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dalle Ore, C. M.; Barucci, M.; Emery, J. P.; Cruikshank, D. P.; Merlin, F.; Perna, D.</p> <p>2012-12-01</p> <p>We present an analysis of the reddest trans-neptunian objects (TNOs) and Centaurs - those belonging to the RR taxon. The RR class contains more than ¼ of the population of TNOs for which photometric colors are available, including a variety of dynamically different objects. The available data cover the spectral range from 0.3 to 2.2 μm. Previous work investigated possible relations between spectral characteristics and other physical and dynamical parameters. The distribution of <span class="hlt">ices</span> on TNOs has been analyzed as a function of the object absolute magnitude, taxonomy and dynamical class. In a sample of 76 objects for which visible and near-IR spectroscopic measurements are available, CH3OH <span class="hlt">ice</span> was detected only on three objects belonging to the RR taxonomic class (5145 Pholus, 55638 2002 VE95 and 90377 Sedna). These three objects are among the reddest, they belong to different dynamical classes, and they have different dimensions. However, all three have similar <span class="hlt">compositions</span> with Sedna showing a more significant heterogeneity in the kind of hydrocarbon <span class="hlt">ices</span> found on its surface than the others. To further investigate the presence of hydrocarbon <span class="hlt">ices</span>, and in particular CH3OH, as part of the <span class="hlt">composition</span> of the RR taxon we used Spitzer IRAC data available for a subgroup of nine objects. Both methanol and methane have a strong absorption at 3.6 μm, the first of the Spitzer IRAC channels, and a much higher albedo at the following channel at 4.5 μm. This albedo pattern is characteristic of some hydrocarbon <span class="hlt">ices</span> and is very different from H2O <span class="hlt">ice</span> that shows instead very low albedos at both channels. Our technique makes use of a large database of models including H2O, CH3OH, CH4, and N 2 <span class="hlt">ices</span> combined with tholins, amorphous carbon, hydrogenated amorphous carbon, serpentine and olivine in different combinations of relative abundances and grain sizes. We automatically extract the models that match the observations at all color wavelengths therefore obtaining for each</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016DPS....4851505A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016DPS....4851505A"><span>Solid-State Chemistry as a Formation Mechanism for C 4N 2 <span class="hlt">Ice</span> and Possibly the Haystack (220 cm -1 <span class="hlt">ice</span> emission feature) in Titan's Stratosphere as Observed by Cassini CIRS</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Anderson, Carrie; Samuelson, Robert E.; McLain, Jason L.; Nna Mvondo, Delphine; Romani, Paul; Flasar, F. Michael</p> <p>2016-10-01</p> <p>A profusion of organic <span class="hlt">ices</span> containing hydrocarbons, nitriles, and combinations of their mixtures comprise Titan's complex stratospheric cloud systems, and are typically formed via vapor condensation. These <span class="hlt">ice</span> particles are then distributed throughout the mid-to-lower stratosphere, with an increased abundance near the winter poles (see Anderson et al., 2016). The cold temperatures and the associated strong circumpolar winds that isolate polar air act in much the same way as on Earth, giving rise to <span class="hlt">compositional</span> anomalies and stratospheric clouds that provide heterogeneous chemistry sites.Titan's C4N2 <span class="hlt">ice</span> emission feature at 478 cm-1 and "the Haystack," a strong unidentified stratospheric <span class="hlt">ice</span> emission feature centered at 220 cm-1, share a common characteristic. Even though both are distinctive <span class="hlt">ice</span> emission features evident in Cassini <span class="hlt">Composite</span> InfraRed (CIRS) far-IR spectra, no associated vapor emission features can be found in Titan's atmosphere. Without a vapor phase, solid-state chemistry provides an alternate mechanism beside vapor condensation for producing these observed stratospheric <span class="hlt">ices</span>.Anderson et al., (2016) postulated that C4N2 <span class="hlt">ice</span> formed in Titan's stratosphere via the solid-state photochemical reaction HCN + HC3N → C4N2 + H2 can occur within extant HCN-HC3N <span class="hlt">composite</span> <span class="hlt">ice</span> particles. Such a reaction, and potentially similar reactions that may produce the Haystack <span class="hlt">ice</span>, are specific examples of solid-state chemistry in solar system atmospheres. This is in addition to the reaction HCl + ClONO2 → HNO3 + Cl2, which is known to produce HNO3 coatings on terrestrial water <span class="hlt">ice</span> particles, a byproduct of the catalytic chlorine chemistry that produces ozone holes in Earth's polar stratosphere (see for example, Molina et al., 1987 Soloman, 1999).A combination of radiative transfer modeling of CIRS far-IR spectra, coupled with optical constants derived from thin film transmittance spectra of organic <span class="hlt">ice</span> mixtures obtained in our Spectroscopy for Planetary <span class="hlt">ICes</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20000074968','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20000074968"><span>Non-Asbestos <span class="hlt">Insulation</span> Testing Using a Plasma Torch</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Morgan, R. E.; Prince, A. S.; Selvidge, S. A.; Phelps, J.; Martin, C. L.; Lawrence, T. W.</p> <p>2000-01-01</p> <p><span class="hlt">Insulation</span> obsolescence issues are a major concern for the Reusable Solid Rocket Motor (RSRM). As old sources of raw materials disappear, new sources must be found and qualified. No simple, inexpensive test presently exists for predicting the erosion performance of a candidate <span class="hlt">insulation</span> in the full-scale motor, Large motor tests cost million of dollars and therefore can only be used on a few very select candidates. There is a need for a simple, low cost method of screening <span class="hlt">insulation</span> performance that can simulate some of the different erosion environments found in the RSRM. This <span class="hlt">paper</span> describes a series of erosion tests on two different non-asbestos <span class="hlt">insulation</span> formulations, a KEVLAR(registered) fiber-filled and a carbon fiber-filled <span class="hlt">insulation</span> containing Ethylene-Propylene-Diene Monomer (EPDM) rubber as the binder. The test instrument was a plasma torch device. The two main variables investigated were heat flux and alumina particle impingement concentration. Statistical analysis revealed that the two different formulations had very different responses to the main variable. The results of this work indicate that there may be fundamental differences in how these <span class="hlt">insulation</span> formulations perform in the motor operating environment. The plasma torch appears to offer a low-cost means of obtaining a fundamental understanding of <span class="hlt">insulation</span> response to critical factors in a series of statistically designed experiments.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013GMD.....6.1299G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013GMD.....6.1299G"><span>Capabilities and performance of Elmer/<span class="hlt">Ice</span>, a new-generation <span class="hlt">ice</span> sheet model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gagliardini, O.; Zwinger, T.; Gillet-Chaulet, F.; Durand, G.; Favier, L.; de Fleurian, B.; Greve, R.; Malinen, M.; Martín, C.; Råback, P.; Ruokolainen, J.; Sacchettini, M.; Schäfer, M.; Seddik, H.; Thies, J.</p> <p>2013-08-01</p> <p>The Fourth IPCC Assessment Report concluded that <span class="hlt">ice</span> sheet flow models, in their current state, were unable to provide accurate forecast for the increase of polar <span class="hlt">ice</span> sheet discharge and the associated contribution to sea level rise. Since then, the glaciological community has undertaken a huge effort to develop and improve a new generation of <span class="hlt">ice</span> flow models, and as a result a significant number of new <span class="hlt">ice</span> sheet models have emerged. Among them is the parallel finite-element model Elmer/<span class="hlt">Ice</span>, based on the open-source multi-physics code Elmer. It was one of the first full-Stokes models used to make projections for the evolution of the whole Greenland <span class="hlt">ice</span> sheet for the coming two centuries. Originally developed to solve local <span class="hlt">ice</span> flow problems of high mechanical and physical complexity, Elmer/<span class="hlt">Ice</span> has today reached the maturity to solve larger-scale problems, earning the status of an <span class="hlt">ice</span> sheet model. Here, we summarise almost 10 yr of development performed by different groups. Elmer/<span class="hlt">Ice</span> solves the full-Stokes equations, for isotropic but also anisotropic <span class="hlt">ice</span> rheology, resolves the grounding line dynamics as a contact problem, and contains various basal friction laws. Derived fields, like the age of the <span class="hlt">ice</span>, the strain rate or stress, can also be computed. Elmer/<span class="hlt">Ice</span> includes two recently proposed inverse methods to infer badly known parameters. Elmer is a highly parallelised code thanks to recent developments and the implementation of a block preconditioned solver for the Stokes system. In this <span class="hlt">paper</span>, all these components are presented in detail, as well as the numerical performance of the Stokes solver and developments planned for the future.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20080022412','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20080022412"><span><span class="hlt">Ice</span>Val DatAssistant: An Interactive, Automated <span class="hlt">Icing</span> Data Management System</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Levinson, Laurie H.; Wright, William B.</p> <p>2008-01-01</p> <p>As with any scientific endeavor, the foundation of <span class="hlt">icing</span> research at the NASA Glenn Research Center (GRC) is the data acquired during experimental testing. In the case of the GRC <span class="hlt">Icing</span> Branch, an important part of this data consists of <span class="hlt">ice</span> tracings taken following tests carried out in the GRC <span class="hlt">Icing</span> Research Tunnel (IRT), as well as the associated operational and environmental conditions documented during these tests. Over the years, the large number of experimental runs completed has served to emphasize the need for a consistent strategy for managing this data. To address the situation, the <span class="hlt">Icing</span> Branch has recently elected to implement the <span class="hlt">Ice</span>Val DatAssistant automated data management system. With the release of this system, all publicly available IRT-generated experimental <span class="hlt">ice</span> shapes with complete and verifiable conditions have now been compiled into one electronically-searchable database. Simulation software results for the equivalent conditions, generated using the latest version of the LEWICE <span class="hlt">ice</span> shape prediction code, are likewise included and are linked to the corresponding experimental runs. In addition to this comprehensive database, the <span class="hlt">Ice</span>Val system also includes a graphically-oriented database access utility, which provides reliable and easy access to all data contained in the database. In this <span class="hlt">paper</span>, the issues surrounding historical <span class="hlt">icing</span> data management practices are discussed, as well as the anticipated benefits to be achieved as a result of migrating to the new system. A detailed description of the software system features and database content is also provided; and, finally, known issues and plans for future work are presented.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20070031804','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20070031804"><span><span class="hlt">Ice</span>Val DatAssistant: An Interactive, Automated <span class="hlt">Icing</span> Data Management System</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Levinson, Laurie H.; Wright, William B.</p> <p>2008-01-01</p> <p>As with any scientific endeavor, the foundation of <span class="hlt">icing</span> research at the NASA Glenn Research Center (GRC) is the data acquired during experimental testing. In the case of the GRC <span class="hlt">Icing</span> Branch, an important part of this data consists of <span class="hlt">ice</span> tracings taken following tests carried out in the GRC <span class="hlt">Icing</span> Research Tunnel (IRT), as well as the associated operational and environmental conditions during those tests. Over the years, the large number of experimental runs completed has served to emphasize the need for a consistent strategy to manage the resulting data. To address this situation, the <span class="hlt">Icing</span> Branch has recently elected to implement the <span class="hlt">Ice</span>Val DatAssistant automated data management system. With the release of this system, all publicly available IRT-generated experimental <span class="hlt">ice</span> shapes with complete and verifiable conditions have now been compiled into one electronically-searchable database; and simulation software results for the equivalent conditions, generated using the latest version of the LEWICE <span class="hlt">ice</span> shape prediction code, are likewise included and linked to the corresponding experimental runs. In addition to this comprehensive database, the <span class="hlt">Ice</span>Val system also includes a graphically-oriented database access utility, which provides reliable and easy access to all data contained in the database. In this <span class="hlt">paper</span>, the issues surrounding historical <span class="hlt">icing</span> data management practices are discussed, as well as the anticipated benefits to be achieved as a result of migrating to the new system. A detailed description of the software system features and database content is also provided; and, finally, known issues and plans for future work are presented.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22408297-mechanism-influencing-factors-critical-pulse-width-oil-immersed-polymer-insulators-under-short-pulses','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22408297-mechanism-influencing-factors-critical-pulse-width-oil-immersed-polymer-insulators-under-short-pulses"><span>Mechanism and influencing factors on critical pulse width of oil-immersed polymer <span class="hlt">insulators</span> under short pulses</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Zhao, Liang, E-mail: zhaoliang@ninit.ac.cn; Li, Rui; Zheng, Lei</p> <p>2015-04-15</p> <p>The critical pulse width (τ{sub c}) is a pulse width at which the surface flashover threshold (E{sub f}) is equal to the bulk breakdown threshold (E{sub BD}) for liquid-polymer <span class="hlt">composite</span> <span class="hlt">insulation</span> systems, which is discovered by Zhao et al. [Annual Report Conference on Electrical <span class="hlt">Insulation</span> and Dielectric Phenomena (IEEE Dielectrics and Electrical <span class="hlt">Insulation</span> Society, Shenzhen, China, 2013), Vol. 2, pp. 854–857]. In this <span class="hlt">paper</span>, the mechanism of τ{sub c} is interpreted in perspective of the threshold and the time delay (t{sub d}) of surface flashover and bulk breakdown, respectively. It is found that two changes appear as the pulse widthmore » decreases which are responsible for the existence of τ{sub c}: (1) E{sub BD} is lower than E{sub f}; (2) t{sub d} of bulk breakdown is shorter than t{sub d} of surface flashover. In addition, factors which have influences on τ{sub c} are investigated, such as the dielectric type, the <span class="hlt">insulation</span> length, the dielectric thickness, the dielectrics configuration, the pulse number, and the liquid purity. These influences of factors are generalized as three types if τ{sub c} is expected to increase: (1) factors causing E{sub BD} to decrease, such as increasing the pulse number or employing a dielectric of lower E{sub BD}; (2) factors causing E{sub f} to increase, such as complicating the <span class="hlt">insulator</span>'s configuration or increasing the liquid purity; (3) factors causing E{sub BD} and E{sub f} to increase together, but E{sub f} increases faster than E{sub BD}, such as decreasing the dielectric thickness or the <span class="hlt">insulation</span> length. With the data in references, all the three cases are verified experimentally. In the end, a general method based on τ{sub c} for solid <span class="hlt">insulation</span> design is presented and the significance of τ{sub c} on solid <span class="hlt">insulation</span> design and on solid demolition are discussed.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28518108','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28518108"><span>Identification of Plant <span class="hlt">Ice</span>-binding Proteins Through Assessment of <span class="hlt">Ice</span>-recrystallization Inhibition and Isolation Using <span class="hlt">Ice</span>-affinity Purification.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Bredow, Melissa; Tomalty, Heather E; Walker, Virginia K</p> <p>2017-05-05</p> <p><span class="hlt">Ice</span>-binding proteins (IBPs) belong to a family of stress-induced proteins that are synthesized by certain organisms exposed to subzero temperatures. In plants, freeze damage occurs when extracellular <span class="hlt">ice</span> crystals grow, resulting in the rupture of plasma membranes and possible cell death. Adsorption of IBPs to <span class="hlt">ice</span> crystals restricts further growth by a process known as <span class="hlt">ice</span>-recrystallization inhibition (IRI), thereby reducing cellular damage. IBPs also demonstrate the ability to depress the freezing point of a solution below the equilibrium melting point, a property known as thermal hysteresis (TH) activity. These protective properties have raised interest in the identification of novel IBPs due to their potential use in industrial, medical and agricultural applications. This <span class="hlt">paper</span> describes the identification of plant IBPs through 1) the induction and extraction of IBPs in plant tissue, 2) the screening of extracts for IRI activity, and 3) the isolation and purification of IBPs. Following the induction of IBPs by low temperature exposure, extracts are tested for IRI activity using a 'splat assay', which allows the observation of <span class="hlt">ice</span> crystal growth using a standard light microscope. This assay requires a low protein concentration and generates results that are quickly obtained and easily interpreted, providing an initial screen for <span class="hlt">ice</span> binding activity. IBPs can then be isolated from contaminating proteins by utilizing the property of IBPs to adsorb to <span class="hlt">ice</span>, through a technique called '<span class="hlt">ice</span>-affinity purification'. Using cell lysates collected from plant extracts, an <span class="hlt">ice</span> hemisphere can be slowly grown on a brass probe. This incorporates IBPs into the crystalline structure of the polycrystalline <span class="hlt">ice</span>. Requiring no a priori biochemical or structural knowledge of the IBP, this method allows for recovery of active protein. <span class="hlt">Ice</span>-purified protein fractions can be used for downstream applications including the identification of peptide sequences by mass spectrometry and the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20150019659','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20150019659"><span>Recent Advances in the LEWICE <span class="hlt">Icing</span> Model</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Wright, William B.; Addy, Gene; Struk, Peter; Bartkus, Tadas</p> <p>2015-01-01</p> <p>This <span class="hlt">paper</span> will describe two recent modifications to the Glenn <span class="hlt">ICE</span> software. First, a capability for modeling <span class="hlt">ice</span> crystals and mixed phase <span class="hlt">icing</span> has been modified based on recent experimental data. Modifications have been made to the <span class="hlt">ice</span> particle bouncing and erosion model. This capability has been added as part of a larger effort to model <span class="hlt">ice</span> crystal ingestion in aircraft engines. Comparisons have been made to <span class="hlt">ice</span> crystal <span class="hlt">ice</span> accretions performed in the NRC Research Altitude Test Facility (RATFac). Second, modifications were made to the run back model based on data and observations from thermal scaling tests performed in the NRC Altitude <span class="hlt">Icing</span> Tunnel.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140010420','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140010420"><span>Sea <span class="hlt">Ice</span> Thickness, Freeboard, and Snow Depth products from Operation <span class="hlt">Ice</span>Bridge Airborne Data</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Kurtz, N. T.; Farrell, S. L.; Studinger, M.; Galin, N.; Harbeck, J. P.; Lindsay, R.; Onana, V. D.; Panzer, B.; Sonntag, J. G.</p> <p>2013-01-01</p> <p>The study of sea <span class="hlt">ice</span> using airborne remote sensing platforms provides unique capabilities to measure a wide variety of sea <span class="hlt">ice</span> properties. These measurements are useful for a variety of topics including model evaluation and improvement, assessment of satellite retrievals, and incorporation into climate data records for analysis of interannual variability and long-term trends in sea <span class="hlt">ice</span> properties. In this <span class="hlt">paper</span> we describe methods for the retrieval of sea <span class="hlt">ice</span> thickness, freeboard, and snow depth using data from a multisensor suite of instruments on NASA's Operation <span class="hlt">Ice</span>Bridge airborne campaign. We assess the consistency of the results through comparison with independent data sets that demonstrate that the <span class="hlt">Ice</span>Bridge products are capable of providing a reliable record of snow depth and sea <span class="hlt">ice</span> thickness. We explore the impact of inter-campaign instrument changes and associated algorithm adaptations as well as the applicability of the adapted algorithms to the ongoing <span class="hlt">Ice</span>Bridge mission. The uncertainties associated with the retrieval methods are determined and placed in the context of their impact on the retrieved sea <span class="hlt">ice</span> thickness. Lastly, we present results for the 2009 and 2010 <span class="hlt">Ice</span>Bridge campaigns, which are currently available in product form via the National Snow and <span class="hlt">Ice</span> Data Center</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22263953-electrically-insulated-mli-thermal-anchor','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22263953-electrically-insulated-mli-thermal-anchor"><span>Electrically <span class="hlt">insulated</span> MLI and thermal anchor</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Kamiya, Koji; Furukawa, Masato; Murakami, Haruyuki</p> <p>2014-01-29</p> <p>The thermal shield of JT-60SA is kept at 80 K and will use the multilayer <span class="hlt">insulation</span> (MLI) to reduce radiation heat load to the superconducting coils at 4.4 K from the cryostat at 300 K. Due to plasma pulse operation, the MLI is affected by eddy current in toroidal direction. The MLI is designed to suppress the current by electrically <span class="hlt">insulating</span> every 20 degree in the toroidal direction by covering the MLI with polyimide films. In this <span class="hlt">paper</span>, two kinds of designs for the MLI system are proposed, focusing on a way to overlap the layers. A boil-off calorimeter methodmore » and temperature measurement has been performed to determine the thermal performance of the MLI system. The design of the electrical <span class="hlt">insulated</span> thermal anchor between the toroidal field (TF) coil and the thermal shield is also explained.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140008692','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140008692"><span>PSL <span class="hlt">Icing</span> Facility Upgrade Overview</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Griffin, Thomas A.; Dicki, Dennis J.; Lizanich, Paul J.