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Sample records for moti yung dongdai

  1. Bell Yung on Music of China.

    ERIC Educational Resources Information Center

    Campbell, Patricia Shehan

    1995-01-01

    Presents an interview with Bell Yung, a scholar of Chinese music and ethnomusicology. Maintains that world music (music from many nations and cultures) should be taught as early as possible in the schools and at home. Includes two lesson plans for teaching about Chinese music. (CFR)

  2. Assessing the Efficacy of MOTI-4 for Reducing the Use of Cannabis Among Youth in the Netherlands: A Randomized Controlled Trial.

    PubMed

    Dupont, Hans B; Candel, Math J J M; Kaplan, Charles D; van de Mheen, Dike; de Vries, Nanne K

    2016-06-01

    The Moti-4 intervention, in which motivational interviewing, self-monitoring, and strengthening behavioral control are used, was developed in the Netherlands in response to several rapid assessments of problematic use of cannabis among vulnerable adolescents. The main goal of the study reported in this article was to determine whether the Moti-4 intervention was able to reduce two outcome measures pertaining to the level of cannabis use; the amount of Euros spent a week on cannabis and the mean number of cannabis joints (cigarettes) smoked in a week. In a randomized controlled trial (RCT) with a 6-month follow-up, 27 trained Dutch prevention workers recruited 71 Moti-4 participants and 60 controls assigned to usual care. Participants were Dutch youth aged 14-24 years who had used cannabis during the preceding month. At baseline (T0), post-test (T1) and 6-month follow-up (T2), participants completed a questionnaire with 51 items. The 27 prevention workers also completed a checklist to assess the fidelity of delivering each item to each participant in the Moti-4 protocol. Multilevel and binary logistic regression was used to assess the impact of the prevention worker and 14 participant variables on the likelihood of drop-out. Mean scores for cannabis use outcome measures by Moti-4 participants and controls at baseline, T1 and T2 were compared using paired sample t-tests. Top-down multiple regression was used to assess relationships between Moti-4 and 13 other variables on the one hand and changes in weekly cannabis use at T1 and T2 on the other. The Moti-4 experimental condition had a significant and positive influence in reducing the level of expenditure on cannabis (p<0.05). There was no significant difference in outcome, neither for the 4 participating institutes nor for the professionals implementing the intervention. Baseline cannabis use was the strongest predictor (p<0.001) of weekly cannabis expenditure at posttest and 6-month follow-up. This effect was still

  3. Combining Persuasive Technology With Behavioral Theory to Support Weight Maintenance Through a Mobile Phone App: Protocol for the MotiMate App

    PubMed Central

    Hendrie, Gilly A; Freyne, Jill

    2016-01-01

    Background The prevalence of health-focused mobile phone apps available for download increases daily, with weight management apps being among the most proliferative. However, most lack theoretic grounding or evidence of efficacy. There is a significant body of literature which provides evidence for behaviors which are associated with successful weight loss maintenance. Behavioral theory also provides further insight regarding successful behavior change and maintenance. Objective We aimed to apply this knowledge to the development of the functionality of an app targeting weight loss maintenance. Methods We have subsequently undertaken the development of a persuasive and behavior targeting mobile app (MotiMate) to assist in maintenance of weight loss. MotiMate combines persuasive and behavior change theories in a practical targeted tool through its motivational messages, personalized feedback, and intelligent supportive tools to manage weight, food, exercise, mood and stress. Results The development and trial of MotiMate received funding support in May 2014. All 88 volunteers started the trial by December 2014 and were in the process of completing their final visits when this paper was submitted (May 2015). Data analysis is currently underway. Conclusions The paper has presented a scientifically informed mobile phone app to support weight loss maintenance. Further evaluation of its efficacy is in progress. Trial Registration ANZCTR 12614000474651; https://www.anzctr.org.au/Trial/Registration/TrialReview.aspx?id=366120 (Archived by WebCite at http://www.webcitation.org/6eJeQiKxi). PMID:26747725

  4. Prevalence of parasitic infection in captive wild animals in Bir Moti Bagh mini zoo (Deer Park), Patiala, Punjab

    PubMed Central

    Mir, A. Q.; Dua, K.; Singla, L. D.; Sharma, S.; Singh, M. P.

    2016-01-01

    Aim: The study was conducted to know the prevalence of gastrointestinal parasites of captive wild animals at Bir Moti Bagh Mini Zoo (Deer Park), Patiala, Punjab. Materials and Methods: A total of 31 fecal samples from eight species of captive animals including Civet cat (Viverra zibetha), Porcupine (Hystrix indica), Nilgai (Boselaphus tragocamelus), Spotted deer (Axis axis), Black buck (Antelope cervicapra), Sambar deer (Cervus unicolor), Hog deer (Axis porcinus), and Barking deer (Muntiacus muntjak) were screened using classical parasitological techniques including sedimentation and floatation technique. Results: Out of 31 fecal samples examined, 20 were positive for parasitic ova/oocysts of different species indicating an overall prevalence of 68.0%. The six different types of parasites observed in the study included strongyle (67%), Strongyloides spp. (14%), coccidia (38%), Trichuris spp. (19%), ascarid (10%), and Capillaria spp. (10%). Strongyles were the most common parasites observed (67%) followed by coccidia (38%). Mixed helminth and protozoan infection were observed in 48% of animals. No cestode or trematodes were detected during the study. Conclusion: The high prevalence of gastrointestinal parasites without overt clinical signs of disease or mortality as observed in this study is suggestive of subclinical infection. The findings will help in formulating the appropriate deworming protocol for parasitic control in these captive animals. PMID:27397973

  5. Investigating Remediation Reagents Injection and Rainfall Effect by using Self-Potential Method in a Soil and Groundwater Contamination Site located in Yung Kang, Taiwan

    NASA Astrophysics Data System (ADS)

    Chuang, Yung-Chieh; Chen, Chien-Chih; Wang, Tzu-Pin; Dong, Tien-Hsing; Chen, Yao-Tsung; Lin, Su-Tien; Ho, Ching-Jen