</p> <p>2014-01-01</p> <p>The NASA Glenn Research Center Propulsion Systems Lab (PSL) was recently upgraded to perform engine inlet <span class="hlt">ice</span> crystal testing in an altitude environment. The system installed 10 spray bars in the inlet plenum for <span class="hlt">ice</span> crystal generation using 222 spray nozzles. As an altitude test chamber, the PSL is capable of simulating <span class="hlt">icing</span> events at altitude in a groundtest facility. The system was designed to operate at altitudes from 4,000 to 40,000 ft at Mach numbers up to 0.8M and inlet total temperatures from -60 to +15 degF. This <span class="hlt">paper</span> and presentation will be part of a series of presentations on PSL <span class="hlt">Icing</span> and will cover the development of the <span class="hlt">icing</span> capability through design, developmental testing, installation, initial calibration, and validation engine testing. Information will be presented on the design criteria and process, spray bar developmental testing at Cox and Co., system capabilities, and initial calibration and engine validation test. The PSL <span class="hlt">icing</span> system was designed to provide NASA and the <span class="hlt">icing</span> community with a facility that could be used for research studies of engine <span class="hlt">icing</span> by duplicating in-flight events in a controlled ground-test facility. With the system and the altitude chamber we can produce flight conditions and cloud environments to simulate those encountered in flight. The <span class="hlt">icing</span> system can be controlled to set various cloud uniformities, droplet median volumetric diameter (MVD), and <span class="hlt">icing</span> water content (IWC) through a wide variety of conditions. The PSL chamber can set altitudes, Mach numbers, and temperatures of interest to the <span class="hlt">icing</span> community and also has the instrumentation capability of measuring engine performance during <span class="hlt">icing</span> testing. PSL last year completed the calibration and initial engine validation of the facility utilizing a Honeywell ALF502-R5 engine and has duplicated in-flight roll back conditions experienced during flight testing. This <span class="hlt">paper</span> will summarize the modifications and buildup of the facility to accomplish these tests.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012Cryo...52..656K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012Cryo...52..656K"><span>High voltage <span class="hlt">insulation</span> of bushing for HTS power equipment</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kim, Woo-Jin; Choi, Jae-Hyeong; Kim, Sang-Hyun</p> <p>2012-12-01</p> <p>For the operation of high temperature superconducting (HTS) power equipments, it is necessary to develop <span class="hlt">insulating</span> materials and high voltage (HV) <span class="hlt">insulation</span> technology at cryogenic temperature of bushing. Liquid nitrogen (LN2) is an attractive dielectric liquid. Also, the polymer <span class="hlt">insulating</span> materials are expected to be used as solid materials such as glass fiber reinforced plastic (GFRP), polytetra-fluoroethylene (PTFE, Teflon), Silicon (Si) rubber, aromatic polyamide (Nomex), EPDM/Silicon alloy compound (EPDM/Si). In this <span class="hlt">paper</span>, the surface flashover characteristics of various <span class="hlt">insulating</span> materials in LN2 are studied. These results are studied at both AC and impulse voltage under a non-uniform field. The use of GFRP and Teflon as <span class="hlt">insulation</span> body for HTS bushing should be much desirable. Especially, GFRP is excellent material not only surface flashover characteristics but also mechanical characteristics at cryogenic temperature. The surface flashover is most serious problem for the shed design in LN2 and operation of superconducting equipments.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27387912','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27387912"><span>Hydrocarbon biodegradation by Arctic sea-<span class="hlt">ice</span> and sub-<span class="hlt">ice</span> microbial communities during microcosm experiments, Northwest Passage (Nunavut, Canada).</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Garneau, Marie-Ève; Michel, Christine; Meisterhans, Guillaume; Fortin, Nathalie; King, Thomas L; Greer, Charles W; Lee, Kenneth</p> <p>2016-10-01</p> <p>The increasing accessibility to navigation and offshore oil exploration brings risks of hydrocarbon releases in Arctic waters. Bioremediation of hydrocarbons is a promising mitigation strategy but challenges remain, particularly due to low microbial metabolic rates in cold, <span class="hlt">ice</span>-covered seas. Hydrocarbon degradation potential of <span class="hlt">ice</span>-associated microbes collected from the Northwest Passage was investigated. Microcosm incubations were run for 15 days at -1.7°C with and without oil to determine the effects of hydrocarbon exposure on microbial abundance, diversity and activity, and to estimate component-specific hydrocarbon loss. Diversity was assessed with automated ribosomal intergenic spacer analysis and Ion Torrent 16S rRNA gene sequencing. Bacterial activity was measured by (3)H-leucine uptake rates. After incubation, sub-<span class="hlt">ice</span> and sea-<span class="hlt">ice</span> communities degraded 94% and 48% of the initial hydrocarbons, respectively. Hydrocarbon exposure changed the <span class="hlt">composition</span> of sea-<span class="hlt">ice</span> and sub-<span class="hlt">ice</span> communities; in sea-<span class="hlt">ice</span> microcosms, Bacteroidetes (mainly Polaribacter) dominated whereas in sub-<span class="hlt">ice</span> microcosms, the contribution of Epsilonproteobacteria increased, and that of Alphaproteobacteria and Bacteroidetes decreased. Sequencing data revealed a decline in diversity and increases in Colwellia and Moritella in oil-treated microcosms. Low concentration of dissolved organic matter (DOM) in sub-<span class="hlt">ice</span> seawater may explain higher hydrocarbon degradation when compared to sea <span class="hlt">ice</span>, where DOM was abundant and composed of labile exopolysaccharides. © Fisheries and Oceans Canada [2016].</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=heat+AND+insulation&pg=2&id=ED205795','ERIC'); return false;" href="https://eric.ed.gov/?q=heat+AND+insulation&pg=2&id=ED205795"><span><span class="hlt">Insulation</span>.</span></a></p> <p><a target="_blank" href="http://www.eric.ed.gov/ERICWebPortal/search/extended.jsp?_pageLabel=advanced">ERIC Educational Resources Information Center</a></p> <p>Rhea, Dennis</p> <p></p> <p>This instructional unit is one of 10 developed by students on various energy-related areas that deals specifically with <span class="hlt">insulation</span>. Its objective is for the student to be able to determine <span class="hlt">insulation</span> needs of new or existing structures, select type to use, use installation techniques, calculate costs, and apply safety factors. Some topics covered…</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li class="active"><span>20</span></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_20 --> <div id="page_21" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li class="active"><span>21</span></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="401"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5885011','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5885011"><span>The diversity of <span class="hlt">ice</span> algal communities on the Greenland <span class="hlt">Ice</span> Sheet as revealed by oligotyping</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Lutz, Stefanie; McCutcheon, Jenine; McQuaid, James B.; Benning, Liane G.</p> <p>2018-01-01</p> <p>The Arctic is being disproportionally affected by climate change compared with other geographic locations, and is currently experiencing unprecedented melt rates. The Greenland <span class="hlt">Ice</span> Sheet (GrIS) can be regarded as the largest supraglacial ecosystem on Earth, and <span class="hlt">ice</span> algae are the dominant primary producers on bare <span class="hlt">ice</span> surfaces throughout the course of a melt season. <span class="hlt">Ice</span>-algal-derived pigments cause a darkening of the <span class="hlt">ice</span> surface, which in turn decreases albedo and increases melt rates. The important role of <span class="hlt">ice</span> algae in changing melt rates has only recently been recognized, and we currently know little about their community <span class="hlt">compositions</span> and functions. Here, we present the first analysis of <span class="hlt">ice</span> algal communities across a 100 km transect on the GrIS by high-throughput sequencing and subsequent oligotyping of the most abundant taxa. Our data reveal an extremely low algal diversity with Ancylonema nordenskiöldii and a Mesotaenium species being by far the dominant taxa at all sites. We employed an oligotyping approach and revealed a hidden diversity not detectable by conventional clustering of operational taxonomic units and taxonomic classification. Oligotypes of the dominant taxa exhibit a site-specific distribution, which may be linked to differences in temperatures and subsequently the extent of the melting. Our results help to better understand the distribution patterns of <span class="hlt">ice</span> algal communities that play a crucial role in the GrIS ecosystem. PMID:29547098</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1394775-investigating-compositional-effects-atomic-layer-deposition-ternary-dielectric-ti-al-metal-insulator-semiconductor-heterojunction-capacitor-structure-gate-insulation-inaln-gan-algan-gan','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1394775-investigating-compositional-effects-atomic-layer-deposition-ternary-dielectric-ti-al-metal-insulator-semiconductor-heterojunction-capacitor-structure-gate-insulation-inaln-gan-algan-gan"><span>Investigating <span class="hlt">compositional</span> effects of atomic layer deposition ternary dielectric Ti-Al-O on metal-<span class="hlt">insulator</span>-semiconductor heterojunction capacitor structure for gate <span class="hlt">insulation</span> of InAlN/GaN and AlGaN/GaN</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Colon, Albert; Stan, Liliana; Divan, Ralu</p> <p></p> <p>Gate <span class="hlt">insulation</span>/surface passivation in AlGaN/GaN and InAlN/GaN heterojunction field-effect transistors is a major concern for passivation of surface traps and reduction of gate leakage current. However, finding the most appropriate gate dielectric materials is challenging and often involves a compromise of the required properties such as dielectric constant, conduction/valence band-offsets, or thermal stability. Creating a ternary compound such as Ti-Al-O and tailoring its <span class="hlt">composition</span> may result in a reasonably good gate material in terms of the said properties. To date, there is limited knowledge of the performance of ternary dielectric compounds on AlGaN/GaN and even less on InAlN/GaN. To approachmore » this problem, the authors fabricated metal-<span class="hlt">insulator</span>-semiconductor heterojunction (MISH) capacitors with ternary dielectrics Ti-Al-O of various <span class="hlt">compositions</span>, deposited by atomic layer deposition (ALD). The film deposition was achieved by alternating cycles of TiO2 and Al2O3 using different ratios of ALD cycles. TiO2 was also deposited as a reference sample. The electrical characterization of the MISH capacitors shows an overall better performance of ternary compounds compared to the pure TiO2. The gate leakage current density decreases with increasing Al content, being similar to 2-3 orders of magnitude lower for a TiO2:Al2O3 cycle ratio of 2:1. Although the dielectric constant has the highest value of 79 for TiO2 and decreases with increasing the number of Al2O3 cycles, it is maintaining a relatively high value compared to an Al2O3 film. Capacitance voltage sweeps were also measured in order to characterize the interface trap density. A decreasing trend in the interface trap density was found while increasing Al content in the film. In conclusion, our study reveals that the desired high-kappa properties of TiO2 can be adequately maintained while improving other <span class="hlt">insulator</span> performance factors. The ternary compounds may be an excellent choice as a gate material</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27455680','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27455680"><span>A Low Temperature, Solution-Processed Poly(4-vinylphenol), YO(x) Nanoparticle <span class="hlt">Composite</span>/Polysilazane Bi-Layer Gate <span class="hlt">Insulator</span> for ZnO Thin Film Transistor.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Shin, Hyeonwoo; Kang, Chan-Mo; Chae, Hyunsik; Kim, Hyun-Gwan; Baek, Kyu-Ha; Choi, Hyoung Jin; Park, Man-Young; Do, Lee-Mi; Lee, Changhee</p> <p>2016-03-01</p> <p>Low temperature, solution-processed metal oxide thin film transistors (MEOTFTs) have been widely investigated for application in low-cost, transparent, and flexible electronics. To enlarge the application area, solution-processed gate <span class="hlt">insulators</span> (GI) have been investigated in recent years. We investigated the effects of the organic/inorganic bi-layer GI to ZnO thin film transistors (TFTs). PVP, YO(x) nanoparticle <span class="hlt">composite</span>, and polysilazane bi-layer showed low leakage current (-10(-8) A/cm2 in 2 MV), which are applicable in low temperature processed MEOTFTs. Polysilazane was used as an interlayer between ZnO and PVP, YO(x) nanoparticle <span class="hlt">composite</span> as a good charge transport interface with ZnO. By applying the PVP, YO(x), nanoparticle <span class="hlt">composite</span>/polysilazane bi-layer structure to ZnO TFTs, we successfully suppressed the off current (I(off)) to -10(-11) and fabricated good MEOTFTs in 180 degrees C.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008AIPC..985.1351L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008AIPC..985.1351L"><span>Heat Flow Measurement and Analysis of Thermal Vacuum <span class="hlt">Insulation</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Laa, C.; Hirschl, C.; Stipsitz, J.</p> <p>2008-03-01</p> <p>A new kind of calorimeter has been developed at Austrian Aerospace to measure specific material parameters needed for the analysis of thermal vacuum <span class="hlt">insulation</span>. A detailed description of the measuring device and the measurement results will be given in this <span class="hlt">paper</span>. This calorimeter facility allows to measure the heat flow through the <span class="hlt">insulation</span> under vacuum conditions in a wide temperature range from liquid nitrogen to ambient. Both boundary temperatures can be chosen within this range. Furthermore the <span class="hlt">insulation</span> can be characterized at high vacuum or under degraded vacuum, the latter is simulated by using helium or nitrogen gas. The mechanisms of heat transfer have been investigated, namely infrared radiation between the reflective layers of the <span class="hlt">insulation</span> and conduction through the interleaving spacer material. A mathematical description of the heat flow through the <span class="hlt">insulation</span> has been derived. Based on this, the heat flow for a typical <span class="hlt">insulation</span> material has been calculated by finite element analysis by use of the sotware tool Ansys®. Such a transient calculation is needed to determine the time to reach thermal equilibrium, which is mandatory for a proper interpretation and evaluation of the measurement. The new <span class="hlt">insulation</span> measurement results combined with the proposed type of analysis can be applied to better understand the thermal behavior of any kind of cryogenic system.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/862812','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/servlets/purl/862812"><span>Orbital disc <span class="hlt">insulator</span> for SF.sub.6 gas-<span class="hlt">insulated</span> bus</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Bacvarov, Dosio C.; Gomarac, Nicholas G.</p> <p>1977-01-01</p> <p>An <span class="hlt">insulator</span> for supporting a high voltage conductor within a gas-filled grounded housing consists of radially spaced <span class="hlt">insulation</span> rings fitted to the exterior of the bus and the interior of the grounded housing respectively, and the spaced rings are connected by trefoil type rings which are integrally formed with the spaced <span class="hlt">insulation</span> rings.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009AcAau..65.1284A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009AcAau..65.1284A"><span>Study of multilayer thermal <span class="hlt">insulation</span> by inverse problems method</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Alifanov, O. M.; Nenarokomov, A. V.; Gonzalez, V. M.</p> <p>2009-11-01</p> <p>The purpose of this <span class="hlt">paper</span> is to introduce a new method in the research of radiative and thermal properties of materials with further applications in the design of thermal control systems (TCS) of spacecrafts. In this <span class="hlt">paper</span> the radiative and thermal properties (emissivity and thermal conductance) of a multilayered thermal-<span class="hlt">insulating</span> blanket (MLI), which is a screen-vacuum thermal <span class="hlt">insulation</span> as a part of the TCS for perspective spacecrafts, are estimated. Properties of the materials under study are determined in the result of temperature and heat flux measurement data processing based on the solution of the inverse heat transfer problem (IHTP) technique. Given are physical and mathematical models of heat transfer processes in a specimen of the multilayered thermal-<span class="hlt">insulating</span> blanket located in the experimental facility. A mathematical formulation of the inverse heat conduction problem is presented as well. The practical approves were made for specimen of the real MLI.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20010095010','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20010095010"><span>Microstructural Investigation of High Emittance Glass Coatings on Fibrous Ceramic <span class="hlt">Insulation</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Ellerby, Don; Leiser, Dan; DiFiore, Robert; Figone, Jeff; Smith, Dane; Loehman, Ron; Kotula, Paul</p> <p>2001-01-01</p> <p>This viewgraph presentation provides an overview of the Space Shuttle Thermal Protection System (TPS) and the various products incorporated in the TPS. There are three tile systems which include pure silica, fibrous refractory <span class="hlt">composite</span> <span class="hlt">insulation</span> (FRCI), and alumina enhanced thermal barrier (AETB). Coating systems include reaction cured glass (RCG) and toughened uni-piece <span class="hlt">insulation</span> (TUFI). The microstructures of these systems are explored as are the manufacturing processes associated with each. Microstructural investigation using methods such as automated X-ray spectral image analysis (AXSIA) is a crucial part of understanding the mechanical nature of these systems.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1338329-origin-transitions-between-metallic-insulating-states-simple-metals','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1338329-origin-transitions-between-metallic-insulating-states-simple-metals"><span>Origin of Transitions between Metallic and <span class="hlt">Insulating</span> States in Simple Metals</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Naumov, Ivan I.; Hemley, Russell J.</p> <p>2015-04-17</p> <p>Unifying principles that underlie recently discovered transitions between metallic and <span class="hlt">insulating</span> states in elemental solids under pressure are developed. Using group theory arguments and first principles calculations, we show that the electronic properties of the phases involved in these transitions are controlled by symmetry principles not previously recognized. The valence bands in these systems are described by simple and <span class="hlt">composite</span> band representations constructed from localized Wannier functions centered on points unoccupied by atoms, and which are not necessarily all symmetrical. The character of the Wannier functions is closely related to the degree of s-p(-d) hybridization and reflects multi-center chemical bondingmore » in these <span class="hlt">insulating</span> states. The conditions under which an <span class="hlt">insulating</span> state is allowed for structures having an integer number of atoms per primitive unit cell as well as re-entrant (i.e., metal-<span class="hlt">insulator</span>-metal) transition sequences are detailed, resulting in predictions of novel behavior such as phases having three-dimensional Dirac-like points. The general principles developed are tested and applied to the alkali and alkaline earth metals, including elements where high-pressure <span class="hlt">insulating</span> phases have been identified or reported (e.g., Li, Na, and Ca).« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.C53B0574L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.C53B0574L"><span><span class="hlt">Ice</span> Shelf-Ocean Interactions Near <span class="hlt">Ice</span> Rises and <span class="hlt">Ice</span> Rumples</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lange, M. A.; Rückamp, M.; Kleiner, T.</p> <p>2013-12-01</p> <p>The stability of <span class="hlt">ice</span> shelves depends on the existence of embayments and is largely influenced by <span class="hlt">ice</span> rises and <span class="hlt">ice</span> rumples, which act as 'pinning-points' for <span class="hlt">ice</span> shelf movement. Of additional critical importance are interactions between <span class="hlt">ice</span> shelves and the water masses underlying them in <span class="hlt">ice</span> shelf cavities, particularly melting and refreezing processes. The present study aims to elucidate the role of <span class="hlt">ice</span> rises and <span class="hlt">ice</span> rumples in the context of climate change impacts on Antarctic <span class="hlt">ice</span> shelves. However, due to their smaller spatial extent, <span class="hlt">ice</span> rumples react more sensitively to climate change than <span class="hlt">ice</span> rises. Different forcings are at work and need to be considered separately as well as synergistically. In order to address these issues, we have decided to deal with the following three issues explicitly: oceanographic-, cryospheric and general topics. In so doing, we paid particular attention to possible interrelationships and feedbacks in a coupled <span class="hlt">ice</span>-shelf-ocean system. With regard to oceanographic issues, we have applied the ocean circulation model ROMBAX to ocean water masses adjacent to and underneath a number of idealized <span class="hlt">ice</span> shelf configurations: wide and narrow as well as laterally restrained and unrestrained <span class="hlt">ice</span> shelves. Simulations were performed with and without small <span class="hlt">ice</span> rises located close to the calving front. For larger configurations, the impact of the <span class="hlt">ice</span> rises on melt rates at the <span class="hlt">ice</span> shelf base is negligible, while for smaller configurations net melting rates at the <span class="hlt">ice</span>-shelf base differ by a factor of up to eight depending on whether <span class="hlt">ice</span> rises are considered or not. We employed the thermo-coupled <span class="hlt">ice</span> flow model TIM-FD3 to simulate the effects of several <span class="hlt">ice</span> rises and one <span class="hlt">ice</span> rumple on the dynamics of <span class="hlt">ice</span> shelf flow. We considered the complete un-grounding of the <span class="hlt">ice</span> shelf in order to investigate the effect of pinning points of different characteristics (interior or near calving front, small and medium sized) on the resulting flow and stress fields</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19890012038','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19890012038"><span>Collisions with <span class="hlt">ice</span>-volatile objects: Geological implications</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Wilde, P.; Quinby-Hunt, M. S.; Berry, W. B. N.</p> <p>1988-01-01</p> <p>The collision of the Earth with extra-terrestrial <span class="hlt">ice</span>-volatile bodies is proposed as a mechanism to produce rapid changes in the geologic record. These bodies would be analogs of the <span class="hlt">ice</span> satellites found for the Jovian planets and suspected for comets and certain low density bodies in the Asteroid belt. Five generic end-members are postulated: (1) water <span class="hlt">ice</span>; (2) dry <span class="hlt">ice</span>: carbon-carbon dioxide rich, (3) oceanic (chloride) <span class="hlt">ice</span>; (4) sulfur-rich <span class="hlt">ice</span>; (5) ammonia hydrate-rich <span class="hlt">ice</span>; and (6) clathrate: methane-rich <span class="hlt">ice</span>. Due to the volatile nature of these bodies, evidence for their impact with the Earth would be subtle and probably best reflected geochemically or in the fossil record. Actual boloids impacting the Earth may have a variable <span class="hlt">composition</span>, generally some admixture with water <span class="hlt">ice</span>. However for discussion purposes, only the effects of a dominant component will be treated. The general geological effects of such collisions, as a function of the dominant component would be: (1) rapid sea level rise unrelated to deglaciation, (2) decreased oceanic pH and rapid climatic warming or deglaciation; (3) increased paleosalinities; (4) increased acid rain; (5) increased oceanic pH and rapid carbonate deposition; and (6) rapid climatic warming or deglaciation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010BGD.....7.1167A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010BGD.....7.1167A"><span>Differences in community <span class="hlt">composition</span> of bacteria in four deep <span class="hlt">ice</span> sheets in western China</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>An, L.; Chen, Y.; Xiang, S.