    2016-04-01

    In this study, we have proposed the use of time-lapse SP (self-potential) monitoring system to investigate a remediation reagents injection and rainfall effect in the soil and groundwater contamination site which was located in Yung Kang, Taiwan. We set up two mutually perpendicular survey lines to continuously record the SP data at a sampling rate of 25 Hz. One extended in N-S direction for a total length of 85 m with 17 potential electrodes and 1 common reference electrode. Another extended in E-W direction for a total length of 35 m with 7 potential electrodes and 1 common reference electrode. By averaging 1 day hourly SP median data, we calculated the time-lapse SPT (self-potential tomography) with a published code SP2DINV, and got the following results. First and foremost, from the daily SPTs, we found some artificial structures at a depth of circa 5 m. Then, by observing the positive and negative electric potential distributions in both N-S and E-W SPTs, we determined that the regional groundwater flow direction was in NE. Besides, making use of interpolation scheme, we filtered the rainfall effect out of the raw SP data. Then from the SPTs within the rainy days, we successfully demonstrated the SP response to the precipitation. And this phenomenon was interpreted as streaming potential which was caused from the enhancement of groundwater pressure. In addition, we correlated the charge density variation above 5m from SPTs with daily rainfall from August to September, to evaluate the Streaming Potential Coupling Coefficient. Last but not the least, by analyzing the SPTs variation from 13th to 18th October 2015 and from 23th to 25th November 2015, we compared the SPTs difference between two remediation reagents injection periods. And we also computed the passing time of the equal-potential lines between two fixed points, to evaluate the apparent hydraulic conductivities in this study area.

  6. Mo/Ti Diffusion Bonding for Making Thermoelectric Devices

    NASA Technical Reports Server (NTRS)

    Sakamoto, Jeffrey; Kisor, Adam; Caillat, Thierry; Lara, Liana; Ravi, Vilupanur; Firdosy, Samad; Fleuiral, Jean-Pierre

    2007-01-01

    An all-solid-state diffusion bonding process that exploits the eutectoid reaction between molybdenum and titanium has been developed for use in fabricating thermoelectric devices based on skutterudite compounds. In essence, the process is one of heating a flat piece of pure titanium in contact with a flat piece of pure molybdenum to a temperature of about 700 C while pushing the pieces together with a slight pressure [a few psi (of the order of 10 kPa)]. The process exploits the energy of mixing of these two metals to form a strong bond between them. These two metals were selected partly because the bonds formed between them are free of brittle intermetallic phases and are mechanically and chemically stable at high temperatures. The process is a solution of the problem of bonding hot-side metallic interconnections (denoted hot shoes in thermoelectric jargon) to titanium-terminated skutterudite n and p legs during the course of fabrication of a unicouple, which is the basic unit cell of a thermoelectric device (see figure). The hot-side operating temperature required for a skutterudite thermoelectric device is 700 C. This temperature precludes the use of brazing to attach the hot shoe; because brazing compounds melt at lower temperatures, the hot shoe would become detached during operation. Moreover, the decomposition temperature of one of the skutterudite compounds is 762 C; this places an upper limit on the temperature used in bonding the hot shoe. Molybdenum was selected as the interconnection metal because the eutectoid reaction between it and the titanium at the ends of the p and n legs has characteristics that are well suited for this application. In addition to being suitable for use in the present bonding process, molybdenum has high electrical and thermal conductivity and excellent thermal stability - characteristics that are desired for hot shoes of thermoelectric devices. The process takes advantage of the chemical potential energy of mixing between molybdenum and titanium. These metals have a strong affinity for each other. They are almost completely soluble in each other and remain in the solid state at temperatures above the eutectoid temperature of 695 C. As a result, bonds formed by interdiffusion of molybdenum and titanium are mechanically stable at and well above the original bonding temperature of about 700 C. Inasmuch as the bonds are made at approximately the operating temperature, thermomechanical stresses associated with differences in thermal expansion are minimized.

  7. 30nm half-pitch metal patterning using Moti CD shrink technique and double patterning

    NASA Astrophysics Data System (ADS)

    Versluijs, Janko; De Marneffe, J.-F.; Goossens, Danny; Op de Beeck, Maaike; Vandeweyer, Tom; Wiaux, Vincent; Struyf, Herbert; Maenhoudt, Mireille; Brouri, Mohand; Vertommen, Johan; Kim, Ji Soo; Zhu, Helen; Sadjadi, Reza

    2008-03-01

    Double patterning lithography appears a likely candidate to bridge the gap between water-based immersion lithography and EUV. A double patterning process is discussed for 30nm half-pitch interconnect structures, using 1.2 NA immersion lithography combined with the Motif TM CD shrink technique. An adjusted OPC calculation is required to model the proximity effects of the Motif shrink technique and subsequent metal hard mask (MHM) etch, on top of the lithography based proximity effects. The litho-etch-litho-etch approach is selected to pattern a TiN metal hard mask. This mask is then used to etch the low-k dielectric. The various process steps and challenges encountered are discussed, with the feasibility of this approach demonstrated by successfully transferring a 30nm half-pitch pattern into the MHM.

  8. Enabling Nanotechnology with Focused Ion Beams from Laser Cooled Atoms

    NASA Astrophysics Data System (ADS)

    Steele, A. V.; Knuffman, B.; Orloff, J.; Maazouz, M.; McClelland, J. J.

    2011-05-01

    The Magneto-Optical Trap Ion Source (MOTIS) being developed at NIST has the potential to enable numerous advances in nanoscale science. In a MOTIS, atoms are captured into a MOT, photoionized, and accelerated to an energy of a few hundred eV to a few tens of kV. A beam formed in this way can be brought to a tight focus, competitive with the commercial focused ion beam machines deployed widely today. Additionally, the unique characteristics of this source, coupled with the user's choice of ion from the long and growing list of laser-coolable atomic species suggest that the MOTIS has the potential to advance the state of the art in applications such as imaging, nanofabrication, secondary ion mass spectrometry, and others. I will present high-resolution images from our lithium and chromium MOTIS-based focused ion beams and discuss applications which we will pursue with these new tools.

  9. Education, Training and Contexts: Studies and Essays.

    ERIC Educational Resources Information Center

    Lauglo, Jon

    This volume provides an overview of some of the outstanding features of the work of the Norwegian sociologist and comparative educationist, Jon Lauglo. After an introduction, "'It Ain't Necessarily So!': Theories and Observations in Jon Lauglo's World of Education and Training" (Se-Yung Lim and Klaus Schaack), essays and studies are presented in…

  10. New Visions in Asian American Studies. Diversity, Community, Power.

    ERIC Educational Resources Information Center

    Ng, Franklin, Ed.; And Others

    This collection of essays from the eighth national conference of the Association for Asian American Studies is organized into four sections: history and women's studies; social science; literature; and Hawaiian studies. The following papers are included: (1) "History and Women Studies" (Yung); (2) "From Old to New Plantations: Labor's Growing…

  11. Measuring Civic Engagement Processes and Youth Civic Empowerment in the Classroom: The CIVVICS Observation Tool

    ERIC Educational Resources Information Center

    Stolte, Laurel Cadwallader; Isenbarger, Molly; Cohen, Alison Klebanoff

    2014-01-01

    Grounded in the context of the gap in civic participation, action-based civics curricula, and how classroom interactions may affect student development, we present the CIVVICS (Civic Interactions motiVating diVerse Individuals in Classroom Settings) observation tool. CIVVICS's four domains--Lesson Planning and Implementation, Classroom…

  12. Deuterium Fractionation on Mars and Evolutionary Implications for Water

    NASA Astrophysics Data System (ADS)

    Pathare, A. V.; Paige, D. A.

    1998-09-01

    Deuterium/Hydrogen (D/H) in the Martian atmosphere is enriched relative to terrestrial Standard Mean Ocean Water (SMOW) by a factor of 5.5. Yung et al. (1) photochemically modeled the escape efficiency (R) of D relative to H and obtained 0.32. Such high R implies that Mars experienced massive water loss early in its history, and cannot have significantly exchanged with juvenile water since. But Yung et al. (1) did not consider solar cycle related variations in both exospheric temperature and ionospheric chemistry, and when we accounted for changes in solar activity we obtained R = 0.17, which as we discussed last year is consistent with episodic juvenile water resupply. However, earlier this year Krasnopolsky et al. (2) obtained an even lower R = 0.02, based on spectroscopic measurements of deuterium which they could only reproduce by assuming that the ratio of (HD/H2) / (HDO/H2O) at the 80 km base of the exosphere was less than 10 based on Yung et al. (1). To explain this significant deviation, Krasnopolsky et al. (2) argued that partitioning of D into HD and HDO is controlled not kinetically but rather thermodynamically. However, as pointed out by Yung and Kass (3), this explanation would require an isotopic exchange rate coefficient over 10 orders of magnitude larger than that measured for this thermodynamic reaction in the laboratory. Therefore, we explore within the confines of the more likely applicable kinetic photochemical theory whether less extreme variations in exospheric and/or lower atmospheric reaction rate constants could result in a resolution to this dilemma. For example, variations in the vertical distribution of D could allow higher densities of HD at 80 km to be consistent with the new spectroscopic observations, or changes in the tropospheric conversion of HDO into HD could lessen the predicted amount of HD at 80 km. In addition, we examine the new climatological implications of R < 0.32 upon the evolution of Martian water, as massive

  13. A Record Book of Open Heart Surgical Cases between 1959 and 1982, Hand-Written by a Cardiac Surgeon.

    PubMed

    Kim, Won-Gon

    2016-08-01

    A book of brief records of open heart surgery underwent between 1959 and 1982 at Seoul National University Hospital was recently found. The book was hand-written by the late professor and cardiac surgeon Yung Kyoon Lee (1921-1994). This book contains valuable information about cardiac patients and surgery at the early stages of the establishment of open heart surgery in Korea, and at Seoul National University Hospital. This report is intended to analyze the content of the book. PMID:27525246

  14. A Record Book of Open Heart Surgical Cases between 1959 and 1982, Hand-Written by a Cardiac Surgeon

    PubMed Central

    Kim, Won-Gon

    2016-01-01

    A book of brief records of open heart surgery underwent between 1959 and 1982 at Seoul National University Hospital was recently found. The book was hand-written by the late professor and cardiac surgeon Yung Kyoon Lee (1921–1994). This book contains valuable information about cardiac patients and surgery at the early stages of the establishment of open heart surgery in Korea, and at Seoul National University Hospital. This report is intended to analyze the content of the book. PMID:27525246

  15. Photochemical modeling of Titan's atmosphere

    PubMed

    Toublanc, D; Parisot, J P; Brillet, J; Gautier, D; Raulin, F; McKay, C P

    1995-01-01

    We have developed a new photochemical model of Titan's atmosphere which includes all the important compounds and reactions in spherical geometry from the surface to 1240 km. Compared to the previous model of Yung et al. (1984, Astrophys. J. Suppl. 55, 465-506), the most significant recent change in the reactions used is the updated methane photodissociation scheme (Mordaunt et al. 1993, J. Chem. Phys. 98(3), 2054-2065). Moreover, the transfer of the solar radiation in the atmosphere and the photolysis rates have been calculated by using a Monte Carlo code. Finally, the eddy diffusion coefficient profile is adjusted in order to fit the mean vertical distribution of HCN retrieved from millimeter groundbased observations of Tanguy et al. (1990, Icarus, 85, 43-57) using new values for the boundary flux of atomic nitrogen (Strobel et al. 1992, Icarus 100, 512-526). We have run the model in both steady-state and diurnal modes, with 62 speices involved in 249 reactions. There is little difference between diurnal and steady-state results. Overall our results are in a closer agreement with the abundances inferred from the Voyager infrared measurements at the equator than the Yung et al. results. We find that the catalytic scheme for H recombination invoked by Yung et al. only slightly improves the model results and we conclude that this scheme is not essential to fit observations. PMID:11538950

  16. Alkali Metal Thermoelectric Conversion (AMTEC) for space nuclear power systems

    NASA Technical Reports Server (NTRS)

    Bankston, C. P.; Cole, T.; Khanna, S. K.; Thakoor, A. P.

    1985-01-01

    Performance parameters of the Alkali Metal Thermoelectric Converter (AMTEC) for a 100 kW electric power system have been calculated at four technological levels assuming a heat pipe-cooled nuclear reactor heat source. The most advanced level considered would operate between 1180 K converter temperature and 711 K radiator temperature at 16 percent efficiency, and would weigh 1850 kg with a radiator area of 43 sq m. In addition, electrode research studies for the AMTEC systems have been conducted utilizing an experimental test cell of Bankston et al. (1983) and Mo and several Mo-Ti electrodes. It was found that the Mo-Ti electrodes offered no improvement in lifetime characteristics over the pure Mo electrodes, however, oxygen treatment of a degraded Mo electrode restored its specific power output to 90 percent of its original specific power and maintained this level for 60 hr, thus offering a potential for lifetime stability.