-R.; Shang, T.-C.; Tian, L.-De</p> <p>2010-02-01</p> <p>Microbial community patterns vary in glaciers world wide, presenting unique responses to global climatic and environmental changes. Four bacterial clone libraries were established by 16S rRNA gene amplification from four <span class="hlt">ice</span> layers along the 42-m-long <span class="hlt">ice</span> core MuztB drilled from the Muztag Ata Glacier. A total of 152 bacterial sequences obtained from the <span class="hlt">ice</span> core MuztB were phylogenetically compared with the 71 previously reported sequences from three <span class="hlt">ice</span> cores extracted from <span class="hlt">ice</span> caps Malan, Dunde, and Puruoganri. The six functional clusters Flavisolibacter, Flexibacter (Bacteroidetes), Acinetobacter, Enterobacter (Gammaproteobacteria), Planococcus/Anoxybacillus (Firmicutes), and Propionibacter/Luteococcus (Actinobacteria) frequently occurred along the Muztag Ata Glacier profile. Sequence analysis showed that most of the sequences from the <span class="hlt">ice</span> core clustered with those from cold environments, and the sequences from the same glacier formed a distinct cluster. Moreover, bacterial communities from the same location or similarly aged <span class="hlt">ice</span> formed a cluster, and were clearly separate from those from other geographically isolated glaciers. In a summary, the findings provide preliminary evidence of zone distribution of microbial community, support our hypothesis of the spatial and temporal biogeography of microorganisms in glacial <span class="hlt">ice</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19990019485','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19990019485"><span>NASA/FAA Tailplane <span class="hlt">Icing</span> Program Overview</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Ratvasky, Thomas P.; VanZante, Judith Foss; Riley, James T.</p> <p>1999-01-01</p> <p>The effects of tailplane <span class="hlt">icing</span> were investigated in a four-year NASA/FAA Tailplane <span class="hlt">Icing</span>, Program (TIP). This research program was developed to improve the understanding, of <span class="hlt">iced</span> tailplane aeroperformance and aircraft aerodynamics, and to develop design and training aides to help reduce the number of incidents and accidents caused by tailplane <span class="hlt">icing</span>. To do this, the TIP was constructed with elements that included <span class="hlt">icing</span>, wind tunnel testing, dry-air aerodynamic wind tunnel testing, flight tests, and analytical code development. This <span class="hlt">paper</span> provides an overview of the entire program demonstrating the interconnectivity of the program elements and reports on current accomplishments.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015IAUGA..2255736F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015IAUGA..2255736F"><span><span class="hlt">Ice</span> Mapping Observations in Galactic Star-Forming Regions: the AKARI Legacy</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fraser, Helen Jane; Suutarinnen, Aleksi; Noble, Jennifer</p> <p>2015-08-01</p> <p>It is becoming increasingly clear that explaining the small-scale distribution of many gas-phase molecules relies on our interpretation of the complex inter-connectivity between gas- and solid-phase interstellar chemistries. Inputs to proto-stellar astrochemical models are required that exploit <span class="hlt">ice</span> <span class="hlt">compositions</span> reflecting the historical physical conditions in pre-stellar environments when the <span class="hlt">ices</span> first formed. Such data are required to translate the near-universe picture of <span class="hlt">ice-composition</span> to our understanding of the role of extra-galactic <span class="hlt">ices</span> in star-formation at higher redshifts.Here we present the first attempts at multi-object <span class="hlt">ice</span> detections, and the subsequent <span class="hlt">ice</span> column density mapping. The AKARI space telescope was uniquely capable of observing all the <span class="hlt">ice</span> features between 2 and 5 microns, thereby detecting H2O, CO and CO2 <span class="hlt">ices</span> concurrently, through their stretching vibrational features. Our group has successfully extracted an unprecedented volume of <span class="hlt">ice</span> spectra from AKARI, including sources with not more than 2 mJy flux at 3 microns, showing:(a) H2O CO and CO2 <span class="hlt">ices</span> on 30 lines of sight towards pre-stellar and star-forming cores, which when combined with laboratory experiments indicate how the chemistries of these three <span class="hlt">ices</span> are interlinked (Noble et al (2013)),(b) <span class="hlt">ice</span> maps showing the spatial distribution of water <span class="hlt">ice</span> across 12 pre-stellar cores, in different molecular clouds (Suutarinnen et al (2015)), and the distribution of <span class="hlt">ice</span> components within these cores on 1000 AU scales (Noble et al (2015)),(c) over 200 new detections of water <span class="hlt">ice</span>, mostly on lines of sight towards background sources (> 145), indicating that water <span class="hlt">ice</span> column density has a minimum value as a function of Av, but on a cloud-by-cloud basis typically correlates with Av, and dust emissivity at 250 microns (Suutarinnen et al (2015)),(d) the first detections of HDO <span class="hlt">ice</span> towards background stars (Fraser et al (2015)).We discuss whether these results support the picture of a generic chemical</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20170008731','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20170008731"><span><span class="hlt">Ice</span> Accretion Roughness Measurements and Modeling</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>McClain, Stephen T.; Vargas, Mario; Tsao, Jen-Ching; Broeren, Andy P.; Lee, Sam</p> <p>2017-01-01</p> <p>Roughness on aircraft <span class="hlt">ice</span> accretions is very important to the overall <span class="hlt">ice</span> accretion process and to the resulting degradation in aircraft aerodynamic performance. Roughness enhances the local convection leading to more rapid <span class="hlt">ice</span> accumulation rates, and roughness generates local flow perturbations that lead to higher skin friction. This <span class="hlt">paper</span> presents 1) a review of the developments in <span class="hlt">ice</span> shape three-dimensional laser scanning developed at NASA Glenn, 2) a review of the approach of McClain and Kreeger employed to characterize <span class="hlt">ice</span> roughness evolution on an airfoil surface, and 3) a review of the experimental efforts that have been performed over the last five years to characterize, scale, and model <span class="hlt">ice</span> roughness evolution physics.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.C31D..01L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C31D..01L"><span>Gas exchange in the <span class="hlt">ice</span> zone: the role of small waves and big animals</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Loose, B.; Takahashi, A.; Bigdeli, A.</p> <p>2016-12-01</p> <p>The balance of air-sea gas exchange and net biological carbon fixation determine the transport and transformation of carbon dioxide and methane in the ocean. Air-sea gas exchange is mostly driven by upper ocean physics, but biology can also play a role. In the open ocean, gas exchange increases proportionate to the square of wind speed. When sea <span class="hlt">ice</span> is present, this dependence breaks down in part because breaking waves and air bubble entrainment are damped out by interactions between sea <span class="hlt">ice</span> and the wave field. At the same time, sea <span class="hlt">ice</span> motions, formation, melt, and even sea <span class="hlt">ice</span>-associated organisms can act to introduce turbulence and air bubbles into the upper ocean, thereby enhancing air-sea gas exchange. We take advantage of the knowledge advances of upper ocean physics including bubble dynamics to formulate a model for air-sea gas exchange in the sea <span class="hlt">ice</span> zone. Here, we use the model to examine the role of small-scale waves and diving animals that trap air for <span class="hlt">insulation</span>, including penguins, seals and polar bears. We compare these processes to existing parameterizations of wave and bubble dynamics in the open ocean, to observe how sea <span class="hlt">ice</span> both mitigates and locally enhances air-sea gas transfer.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20020039858&hterms=nucleation+humidity&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dnucleation%2Bhumidity','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20020039858&hterms=nucleation+humidity&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dnucleation%2Bhumidity"><span>SUCCESS Evidence for Cirrus Cloud <span class="hlt">Ice</span> Nucleation Mechanisms</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Jensen, Eric; Gore, Warren J. Y. (Technical Monitor)</p> <p>1997-01-01</p> <p>During the SUCCESS mission, several measurements were made which should improve our understanding of <span class="hlt">ice</span> nucleation processes in cirrus clouds. Temperature and water vapor concentration were made with a variety of instruments on the NASA DC-8. These observations should provide accurate upper tropospheric humidities. In particular, we will evaluate what humidities are required for <span class="hlt">ice</span> nucleation. Preliminary results suggest that substantial supersaturations frequently exist in the upper troposphere. The leading-edge region of wave-clouds (where <span class="hlt">ice</span> nucleation occurs) was sampled extensively at temperatures near -40 and -60C. These observations should give precise information about conditions required for <span class="hlt">ice</span> nucleation. In addition, we will relate the observed aerosol <span class="hlt">composition</span> and size distributions to the <span class="hlt">ice</span> formation observed to evaluate the role of soot or mineral particles on <span class="hlt">ice</span> nucleation. As an alternative technique for determining what particles act as <span class="hlt">ice</span> nuclei, numerous samples of aerosols inside <span class="hlt">ice</span> crystals were taken. In some cases, large numbers of aerosols were detected in each crystal, indicating that efficient scavenging occurred. Analysis of aerosols in <span class="hlt">ice</span> crystals when only one particle per crystal was detected should help with the <span class="hlt">ice</span> nucleation issue. Direct measurements of the <span class="hlt">ice</span> nucleating activity of ambient aerosols drawn into airborne cloud chambers were also made. Finally, measurements of aerosols and <span class="hlt">ice</span> crystals in contrails should indicate whether aircraft exhaust soot particles are effective <span class="hlt">ice</span> nuclei.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22273601-spin-transport-normal-metal-insulator-topological-insulator-coupled-ferromagnetic-insulator-structures','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22273601-spin-transport-normal-metal-insulator-topological-insulator-coupled-ferromagnetic-insulator-structures"><span>Spin transport in normal metal/<span class="hlt">insulator</span>/topological <span class="hlt">insulator</span> coupled to ferromagnetic <span class="hlt">insulator</span> structures</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Kondo, Kenji, E-mail: kkondo@es.hokudai.ac.jp</p> <p></p> <p>In this study, we investigate the spin transport in normal metal (NM)/<span class="hlt">insulator</span> (I)/topological <span class="hlt">insulator</span> (TI) coupled to ferromagnetic <span class="hlt">insulator</span> (FI) structures. In particular, we focus on the barrier thickness dependence of the spin transport inside the bulk gap of the TI with FI. The TI with FI is described by two-dimensional (2D) Dirac Hamiltonian. The energy profile of the <span class="hlt">insulator</span> is assumed to be a square with barrier height V and thickness d along the transport-direction. This structure behaves as a tunnel device for 2D Dirac electrons. The calculation is performed for the spin conductance with changing the barrier thicknessmore » and the components of magnetization of FI layer. It is found that the spin conductance decreases with increasing the barrier thickness. Also, the spin conductance is strongly dependent on the polar angle θ, which is defined as the angle between the axis normal to the FI and the magnetization of FI layer. These results indicate that the structures are promising candidates for novel tunneling magnetoresistance devices.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ApSS..409...45C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ApSS..409...45C"><span>Durable superhydrophobic <span class="hlt">paper</span> enabled by surface sizing of starch-based <span class="hlt">composite</span> films</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chen, Gang; Zhu, Penghui; Kuang, Yudi; Liu, Yu; Lin, Donghan; Peng, Congxing; Wen, Zhicheng; Fang, Zhiqiang</p> <p>2017-07-01</p> <p>Superhydrophobic <span class="hlt">paper</span> with remarkable durability is of considerable interest for its practical applications. In this study, a scalable, inexpensive, and universal surface sizing technique was implemented to prepare superhydrophobic <span class="hlt">paper</span> with enhanced durability. A thin layer of starch-based <span class="hlt">composite</span>, acting as a bio-binder, was first coated onto the <span class="hlt">paper</span> surface by a sophisticated manufacturing technique called surface sizing, immediately followed by a spray coating of hexamethyl disilazane treated silica nanoparticles (HMDS-SiNPs) dispersed in ethanol on the surface of the wet starch-coated sheet, and the dual layers dried at the same time. Consequently, durable superhydrophobic <span class="hlt">paper</span> with bi-layer structure was obtained after air drying. The as-prepared superhydrophobic <span class="hlt">paper</span> not only exhibited a self-cleaning behavior, but also presented an enhanced durability against scratching, bending/deformation, as well as moisture. The universal surface sizing of starch-based <span class="hlt">composites</span> may pave the way for the up-scaled and cost-effective production of durable superhydrophobic <span class="hlt">paper</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/869483','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/servlets/purl/869483"><span>Multiple density layered <span class="hlt">insulator</span></span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Alger, Terry W.</p> <p>1994-01-01</p> <p>A multiple density layered <span class="hlt">insulator</span> for use with a laser is disclosed wh provides at least two different <span class="hlt">insulation</span> materials for a laser discharge tube, where the two <span class="hlt">insulation</span> materials have different thermoconductivities. The multiple layer <span class="hlt">insulation</span> materials provide for improved thermoconductivity capability for improved laser operation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/7242057','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/biblio/7242057"><span>Multiple density layered <span class="hlt">insulator</span></span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Alger, T.W.</p> <p>1994-09-06</p> <p>A multiple density layered <span class="hlt">insulator</span> for use with a laser is disclosed which provides at least two different <span class="hlt">insulation</span> materials for a laser discharge tube, where the two <span class="hlt">insulation</span> materials have different thermoconductivities. The multiple layer <span class="hlt">insulation</span> materials provide for improved thermoconductivity capability for improved laser operation. 4 figs.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li class="active"><span>21</span></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_21 --> <div id="page_22" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li class="active"><span>22</span></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="421"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016ISPAr41B8..481B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016ISPAr41B8..481B"><span>Mass Balance Changes and <span class="hlt">Ice</span> Dynamics of Greenland and Antarctic <span class="hlt">Ice</span> Sheets from Laser Altimetry</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Babonis, G. S.; Csatho, B.; Schenk, T.</p> <p>2016-06-01</p> <p>During the past few decades the Greenland and Antarctic <span class="hlt">ice</span> sheets have lost <span class="hlt">ice</span> at accelerating rates, caused by increasing surface temperature. The melting of the two big <span class="hlt">ice</span> sheets has a big impact on global sea level rise. If the <span class="hlt">ice</span> sheets would melt down entirely, the sea level would rise more than 60 m. Even a much smaller rise would cause dramatic damage along coastal regions. In this <span class="hlt">paper</span> we report about a major upgrade of surface elevation changes derived from laser altimetry data, acquired by NASA's <span class="hlt">Ice</span>, Cloud and land Elevation Satellite mission (ICESat) and airborne laser campaigns, such as Airborne Topographic Mapper (ATM) and Land, Vegetation and <span class="hlt">Ice</span> Sensor (LVIS). For detecting changes in <span class="hlt">ice</span> sheet elevations we have developed the Surface Elevation Reconstruction And Change detection (SERAC) method. It computes elevation changes of small surface patches by keeping the surface shape constant and considering the absolute values as surface elevations. We report about important upgrades of earlier results, for example the inclusion of local <span class="hlt">ice</span> caps and the temporal extension from 1993 to 2014 for the Greenland <span class="hlt">Ice</span> Sheet and for a comprehensive reconstruction of <span class="hlt">ice</span> thickness and mass changes for the Antarctic <span class="hlt">Ice</span> Sheets.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PhyEd..53b3001E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PhyEd..53b3001E"><span>Investigating the effect of multiple layers of <span class="hlt">insulation</span> with a bubble wrap experiment</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Eggers, Dolores; Ruiz, Michael J.</p> <p>2018-03-01</p> <p>We provide a fun, inexpensive laboratory experiment for students to investigate the effects of multiple layers of <span class="hlt">insulation</span> and observe diminishing values for additional layers using bubble wrap. This experiment provides an opportunity for students to learn about heat transfer through conduction using readily available materials. A water-<span class="hlt">ice</span> pack is placed on top of five layers of bubble wrap. The temperature is taken between each layer periodically for at least 15 min. Students determine asymptotic temperatures for varying layers. This experiment also suggests a real world application.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19930006213','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19930006213"><span>Advancements in the LEWICE <span class="hlt">Ice</span> Accretion Model</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Wright, William B.</p> <p>1993-01-01</p> <p>Recent evidence has shown that the NASA/Lewis <span class="hlt">Ice</span> Accretion Model, LEWICE, does not predict accurate <span class="hlt">ice</span> shapes for certain glaze <span class="hlt">ice</span> conditions. This <span class="hlt">paper</span> will present the methodology used to make a first attempt at improving the <span class="hlt">ice</span> accretion prediction in these regimes. Importance is given to the correlations for heat transfer coefficient and <span class="hlt">ice</span> density, as well as runback flow, selection of the transition point, flow field resolution, and droplet trajectory models. Further improvements and refinement of these modules will be performed once tests in NASA's <span class="hlt">Icing</span> Research Tunnel, scheduled for 1993, are completed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20170000875','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20170000875"><span>Plans and Preliminary Results of Fundamental Studies of <span class="hlt">Ice</span> Crystal <span class="hlt">Icing</span> Physics in the NASA Propulsion Systems Laboratory</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Struk, Peter; Tsao, Jen-Ching; Bartkus, Tadas</p> <p>2017-01-01</p> <p>This <span class="hlt">paper</span> describes plans and preliminary results for using the NASA Propulsion Systems Lab (PSL) to experimentally study the fundamental physics of <span class="hlt">ice</span>-crystal <span class="hlt">ice</span> accretion. NASA is evaluating whether this facility, in addition to full-engine and motor-driven-rig tests, can be used for more fundamental <span class="hlt">ice</span>-accretion studies that simulate the different mixed-phase <span class="hlt">icing</span> conditions along the core flow passage of a turbo-fan engine compressor. The data from such fundamental accretion tests will be used to help develop and validate models of the accretion process. This <span class="hlt">paper</span> presents data from some preliminary testing performed in May 2015 which examined how a mixed-phase cloud could be generated at PSL using evaporative cooling in a warmer-than-freezing environment.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20170001732','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20170001732"><span>Plans and Preliminary Results of Fundamental Studies of <span class="hlt">Ice</span> Crystal <span class="hlt">Icing</span> Physics in the NASA Propulsion Systems Laboratory</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Struk, Peter; Tsao, Jen-Ching; Bartkus, Tadas</p> <p>2016-01-01</p> <p>This presentation accompanies the <span class="hlt">paper</span> titled Plans and Preliminary Results of Fundamental Studies of <span class="hlt">Ice</span> Crystal <span class="hlt">Icing</span> Physics in the NASA Propulsion Systems Laboratory. NASA is evaluating whether PSL, in addition to full-engine and motor-driven-rig tests, can be used for more fundamental <span class="hlt">ice</span>-accretion studies that simulate the different mixed-phase <span class="hlt">icing</span> conditions along the core flow passage of a turbo-fan engine compressor. The data from such fundamental accretion tests will be used to help develop and validate models of the accretion process. This presentation (and accompanying <span class="hlt">paper</span>) presents data from some preliminary testing performed in May 2015 which examined how a mixed-phase cloud could be generated at PSL using evaporative cooling in a warmer-than-freezing environment.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19890013198','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19890013198"><span>NASA's program on <span class="hlt">icing</span> research and technology</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Reinmann, John J.; Shaw, Robert J.; Ranaudo, Richard J.</p> <p>1989-01-01</p> <p>NASA's program in aircraft <span class="hlt">icing</span> research and technology is reviewed. The program relies heavily on computer codes and modern applied physics technology in seeking <span class="hlt">icing</span> solutions on a finer scale than those offered in earlier programs. Three major goals of this program are to offer new approaches to <span class="hlt">ice</span> protection, to improve our ability to model the response of an aircraft to an <span class="hlt">icing</span> encounter, and to provide improved techniques and facilities for ground and flight testing. This <span class="hlt">paper</span> reviews the following program elements: (1) new approaches to <span class="hlt">ice</span> protection; (2) numerical codes for deicer analysis; (3) measurement and prediction of <span class="hlt">ice</span> accretion and its effect on aircraft and aircraft components; (4) special wind tunnel test techniques for rotorcraft <span class="hlt">icing</span>; (5) improvements of <span class="hlt">icing</span> wind tunnels and research aircraft; (6) ground de-<span class="hlt">icing</span> fluids used in winter operation; (7) fundamental studies in <span class="hlt">icing</span>; and (8) droplet sizing instruments for <span class="hlt">icing</span> clouds.