  17. On the parameterization of 1D vertical mixing in planetary atmospheres: insights from 2D and 3D simulations

    NASA Astrophysics Data System (ADS)

    Zhang, Xi; Showman, Adam P.

    2015-11-01

    Most of the current atmospheric chemistry models for planets (e.g., Krasnopolsky & Parshev 1981; Yung & Demore 1982; Yung, Allen & Pinto 1984; Lavvas et al. 2008; Zhang et al. 2012) and exoplanets (e.g., Line, Liang & Yung 2010; Moses et al. 2011; Hu & Seager 2014) adopt a one-dimensional (1D) chemical-diffusion approach in the vertical coordinate. Although only a crude approximation, these 1D models have succeeded in explaining the global-averaged vertical profiles of many chemical species in observations. One of the important assumptions of these models is that all chemical species are transported via the same eddy diffusion profile--that is, the assumption is made that the eddy diffusivity is a fundamental property of the dynamics alone, and does not depend on the chemistry. Here we show that, as also noticed in the Earth community (e.g., Holton 1986), this “homogenous eddy diffusion” assumption generally breaks down. We first show analytically why the 1D eddy diffusivity must generally depend both on the horizontal eddy mixing and the chemical lifetime of the species. This implies that the long-lived species and short-lived chemical species will generally exhibit different eddy diffusion profiles, even in a given atmosphere with identical dynamics. Next, we present tracer-transport simulations in a 2D chemical-diffusion-advection model (Shia et al. 1989; Zhang, Shia & Yung 2013) and a 3D general circulation model (MITgcm, e.g., Liu & Showman 2013), for both rapid-rotating planets and tidally-locked exoplanets, to further explore the effect of chemical timescales on the eddy diffusivity. From the 2D and 3D simulation outputs, we derive effective 1D eddy diffusivity profiles for chemical tracers exhibiting a range of chemical timescales. We show that the derived eddy diffusivity can depend strongly on the horizontal eddy mixing and chemistry, although the dependences are more complex than the analytic model predicts. Overall, these results suggest that

  18. AGU membership applications

    NASA Astrophysics Data System (ADS)

    Applications for membership have been received from the following individuals. The letter after the name denotes the proposed primary section affiliation.Henry D. I. Abarbanel (O), Julia C. Allen (H), Gwendolyn L. Anson (GP), Andrew Bakun (O), C. A. Bengtson (T), Patricia A. Berge (S), Peter R. Betzer (O), Pierre Boivin (V), Michael V. Capobianco (P), Martin C. Chapman (S), Chu-Yung Chen (V), Timothy J. Clarke (S), Steven C. Constable (GP), Michele Dermer (H), G. M. Dow (T), Carl E. Draper (G), Dean A. Dunn (O), I. B. Everingham (S).

  19. High-Temperature Compressive Properties of TiC-Added Mo-Si-B Alloys

    NASA Astrophysics Data System (ADS)

    Yoshimi, Kyosuke; Nakamura, Junya; Kanekon, Daiki; Yamamoto, Shiho; Maruyama, Kouichi; Katsui, Hirokazu; Goto, Takashi

    2014-09-01

    High-temperature compressive properties of two TiC-added Mo-Si-B alloys with nominal compositions of Mo-5Si-10B-7.5TiC (70Mo alloy) and Mo-6.7Si-13.3B-7.5TiC (65Mo alloy) (at.%) were investigated. The alloys were composed of four constituent phases: Mo solid solution (Moss), Mo5SiB2, (Mo,Ti)C, and (Mo,Ti)2C. The primary phases of the 70Mo and 65Mo alloys were Moss and T2, respectively. The compressive deformability of the 65Mo alloy was significantly limited even at 1600°C because of the elongated, coarse primary T2 phase, whereas the 70Mo alloy had good compressive deformability and a high strength in the test-temperature range of 1000-1600°C; the peak stresses were 1800 MPa at 1000°C, 1230 MPa at 1200°C, and 350 MPa at 1600°C. At and above 1200°C, the peak stress values were more than double those of Mo-6.7Si-7.9B, Ti-Zr-Mo, and Mo-Hf-C alloys. The plastic strain in the 70Mo alloy at temperatures lower than the ductile-brittle transition temperature of T2 was generated by plastic deformation of not only Moss but also of (Mo,Ti)C and (Mo,Ti)2C. This work indicates that (Mo,Ti)C and (Mo,Ti)2C play an important role in determining the high-temperature strength and deformation properties of TiC-added Mo-Si-B alloys.

  20. Avian artificial insemination and semen preservation

    USGS Publications Warehouse

    Gee, G.F.

    1983-01-01

    Summary: Artificial insemination is a practical propagation tool that has been successful with a variety of birds. Cooperative, massage, and electroejaculation and modifications of these three basic methods of semen collection are described for a variety of birds. Semen color and consistency and sperm number, moti!ity, and morphology, as discussed, are useful indicators of semen quality, but the most reliable test of semen quality is the production of fertile eggs. Successful cryogenic preservation of avian semen with DMSO or glycerol as the cryoprotectant has been possible. Although the methods for preservation require special equipment, use of frozen semen requires only simple insemination supplies

  1. Authigenesis of vivianite as influenced by methane-induced sulfidization in cold-seep sediments off southwestern Taiwan

    NASA Astrophysics Data System (ADS)

    Hsu, Ta-Wei; Jiang, Wei-Teh; Wang, Yunshuen

    2014-08-01

    Authigenesis of iron-rich phosphate nodules occurs in iron-rich cold-seep sediments (MD052911 core) at Yung-An Ridge offshore southwestern Taiwan. Raman, FTIR, and quantitative X-ray energy-dispersive spectroscopic analyses indicate that the phosphate mineral is vivianite (or barićite) and shows Fe/Mg molar ratios spanning from ca. 0.6 to 4.0 and a general down core trend of increasing Fe/Mg ratios. The formation of vivianite is limited to a depth interval of 13-17 mbsf (meters below seafloor) and is most prominent at ∼16 mbsf in association with high dissolved iron concentrations and depleted dissolved sulfide below a peak sulfidization zone (enriched in mackinawite and greigite). Alternate growths of vivianite and iron monosulfides and compositional zoning with Mg enriched towards the peripheries of individual nodules occur in the transition from the zone of vivianite mineralization to the sulfidization zone. The crystallization of vivianite below the sulfidization front could have been favored by scavenging of downward diffusive dissolved sulfide from pore waters in the sulfidization zone. Alternate growths and overlapping of the zones of iron monosulfides and vivianite can be attributed to fluctuations of the sulfidization front and methane flux. The discovery of vivianite in the Yung-An Ridge sediments implies that authigenic vivianite can be an important sink for phosphorus burial in cold-seep sediments that have high reactive-iron contents and high sedimentation rates.

  2. Oxygen isotope fractionation in stratospheric CO2

    NASA Technical Reports Server (NTRS)

    Thiemens, M. H.; Jackson, T.; Mauersberger, K.; Schueler, B.; Morton, J.

    1991-01-01

    A new cryogenic collection system has been flown on board a balloon gondola to obtain separate samples of ozone and carbon dioxide without entrapping major atmospheric gases. Precision laboratory isotopic analysis of CO2 samples collected between 26 and 35.5 km show a mass-independent enrichment in both O-17 and O-18 of about 11 per mil above tropospheric values. Ozone enrichment in its heavy isotopes was 9 to 16 percent in O3-50 and 8 to 11 percent in O3-49, respectively (Schueler et al., 1990). A mechanism to explain the isotope enrichment in CO2 has been recently proposed by Yung et al. (1991). The model is based on the isotope exchange between CO2 and O3 via O(1D), resulting in a transfer of the ozone isotope enrichment to carbon dioxide. Predicted enrichment and measured values agree well.

  3. Recovery of Weak Factor Loadings When Adding the Mean Structure in Confirmatory Factor Analysis: A Simulation Study

    PubMed Central

    Ximénez, Carmen

    2016-01-01

    This article extends previous research on the recovery of weak factor loadings in confirmatory factor analysis (CFA) by exploring the effects of adding the mean structure. This issue has not been examined in previous research. This study is based on the framework of Yung and Bentler (1999) and aims to examine the conditions that affect the recovery of weak factor loadings when the model includes the mean structure, compared to analyzing the covariance structure alone. A simulation study was conducted in which several constraints were defined for one-, two-, and three-factor models. Results show that adding the mean structure improves the recovery of weak factor loadings and reduces the asymptotic variances for the factor loadings, particularly for the models with a smaller number of factors and a small sample size. Therefore, under certain circumstances, modeling the means should be seriously considered for covariance models containing weak factor loadings. PMID:26779071

  4. The critical surface fugacity of self-avoiding walks on a rotated honeycomb lattice

    NASA Astrophysics Data System (ADS)

    Beaton, Nicholas R.

    2014-02-01

    In a recent paper by Beaton et al, it was proved that a model of self-avoiding walks on the honeycomb lattice, interacting with an impenetrable surface, undergoes an adsorption phase transition when the surface fugacity is 1+\\sqrt{2}. Their proof used a generalization of an identity obtained by Duminil-Copin and Smirnov, and confirmed a conjecture of Batchelor and Yung. We consider a similar model of self-avoiding walk adsorption on the honeycomb lattice, but with the lattice rotated by π/2. For this model there also exists a conjecture for the critical surface fugacity, made in 1998 by Batchelor, Bennett-Wood and Owczarek. Using similar methods to Beaton et al, we prove that this is indeed the critical fugacity.

  5. Comparative genomics of Cluster O mycobacteriophages.

    PubMed

    Cresawn, Steven G; Pope, Welkin H; Jacobs-Sera, Deborah; Bowman, Charles A; Russell, Daniel A; Dedrick, Rebekah M; Adair, Tamarah; Anders, Kirk R; Ball, Sarah; Bollivar, David; Breitenberger, Caroline; Burnett, Sandra H; Butela, Kristen; Byrnes, Deanna; Carzo, Sarah; Cornely, Kathleen A; Cross, Trevor; Daniels, Richard L; Dunbar, David; Findley, Ann M; Gissendanner, Chris R; Golebiewska, Urszula P; Hartzog, Grant A; Hatherill, J Robert; Hughes, Lee E; Jalloh, Chernoh S; De Los Santos, Carla; Ekanem, Kevin; Khambule, Sphindile L; King, Rodney A; King-Smith, Christina; Klyczek, Karen; Krukonis, Greg P; Laing, Christian; Lapin, Jonathan S; Lopez, A Javier; Mkhwanazi, Sipho M; Molloy, Sally D; Moran, Deborah; Munsamy, Vanisha; Pacey, Eddie; Plymale, Ruth; Poxleitner, Marianne; Reyna, Nathan; Schildbach, Joel F; Stukey, Joseph; Taylor, Sarah E; Ware, Vassie C; Wellmann, Amanda L; Westholm, Daniel; Wodarski, Donna; Zajko, Michelle; Zikalala, Thabiso S; Hendrix, Roger W; Hatfull, Graham F

    2015-01-01

    Mycobacteriophages--viruses of mycobacterial hosts--are genetically diverse but morphologically are all classified in the Caudovirales with double-stranded DNA and tails. We describe here a group of five closely related mycobacteriophages--Corndog, Catdawg, Dylan, Firecracker, and YungJamal--designated as Cluster O with long flexible tails but with unusual prolate capsids. Proteomic analysis of phage Corndog particles, Catdawg particles, and Corndog-infected cells confirms expression of half of the predicted gene products and indicates a non-canonical mechanism for translation of the Corndog tape measure protein. Bioinformatic analysis identifies 8-9 strongly predicted SigA promoters and all five Cluster O genomes contain more than 30 copies of a 17 bp repeat sequence with dyad symmetry located throughout the genomes. Comparison of the Cluster O phages provides insights into phage genome evolution including the processes of gene flux by horizontal genetic exchange. PMID:25742016