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011IJTPE.131..139K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011IJTPE.131..139K"><span>Study on <span class="hlt">Insulating</span> Material by Renewable Resources</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kurata, Yasuyuki; Kurosumi, Akihiro; Ishikawa, Keita</p> <p></p> <p>Under circumstances such as global warming caused by carbon dioxide and other green house gas and crisis of depletion of fossil resources, recyclable resources such as biomass have captured the world's attention as reproducible resources alternative to petroleum. Therefore the technologies such to manufacture chemicals from recyclable resources have been developed for the achievement of measures for controlling global warming and the low carbon society. Recently, the bioplastic such as polylactic resin is applied to the home appliances and the automobile interior part as substitution of general-purpose plastic Moreover, the <span class="hlt">insulation</span> oil from the vegetable oil has been put to practical use. The application of recyclable resources is extending in an electric field. In this <span class="hlt">paper</span>, we introduce the characteristic and the problem of the <span class="hlt">insulating</span> material made from recyclable resources in the field of the solid <span class="hlt">insulation</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1983STIN...8416513A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1983STIN...8416513A"><span>Reduction of heat <span class="hlt">insulation</span> upon soaking of the <span class="hlt">insulation</span> layer</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Achtliger, J.</p> <p>1983-09-01</p> <p>Improved thermal protection of hollow masonry by introduction of a core <span class="hlt">insulation</span> between the inner and outer shell is discussed. The thermal conductivity of <span class="hlt">insulation</span> materials was determined in dry state and after soaking by water with different volume-related moisture contents. The interpolated thermal conductivity values from three measured values at 10 C average temperature are presented as a function of the pertinent moisture content. Fills of expanded polystyrene, perlite and granulated mineral fibers, <span class="hlt">insulating</span> boards made of mineral fibers and in situ cellular plastics produced from urea-formaldehyde resin were investigated. Test results show a confirmation of thermal conductivity values for <span class="hlt">insulating</span> materials in hollow masonry.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/20543730','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/20543730"><span>Relationship between body <span class="hlt">composition</span>, leg strength, anaerobic power, and on-<span class="hlt">ice</span> skating performance in division I men's hockey athletes.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Potteiger, Jeffrey A; Smith, Dean L; Maier, Mark L; Foster, Timothy S</p> <p>2010-07-01</p> <p>The purpose of this study was to examine relationships between laboratory tests and on-<span class="hlt">ice</span> skating performance in division I men's hockey athletes. Twenty-one men (age 20.7 +/- 1.6 years) were assessed for body <span class="hlt">composition</span>, isokinetic force production in the quadriceps and hamstring muscles, and anaerobic muscle power via the Wingate 30-second cycle ergometer test. Air displacement plethysmography was used to determine % body fat (%FAT), fat-free mass (FFM), and fat mass. Peak torque and total work during 10 maximal effort repetitions at 120 degrees .s were measured during concentric muscle actions using an isokinetic dynamometer. Muscle power was measured using a Monark cycle ergometer with resistance set at 7.5% of body mass. On-<span class="hlt">ice</span> skating performance was measured during 6 timed 89-m sprints with subjects wearing full hockey equipment. First length skate (FLS) was 54 m, and total length skate (TLS) was 89 m with fastest and average skating times used in the analysis. Correlation coefficients were used to determine relationships between laboratory testing and on-<span class="hlt">ice</span> performance. Subjects had a body mass of 88.8 +/- 7.8 kg and %FAT of 11.9 +/- 4.6. First length skate-Average and TLS-Average skating times were moderately correlated to %FAT ([r = 0.53; p = 0.013] and [r = 0.57; p = 0.007]) such that a greater %FAT was related to slower skating speeds. First length skate-Fastest was correlated to Wingate percent fatigue index (r = -0.48; p = 0.027) and FLS-Average was correlated to Wingate peak power per kilogram body mass (r = -0.43; p = 0.05). Laboratory testing of select variables can predict skating performance in <span class="hlt">ice</span> hockey athletes. This information can be used to develop targeted and effective strength and conditioning programs that will improve on-<span class="hlt">ice</span> skating speed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018AcAau.145..141G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018AcAau.145..141G"><span>Influence of different propellant systems on ablation of EPDM <span class="hlt">insulators</span> in overload state</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Guan, Yiwen; Li, Jiang; Liu, Yang; Xu, Tuanwei</p> <p>2018-04-01</p> <p>This study examines the propellants used in full-scale solid rocket motors (SRM) and investigates how <span class="hlt">insulator</span> ablation is affected by two propellant formulations (A and B) during flight overload conditions. An experimental study, theoretical analysis, and numerical simulations were performed to discover the intrinsic causes of <span class="hlt">insulator</span> ablation rates from the perspective of lab-scaled ground-firing tests, the decoupling of thermochemical ablation, and particle erosion. In addition, the difference in propellant <span class="hlt">composition</span>, and the <span class="hlt">insulator</span> charring layer microstructure were analyzed. Results reveal that the degree of <span class="hlt">insulator</span> ablation is positively correlated with the propellant burn rate, particle velocity, and aggregate concentrations during the condensed phase. A lower ratio of energetic additive material in the AP oxidizer of the propellant is promising for the reduction in particle size and increase in the burn rate and pressure index. However, the overall higher velocity of a two-phase flow causes severe erosion of the <span class="hlt">insulation</span> material. While the higher ratio of energetic additive to the AP oxidizer imparts a smaller ablation rate to the <span class="hlt">insulator</span> (under lab-scale test conditions), the slag deposition problem in the combustion chamber may cause catastrophic consequences for future large full-scale SRM flight experiments.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018E%26ES..121b2032X','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018E%26ES..121b2032X"><span>Growing and testing mycelium bricks as building <span class="hlt">insulation</span> materials</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Xing, Yangang; Brewer, Matthew; El-Gharabawy, Hoda; Griffith, Gareth; Jones, Phil</p> <p>2018-02-01</p> <p>In order to improve energy performance of buildings, <span class="hlt">insulation</span> materials (such as mineral glass and rock wools, or fossil fuel-based plastic foams) are being used in increasing quantities, which may lead to potential problem with materials depletions and landfill disposal. One sustainable solution suggested is the use of bio-based, biodegradable materials. A number of attempts have been made to develop biomaterials, such as sheep wood, hemcrete or recycled <span class="hlt">papers</span>. In this <span class="hlt">paper</span>, a novel type of bio <span class="hlt">insulation</span> materials - mycelium is examined. The aim is to produce mycelium materials that could be used as <span class="hlt">insulations</span>. The bio-based material was required to have properties that matched existing alternatives, such as expanded polystyrene, in terms of physical and mechanical characteristics but with an enhanced level of biodegradability. The testing data showed mycelium bricks exhibited good thermal performance. Future work is planned to improve growing process and thermal performance of the mycelium bricks.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1989ESASP.302...65S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1989ESASP.302...65S"><span>Laboratory studies of cometary <span class="hlt">ice</span> analogues</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schmitt, B.; Espinasse, S.; Grim, R. J. A.; Greenberg, J. M.; Klinger, J.</p> <p>1989-12-01</p> <p>Laboratory studies were performed in order to simulate the physico-chemical processes that are likely to occur in the near surface layers of short and intermediate period comets. Pure H2O <span class="hlt">ice</span> as well as CO:H2O, CO2:H2O, CH4:H2O, CO:CO2:H2O, and NH3:H2O <span class="hlt">ice</span> mixtures were studied in the temperature range between 10 and 180 K. The evolution of the <span class="hlt">composition</span> of <span class="hlt">ice</span> mixtures, the crystallization of H2O <span class="hlt">ice</span> as well as the formation and decompostion of clathrate hydrate by different processes were studied as a function of temperature and time. Using the results together with numerical modeling, predictions are made about the survival of amorphous <span class="hlt">ice</span>, CO, CO2, CH4, and NH3 in the near surface layers of short period comets. The likeliness of finding clathrate and molecular hydrates is discussed. It is proposed that the analytical methods developed here could be fruitfully adapted to the analysis of returned comet samples.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20020076124','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20020076124"><span>Automotive <span class="hlt">Insulation</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>1997-01-01</p> <p>Under a Space Act Agreement between Boeing North America and BSR Products, Space Shuttle Thermal Protection System (TPS) materials are now used to <span class="hlt">insulate</span> race cars. BSR has created special TPS blanket <span class="hlt">insulation</span> kits for use on autos that take part in NASCAR events, and other race cars through its nationwide catalog distribution system. Temperatures inside a race car's cockpit can soar to a sweltering 140 to 160 degrees, with the extreme heat coming through the engine firewall, transmission tunnel, and floor. It is common for NASCAR drivers to endure blisters and burns due to the excessive heat. Tests on a car <span class="hlt">insulated</span> with the TPS material showed a temperature drop of some 50 degrees in the driver's cockpit. BSR-TPS Products, Inc. now manufactures <span class="hlt">insulation</span> kits for distribution to race car teams around the world.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009MCM....45..105M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009MCM....45..105M"><span>A <span class="hlt">composite</span> material based on recycled tires</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Malers, L.; Plesuma, R.; Locmele, L.</p> <p>2009-01-01</p> <p>The present study is devoted to the elaboration and investigation of a <span class="hlt">composite</span> material based on mechanically grinded recycled tires and a polymer binder. The correlation between the content of the binder, some technological parameters, and material properties of the <span class="hlt">composite</span> was clarified. The apparent density, the compressive stress at a 10% strain, the compressive elastic modulus in static and cyclic loadings, and the <span class="hlt">insulating</span> properties (acoustic and thermal) were the parameters of special interest of the present investigation. It is found that a purposeful variation of material <span class="hlt">composition</span> and some technological parameters leads to multifunctional <span class="hlt">composite</span> materials with different and predictable mechanical and <span class="hlt">insulation</span> properties.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70190395','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70190395"><span>Polar bears and sea <span class="hlt">ice</span> habitat change</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Durner, George M.; Atwood, Todd C.; Butterworth, Andy</p> <p>2017-01-01</p> <p>The polar bear (Ursus maritimus) is an obligate apex predator of Arctic sea <span class="hlt">ice</span> and as such can be affected by climate warming-induced changes in the extent and <span class="hlt">composition</span> of pack <span class="hlt">ice</span> and its impacts on their seal prey. Sea <span class="hlt">ice</span> declines have negatively impacted some polar bear subpopulations through reduced energy input because of loss of hunting habitats, higher energy costs due to greater <span class="hlt">ice</span> drift, <span class="hlt">ice</span> fracturing and open water, and ultimately greater challenges to recruit young. Projections made from the output of global climate models suggest that polar bears in peripheral Arctic and sub-Arctic seas will be reduced in numbers or become extirpated by the end of the twenty-first century if the rate of climate warming continues on its present trajectory. The same projections also suggest that polar bears may persist in the high-latitude Arctic where heavy multiyear sea <span class="hlt">ice</span> that has been typical in that region is being replaced by thinner annual <span class="hlt">ice</span>. Underlying physical and biological oceanography provides clues as to why polar bear in some regions are negatively impacted, while bears in other regions have shown no apparent changes. However, continued declines in sea <span class="hlt">ice</span> will eventually challenge the survival of polar bears and efforts to conserve them in all regions of the Arctic.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19970019307','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19970019307"><span><span class="hlt">Ices</span> on the Satellites of Jupiter, Saturn, and Uranus</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Cruikshank, Dale P.; Brown, Robert H.; Calvin, Wendy M.; Roush, Ted L.</p> <p>1995-01-01</p> <p>Three satellites of Jupiter, seven satellites of Saturn, and five satellites of Uranus show spectroscopic evidence of H2O <span class="hlt">ice</span> on their surfaces, although other details of their surfaces are highly diverse. The icy surfaces contain contaminants of unknown <span class="hlt">composition</span> in varying degrees of concentration, resulting in coloration and large differences in albedo. In addition to H2O, Europa has frozen SO2, and Ganymede has O2 in the surface; in both of these cases external causes are implicated in the deposition or formation of these trace components. Variations in <span class="hlt">ice</span> exposure across the surfaces of the satellites are measured from the spectroscopic signatures. While H2O <span class="hlt">ice</span> occurs on the surfaces of many satellites, the range of bulk densities of these bodies shows that its contribution to their overall <span class="hlt">compositions</span> is highly variable from one object to another.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.P31D2854F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.P31D2854F"><span>Longevity of <span class="hlt">Compositionally</span> Stratified Layers in <span class="hlt">Ice</span> Giants</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Friedson, A. J.</p> <p>2017-12-01</p> <p>In the hydrogen-rich atmospheres of gas giants, a decrease with radius in the mixing ratio of a heavy species (e.g. He, CH4, H2O) has the potential to produce a density stratification that is convectively stable if the heavy species is sufficiently abundant. Formation of stable layers in the interiors of these planets has important implications for their internal structure, chemical mixing, dynamics, and thermal evolution, since vertical transport of heat and constituents in such layers is greatly reduced in comparison to that in convecting layers. Various processes have been suggested for creating <span class="hlt">compositionally</span> stratified layers. In the interiors of Jupiter and Saturn, these include phase separation of He from metallic hydrogen and dissolution of dense core material into the surrounding metallic-H envelope. Condensation of methane and water has been proposed as a mechanism for producing stable zones in the atmospheres of Saturn and the <span class="hlt">ice</span> giants. However, if a stably stratified layer is formed adjacent to an active region of convection, it may be susceptible to progressive erosion as the convection intrudes and entrains fluid into the unstable envelope. We discuss the principal factors that control the rate of entrainment and associated erosion and present a specific example concerning the longevity of stable layers formed by condensation of methane and water in Uranus and Neptune. We also consider whether the temporal variability of such layers may engender episodic behavior in the release of the internal heat of these planets. This research is supported by a grant from the NASA Solar System Workings Program.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ApPhA.123..566L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ApPhA.123..566L"><span>Preparation of nitrogen-doped graphene/activated carbon <span class="hlt">composite</span> <span class="hlt">papers</span> to enhance energy storage in supercapacitors</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Li, Yong-feng; Liu, Yan-zhen; Liang, Yu; Guo, Xiao-hui; Chen, Cheng-meng</p> <p>2017-09-01</p> <p>This report presents a facile and effective method to synthesize freestanding nitrogen-doped reduced graphene oxide (rGO)/activated carbon (AC) <span class="hlt">composite</span> <span class="hlt">papers</span> for supercapacitors by a method combining vacuum filtration with post-annealing in NH3 atmosphere. The effect of activated carbon contents on the microstructure and capacitive behavior of the resulting <span class="hlt">composite</span> <span class="hlt">papers</span> before and after the annealing was investigated by X-ray diffraction, scanning electron microscopy, and Raman and X-ray photoelectron spectroscopy. Results show that the <span class="hlt">composite</span> <span class="hlt">paper</span> with a 30% activated carbon loading has a high nitrogen content of 14.6 at% and superior capacitive performance (308 F/g, 1 A/g) to the other <span class="hlt">composite</span> <span class="hlt">papers</span> with various activated carbon loadings. Nitrogen was doped and GO reduced during the annealing. The rGO nanosheets acted as a framework, and the AC particles served as spacers to avoid agglomeration of graphene sheets. The high capacitance of the <span class="hlt">composite</span> <span class="hlt">paper</span> is ascribed to the electric double-layer behavior and the reversible redox reactions of the nitrogen and oxygen groups. The entire process is simple, environmental friendly and easily scalable for mass production.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19970009491','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19970009491"><span>Tests of the Performance of Coatings for Low <span class="hlt">Ice</span> Adhesion</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Anderson, David N.; Reich, Allen D.</p> <p>1997-01-01</p> <p>This <span class="hlt">paper</span> reports studies of the performance of low-<span class="hlt">ice</span>-adhesion coatings by NASA Lewis and BFGoodrich. Studies used impact <span class="hlt">ice</span> accreted both in the NASA Lewis <span class="hlt">Icing</span> Research Tunnel (IRT) and in the BFGoodrich <span class="hlt">Icing</span> Wind Tunnel (IWT) and static <span class="hlt">ice</span> in a BFGoodrich bench-top parallel-plate shear rig. Early tests at NASA Lewis involved simple qualitative evaluations of the ease of removing impact <span class="hlt">ice</span> from a surface. Coated surfaces were compared with uncoated ones. Some of the coatings were tested again with static <span class="hlt">ice</span> at BFGoodrich to obtain quantitative measurements. Later, methods to establish the adhesion force on surfaces subjected to impact <span class="hlt">ice</span> were explored at Lewis. This <span class="hlt">paper</span> describes the various test programs and the results of testing some of the coatings looked at over the past 5 years. None of the coatings were found to be truly <span class="hlt">ice</span>-phobic; however, the most effective coatings were found to reduce the adhesion of <span class="hlt">ice</span> to about 1/2 that of an uncoated aluminum sample.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFM.C11B..03P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFM.C11B..03P"><span>Airborne radar surveys of snow depth over Antarctic sea <span class="hlt">ice</span> during Operation <span class="hlt">Ice</span>Bridge</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Panzer, B.; Gomez-Garcia, D.; Leuschen, C.; Paden, J. D.; Gogineni, P. S.</p> <p>2012-12-01</p> <p>Over the last decade, multiple satellite-based laser and radar altimeters, optimized for polar observations, have been launched with one of the major objectives being the determination of global sea <span class="hlt">ice</span> thickness and distribution [5, 6]. Estimation of sea-<span class="hlt">ice</span> thickness from these altimeters relies on freeboard measurements and the presence of snow cover on sea <span class="hlt">ice</span> affects this estimate. Current means of estimating the snow depth rely on daily precipitation products and/or data from passive microwave sensors [2, 7]. Even a small uncertainty in the snow depth leads to a large uncertainty in the sea-<span class="hlt">ice</span> thickness estimate. To improve the accuracy of the sea-<span class="hlt">ice</span> thickness estimates and provide validation for measurements from satellite-based sensors, the Center for Remote Sensing of <span class="hlt">Ice</span> Sheets deploys the Snow Radar as a part of NASA Operation <span class="hlt">Ice</span>Bridge. The Snow Radar is an ultra-wideband, frequency-modulated, continuous-wave radar capable of resolving snow depth on sea <span class="hlt">ice</span> from 5 cm to more than 2 meters from long-range, airborne platforms [4]. This <span class="hlt">paper</span> will discuss the algorithm used to directly extract snow depth estimates exclusively using the Snow Radar data set by tracking both the air-snow and snow-<span class="hlt">ice</span> interfaces. Prior work in this regard used data from a laser altimeter for tracking the air-snow interface or worked under the assumption that the return from the snow-<span class="hlt">ice</span> interface was greater than that from the air-snow interface due to a larger dielectric contrast, which is not true for thick or higher loss snow cover [1, 3]. This <span class="hlt">paper</span> will also present snow depth estimates from Snow Radar data during the NASA Operation <span class="hlt">Ice</span>Bridge 2010-2011 Antarctic campaigns. In 2010, three sea <span class="hlt">ice</span> flights were flown, two in the Weddell Sea and one in the Amundsen and Bellingshausen Seas. All three flight lines were repeated in 2011, allowing an annual comparison of snow depth. In 2011, a repeat pass of an earlier flight in the Weddell Sea was flown, allowing for a</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li class="active"><span>22</span></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_22 --> <div id="page_23" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li class="active"><span>23</span></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li><a href="#" onclick='return showDiv("page_25");'>25</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="441"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/6085044-arctic-ice-shelves-ice-islands-origin-growth-disintegration-physical-characteristics-structural-stratigraphic-variability-dynamics','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/6085044-arctic-ice-shelves-ice-islands-origin-growth-disintegration-physical-characteristics-structural-stratigraphic-variability-dynamics"><span>Arctic <span class="hlt">ice</span> shelves and <span class="hlt">ice</span> islands: Origin, growth and disintegration, physical characteristics, structural-stratigraphic variability, and dynamics</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Jeffries, M.O.</p> <p>1992-08-01</p> <p><span class="hlt">Ice</span> shelves are thick, floating <span class="hlt">ice</span> masses most often associated with Antarctica where they are seaward extensions of the grounded Antarctic <span class="hlt">ice</span> sheet and sources of many icebergs. However, there are also <span class="hlt">ice</span> shelves in the Arctic, primarily located along the north coast of Ellesmere Island in the Canadian High Arctic. The only <span class="hlt">ice</span> shelves in North America and the most extensive in the north polar region, the Ellesmere <span class="hlt">ice</span> shelves originate from glaciers and from sea <span class="hlt">ice</span> and are the source of <span class="hlt">ice</span> islands, the tabular icebergs of the Arctic Ocean. The present state of knowledge and understanding ofmore » these <span class="hlt">ice</span> features is summarized in this <span class="hlt">paper</span>. It includes historical background to the discovery and early study of <span class="hlt">ice</span> shelves and <span class="hlt">ice</span> islands, including the use of <span class="hlt">ice</span> islands as floating laboratories for polar geophysical research. Growth mechanisms and age, the former extent and the twentieth century disintegration of the Ellesmere <span class="hlt">ice</span> shelves, and the processes and mechanisms of <span class="hlt">ice</span> island calving are summarized. Surface features, thickness, thermal regime, and the size, shape, and numbers of <span class="hlt">ice</span> islands are discussed. The structural-stratigraphic variability of <span class="hlt">ice</span> islands and <span class="hlt">ice</span> shelves and the complex nature of their growth and development are described. Large-scale and small-scale dynamics of <span class="hlt">ice</span> islands are described, and the results of modeling their drift and recurrence intervals are presented. The conclusion identifies some unanswered questions and future research opportunities and needs. 97 refs., 18 figs.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/543464-innovative-self-drying-concept-thermal-insulation-cold-piping','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/543464-innovative-self-drying-concept-thermal-insulation-cold-piping"><span>Innovative self-drying concept for thermal <span class="hlt">insulation</span> of cold piping</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Korsgaard, V.</p> <p>1997-11-01</p> <p>In the <span class="hlt">paper</span> an innovative Self-Drying concept, the Hygro-Wick concept, for thermal <span class="hlt">insulation</span> of cold piping is described. The concept is based on the wicking action of certain fabrics to remove by capillary suction condensed water vapor from the pipe surface to the outer surface of the <span class="hlt">insulation</span>/jacket, from whence it will evaporate/diffuse into the ambient air. Hence the concept will prevent long term accumulation of moisture in the <span class="hlt">insulation</span> material. Theoretical and experimental results for two different embodiments of the concept is given: The Self-Drying system and the Self-Sealing system.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.P13A2117K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.P13A2117K"><span>Identification of Organics in <span class="hlt">Ice</span> Grains from Enceladus</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Khawaja, N.; Postberg, F.; Reviol, R.; Nölle, L.; Klenner, F.; Srama, R.</p> <p>2015-12-01</p> <p>The Cosmic Dust Analyzer (CDA) aboard the Cassini spacecraft performs in-situ measurements of the chemical <span class="hlt">composition</span> of icy dust grains impinging onto the target surface. The instrument recorded cationic Time-of-Flight (ToF) mass spectra of organic-bearing <span class="hlt">ice</span> grains emitted from Enceladus at different impact velocities causing different molecular fragmentation patterns [1,2]. Here we present a detailed analysis of these spectra (Type-2) to identify the <span class="hlt">composition</span> of organic material embedded in Enceladus <span class="hlt">ice</span> grains. The organic compounds display a great <span class="hlt">compositional</span> diversity, which indicates varying contributions of several organic species. The spectra analysis is supported by a large-scale laboratory ground campaign yielding a library of analogue spectra for organic material embedded in a water <span class="hlt">ice</span> matrix. To mimic the identified pattern of cationic fragments in organic enriched spectra we use a laboratory setup: Infrared Free Liquid MALDI ToF Mass Spectrometer (IR-FL-MALDI-ToF-MS). An infrared laser is used to disperse a liquid micro-beam of a water-solution to get cationic fragments. The laser energy is adjusted to simulate different impact velocities of <span class="hlt">ice</span> particles on CDA [3]. So far we have identified characteristic fragment patterns of at least three classes of organic molecules: (i) aromatic species, (ii) amines, and (iii) carbonyl group species. (i) <span class="hlt">ice</span> grains containing aromatic species are identified by a series of characteristic aromatic fragment cations (ii) <span class="hlt">ice</span> grains containing amines are identified by a pronounced ammonium cation and (iii) <span class="hlt">ice</span> grains containing carbonyl compounds are specified by a characteristic acylium cation in conjunction with certain others mass lines. Besides aromatic, amine and carbonyl species, Type-2 spectra also show contributions from other, yet un-specified, organic species. Typically, fragment cations of aromatic compounds are stable at impact velocities up-to 15km/s whereas cations of amines and carbonyl species</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=2952892','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=2952892"><span>Low Voltage Electrowetting-on-Dielectric Platform using Multi-Layer <span class="hlt">Insulators</span></span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Lin, Yan-You; Evans, Randall D.; Welch, Erin; Hsu, Bang-Ning; Madison, Andrew C.; Fair, Richard B.</p> <p>2010-01-01</p> <p>A low voltage, two-level-metal, and multi-layer <span class="hlt">insulator</span> electrowetting-on-dielectric (EWD) platform is presented. Dispensing 300pl droplets from 140nl closed on-chip reservoirs was accomplished with as little as 11.4V solely through EWD forces, and the actuation threshold voltage was 7.2V with a 1Hz voltage switching rate between electrodes. EWD devices were fabricated with a multilayer <span class="hlt">insulator</span> consisting of 135nm sputtered tantalum pentoxide (Ta2O5) and 180nm parylene C coated with 70nm of CYTOP. Furthermore, the minimum actuation threshold voltage followed a previously published scaling model for the threshold voltage, VT, which is proportional to (t/εr)1/2, where t and εr are the <span class="hlt">insulator</span> thickness and dielectric constant respectively. Device threshold voltages are compared for several <span class="hlt">insulator</span> thicknesses (200nm, 500nm, and 1µm), different dielectric materials (parylene C and tantalum pentoxide), and homogeneous versus heterogeneous <span class="hlt">compositions</span>. Additionally, we used a two-level-metal fabrication process, which enables the fabrication of smaller and denser electrodes with high interconnect routing flexibility. We also have achieved low dispensing and actuation voltages for scaled devices with 30pl droplets. PMID:20953362</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018TCry...12...25R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018TCry...12...25R"><span>Frazil-<span class="hlt">ice</span> growth rate and dynamics in mixed layers and sub-<span class="hlt">ice</span>-shelf plumes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rees Jones, David W.; Wells, Andrew J.</p> <p>2018-01-01</p> <p>The growth of frazil or granular <span class="hlt">ice</span> is an important mode of <span class="hlt">ice</span> formation in the cryosphere. Recent advances have improved our understanding of the microphysical processes that control the rate of <span class="hlt">ice</span>-crystal growth when water is cooled beneath its freezing temperature. These advances suggest that crystals grow much faster than previously thought. In this <span class="hlt">paper</span>, we consider models of a population of <span class="hlt">ice</span> crystals with different sizes to provide insight into the treatment of frazil <span class="hlt">ice</span> in large-scale models. We consider the role of crystal growth alongside the other physical processes that determine the dynamics of frazil <span class="hlt">ice</span>. We apply our model to a simple mixed layer (such as at the surface of the ocean) and to a buoyant plume under a floating <span class="hlt">ice</span> shelf. We provide numerical calculations and scaling arguments to predict the occurrence of frazil-<span class="hlt">ice</span> explosions, which we show are controlled by crystal growth, nucleation, and gravitational removal. Faster crystal growth, higher secondary nucleation, and slower gravitational removal make frazil-<span class="hlt">ice</span> explosions more likely. We identify steady-state crystal size distributions, which are largely insensitive to crystal growth rate but are affected by the relative importance of secondary nucleation to gravitational removal. Finally, we show that the fate of plumes underneath <span class="hlt">ice</span> shelves is dramatically affected by frazil-<span class="hlt">ice</span> dynamics. Differences in the parameterization of crystal growth and nucleation give rise to radically different predictions of basal accretion and plume dynamics, and can even impact whether a plume reaches the end of the <span class="hlt">ice</span> shelf or intrudes at depth.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/869794','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/servlets/purl/869794"><span>Calcium silicate <span class="hlt">insulation</span> structure</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Kollie, Thomas G.; Lauf, Robert J.</p> <p>1995-01-01</p> <p>An <span class="hlt">insulative</span> structure including a powder-filled evacuated casing utilizes a quantity of finely divided synthetic calcium silicate having a relatively high surface area. The resultant structure-provides superior thermal <span class="hlt">insulating</span> characteristics over a broad temperature range and is particularly well-suited as a panel for a refrigerator or freezer or the <span class="hlt">insulative</span> barrier for a cooler or a <span class="hlt">insulated</span> bottle.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20050182000&hterms=asbestos&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dasbestos','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20050182000&hterms=asbestos&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dasbestos"><span>NASA Lewis' <span class="hlt">Icing</span> Research Tunnel Works With Small Local Company to Test Coatings</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>1998-01-01</p> <p>Dynamic Coatings, Inc., wanted to test coating products that would enable the company to approach new markets. A Space Act Agreement with NASA Lewis Research Center afforded them this opportunity. They used Lewis' <span class="hlt">Icing</span> Research Tunnel to test coating products for reduced <span class="hlt">ice</span> adhesion, industrial and aerospace lubrication applications, a tiremold release coating now used in the production of tires for the Boeing 777, and a product that solidifies asbestos fibers (which is being tested as an <span class="hlt">insulator</span> in a power plant in Iowa). Not only was the testing a success, but during these activities, Dynamic Coatings met another coating company with whom they now have a joint venture offering a barnacle-repellent coating for marine applications, now on the market in Florida.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1321732','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1321732"><span>Computational Search for Strong Topological <span class="hlt">Insulators</span>: An Exercise in Data Mining and Electronic Structure</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Klintenberg, M.; Haraldsen, Jason T.; Balatsky, Alexander V.</p> <p></p> <p>In this <span class="hlt">paper</span>, we report a data-mining investigation for the search of topological <span class="hlt">insulators</span> by examining individual electronic structures for over 60,000 materials. Using a data-mining algorithm, we survey changes in band inversion with and without spin-orbit coupling by screening the calculated electronic band structure for a small gap and a change concavity at high-symmetry points. Overall, we were able to identify a number of topological candidates with varying structures and <span class="hlt">composition</span>. Lastly, our overall goal is expand the realm of predictive theory into the determination of new and exotic complex materials through the data mining of electronic structure.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1321732-computational-search-strong-topological-insulators-exercise-data-mining-electronic-structure','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1321732-computational-search-strong-topological-insulators-exercise-data-mining-electronic-structure"><span>Computational Search for Strong Topological <span class="hlt">Insulators</span>: An Exercise in Data Mining and Electronic Structure</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Klintenberg, M.; Haraldsen, Jason T.; Balatsky, Alexander V.</p> <p>2014-06-19</p> <p>In this <span class="hlt">paper</span>, we report a data-mining investigation for the search of topological <span class="hlt">insulators</span> by examining individual electronic structures for over 60,000 materials. Using a data-mining algorithm, we survey changes in band inversion with and without spin-orbit coupling by screening the calculated electronic band structure for a small gap and a change concavity at high-symmetry points. Overall, we were able to identify a number of topological candidates with varying structures and <span class="hlt">composition</span>. Lastly, our overall goal is expand the realm of predictive theory into the determination of new and exotic complex materials through the data mining of electronic structure.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20100041307','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20100041307"><span>Aerogel/polymer <span class="hlt">composite</span> materials</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Williams, Martha K. (Inventor); Smith, Trent M. (Inventor); Fesmire, James E. (Inventor); Roberson, Luke B. (Inventor); Clayton, LaNetra M. (Inventor)</p> <p>2010-01-01</p> <p>The invention provides new <span class="hlt">composite</span> materials containing aerogels blended with thermoplastic polymer materials at a weight ratio of aerogel to thermoplastic polymer of less than 20:100. The <span class="hlt">composite</span> materials have improved thermal <span class="hlt">insulation</span> ability. The <span class="hlt">composite</span> materials also have better flexibility and less brittleness at low temperatures than the parent thermoplastic polymer materials.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20170010458','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20170010458"><span>Aerogel / Polymer <span class="hlt">Composite</span> Materials</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Smith, Trent M. (Inventor); Clayton, LaNetra M. (Inventor); Fesmire, James E. (Inventor); Williams, Martha K. (Inventor); Roberson, Luke B. (Inventor)</p> <p>2017-01-01</p> <p>The invention provides new <span class="hlt">composite</span> materials containing aerogels blended with thermoplastic polymer materials at a weight ratio of aerogel to thermoplastic polymer of less than 20:100. The <span class="hlt">composite</span> materials have improved thermal <span class="hlt">insulation</span> ability. The <span class="hlt">composite</span> materials also have better flexibility and less brittleness at low temperatures than the parent thermoplastic polymer materials.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012MPLB...2650095L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012MPLB...2650095L"><span>Lightning Impulse Breakdown Characteristics and Electrodynamic Process of <span class="hlt">Insulating</span> Vegetable Oil-Based Nanofluid</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Li, Jian; Zhang, Zhao-Tao; Zou, Ping; Du, Bin; Liao, Rui-Jin</p> <p>2012-06-01</p> <p><span class="hlt">Insulating</span> vegetable oils are considered environment-friendly and fire-resistant substitutes for <span class="hlt">insulating</span> mineral oils. This <span class="hlt">paper</span> presents the lightning impulse breakdown characteristic of <span class="hlt">insulating</span> vegetable oil and <span class="hlt">insulating</span> vegetable oil-based nanofluids. It indicates that Fe3O4 nanoparticles can increase the negative lightning impulse breakdown voltages of <span class="hlt">insulating</span> vegetable oil by 11.8% and positive lightning impulse breakdown voltages by 37.4%. The propagation velocity of streamer is reduced by the presence of nanoparticles. The propagation velocities of streamer to positive and negative lightning impulse breakdown in the <span class="hlt">insulating</span> vegetable oil-based nanofluids are 21.2% and 14.4% lesser than those in <span class="hlt">insulating</span> vegetable oils, respectively. The higher electrical breakdown strength and lower streamer velocity is explained by the charging dynamics of nanoparticles in <span class="hlt">insulating</span> vegetable oil. Space charge build-up and space charge distorted filed in point-sphere gap is also described. The field strength is reduced at the streamer tip due to the low mobility of negative nanoparticles.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29469238','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29469238"><span>Fire-Retardant and Thermally <span class="hlt">Insulating</span> Phenolic-Silica Aerogels.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Yu, Zhi-Long; Yang, Ning; Apostolopoulou-Kalkavoura, Varvara; Qin, Bing; Ma, Zhi-Yuan; Xing, Wei-Yi; Qiao, Chan; Bergström, Lennart; Antonietti, Markus; Yu, Shu-Hong</p> <p>2018-04-16</p> <p>Energy efficient buildings require materials with a low thermal conductivity and a high fire resistance. Traditional organic <span class="hlt">insulation</span> materials are limited by their poor fire resistance and inorganic <span class="hlt">insulation</span> materials are either brittle or display a high thermal conductivity. Herein we report a mechanically resilient organic/inorganic <span class="hlt">composite</span> aerogel with a thermal conductivity significantly lower than expanded polystyrene and excellent fire resistance. Co-polymerization and nanoscale phase separation of the phenol-formaldehyde-resin (PFR) and silica generate a binary network with domain sizes below 20 nm. The PFR/SiO 2 aerogel can resist a high-temperature flame without disintegration and prevents the temperature on the non-exposed side from increasing above the temperature critical for the collapse of reinforced concrete structures. © 2018 Wiley-VCH Verlag GmbH & Co. KGaA, Weinheim.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017SPJCE..12...97B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017SPJCE..12...97B"><span>Technology of Double Thermal <span class="hlt">Insulation</span> for the Repair and Energy Optimization of Existing Thermal <span class="hlt">Insulation</span> <span class="hlt">Composite</span> Systems</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Belániová, Barbora; Antošová, Naďa</p> <p>2017-06-01</p> <p>The theme of improvement thermal proprieties of external cladding according to the New EU Directive is still a hot topic, which needs to be answered necessarily till December 2020. Maintenance and repair of existing ETICS became to also an actual open theme in search solutions for existing constructions. The aim of the research in this review is to analyze influence of layers the alternative thermal materials in technology "double thermal <span class="hlt">insulation</span>". Humidity and temperature conditions will be further examined in connection with the development and colonization of microorganisms on surface construction.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015DPS....4720001G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015DPS....4720001G"><span>Configuration of Pluto's Volatile <span class="hlt">Ices</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Grundy, William M.; Binzel, R. P.; Cook, J. C.; Cruikshank, D. P.; Dalle Ore, C. M.; Earle, A. M.; Ennico, K.; Jennings, D. E.; Howett, C. J. A.; Linscott, I. R.; Lunsford, A. W.; Olkin, C. B.; Parker, A. H.; Parker, J. Wm; Protopapa, S.; Reuter, D. C.; Singer, K. N.; Spencer, J. R.; Stern, S. A.; Tsang, C. C. C.; Verbiscer, A. J.; Weaver, H. A.; Young, L. A.; Berry, K.; Buie, M. W.; Stansberry, J. A.</p> <p>2015-11-01</p> <p>We report on near-infrared remote sensing by New Horizons' Ralph instrument (Reuter et al. 2008, Space Sci. Rev. 140, 129-154) of Pluto's N2, CO, and CH4 <span class="hlt">ices</span>. These especially volatile <span class="hlt">ices</span> are mobile even at Pluto's cryogenic surface temperatures. Sunlight reflected from these <span class="hlt">ices</span> becomes imprinted with their characteristic spectral absorption bands. The detailed appearance of these absorption features depends on many aspects of local <span class="hlt">composition</span>, thermodynamic state, and texture. Multiple-scattering radiative transfer models are used to retrieve quantitative information about these properties and to map how they vary across Pluto's surface. Using parameter maps derived from New Horizons observations, we investigate the striking regional differences in the abundances and scattering properties of Pluto's volatile <span class="hlt">ices</span>. Comparing these spatial patterns with the underlying geology provides valuable constraints on processes actively modifying the planet's surface, over a variety of spatial scales ranging from global latitudinal patterns to more regional and local processes within and around the feature informally known as Sputnik Planum. This work was supported by the NASA New Horizons Project.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EPSC...11..423N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EPSC...11..423N"><span>Laboratory investigation of nitrile <span class="hlt">ices</span> of Titan's stratospheric clouds</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nna Mvondo, D.; Anderson, C. M.; McLain, J. L.; Samuelson, R. E.</p> <p>2017-09-01</p> <p>Titan's mid to lower stratosphere contains complex cloud systems of numerous organic <span class="hlt">ice</span> particles comprised of both hydrocarbon and nitrile compounds. Most of these stratospheric <span class="hlt">ice</span> clouds form as a result of vapor condensation formation processes. However, there are additional <span class="hlt">ice</span> emission features such as dicyanoacetylene (C4N2) and the 220 cm-1 <span class="hlt">ice</span> emission feature (the "Haystack") that are difficult to explain since there are no observed vapor emission features associated with these <span class="hlt">ices</span>. In our laboratory, using a high-vacuum chamber coupled to a FTIR spectrometer, we are engaged in a dedicated investigation of Titan's stratospheric <span class="hlt">ices</span> to interpret and constrain Cassini <span class="hlt">Composite</span> InfraRed Spectrometer (CIRS) far-IR data. We will present laboratory transmittance spectra obtained for propionitrile (CH3CH2CN), cyanogen (C2N2) and hydrogen cyanide (HCN) <span class="hlt">ices</span>, as well as various combinations of their mixtures, to better understand the cloud chemistry occurring in Titan's stratosphere.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5512346','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5512346"><span>Doping Effect of Graphene Nanoplatelets on Electrical <span class="hlt">Insulation</span> Properties of Polyethylene: From Macroscopic to Molecular Scale</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Jing, Ziang; Li, Changming; Zhao, Hong; Zhang, Guiling; Han, Baozhong</p> <p>2016-01-01</p> <p>The doping effect of graphene nanoplatelets (GNPs) on electrical <span class="hlt">insulation</span> properties of polyethylene (PE) was studied by combining experimental and theoretical methods. The electric conduction properties and trap characteristics were tested for pure PE and PE/GNPs <span class="hlt">composites</span> by using a direct measurement method and a thermal stimulated current (TSC) method. It was found that doping smaller GNPs is more beneficial to decrease the conductivity of PE/GNPs. The PE/GNPs <span class="hlt">composite</span> with smaller size GNPs mainly introduces deep energy traps, while with increasing GNPs size, besides deep energy traps, shallow energy traps are also introduced. These results were also confirmed by density functional theory (DFT) and the non-equilibrium Green’s function (NEGF) method calculations. Therefore, doping small size GNPs is favorable for trapping charge carriers and enhancing <span class="hlt">insulation</span> ability, which is suggested as an effective strategy in exploring powerful <span class="hlt">insulation</span> materials. PMID:28773802</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012EGUGA..1410810P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012EGUGA..1410810P"><span>Palaeoclimate signal recorded by stable isotopes in cave <span class="hlt">ice</span>: a modeling approach</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Perşoiu, A.; Bojar, A.-V.</p> <p>2012-04-01</p> <p><span class="hlt">Ice</span> accumulations in caves preserve a large variety of geochemical information as candidate proxies for both past climate and environmental changes, one of the most significant being the stable isotopic <span class="hlt">composition</span> of the <span class="hlt">ice</span>. A series of recent studies have targeted oxygen and hydrogen stable isotopes in cave <span class="hlt">ice</span> as proxies for past air temperatures, but the results are far from being as straightforward as they are in high latitude and altitude glaciers and <span class="hlt">ice</span> caps. The main problems emerging from these studies are related to the mechanisms of cave <span class="hlt">ice</span> formation (i.e., freezing of water) and post-formation processes (melting and refreezing), which both alter the original isotopic signal in water. Different methods have been put forward to solve these issues and a fair understanding of the present-day link between stable isotopes in precipitation and cave <span class="hlt">ice</span> exists now. However, the main issues still lays unsolved: 1) is it possible to extend this link to older <span class="hlt">ice</span> and thus reconstruct past changes in air temperature?; 2) to what extent are <span class="hlt">ice</span> dynamics processes modifying the original climatic signal and 3) what is the best method to be used in extracting a climatic signal from stable isotopes in cave <span class="hlt">ice</span>? To respond to these questions, we have conducted a modeling experiment, in which a theoretical cave <span class="hlt">ice</span> stable isotope record was constructed using present-day observations on stable isotope behavior in cave <span class="hlt">ice</span> and <span class="hlt">ice</span> dynamics, and different methods (presently used for both polar and cave glaciers), were used to reconstruct the original, known, isotopic values. Our results show that it is possible to remove the effects of <span class="hlt">ice</span> melting and refreezing on stable isotope <span class="hlt">composition</span> of cave <span class="hlt">ice</span>, and thus reconstruct the original isotopic signal, and further the climatic one.