  6. Comparative Genomics of Cluster O Mycobacteriophages

    PubMed Central

    Cresawn, Steven G.; Pope, Welkin H.; Jacobs-Sera, Deborah; Bowman, Charles A.; Russell, Daniel A.; Dedrick, Rebekah M.; Adair, Tamarah; Anders, Kirk R.; Ball, Sarah; Bollivar, David; Breitenberger, Caroline; Burnett, Sandra H.; Butela, Kristen; Byrnes, Deanna; Carzo, Sarah; Cornely, Kathleen A.; Cross, Trevor; Daniels, Richard L.; Dunbar, David; Findley, Ann M.; Gissendanner, Chris R.; Golebiewska, Urszula P.; Hartzog, Grant A.; Hatherill, J. Robert; Hughes, Lee E.; Jalloh, Chernoh S.; De Los Santos, Carla; Ekanem, Kevin; Khambule, Sphindile L.; King, Rodney A.; King-Smith, Christina; Klyczek, Karen; Krukonis, Greg P.; Laing, Christian; Lapin, Jonathan S.; Lopez, A. Javier; Mkhwanazi, Sipho M.; Molloy, Sally D.; Moran, Deborah; Munsamy, Vanisha; Pacey, Eddie; Plymale, Ruth; Poxleitner, Marianne; Reyna, Nathan; Schildbach, Joel F.; Stukey, Joseph; Taylor, Sarah E.; Ware, Vassie C.; Wellmann, Amanda L.; Westholm, Daniel; Wodarski, Donna; Zajko, Michelle; Zikalala, Thabiso S.; Hendrix, Roger W.; Hatfull, Graham F.

    2015-01-01

    Mycobacteriophages – viruses of mycobacterial hosts – are genetically diverse but morphologically are all classified in the Caudovirales with double-stranded DNA and tails. We describe here a group of five closely related mycobacteriophages – Corndog, Catdawg, Dylan, Firecracker, and YungJamal – designated as Cluster O with long flexible tails but with unusual prolate capsids. Proteomic analysis of phage Corndog particles, Catdawg particles, and Corndog-infected cells confirms expression of half of the predicted gene products and indicates a non-canonical mechanism for translation of the Corndog tape measure protein. Bioinformatic analysis identifies 8–9 strongly predicted SigA promoters and all five Cluster O genomes contain more than 30 copies of a 17 bp repeat sequence with dyad symmetry located throughout the genomes. Comparison of the Cluster O phages provides insights into phage genome evolution including the processes of gene flux by horizontal genetic exchange. PMID:25742016

  7. Laboratory studies on the reactions between chlorine, sulfur dioxide, and oxygen - Implications for the Venus stratosphere

    NASA Technical Reports Server (NTRS)

    Demore, W. B.; Leu, M.-T.; Smith, R. H.; Yung, Y. L.

    1985-01-01

    Fourier transform IR spectrophotometry is used to monitor the reactants and products in a Venus stratosphere simulation study involving the photolysis of mixtures of Cl2 and SO2, with and without O2 present in an atmosphere of N2. When several speculative reactions inferred from these experiments are incorporated by the Yung and DeMore (1982) model of Venus stratospheric chemistry, it emerges that SO2Cl2 is a key reservoir species for chlorine, and that the reaction between Cl and SO2 furnishes an important cycle for the destruction of O2 and the conversion of SO2 to H2SO4, thereby providing a possible solution to the photochemistry of the Venus stratosphere.

  8. Heavy hydrogen isotopes penetration through austenitic and martensitic steels

    NASA Astrophysics Data System (ADS)

    Dolinski, Yu.; Lyasota, I.; Shestakov, A.; Repritsev, Yu.; Zouev, Yu.

    2000-12-01

    Experimental results are presented of deuterium and tritium permeability through samples of nickel, austenitic steel (16Cr-15Ni-3Mo-Ti), and martensitic steel DIN 1.4914 (MANET) exposed to a gaseous phase. Experiments were carried out at the RFNC-VNHTF installation, which has the capability of measuring the permeability of hydrogen isotopes by mass spectrometry over a temperature range of 293-1000 K, hydrogen isotope pressure ranges of 50-1000 Pa. Sample disks (30 and 40 mm diam.) can be assembled in the test chamber by electron-beam welding or mounted (30-mm diam. disks) on gaskets. Diffusion and permeability dependencies on temperature and pressure are determined and corresponding activation energies are presented.

  9. List mode reconstruction for PET with motion compensation: A simulation study

    SciTech Connect

    Qi, Jinyi; Huesman, Ronald H.

    2002-07-03

    Motion artifacts can be a significant factor that limits the image quality in high-resolution PET. Surveillance systems have been developed to track the movements of the subject during a scan. Development of reconstruction algorithms that are able to compensate for the subject motion will increase the potential of PET. In this paper we present a list mode likelihood reconstruction algorithm with the ability of motion compensation. The subject moti is explicitly modeled in the likelihood function. The detections of each detector pair are modeled as a Poisson process with time vary ingrate function. The proposed method has several advantages over the existing methods. It uses all detected events and does not introduce any interpolation error. Computer simulations show that the proposed method can compensate simulated subject movements and that the reconstructed images have no visible motion artifacts.

  10. [Polyetheretherketone (PEEK). Part II: application in clinical practice].

    PubMed

    Pokorný, D; Fulín, P; Slouf, M; Jahoda, D; Landor, I; Sosna, A

    2010-01-01

    Polyetheretherketone (PEEK) is one of the up-to-date organic polymer thermoplastics with applications in orthopaedics and trauma medicine. This study presents a detailed analysis of its tests and applications in clinical medicine. A wide range of PEEK modifications and composites are commercially available, e.g., PEEK-Classix, PEEK-Optima, Endolign and Motis. They differ in their physical properties, which makes them suitable for different applications. Other forms, so-called PEEK bioactive composites, contain beta-tricalcium phosphate and hydroxyapatite. Research in this field is also concerned with the surface finish of this polymer thermoplastic and involves macroporous titanium and hydroxyapatite layers, or treatment with laser for an exactly defined surface structure. The clinical applications of PEEK and its composites include, in addition to components for spinal surgery, osteosynthesis plates, screws, intramedullary nails or external fixators, which are implants still at the stage of prototypes. In this review, attention is paid to the use of PEEK thermoplastics for joint replacement. Mid-term studies involving hundreds of patients have shown that, for instance, the VerSys Epoch Fullcoat Hip System (Zimmer) has a markedly lower stress-shielding effect. Carbon fibre-reinforced (CFR-PEEK) composites are used to make articulating components for total hip replacement. Their convenient properties allow for production of much thinner liners and an enlargement of the femoral head diameter, thus reducing the wear of joint implants. CFR-PEEK composites are particularly effective for hip resurfacing in which the Mitch PCR (Stryker) acetabular component has been used with good results. The MOTIS polymer acetabular cup (Invibio Ltd.) is another example. Further PEEK applications include the construction of finger-joint prostheses (Mathys AG), suture anchors (Stryker) and various kinds of augmentations (Medin). Based on the information obtained, the authors suggest

  11. Putative channel components for the fast-rotating sodium-driven flagellar motor of a marine bacterium.

    PubMed Central

    Asai, Y; Kojima, S; Kato, H; Nishioka, N; Kawagishi, I; Homma, M

    1997-01-01

    The polar flagellum of Vibrio alginolyticus rotates remarkably fast (up to 1,700 revolutions per second) by using a motor driven by sodium ions. Two genes, motX and motY, for the sodium-driven flagellar motor have been identified in marine bacteria, Vibrio parahaemolyticus and V. alginolyticus. They have no similarity to the genes for proton-driven motors, motA and motB, whose products constitute a proton channel. MotX was proposed to be a component of a sodium channel. Here we identified additional sodium motor genes, pomA and pomB, in V. alginolyticus. Unexpectedly, PomA and PomB have similarities to MotA and MotB, respectively, especially in the predicted transmembrane regions. These results suggest that PomA and PomB may be sodium-conducting channel components of the sodium-driven motor and that the motor part consists of the products of at least four genes, pomA, pomB, motX, and motY. Furthermore, swimming speed was controlled by the expression level of the pomA gene, suggesting that newly synthesized PomA proteins, which are components of a force-generating unit, were successively integrated into the defective motor complexes. These findings imply that Na+-driven flagellar motors may have similar structure and function as proton-driven motors, but with some interesting differences as well, and it is possible to compare and study the coupling mechanisms of the sodium and proton ion flux for the force generation. PMID:9260952

  12. Cometary Water on Mars

    NASA Astrophysics Data System (ADS)

    Grinspoon, D.

    1999-09-01

    The enhanced deuterium-to-hydrogen (D/H) ratio in the Martian atmosphere (5.25 x terrestrial;1,2) has been interpreted as the signature of water loss based on the assumption that primordial Martian water had Earth-like D/H. Yung et al.(3)considered that atmospheric water may be in steady-state with a crustal source, but rejected this possibility because of the non-terrestrial D/H signature inferred for the source hydrogen. Watson et al (4) measured D/H in SNC meteorites and found evidence for two reservoirs: a fractionated reservoir with values clustered around the measured atmospheric value and an unfractionated reservoir with values clustered at roughly twice the terrestrial D/H value. They interpreted the latter group to represent mixing between primordial hydrogen with Earth-like D/H and the more enhanced atmospheric value. However, this unfractionated reservoir has D/H which is very similar to that measured in three Oort cloud comets (5,6,7). If we assume that this is the D/H value of crustal water on Mars and calculate the predicted D/H value of atmospheric H in steady-state with such a source, we find that the predicted value corresponds closely with both the measured atmospheric value and the fractionated reservoir measured in the SNCs. Thus a cometary source for crustal water on Mars can explain all of the measured values. If Mars formed relatively dry due to its small size, then a late accretional flux of cometary material could have provided 300 meters of water, while leaving Earth's D/H relatively unperturbed. 1) Owen et al.(1988). Science, 240, 1767-1770. 2) Bjoraker et al. (1989). Bull. Am. Astron. Soc., 21, 991. 3) Yung et al. (1988). Icarus, 76, 146-159. 4) Watson et al.(1994). Science, 265, 86-90. 5) Balsinger et al.. (1995) J. Geophys. Res. 100, 5827-5834. 6) Bockelee-Morvan, D. et al. (1999) Icarus, in the press. 7) Meier et al. (1998). Science, 279, 842-844.

  13. Technical Knowledge, Cultural Practices and Social Boundaries: Wan-Nan Scholars and the Recasting of Jesuit Astronomy, 1600-1800

    NASA Astrophysics Data System (ADS)

    Chu, Ping-Yi.

    Taking four Wan-nan Confucian scholars--Yang Kuang -hsien, Mei Wen-ting, Chiang Yung and Tai Chen--as examples, this dissertation studies how an immigrant Jesuit scientific community built and defended itself in a specialized institutional niche located at the Ch'ing court and how a defeated Chinese scientific tradition successfully survived by occupying a broader cultural space, with the Manchu emperor in between. Special attention is paid to how these four Confucian scholars constructed social boundaries between the Chinese and the Westerners in their astronomical discourses and how they domesticated Western astronomy in order to fit the Chinese cultural conditions situated in the power structure built by the Manchus. This inquiry begins with a brief introduction of Wan-nan and the Wan-nan school. I then discuss how the Jesuits legitimated their knowledge during the Ming -Ch'ing transition, and how Jesuit astronomy was situated within the power nexus between the Confucian literati and the emperors. The next chapter focuses on Yang Kuang-hsien and his challenges to the Jesuits. I examine his strategies and the power structure in which Yang carried out his challenge to the Jesuits. The fourth and fifth chapters investigate how Mei Wen-ting restructured the relationship between Confucianism and astronomy. The former chapter focuses on Mei's social networking and his ambivalence towards the Ming and Ch'ing dynasties, on the one hand, and towards Chinese and Western learning on the other. The latter chapter deals with how Mei Wen-ting recast Chinese astronomical tradition and Confucianism. In the sixth chapter, I will compare the fame of Chiang Yung and Tai Chen in order to demonstrate how astronomy was practiced in evidential studies after Mei Wen-ting, and how evidential studies itself conveyed an ideological construction of the other. Through integrating Western astronomy with indigenous tradition while exorcising the otherness contained within the cultural package

  14. Two Dimensional Fluid Flow Models Offshore Southwestern Taiwan

    NASA Astrophysics Data System (ADS)

    Chen, L. W.; Wu, S. K.; Chi, W. C.; Liu, C. S.; Shyu, C. T.; Wang, Y. S.