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20120018032','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20120018032"><span><span class="hlt">Ice</span> Growth Measurements from Image Data to Support <span class="hlt">Ice</span> Crystal and Mixed-Phase Accretion Testing</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Struk, Peter M.; Lynch, Christopher J.</p> <p>2012-01-01</p> <p>This <span class="hlt">paper</span> describes the imaging techniques as well as the analysis methods used to measure the <span class="hlt">ice</span> thickness and growth rate in support of <span class="hlt">ice</span>-crystal <span class="hlt">icing</span> tests performed at the National Research Council of Canada (NRC) Research Altitude Test Facility (RATFac). A detailed description of the camera setup, which involves both still and video cameras, as well as the analysis methods using the NASA Spotlight software, are presented. Two cases, one from two different test entries, showing significant <span class="hlt">ice</span> growth are analyzed in detail describing the <span class="hlt">ice</span> thickness and growth rate which is generally linear. Estimates of the bias uncertainty are presented for all measurements. Finally some of the challenges related to the imaging and analysis methods are discussed as well as methods used to overcome them.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20120014350','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20120014350"><span><span class="hlt">Ice</span> Growth Measurements from Image Data to Support <span class="hlt">Ice</span>-Crystal and Mixed-Phase Accretion Testing</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Struk, Peter, M; Lynch, Christopher, J.</p> <p>2012-01-01</p> <p>This <span class="hlt">paper</span> describes the imaging techniques as well as the analysis methods used to measure the <span class="hlt">ice</span> thickness and growth rate in support of <span class="hlt">ice</span>-crystal <span class="hlt">icing</span> tests performed at the National Research Council of Canada (NRC) Research Altitude Test Facility (RATFac). A detailed description of the camera setup, which involves both still and video cameras, as well as the analysis methods using the NASA Spotlight software, are presented. Two cases, one from two different test entries, showing significant <span class="hlt">ice</span> growth are analyzed in detail describing the <span class="hlt">ice</span> thickness and growth rate which is generally linear. Estimates of the bias uncertainty are presented for all measurements. Finally some of the challenges related to the imaging and analysis methods are discussed as well as methods used to overcome them.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li class="active"><span>23</span></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li><a href="#" onclick='return showDiv("page_25");'>25</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_23 --> <div id="page_24" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li class="active"><span>24</span></li> <li><a href="#" onclick='return showDiv("page_25");'>25</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="461"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20120002028','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20120002028"><span>Electromagnetic Nondestructive Evaluation of Wire <span class="hlt">Insulation</span> and Models of <span class="hlt">Insulation</span> Material Properties</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Bowler, Nicola; Kessler, Michael R.; Li, Li; Hondred, Peter R.; Chen, Tianming</p> <p>2012-01-01</p> <p>Polymers have been widely used as wiring electrical <span class="hlt">insulation</span> materials in space/air-craft. The dielectric properties of <span class="hlt">insulation</span> polymers can change over time, however, due to various aging processes such as exposure to heat, humidity and mechanical stress. Therefore, the study of polymers used in electrical <span class="hlt">insulation</span> of wiring is important to the aerospace industry due to potential loss of life and aircraft in the event of an electrical fire caused by breakdown of wiring <span class="hlt">insulation</span>. Part of this research is focused on studying the mechanisms of various environmental aging process of the polymers used in electrical wiring <span class="hlt">insulation</span> and the ways in which their dielectric properties change as the material is subject to the aging processes. The other part of the project is to determine the feasibility of a new capacitive nondestructive testing method to indicate degradation in the wiring <span class="hlt">insulation</span>, by measuring its permittivity.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016MS%26E..124a2123D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016MS%26E..124a2123D"><span>Basalt fiber <span class="hlt">insulating</span> material with a mineral binding agent for industrial use</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Drozdyuk, T.; Aizenshtadt, A.; Tutygin, A.; Frolova, M.</p> <p>2016-04-01</p> <p>The <span class="hlt">paper</span> considers a possibility of using mining industry waste as a binding agent for heat <span class="hlt">insulating</span> material on the basis of basalt fiber. The main objective of the research is to produce a heat-<span class="hlt">insulating</span> material to be applied in machine building in high-temperature environments. After synthetic binder having been replaced by a mineral one, an environmentally sound thermal <span class="hlt">insulating</span> material having desirable heat-protecting ability and not failing when exposed to high temperatures was obtained.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20130009044','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20130009044"><span>Anti-<span class="hlt">Icing</span> Formulas Prevent Train Delays</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>2013-01-01</p> <p>In the winter of 2009, Washington, DC, workers faced the prospect of a difficult commute due to record-setting snowfalls. But thousands of the city's Metrorail riders found the public transportation system fully functional, thanks in part to a NASA technology invented years before. Just like trains, an airplane must be snow- and <span class="hlt">ice</span>-free to ensure safe travel. Traditionally, fluids containing a compound called ethylene glycol have been used to inhibit <span class="hlt">ice</span> on planes. In 1992, however, the US Air Force banned its purchase of this ingredient due to toxicity concerns. According to the Centers for Disease Control, exposure to large amounts of ethylene glycol through air or water can damage the kidneys, nervous system, lungs, and heart. Urine samples from airport deicing workers have contained traces of the substance. At the time of the Air Force s ban, Robert Lockyer was working at NASA s Ames Research Center in the Advanced <span class="hlt">Composites</span> Model Development Branch, where he says "we decided to pick up the gauntlet and began researching existing fluid <span class="hlt">compositions</span> and the processes used in deicing aircraft." Along with Lockyer, in 1997 Ames researchers Leonard Haslim and John Zuk devised a nontoxic, biodegradable, and cost effective substitute for ethylene glycol. When applied to a dry surface before a snow or <span class="hlt">ice</span> event, the solution prevented <span class="hlt">ice</span> from forming a bond with the surface. This made it easy to wipe away any accumulation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.C33A0684F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.C33A0684F"><span><span class="hlt">Ice</span>911 Research: Preserving and Rebuilding Multi-Year <span class="hlt">Ice</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Field, L. A.; Chetty, S.; Manzara, A.</p> <p>2013-12-01</p> <p>A localized surface albedo modification technique is being developed that shows promise as a method to increase multi-year <span class="hlt">ice</span> using reflective floating materials, chosen so as to have low subsidiary environmental impact. Multi-year <span class="hlt">ice</span> has diminished rapidly in the Arctic over the past 3 decades (Riihela et al, Nature Climate Change, August 4, 2013) and this plays a part in the continuing rapid decrease of summer-time <span class="hlt">ice</span>. As summer-time <span class="hlt">ice</span> disappears, the Arctic is losing its ability to act as the earth's refrigeration system, and this has widespread climatic effects, as well as a direct effect on sea level rise, as oceans heat, and once-land-based <span class="hlt">ice</span> melts into the sea. We have tested the albedo modification technique on a small scale over five Winter/Spring seasons at sites including California's Sierra Nevada Mountains, a Canadian lake, and a small man-made lake in Minnesota, using various materials and an evolving array of instrumentation. The materials can float and can be made to minimize effects on marine habitat and species. The instrumentation is designed to be deployed in harsh and remote locations. Localized snow and <span class="hlt">ice</span> preservation, and reductions in water heating, have been quantified in small-scale testing. Climate modeling is underway to analyze the effects of this method of surface albedo modification in key areas on the rate of oceanic and atmospheric temperature rise. We are also evaluating the effects of snow and <span class="hlt">ice</span> preservation for protection of infrastructure and habitat stabilization. This <span class="hlt">paper</span> will also discuss a possible reduction of sea level rise with an eye to quantification of cost/benefit. The most recent season's experimentation on a man-made private lake in Minnesota saw further evolution in the material and deployment approach. The materials were successfully deployed to shield underlying snow and <span class="hlt">ice</span> from melting; applications of granular materials remained stable in the face of local wind and storms. Localized albedo</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003DPS....35.1502E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003DPS....35.1502E"><span>Are There Oceans Under the <span class="hlt">Ice</span> of Small Saturnian and Uranian Moons?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>England, C.</p> <p>2003-05-01</p> <p>Thermal analysis of the large outer-planetary moons (Titan, Callisto, Ganymede) argue strongly for substantial subsurface oceans if they are made up mostly of rock and <span class="hlt">ice</span>, and if the rock exhibits radioactivity not too different from that of meteoric and lunar material [1]. For Titania, Rhea, Oberon and Iapetus (the TROI moons) with radii just over 700 km, the existence of oceans is less clear. In these bodies, a subsurface ocean may be likely if the rock has sunk to the center of the moon (i.e., the moon is differentiated) and (1) the radiogenic heating rate is on the higher end of that of lunar samples, (2) the bodies experience tidal heating, or (3) the oceans contain compounds such as ammonia that reduce the freezing point of the aqueous environment. A combination of these occurrences would weigh for a subsurface ocean, perhaps of substantial size. That outer-planetary moons with radii larger than about 200 km (e.g.; Enceladus at 250 km) are spherical argues for separation of light and heavy materials, especially in the larger bodies. Otherwise, the moon exhibits an irregular shape (e.g.; Hyperion at 133 km). Primordial radioactivity and collision events may have aided separation. If present-day radiogenicity is that of lunar samples, natural heating is available to maintain global aqueous environments on all of the TROI moons. The ammonia-water eutectics suggested for Titan [2] provide additional margin. The maintenance of oceans in smaller bodies depends on a balance of internal heat generation and thermal isolation by <span class="hlt">ice</span> or other <span class="hlt">insulating</span> material. The more important parameter may be the <span class="hlt">insulating</span> <span class="hlt">ice</span>, without which an outer-planetary ocean is not possible. The reduced thermal conductivity for impure <span class="hlt">ice</span> [3] provides even more likelihood for oceans. Calculations for tidal heating within Europa due to orbital resonances [4] suggest that tidal heating amounts to over 40 times its internal radiogenic heating. A value equal only to natural radiogenic</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5978228','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5978228"><span>Preparation Nano-Structure Polytetrafluoroethylene (PTFE) Functional Film on the Cellulose <span class="hlt">Insulation</span> Polymer and Its Effect on the Breakdown Voltage and Hydrophobicity Properties</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Liu, Cong; Li, Yanqing; Liao, Ruijin; Liao, Qiang; Tang, Chao</p> <p>2018-01-01</p> <p>Cellulose <span class="hlt">insulation</span> polymer is an important component of oil-<span class="hlt">paper</span> <span class="hlt">insulation</span>, which is widely used in power transformer. The weight of the cellulose <span class="hlt">insulation</span> polymer materials is as high as tens of tons in the larger converter transformer. Excellent performance of oil-<span class="hlt">paper</span> <span class="hlt">insulation</span> is very important for ensuring the safe operation of larger converter transformer. An effective way to improve the <span class="hlt">insulation</span> and the physicochemical property of the oil impregnated <span class="hlt">insulation</span> pressboard/<span class="hlt">paper</span> is currently a popular research topic. In this <span class="hlt">paper</span>, the polytetrafluoroethylene (PTFE) functional film was coated on the cellulose <span class="hlt">insulation</span> pressboard by radio frequency (RF) magnetron sputtering to improve its breakdown voltage and the hydrophobicity properties. X-ray photoelectron spectroscopy (XPS) results show that the nano-structure PTFE functional film was successfully fabricated on the cellulose <span class="hlt">insulation</span> pressboard surface. The scanning electron microscopy (SEM) and X-ray diffraction (XRD) present that the nanoscale size PTFE particles were attached to the pressboard surface and it exists in the amorphous form. Atomic force microscopy (AFM) shows that the sputtered pressboard surface is still rough. The rough PTFE functional film and the reduction of the hydrophilic hydroxyl of the surface due to the shielding effect of PTFE improve the breakdown and the hydrophobicity properties of the cellulose <span class="hlt">insulation</span> pressboard obviously. This <span class="hlt">paper</span> provides an innovative way to improve the performance of the cellulose <span class="hlt">insulation</span> polymer. PMID:29883376</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29883376','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29883376"><span>Preparation Nano-Structure Polytetrafluoroethylene (PTFE) Functional Film on the Cellulose <span class="hlt">Insulation</span> Polymer and Its Effect on the Breakdown Voltage and Hydrophobicity Properties.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Hao, Jian; Liu, Cong; Li, Yanqing; Liao, Ruijin; Liao, Qiang; Tang, Chao</p> <p>2018-05-21</p> <p>Cellulose <span class="hlt">insulation</span> polymer is an important component of oil-<span class="hlt">paper</span> <span class="hlt">insulation</span>, which is widely used in power transformer. The weight of the cellulose <span class="hlt">insulation</span> polymer materials is as high as tens of tons in the larger converter transformer. Excellent performance of oil-<span class="hlt">paper</span> <span class="hlt">insulation</span> is very important for ensuring the safe operation of larger converter transformer. An effective way to improve the <span class="hlt">insulation</span> and the physicochemical property of the oil impregnated <span class="hlt">insulation</span> pressboard/<span class="hlt">paper</span> is currently a popular research topic. In this <span class="hlt">paper</span>, the polytetrafluoroethylene (PTFE) functional film was coated on the cellulose <span class="hlt">insulation</span> pressboard by radio frequency (RF) magnetron sputtering to improve its breakdown voltage and the hydrophobicity properties. X-ray photoelectron spectroscopy (XPS) results show that the nano-structure PTFE functional film was successfully fabricated on the cellulose <span class="hlt">insulation</span> pressboard surface. The scanning electron microscopy (SEM) and X-ray diffraction (XRD) present that the nanoscale size PTFE particles were attached to the pressboard surface and it exists in the amorphous form. Atomic force microscopy (AFM) shows that the sputtered pressboard surface is still rough. The rough PTFE functional film and the reduction of the hydrophilic hydroxyl of the surface due to the shielding effect of PTFE improve the breakdown and the hydrophobicity properties of the cellulose <span class="hlt">insulation</span> pressboard obviously. This <span class="hlt">paper</span> provides an innovative way to improve the performance of the cellulose <span class="hlt">insulation</span> polymer.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23571922','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23571922"><span>Phase modulation in horizontal metal-<span class="hlt">insulator-silicon-insulator</span>-metal plasmonic waveguides.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Zhu, Shiyang; Lo, G Q; Kwong, D L</p> <p>2013-04-08</p> <p>An extremely compact Si phase modulator is proposed and validated, which relies on effective modulation of the real part of modal index of horizontal metal-<span class="hlt">insulator-Si-insulator</span>-metal plasmonic waveguides by a voltage applied between the metal cover and the Si core. Proof-of-concept devices are fabricated on silicon-on-<span class="hlt">insulator</span> substrates using standard complementary metal-oxide-semiconductor technology using copper as the metal and thermal silicon dioxide as the <span class="hlt">insulator</span>. A modulator with a 1-μm-long phase shifter inserted in an asymmetric Si Mach-Zehnder interferometer exhibits 9-dB extinction ratio under a 6-V/10-kHz voltage swing. Numerical simulations suggest that high speed and low driving voltage could be achieved by shortening the distance between the Si core and the n(+)-contact and by using a high-κ dielectric as the <span class="hlt">insulator</span>, respectively.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20100028890','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20100028890"><span>Nearly Seamless Vacuum-<span class="hlt">Insulated</span> Boxes</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Stepanian, Christopher J.; Ou, Danny; Hu, Xiangjun</p> <p>2010-01-01</p> <p>A design concept, and a fabrication process that would implement the design concept, have been proposed for nearly seamless vacuum-<span class="hlt">insulated</span> boxes that could be the main structural components of a variety of controlled-temperature containers, including common household refrigerators and <span class="hlt">insulating</span> containers for shipping foods. In a typical case, a vacuum-<span class="hlt">insulated</span> box would be shaped like a rectangular parallelepiped conventional refrigerator box having five fully closed sides and a hinged door on the sixth side. Although it is possible to construct the five-closed-side portion of the box as an assembly of five unitary vacuum-<span class="hlt">insulated</span> panels, it is not desirable to do so because the relatively high thermal conductances of the seams between the panels would contribute significant amounts of heat leakage, relative to the leakage through the panels themselves. In contrast, the proposal would make it possible to reduce heat leakage by constructing the five-closed-side portion of the box plus the stationary portion (if any) of the sixth side as a single, seamless unit; the only remaining seam would be the edge seal around the door. The basic cross-sectional configuration of each side of a vacuum-<span class="hlt">insulated</span> box according to the proposal would be that of a conventional vacuum-<span class="hlt">insulated</span> panel: a low-density, porous core material filling a partially evacuated space between face sheets. However, neither the face sheets nor the core would be conventional. The face sheets would be opposite sides of a vacuum bag. The core material would be a flexible polymer-modified silica aerogel of the type described in Silica/Polymer and Silica/Polymer/Fiber <span class="hlt">Composite</span> Aero - gels (MSC-23736) in this issue of NASA Tech Briefs. As noted in that article, the stiffness of this core material against compression is greater than that of prior aerogels. This is an important advantage because it translates to greater retention of thickness and, hence, of <span class="hlt">insulation</span> performance when pressure is</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/15207296','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/15207296"><span>Possibility of using waste tire <span class="hlt">composites</span> reinforced with rice straw as construction materials.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Yang, Han-Seung; Kim, Dae-Jun; Lee, Young-Kyu; Kim, Hyun-Joong; Jeon, Jin-Yong; Kang, Chun-Won</p> <p>2004-10-01</p> <p>Agricultural lignocellulosic fiber (rice straw)-waste tire particle <span class="hlt">composite</span> boards were manufactured for use as <span class="hlt">insulation</span> boards in construction, using the same method as that used in the wood-based panel industry. The manufacturing parameters were: a specific gravity of 0.8 and a rice straw content (10/90, 20/80 and 30/70 by wt.% of rice straw/waste tire particle). A commercial polyurethane adhesive for rubber was used as the <span class="hlt">composite</span> binder. The water proof, water absorption and thickness swelling properties of the <span class="hlt">composite</span> boards were better than those of wood particleboard. Furthermore, the flexibility and flexural properties of the <span class="hlt">composite</span> boards were superior to those of other wood-based panel products. The <span class="hlt">composite</span> boards also demonstrated good acoustical <span class="hlt">insulation</span>, electrical <span class="hlt">insulation</span>, anti-caustic and anti-rot properties. These boards can be used to prevent impact damage, are easily modifiable and are inexpensive. They are able to be used as a substitute for <span class="hlt">insulation</span> boards and other flexural materials in construction.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19890003370','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19890003370"><span>Cryogenic <span class="hlt">Insulation</span> System</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Davis, Randall C. (Inventor); Taylor, Allan H. (Inventor); Jackson, L. Robert (Inventor); Mcauliffe, Patrick S. (Inventor)</p> <p>1988-01-01</p> <p>This invention relates to reusable, low density, high temperature cryogenic foam <span class="hlt">insulation</span> systems and the process for their manufacture. A pacing technology for liquid hydrogen fueled, high speed aircraft is the development of a fully reusable, flight weight cryogenic <span class="hlt">insulation</span> system for propellant tank structures. In the invention cryogenic foam <span class="hlt">insulation</span> is adhesively bonded to the outer wall of the fuel tank structure. The cryogenic <span class="hlt">insulation</span> consists of square sheets fabricated from an array of abutting square blocks. Each block consists of a sheet of glass cloth adhesively bonded between two layers of polymethacrylimide foam. Each block is wrapped in a vapor impermeable membrane, such as Kapton(R) aluminum Kapton(R), to provide a vapor barrier. Very beneficial results can be obtained by employing the present invention in conjunction with fibrous <span class="hlt">insulation</span> and an outer aeroshell, a hot fuselage structure with an internal thermal protection system.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26339489','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26339489"><span><span class="hlt">Ice</span> swimming - '<span class="hlt">Ice</span> Mile' and '1 km <span class="hlt">Ice</span> event'.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Knechtle, Beat; Rosemann, Thomas; Rüst, Christoph A</p> <p>2015-01-01</p> <p><span class="hlt">Ice</span> swimming for 1 mile and 1 km is a new discipline in open-water swimming since 2009. This study examined female and male performances in swimming 1 mile ('<span class="hlt">Ice</span> Mile') and 1 km ('1 km <span class="hlt">Ice</span> event') in water of 5 °C or colder between 2009 and 2015 with the hypothesis that women would be faster than men. Between 2009 and 2015, 113 men and 38 women completed one '<span class="hlt">Ice</span> Mile' and 26 men and 13 completed one '1 km <span class="hlt">Ice</span> event' in water colder than +5 °C following the rules of International <span class="hlt">Ice</span> Swimming Association (IISA). Differences in performance between women and men were determined. Sex difference (%) was calculated using the equation ([time for women] - [time for men]/[time for men] × 100). For '<span class="hlt">Ice</span> Mile', a mixed-effects regression model with interaction analyses was used to investigate the influence of sex and environmental conditions on swimming speed. The association between water temperature and swimming speed was assessed using Pearson correlation analyses. For '<span class="hlt">Ice</span> Mile' and '1 km <span class="hlt">Ice</span> event', the best men were faster than the best women. In '<span class="hlt">Ice</span> Mile', calendar year, number of attempts, water temperature and wind chill showed no association with swimming speed for both women and men. For both women and men, water temperature was not correlated to swimming speed in both '<span class="hlt">Ice</span> Mile' and '1 km <span class="hlt">Ice</span> event'. In water colder than 5 °C, men were faster than women in '<span class="hlt">Ice</span> Mile' and '1 km <span class="hlt">Ice</span> event'. Water temperature showed no correlation to swimming speed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008E%26PSL.265..246N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008E%26PSL.265..246N"><span>Conditions for a steady <span class="hlt">ice</span> sheet <span class="hlt">ice</span> shelf junction</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nowicki, S. M. J.; Wingham, D. J.</p> <p>2008-01-01</p> <p>This <span class="hlt">paper</span> investigates the conditions under which a marine <span class="hlt">ice</span> sheet may adopt a steady profile. The <span class="hlt">ice</span> is treated as a linear viscous fluid caused to flow from a rigid base to and over water, treated as a denser but inviscid fluid. The solutions in the region around the point of flotation, or 'transition' zone, are calculated numerically. In-flow and out-flow conditions appropriate to <span class="hlt">ice</span> sheet and <span class="hlt">ice</span> shelf flow are applied at the ends of the transition zone and the rigid base is specified; the flow and steady free surfaces are determined as part of the solutions. The basal stress upstream, and the basal deflection downstream, of the flotation point are examined to determine which of these steady solutions satisfy 'contact' conditions that would prevent (i) the steady downstream basal deflection contacting the downstream base, and (ii) the upstream <span class="hlt">ice</span> commencing to float in the event it was melted at the base. In the case that the upstream bed is allowed to slide, we find only one mass flux that satisfies the contact conditions. When no sliding is allowed at the bed, however, we find a range of mass fluxes satisfy the contact conditions. The effect of 'backpressure' on the solutions is investigated, and is found to have no affect on the qualitative behaviour of the junctions. To the extent that the numerical, linearly viscous treatment may be applied to the case of <span class="hlt">ice</span> flowing out over the ocean, we conclude that when sliding is present, Weertman's 'instability' hypothesis holds.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-200910220008HQ.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-200910220008HQ.html"><span><span class="hlt">Ice</span> Bridge Antarctic Sea <span class="hlt">Ice</span></span></a></p> <p><a target="_blank" href="https://images.nasa.gov/">NASA Image and Video Library</a></p> <p></p> <p>2009-10-21</p> <p>Sea <span class="hlt">ice</span> is seen out the window of NASA's DC-8 research aircraft as it flies 2,000 feet above the Bellingshausen Sea in West Antarctica on Wednesday, Oct., 21, 2009. This was the fourth science flight of NASA’s Operation <span class="hlt">Ice</span> Bridge airborne Earth science mission to study Antarctic <span class="hlt">ice</span> sheets, sea <span class="hlt">ice</span>, and <span class="hlt">ice</span> shelves. Photo Credit: (NASA/Jane Peterson)</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.ars.usda.gov/research/publications/publication/?seqNo115=271960','TEKTRAN'); return false;" href="http://www.ars.usda.gov/research/publications/publication/?seqNo115=271960"><span>Reclaiming fiberglass from faced <span class="hlt">insulation</span> batts</span></a></p> <p><a target="_blank" href="https://www.ars.usda.gov/research/publications/find-a-publication/">USDA-ARS?s Scientific Manuscript database</a></p> <p></p> <p></p> <p>In the manufacture of <span class="hlt">paper</span>-backed fiberglass <span class="hlt">insulation</span>, defects may occur that cause the manufacturer to reject approximately 45 metric tons (50 tons) of material on average each month. This material is currently hauled to a landfill, placing both a financial burden on the company and an environm...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20170007924','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20170007924"><span>An Initial Study of the Fundamentals of <span class="hlt">Ice</span> Crystal <span class="hlt">Icing</span> Physics in the NASA Propulsion Systems Laboratory</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Struk, Peter M.; Ratvasky, Thomas P.; Bencic, Timothy J.; Van Zante, Judith F.; King, Michael C.; Tsao, Jen-Ching; Bartkus, Tadas P.</p> <p>2017-01-01</p> <p>This <span class="hlt">paper</span> presents results from an initial study of the fundamental physics of <span class="hlt">ice</span>-crystal <span class="hlt">ice</span> accretion using the NASA Propulsion Systems Lab (PSL). <span class="hlt">Ice</span> accretion due to the ingestion of <span class="hlt">ice</span>-crystals is being attributed to numerous jet-engine power-loss events. The NASA PSL is an altitude jet-engine test facility which has recently added a capability to inject <span class="hlt">ice</span> particles into the flow. NASA is evaluating whether this facility, in addition to full-engine and motor-driven-rig tests, can be used for more fundamental <span class="hlt">ice</span>-accretion studies that simulate the different mixed-phase <span class="hlt">icing</span> conditions along the core flow passage of a turbo-fan engine compressor. The data from such fundamental accretion tests will be used to help develop and validate models of the accretion process. The present study utilized a NACA0012 airfoil. The mixed-phase conditions were generated by partially freezing the liquid-water droplets ejected from the spray bars. This <span class="hlt">paper</span> presents data regarding (1) the freeze out characteristics of the cloud, (2) changes in aerothermal conditions due to the presence of the cloud, and (3) the <span class="hlt">ice</span> accretion characteristics observed on the airfoil model. The primary variable in this test was the PSL plenum humidity which was systematically varied for two duct-exit-plane velocities (85 and 135 ms) as well as two particle size clouds (15 and 50 m MVDi). The observed clouds ranged from fully glaciated to fully liquid, where the liquid clouds were at least partially supercooled. The air total temperature decreased at the test section when the cloud was activated due to evaporation. The <span class="hlt">ice</span> accretions observed ranged from sharp arrow-like accretions, characteristic of <span class="hlt">ice</span>-crystal erosion, to cases with double-horn shapes, characteristic of supercooled water accretions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ACP....18.7843P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ACP....18.7843P"><span>Observing <span class="hlt">ice</span> particle growth along fall streaks in mixed-phase clouds using spectral polarimetric radar data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pfitzenmaier, Lukas; Unal, Christine M. H.; Dufournet, Yann; Russchenberg, Herman W. J.</p> <p>2018-06-01</p> <p>The growth of <span class="hlt">ice</span> crystals in presence of supercooled liquid droplets represents the most important process for precipitation formation in the mid-latitudes. However, such mixed-phase interaction processes remain relatively unknown, as capturing the complexity in cloud dynamics and microphysical variabilities turns to be a real observational challenge. Ground-based radar systems equipped with fully polarimetric and Doppler capabilities in high temporal and spatial resolutions such as the S-band transportable atmospheric radar (TARA) are best suited to observe mixed-phase growth processes. In this <span class="hlt">paper</span>, measurements are taken with the TARA radar during the ACCEPT campaign (analysis of the <span class="hlt">composition</span> of clouds with extended polarization techniques). Besides the common radar observables, the 3-D wind field is also retrieved due to TARA unique three beam configuration. The novelty of this <span class="hlt">paper</span> is to combine all these observations with a particle evolution detection algorithm based on a new fall streak retrieval technique in order to study <span class="hlt">ice</span> particle growth within complex precipitating mixed-phased cloud systems. In the presented cases, three different growth processes of <span class="hlt">ice</span> crystals, plate-like crystals, and needles are detected and related to the presence of supercooled liquid water. Moreover, TARA observed signatures are assessed with co-located measurements obtained from a cloud radar and radiosondes. This <span class="hlt">paper</span> shows that it is possible to observe <span class="hlt">ice</span> particle growth processes within complex systems taking advantage of adequate technology and state of the art retrieval algorithms. A significant improvement is made towards a conclusive interpretation of <span class="hlt">ice</span> particle growth processes and their contribution to rain production using fall streak rearranged radar data.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/AD1008292','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/AD1008292"><span>Strongly Correlated Topological <span class="hlt">Insulators</span></span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2016-02-03</p> <p>Strongly Correlated Topological <span class="hlt">Insulators</span> In the past year, the grant was used for work in the field of topological phases, with emphasis on finding...surface of topological <span class="hlt">insulators</span> . In the past 3 years, we have started a new direction, that of fractional topological <span class="hlt">insulators</span> . These are materials...Strongly Correlated Topological <span class="hlt">Insulators</span> Report Title In the past year, the grant was used for work in the field of topological phases, with emphasis</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23218317','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23218317"><span>Flame retardancy of polyaniline-deposited <span class="hlt">paper</span> <span class="hlt">composites</span> prepared via in situ polymerization.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wu, Xianna; Qian, Xueren; An, Xianhui</p> <p>2013-01-30</p> <p>Polyaniline-deposited <span class="hlt">paper</span> <span class="hlt">composites</span> doped with three inorganic acids were prepared via in situ polymerization, and their flame-retardant properties were investigated. Both the conductivity and flame retardancy of the <span class="hlt">composite</span> increased with the increase of the amount of the polyaniline deposited. The doping acid played a very key role in both the conductivity and flame retardancy of the <span class="hlt">composite</span>. The comprehensive properties of the <span class="hlt">composite</span> could be improved when codoped with an equimolar mixture of H(3)PO(4) and H(2)SO(4) or H(3)PO(4) and HCl. The decay of the flame retardancy of the <span class="hlt">composite</span> in atmosphere was due to the dedoping of the polyaniline deposited on cellulose fibers. Copyright © 2012 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018CliPa..14..619B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018CliPa..14..619B"><span>Simulation of the Greenland <span class="hlt">Ice</span> Sheet over two glacial-interglacial cycles: investigating a sub-<span class="hlt">ice</span>-shelf melt parameterization and relative sea level forcing in an <span class="hlt">ice-sheet-ice</span>-shelf model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bradley, Sarah L.; Reerink, Thomas J.; van de Wal, Roderik S. W.; Helsen, Michiel M.</p> <p>2018-05-01</p> <p>Observational evidence, including offshore moraines and sediment cores, confirm that at the Last Glacial Maximum (LGM) the Greenland <span class="hlt">ice</span> sheet (GrIS) expanded to a significantly larger spatial extent than seen at present, grounding into Baffin Bay and out onto the continental shelf break. Given this larger spatial extent and its close proximity to the neighbouring Laurentide <span class="hlt">Ice</span> Sheet (LIS) and Innuitian <span class="hlt">Ice</span> Sheet (IIS), it is likely these <span class="hlt">ice</span> sheets will have had a strong non-local influence on the spatial and temporal behaviour of the GrIS. Most previous paleo <span class="hlt">ice</span>-sheet modelling simulations recreated an <span class="hlt">ice</span> sheet that either did not extend out onto the continental shelf or utilized a simplified marine <span class="hlt">ice</span> parameterization which did not fully include the effect of <span class="hlt">ice</span> shelves or neglected the sensitivity of the GrIS to this non-local bedrock signal from the surrounding <span class="hlt">ice</span> sheets. In this <span class="hlt">paper</span>, we investigated the evolution of the GrIS over the two most recent glacial-interglacial cycles (240 ka BP to the present day) using the <span class="hlt">ice-sheet-ice</span>-shelf model IMAU-<span class="hlt">ICE</span>. We investigated the solid earth influence of the LIS and IIS via an offline relative sea level (RSL) forcing generated by a glacial isostatic adjustment (GIA) model. The RSL forcing governed the spatial and temporal pattern of sub-<span class="hlt">ice</span>-shelf melting via changes in the water depth below the <span class="hlt">ice</span> shelves. In the ensemble of simulations, at the glacial maximums, the GrIS coalesced with the IIS to the north and expanded to the continental shelf break to the southwest but remained too restricted to the northeast. In terms of the global mean sea level contribution, at the Last Interglacial (LIG) and LGM the <span class="hlt">ice</span> sheet added 1.46 and -2.59 m, respectively. This LGM contribution by the GrIS is considerably higher (˜ 1.26 m) than most previous studies whereas the contribution to the LIG highstand is lower (˜ 0.7 m). The spatial and temporal behaviour of the northern margin was highly variable in all simulations</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li class="active"><span>24</span></li> <li><a href="#" onclick='return showDiv("page_25");'>25</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_24 --> <div id="page_25" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li class="active"><span>25</span></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="481"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.1793H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.1793H"><span>Effect of Mantle Rheology on Viscous Heating induced during <span class="hlt">Ice</span> Sheet Cycles</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Huang, Pingping; Wu, Patrick; van der Wal, Wouter</p> <p>2017-04-01</p> <p>Hanyk et al. (2005) studied the viscous shear heating in the mantle induced by the surface loading and unloading of a parabolic-shaped Laurentide-size <span class="hlt">ice</span> sheet. They found that for linear rheology, viscous heating is mainly concentrated below the <span class="hlt">ice</span> sheet. The depth extent of the heating in the mantle is determined by the viscosity distribution. Also, the magnitude of viscous heating is significantly affected by the rate of <span class="hlt">ice</span> thickness change. However, only one <span class="hlt">ice</span> sheet has been considered in their work and the interactions between <span class="hlt">ice</span> sheets and ocean loading have been neglected. Furthermore, only linear rheology has been considered, although they suggested that non-Newtonian rheology may have a stronger effect. Here we follow Hanyk et al. (2005) and computed the viscous dissipation for viscoelastic models using the finite element methodology of Wu (2004) and van der Wal et al. (2010). However, the global <span class="hlt">ICE</span>6G model (Peltier et al. 2015) with realistic oceans is used here to provide the surface loading. In addition, viscous heating in non-linear rheology, <span class="hlt">composite</span> rheology, in addition to linear rheology with uniform or VM5a profile are computed and compared. Our results for linear rheology mainly confirm the findings of Hanyk et al. (2005). For both non-linear and <span class="hlt">composite</span> rheologies, viscous heating is also mainly distributed near and under the <span class="hlt">ice</span> sheets, but, more concentrated; depending on the horizontal dimension of the <span class="hlt">ice</span> sheet, it can extend into the lower mantle, but for some of the time, not as deep as that for linear rheology. For <span class="hlt">composite</span> rheology, the viscous heating is dominated by the effect of non-linear relation between the stress and the strain. The <span class="hlt">ice</span> history controls the time when the local maximum in viscous heating appears. However, the magnitude of the viscous heating is affected by mantle rheology as well as the <span class="hlt">ice</span> loading. Due to viscosity stratification, the shape of the region with high viscous heating in model VM5a is a</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/9775451','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/9775451"><span>A methodology to select a wire <span class="hlt">insulation</span> for use in habitable spacecraft.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Paulos, T; Apostolakis, G</p> <p>1998-08-01</p> <p>This <span class="hlt">paper</span> investigates electrical overheating events aboard a habitable spacecraft. The wire <span class="hlt">insulation</span> involved in these failures plays a major role in the entire event scenario from threat development to detection and damage assessment. Ideally, if models of wire overheating events in microgravity existed, the various wire <span class="hlt">insulations</span> under consideration could be quantitatively compared. However, these models do not exist. In this <span class="hlt">paper</span>, a methodology is developed that can be used to select a wire <span class="hlt">insulation</span> that is best suited for use in a habitable spacecraft. The results of this study show that, based upon the Analytic Hierarchy Process and simplifying assumptions, the criteria selected, and data used in the analysis, Tefzel is better than Teflon for use in a habitable spacecraft.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23508863','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23508863"><span>Glucose oxidase/cellulose-carbon nanotube <span class="hlt">composite</span> <span class="hlt">paper</span> as a biocompatible bioelectrode for biofuel cells.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Won, Keehoon; Kim, Young-Hoo; An, Seulji; Lee, Hye Jung; Park, Saerom; Choi, Yong-Keun; Kim, Ji Hyeon; Hwang, Hak-In; Kim, Hyung Joo; Kim, Hyungsup; Lee, Sang Hyun</p> <p>2013-11-01</p> <p>Biofuel cells are devices for generating electrical energy directly from chemical energy of renewable biomass using biocatalysts such as enzymes. Efficient electrical communication between redox enzymes and electrodes is essential for enzymatic biofuel cells. Carbon nanotubes (CNTs) have been recognized as ideal electrode materials because of their high electrical conductivity, large surface area, and inertness. Electrodes consisting entirely of CNTs, which are known as CNT <span class="hlt">paper</span>, have high surface areas but are typically weak in mechanical strength. In this study, cellulose (CL)-CNT <span class="hlt">composite</span> <span class="hlt">paper</span> was fabricated as electrodes for enzymatic biofuel cells. This <span class="hlt">composite</span> electrode was prepared by vacuum filtration of CNTs followed by reconstitution of cellulose dissolved in ionic liquid, 1-ethyl-3-methylimidazolium acetate. Glucose oxidase (GOx), which is a redox enzyme capable of oxidizing glucose as a renewable fuel using oxygen, was immobilized on the CL-CNT <span class="hlt">composite</span> <span class="hlt">paper</span>. Cyclic voltammograms revealed that the GOx/CL-CNT <span class="hlt">paper</span> electrode showed a pair of well-defined peaks, which agreed well with that of FAD/FADH2, the redox center of GOx. This result clearly shows that the direct electron transfer (DET) between the GOx and the <span class="hlt">composite</span> electrode was achieved. However, this DET was dependent on the type of CNTs. It was also found that the GOx immobilized on the <span class="hlt">composite</span> electrode retained catalytic activity for the oxidation of glucose.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27228106','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27228106"><span>Bioinspired Multifunctional <span class="hlt">Paper</span>-Based rGO <span class="hlt">Composites</span> for Solar-Driven Clean Water Generation.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Lou, Jinwei; Liu, Yang; Wang, Zhongyong; Zhao, Dengwu; Song, Chengyi; Wu, Jianbo; Dasgupta, Neil; Zhang, Wang; Zhang, Di; Tao, Peng; Shang, Wen; Deng, Tao</p> <p>2016-06-15</p> <p>Reusing polluted water through various decontamination techniques has appeared as one of the most practical approaches to address the global shortage of clean water. Rather than relying on single decontamination mechanism, herein we report the preparation and utilization of <span class="hlt">paper</span>-based <span class="hlt">composites</span> for multifunctional solar-driven clean water generation that is inspired by the multiple water purification approaches in biological systems. The reduced graphene oxide (rGO) sheets within such <span class="hlt">composites</span> can efficiently remove organic contaminants through physical adsorption mechanism. Under solar irradiation, the floating rGO <span class="hlt">composites</span> can instantly generate localized heating, which not only can directly generate clean water through distillation mechanism but also significantly enhance adsorption removal performance with the assistance of upward vapor flow. Such porous-structured <span class="hlt">paper</span>-based <span class="hlt">composites</span> allow for facile incorporation of photocatalysts to regenerate clean water out of contaminated water with combined adsorption, photodegradation, and interfacial heat-assisted distillation mechanisms. Within a homemade all-in-one water treatment device, the practical applicability of the <span class="hlt">composites</span> for multifunctional clean water generation has been demonstrated.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19760039698&hterms=1103&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3D%2526%25231103','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19760039698&hterms=1103&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3D%2526%25231103"><span>Beaufort Sea <span class="hlt">ice</span> zones as delineated by microwave imagery</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Campbell, W. J.; Gloersen, P.; Webster, W. J.; Wilheit, T. T.; Ramseier, R. O.</p> <p>1976-01-01</p> <p>Microwave and infrared data were obtained from a research aircraft over the Beaufort Sea <span class="hlt">ice</span> from the shoreline of Harrison Bay northward to a latitude of almost 81 deg N. The data acquired were compared with microwave data obtained on the surface at an approximate position of 75 deg N, 150 deg W. Over this north-south transect of the polar <span class="hlt">ice</span> canopy it was discovered that the sea <span class="hlt">ice</span> could be divided into five distinct zones. The shorefast sea <span class="hlt">ice</span> was found to consist uniformly of first-year sea <span class="hlt">ice</span>. The second zone was found to be a mixture of first-year sea <span class="hlt">ice</span>, medium size multiyear floes, and many recently refrozen leads, polynyas, and open water; considerable shearing activity was evident in this zone. The third zone was a mixture of first-year and multiyear sea <span class="hlt">ice</span> which had a uniform microwave signature. The fourth zone was found to be a mixture of first-year sea <span class="hlt">ice</span> and medium-to-large size multiyear floes which was similar in <span class="hlt">composition</span> to the second zone. The fifth zone was almost exclusively multiyear <span class="hlt">ice</span> extending to the North Pole.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/21174462','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/21174462"><span>Externally applied electric fields up to 1.6 × 10(5) V/m do not affect the homogeneous nucleation of <span class="hlt">ice</span> in supercooled water.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Stan, Claudiu A; Tang, Sindy K Y; Bishop, Kyle J M; Whitesides, George M</p> <p>2011-02-10</p> <p>The freezing of water can initiate at electrically conducting electrodes kept at a high electric potential or at charged electrically <span class="hlt">insulating</span> surfaces. The microscopic mechanisms of these phenomena are unknown, but they must involve interactions between water molecules and electric fields. This <span class="hlt">paper</span> investigates the effect of uniform electric fields on the homogeneous nucleation of <span class="hlt">ice</span> in supercooled water. Electric fields were applied across drops of water immersed in a perfluorinated liquid using a parallel-plate capacitor; the drops traveled in a microchannel and were supercooled until they froze due to the homogeneous nucleation of <span class="hlt">ice</span>. The distribution of freezing temperatures of drops depended on the rate of nucleation of <span class="hlt">ice</span>, and the sensitivity of measurements allowed detection of changes by a factor of 1.5 in the rate of nucleation. Sinusoidal alternation of the electric field at frequencies from 3 to 100 kHz prevented free ions present in water from screening the electric field in the bulk of drops. Uniform electric fields in water with amplitudes up to (1.6 ± 0.4) × 10(5) V/m neither enhanced nor suppressed the homogeneous nucleation of <span class="hlt">ice</span>. Estimations based on thermodynamic models suggest that fields in the range of 10(7)-10(8) V/m might cause an observable increase in the rate of nucleation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19980000580','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19980000580"><span>Scaling Methods for Simulating Aircraft In-Flight <span class="hlt">Icing</span> Encounters</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Anderson, David N.; Ruff, Gary A.</p> <p>1997-01-01</p> <p>This <span class="hlt">paper</span> discusses scaling methods which permit the use of subscale models in <span class="hlt">icing</span> wind tunnels to simulate natural flight in <span class="hlt">icing</span>. Natural <span class="hlt">icing</span> conditions exist when air temperatures are below freezing but cloud water droplets are super-cooled liquid. Aircraft flying through such clouds are susceptible to the accretion of <span class="hlt">ice</span> on the leading edges of unprotected components such as wings, tailplane and engine inlets. To establish the aerodynamic penalties of such <span class="hlt">ice</span> accretion and to determine what parts need to be protected from <span class="hlt">ice</span> accretion (by heating, for example), extensive flight and wind-tunnel testing is necessary for new aircraft and components. Testing in <span class="hlt">icing</span> tunnels is less expensive than flight testing, is safer, and permits better control of the test conditions. However, because of limitations on both model size and operating conditions in wind tunnels, it is often necessary to perform tests with either size or test conditions scaled. This <span class="hlt">paper</span> describes the theoretical background to the development of <span class="hlt">icing</span> scaling methods, discusses four methods, and presents results of tests to validate them.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017MS%26E..251a2070R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017MS%26E..251a2070R"><span>Impact of moisture content in AAC on its heat <span class="hlt">insulation</span> properties</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rubene, S.; Vilnitis, M.</p> <p>2017-10-01</p> <p>One of the most popular trends in construction industry is sustainable construction. Therefore, application of construction materials with high <span class="hlt">insulation</span> characteristics has significantly increased during the past decade. Requirements for application of construction materials with high <span class="hlt">insulation</span> parameters are required not only by means of energy saving and idea of sustainable construction but also by legislative requirements. Autoclaved aerated concrete (AAC) is a load bearing construction material, which has high heat <span class="hlt">insulation</span> parameters. However, if the AAC masonry construction has high moisture content the heat <span class="hlt">insulation</span> properties of the material decrease significantly. This fact lead to the necessity for the on-site control of moisture content in AAC in order to avoid inconsistency between the designed and actual thermal resistivity values of external delimiting constructions. Research of the impact of moisture content in AAC on its heat <span class="hlt">insulation</span> properties has been presented in this <span class="hlt">paper</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19990046048','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19990046048"><span>Software Development Processes Applied to Computational <span class="hlt">Icing</span> Simulation</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Levinson, Laurie H.; Potapezuk, Mark G.; Mellor, Pamela A.</p> <p>1999-01-01</p> <p>The development of computational <span class="hlt">icing</span> simulation methods is making the transition form the research to common place use in design and certification efforts. As such, standards of code management, design validation, and documentation must be adjusted to accommodate the increased expectations of the user community with respect to accuracy, reliability, capability, and usability. This <span class="hlt">paper</span> discusses these concepts with regard to current and future <span class="hlt">icing</span> simulation code development efforts as implemented by the <span class="hlt">Icing</span> Branch of the NASA Lewis Research Center in collaboration with the NASA Lewis Engineering Design and Analysis Division. With the application of the techniques outlined in this <span class="hlt">paper</span>, the LEWICE <span class="hlt">ice</span> accretion code has become a more stable and reliable software product.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018QSRv..189....1M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018QSRv..189....1M"><span>Reconciling records of <span class="hlt">ice</span> streaming and <span class="hlt">ice</span> margin retreat to produce a palaeogeographic reconstruction of the deglaciation of the Laurentide <span class="hlt">Ice</span> Sheet</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Margold, Martin; Stokes, Chris R.; Clark, Chris D.</p> <p>2018-06-01</p> <p>This <span class="hlt">paper</span> reconstructs the deglaciation of the Laurentide <span class="hlt">Ice</span> Sheet (LIS; including the Innuitian <span class="hlt">Ice</span> Sheet) from the Last Glacial Maximum (LGM), with a particular focus on the spatial and temporal variations in <span class="hlt">ice</span> streaming and the associated changes in flow patterns and <span class="hlt">ice</span> divides. We build on a recent inventory of Laurentide <span class="hlt">ice</span> streams and use an existing <span class="hlt">ice</span> margin chronology to produce the first detailed transient reconstruction of the <span class="hlt">ice</span> stream drainage network in the LIS, which we depict in a series of palaeogeographic maps. Results show that the drainage network at the LGM was similar to modern-day Antarctica. The majority of the <span class="hlt">ice</span> streams were marine terminating and topographically-controlled and many of these continued to function late into the deglaciation, until the <span class="hlt">ice</span> sheet lost its marine margin. <span class="hlt">Ice</span> streams with a terrestrial <span class="hlt">ice</span> margin in the west and south were more transient and <span class="hlt">ice</span> flow directions changed with the build-up, peak-phase and collapse of the Cordilleran-Laurentide <span class="hlt">ice</span> saddle. The south-eastern marine margin in Atlantic Canada started to retreat relatively early and some of the <span class="hlt">ice</span> streams in this region switched off at or shortly after the LGM. In contrast, the <span class="hlt">ice</span> streams draining towards the north-western and north-eastern marine margins in the Beaufort Sea and in Baffin Bay appear to have remained stable throughout most of the Late Glacial, and some of them continued to function until after the Younger Dryas (YD). The YD influenced the dynamics of the deglaciation, but there remains uncertainty about the response of the <span class="hlt">ice</span> sheet in several sectors. We tentatively ascribe the switching-on of some major <span class="hlt">ice</span> streams during this period (e.g. M'Clintock Channel <span class="hlt">Ice</span> Stream at the north-west margin), but for other large <span class="hlt">ice</span> streams whose timing partially overlaps with the YD, the drivers are less clear and <span class="hlt">ice</span>-dynamical processes, rather than effects of climate and surface mass balance are viewed as more likely drivers. Retreat</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20120002954','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20120002954"><span>Self-Healing Wire <span class="hlt">Insulation</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Parrish, Clyde F. (Inventor)</p> <p>2012-01-01</p> <p>A self-healing system for an <span class="hlt">insulation</span> material initiates a self-repair process by rupturing a plurality of microcapsules disposed on the <span class="hlt">insulation</span> material. When the plurality of microcapsules are ruptured, reactants within the plurality of microcapsules react to form a replacement polymer in a break of the <span class="hlt">insulation</span> material. This self-healing system has the ability to repair multiple breaks in a length of <span class="hlt">insulation</span> material without exhausting the repair properties of the material.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20120016401','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20120016401"><span>Near-Infrared Band Strengths of Molecules Diluted in N2 and H20 <span class="hlt">Ice</span> Mixtures Relevant to Interstellar and Planetary <span class="hlt">Ices</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Richey, C. R.; Richey, Christina R.</p> <p>2012-01-01</p> <p>In order to determine the column density of a component of an <span class="hlt">ice</span> from its infrared absorption features, the strengths of these features must be known. The peak positions, widths, profiles, and strengths of a certain <span class="hlt">ice</span> component's infrared absorption features are affected be the overall <span class="hlt">composition</span> of the <span class="hlt">ice</span>. Many satellites within the solar system have surfaces that are dominated by H2O or N2 and <span class="hlt">ices</span> in the interstellar medium (ISM) are primarily composed of H2O. The experiments presented here focus on the near-infrared absorption features of CO, CO2, CH4, and NH3 (nu=10,000-4,000/cm, lambda=1-2.5 microns) and the effects of diluting these molecules in N2 or H2O <span class="hlt">ice</span> (mixture ratio of 5:1). This is a continuation of previous results published by our research group.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20040085972','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20040085972"><span>Investigating the Use of Ultrasound for Evaluating Aging Wiring <span class="hlt">Insulation</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Madaras, Eric I.; Anastasi, Robert F.</p> <p>2001-01-01</p> <p>This <span class="hlt">paper</span> reviews our initial efforts to investigate the use of ultrasound to evaluate wire <span class="hlt">insulation</span>. Our initial model was a solid conductor with heat shrink tubing applied. In this model, various wave modes were identified. Subsequently, several aviation classes of wires (MIL-W- 81381, MIL-W-22759/34, and MIL-W-22759/87) were measured. The wires represented polyimide and ethylene-tetraflouroethylene <span class="hlt">insulations</span>, and combinations of polyimide and flouropolymer plastics. Wire gages of 12, 16, and 20 AWG sizes were measured. Finally, samples of these wires were subjected to high temperatures for short periods of time to cause the <span class="hlt">insulation</span> to degrade. Subsequent measurements indicated easily detectable changes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/863577','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/servlets/purl/863577"><span>Glassy <span class="hlt">composition</span> for hermetic seals</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Wilder, Jr., James A.</p> <p>1980-01-01</p> <p>The invention relates to a glassy <span class="hlt">composition</span> adaptable for sealing to aluminum-based alloys to form a hermetically-sealed <span class="hlt">insulator</span> body. The <span class="hlt">composition</span> may either be employed as a glass or, after devitrifying heat treatment, as a glass-ceramic.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018MS%26E..299a2037A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018MS%26E..299a2037A"><span>Strategies for characterizing <span class="hlt">compositions</span> of industrial pulp and <span class="hlt">paper</span> sludge</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Aslanzadeh, Solmaz; Kemal, Rahmat A.; Pribowo, Amadeus Y.</p> <p>2018-01-01</p> <p>The large quantities of waste sludge produced by the pulp and <span class="hlt">paper</span> industry present significant environmental challenges. In order to minimize the amounts of waste, the pulp sludge should be utilized for productive applications. In order to find feasible solutions, the sludge need to be characterized. In this study, the potential of using acid pretreatment and ashing method to determine the chemical <span class="hlt">compositions</span> of the sludge is investigated. This study shows that acid pretreatment could be used to dissolve and determine the <span class="hlt">composition</span> of CaCO3 in the pulp sludge. CaCO3 removal also facilitates the measurement of fiber and ash (clay) contents by using the ashing method. The optimum acid concentration used to completely dissolve CaCO3 was determined using a titration method. Using this method, the measurement of the chemical <span class="hlt">composition</span> of the sludge sample revealed that it consisted primarily of CaCO3 (55% w/w), clay (25%, w/w), and fibers (18%, w/w). Based on these chemical <span class="hlt">compositions</span>, potential utilization for the sludge could be determined.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20170011211','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20170011211"><span><span class="hlt">Ice</span> Crystal <span class="hlt">Icing</span> Research at NASA</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Flegel, Ashlie B.</p> <p>2017-01-01</p> <p><span class="hlt">Ice</span> crystals found at high altitude near convective clouds are known to cause jet engine power-loss events. These events occur due to <span class="hlt">ice</span> crystals entering a propulsion system's core flowpath and accreting <span class="hlt">ice</span> resulting in events such as uncommanded loss of thrust (rollback), engine stall, surge, and damage due to <span class="hlt">ice</span> shedding. As part of a community with a growing need to understand the underlying physics of <span class="hlt">ice</span> crystal <span class="hlt">icing</span>, NASA has been performing experimental efforts aimed at providing datasets that can be used to generate models to predict the <span class="hlt">ice</span> accretion inside current and future engine designs. Fundamental <span class="hlt">icing</span> physics studies on particle impacts, accretion on a single airfoil, and <span class="hlt">ice</span> accretions observed during a rollback event inside a full-scale engine in the Propulsion Systems Laboratory are summarized. Low fidelity code development using the results from the engine tests which identify key parameters for <span class="hlt">ice</span> accretion risk and the development of high fidelity codes are described. These activities have been conducted internal to NASA and through collaboration efforts with industry, academia, and other government agencies. The details of the research activities and progress made to date in addressing <span class="hlt">ice</span> crystal <span class="hlt">icing</span> research challenges are discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20170006539','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20170006539"><span><span class="hlt">Ice</span> Crystal <span class="hlt">Icing</span> Research at NASA</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Flegel, Ashlie B.</p> <p>2017-01-01</p> <p><span class="hlt">Ice</span> crystals found at high altitude near convective clouds are known to cause jet engine power-loss events. These events occur due to <span class="hlt">ice</span> crystals entering a propulsion systems core flowpath and accreting <span class="hlt">ice</span> resulting in events such as uncommanded loss of thrust (rollback), engine stall, surge, and damage due to <span class="hlt">ice</span> shedding. As part of a community with a growing need to understand the underlying physics of <span class="hlt">ice</span> crystal <span class="hlt">icing</span>, NASA has been performing experimental efforts aimed at providing datasets that can be used to generate models to predict the <span class="hlt">ice</span> accretion inside current and future engine designs. Fundamental <span class="hlt">icing</span> physics studies on particle impacts, accretion on a single airfoil, and <span class="hlt">ice</span> accretions observed during a rollback event inside a full-scale engine in the Propulsion Systems Laboratory are summarized. Low fidelity code development using the results from the engine tests which identify key parameters for <span class="hlt">ice</span> accretion risk and the development of high fidelity codes are described. These activities have been conducted internal to NASA and through collaboration efforts with industry, academia, and other government agencies. The details of the research activities and progress made to date in addressing <span class="hlt">ice</span> crystal <span class="hlt">icing</span> research challenges are discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018AAS...23114403L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018AAS...23114403L"><span>Topographic and Other Influences on Pluto's Volatile <span class="hlt">Ices</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lewis, Briley Lynn; Stansberry, John; Grundy, William M.; Schmitt, Bernard; Protopapa, Silvia; Trafton, Laurence M.; Holler, Bryan J.; McKinnon, William B.; Schenk, Paul M.; Stern, S. Alan; Young, Leslie; Weaver, Harold A.; Olkin, Catherine; Ennico, Kimberly; New Horizons Science Team, The New Horizons Composition Team</p> <p>2018-01-01</p> <p>Pluto’s surface is known to consist of various volatile <span class="hlt">ices</span>, mostly N2, CH4, and CO, which sublimate and condense on varying timescales, generally moving from points of high insolation to those of low insolation. The New Horizons Pluto encounter data provide multiple lenses through which to view Pluto’s detailed surface topography and <span class="hlt">composition</span> and to investigate the distribution of volatiles on its surface, including albedo and elevation maps from the imaging instruments and <span class="hlt">composition</span> maps from the LEISA spectral imager. The volatile surface <span class="hlt">ice</span> is expected to be generally isothermal, due to the fact that their vapor pressures are in equilibrium with the atmosphere. Although secular topographic transport mechanisms suggest that points at low elevation should slowly fill with volatile <span class="hlt">ices</span> (Trafton 2015 DPS abstract, Bertrand and Forget 2017), there are counter-examples of this across the surface, implying that energy discrepancies caused by insolation differences, albedo variations, local slopes, and other effects may take precedence at shorter timescales. Using data from the 2015 New Horizons flyby, we present our results of this investigation into the effects of variations in insolation, albedo, and topography on the presence of the different volatile <span class="hlt">ices</span> across the surface of Pluto.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017DPS....4921502L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017DPS....4921502L"><span>Topographic and Other Influences on Pluto's Volatile <span class="hlt">Ices</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lewis, Briley Lynn; Stansberry, John; Grundy, William M.; Schmitt, Bernard; Protopapa, Silvia; Trafton, Laurence M.; Holler, Bryan J.; McKinnon, William B.; Schenk, Paul M.; Stern, S. Alan; Young, Leslie; Weaver, Harold A.; Olkin, Catherine; Ennico, Kimberly; New Horizons Science Team</p> <p>2017-10-01</p> <p>Pluto’s surface is known to consist of various volatile <span class="hlt">ices</span>, mostly N2, CH4, and CO, which sublimate and condense on varying timescales, generally moving from points of high insolation to those of low insolation. The New Horizons Pluto encounter data provide multiple lenses through which to view Pluto’s detailed surface topography and <span class="hlt">composition</span> and to investigate the distribution of volatiles on its surface, including albedo and elevation maps from the imaging instruments and <span class="hlt">composition</span> maps from the LEISA spectral imager. The volatile surface <span class="hlt">ice</span> is expected to be generally isothermal, due to the fact that their vapor pressures are in equilibrium with the atmosphere. Although secular topographic transport mechanisms suggest that points at low elevation should slowly fill with volatile <span class="hlt">ices</span> (Trafton 2015 DPS abstract, Bertrand and Forget 2017), there are counter-examples of this across the surface, implying that energy discrepancies caused by insolation differences, albedo variations, local slopes, and other effects may take precedence at shorter timescales. Using data from the 2015 New Horizons flyby, we present our results of this investigation into the effects of variations in insolation, albedo, and topography on the presence of the different volatile <span class="hlt">ices</span> across the surface of Pluto.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015ApJ...801..118L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015ApJ...801..118L"><span>CO Diffusion into Amorphous H2O <span class="hlt">Ices</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lauck, Trish; Karssemeijer, Leendertjan; Shulenberger, Katherine; Rajappan, Mahesh; Öberg, Karin I.; Cuppen, Herma M.</p> <p>2015-03-01</p> <p>The mobility of atoms, molecules, and radicals in icy grain mantles regulates <span class="hlt">ice</span> restructuring, desorption, and chemistry in astrophysical environments. Interstellar <span class="hlt">ices</span> are dominated by H2O, and diffusion on external and internal (pore) surfaces of H2O-rich <span class="hlt">ices</span> is therefore a key process to constrain. This study aims to quantify the diffusion kinetics and barrier of the abundant <span class="hlt">ice</span> constituent CO into H2O-dominated <span class="hlt">ices</span> at low temperatures (15-23 K), by measuring the mixing rate of initially layered H2O(:CO2)/CO <span class="hlt">ices</span>. The mixed fraction of CO as a function of time is determined by monitoring the shape of the infrared CO stretching band. Mixing is observed at all investigated temperatures on minute timescales and can be ascribed to CO diffusion in H2O <span class="hlt">ice</span> pores. The diffusion coefficient and final mixed fraction depend on <span class="hlt">ice</span> temperature, porosity, thickness, and <span class="hlt">composition</span>. The experiments are analyzed by applying Fick’s diffusion equation under the assumption that mixing is due to CO diffusion into an immobile H2O <span class="hlt">ice</span>. The extracted energy barrier for CO diffusion into amorphous H2O <span class="hlt">ice</span> is ˜160 K. This is effectively a surface diffusion barrier. The derived barrier is low compared to current surface diffusion barriers in use in astrochemical models. Its adoption may significantly change the expected timescales for different <span class="hlt">ice</span> processes in interstellar environments.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li class="active"><span>25</span></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_25 --> <div class="footer-extlink text-muted" style="margin-bottom:1rem; text-align:center;">Some links on this page may take you to non-federal websites. 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