    2012-04-01

    Fluid migration rates are important parameters for understanding the structural characteristics and evolution of the crustal tectonics and hydrocarbon exploration. However, they are difficult to measure on the seafloor. Dense distribution of bottom-simulating reflectors (BSRs) as the index of fluid existence to shed light on our study of the fluid migration. In this study, We acquired 2D fluid flow patterns in two potential gas hydrate prospect sites offshore southwestern Taiwan, and respectively modeled across Yung-An and Formosa ridge in N-S and E-W direction southwestern Taiwan. Temperature field in the shallow crust is used as a tracer to examine the fluid flow patterns. We use thermal information directly measured by thermal probes and topography data to develop the theoretical 2D temperature field using a thermal conduction model, which was derived from a finite element method. The discrepancy between the observed temperature data and the conductive model is attributed to advection heat transfer due to fluid migration. For Yung-An Ridge, we found the BSR-based temperatures are about 2oC higher than the conduction model in the following zones: (1) near a fault zone, (2) on the eastern flank where there are strong seismic reflectors in a pseudo 3D seismic dataset, (3) a seismic chimney zone. We interpret that there is possible active dewatering inside the accretionary prism to allow fluid to migrate upward here. For Formosa Ridge in the passive margin, the BSR-based temperatures are about 2oC colder than the theoretical model, especially on the flanks. We interpret that cold seawater is moving into the ridge from the flanks, cooling the ridge, and then some of the fluid is expelled at the ridge top. The shallow temperature fields are strongly affected by 2D or even 3D bathymetry effects. But we can still gain much information regarding fluid flow patterns through modeling. In the near future, we will extend such study into 3D. Keywords: fluid migration

  15. Titan's Surface Properties: Correlations Among DISR, RADAR And VIMS Observations

    NASA Astrophysics Data System (ADS)

    Soderblom, Laurence A.; DISR, Cassini-Huygens; RADAR; VIMS Teams

    2006-09-01

    Titan's vast equatorial fields of longitudinal dunes seen in radar images (Lorenz et al. 2006) correlate with one of two dark surface units discriminated as “ brown” and "blue” in color composites (RGB as 2.0, 1.6, 1.3 μm) of near-IR spectral cubes. Earth-based spectroscopy (Griffith et al. 2003) shows a surface consistent with dirty H2O ice; VIMS data show more evidence of H2O ice in darker than brighter units (McCord et al. 2006). Our work shows that relative to the VIMS dark blue unit, the albedo of the dark brown unit is lower at 1.3 μm, higher at 2.0 μm, shows less evidence of water ice, and correlates with the radar-dark dunes. This suggests that the dunes are dryer, higher in hydrocarbon or nitrile composition. VIMS bright units show even less evidence of H2O, inferred to consist of very fine tholin dust. If the rate of deposition of hydrocarbons is 0.1 μm/yr (Yung et al. 1984), the surface would be coated (optically) in a few years unless cleansing processes are active. The dunes must be mobile on this timescale to prevent accumulation of bright coatings. Likewise fluvial/pluvial processes every few decades must be cleaning the dark floors of the incised channels and dark scoured plains at the Huygens landing site. In this model Xanadu is a large inactive region where eolian, fluvial, pluvial activity is currently at a low ebb. Huygens landing in a region of the dark blue materials a few kilometers south of bright highlands and about 30 km south of the nearest occurrence of the VIMS-dark-brown Radar-dunes unit. References: Lorenz, R. D., et al., Science, 312, 2006; Griffith, C. A., et al., Science 300, 2003; McCord, T. B., et al., Pl. Sp. Sci. in press, 2006; Yung, Y. L., et al., Ap. J. Supp, 55, 1984.

  16. Comparison of the rotationally adiabatic and vibrationally adiabatic distorted wave methods for the H H2(v=0, j=0)→') H chemical reactions

    NASA Astrophysics Data System (ADS)

    Clary, D. C.; Connor, J. N. L.

    Rotationally adiabatic distorted wave (RADW) and vibrationally adiabatic distorted wave (VADW) calculations of total and differential cross sections are reported for the three-dimensional H + H2(v=0, j=0) →H2(v'=0, j') + H and D + H2(v=0, j=0) →DH(v'=0, j') + H chemical reactions. Both the Porter-Karplus (PK) and the Siegbahn-Liu-Truhlar-Horowitz (SLTH) potential energy surfaces are used. The RADW results for D+H2 on the SLTH potential surface agree well with those obtained by Yung et al. In calculations using the PK surface, we obtain poor agreement with the RADW results reported for the H + H2 reaction by Choi and Tang, and for the D + H2 reaction by Tang and Choi. Reasons for these discrepancies are discussed. The absolute total RADW cross sections for the H + H2 reaction using both potential surfaces fall well below those obtained in accurate quantum calculations while the VADW total cross sections are smaller in magnitude than the RADW cross sections. The RADW and VADW results for relative rotational population distributions and for normalized differential cross sections are almost identical, and agree well with accurate quantum calculations for these quantities for the H + H2 reaction using the PK potential surface.

  17. Schrödinger

    NASA Astrophysics Data System (ADS)

    Kilmister, C. W.

    1989-03-01

    1. Introduction C. W. Kilmister; 2. Boltzmann's influence on Schrödinger Dieter Flamm; 3. Schrödinger's original interpretation of the Schrödinger equation: a rescue attempt Jon Dorling; 4. Are there quantum jumps? J. S. Bell; 5. Square root of minus one, complex phases and Erwin Schrödinger Chen Ning Yung; 6. Consequences of the Schrödinger equation for atomic and molecular physics W. E. Thirring; 7. Molecular dynamics: from H + H, to biomolecules Martin Karplus; 8. Orbital presentation of chemical reactions Kenichi Fukui; 9. Quantum chemistry A. D. Buckingham; 10. Eamon de Valera, Erwin Schrödinger and the Dublin Institute Sir William McCrea; 11. Do bosons condense? J. T. Lewis; 12. Schrödinger's nonlinear optics James McConnell; 13. Schrödinger's unified field theory seen 40 years later O. Hittmair; 14. The Schrödinger equation of the Universe S. W. Hawking; 15. Overview of particle physics A. Salam; 16. Gauge fields, topological defects and cosmology T. W. B. Kibble; 17. Quantum theory and astronomy M. J. Seaton; 18. Schrödinger's contributions to chemistry and biology Linus Pawling; 19. Erwin Schrödinger's What is Life? and molecular biology M. F. Perutz.

  18. Mars atmospheric D/H - Consistent with polar volatile theory?

    NASA Technical Reports Server (NTRS)

    Jakosky, Bruce M.

    1990-01-01

    Current theories on the Martian water history are discussed on the basis of data for the D/H ratio in the Martian atmosphere (which was found to be enhanced by a factor of 6 + or - relative to the value on earth). In particular, the calculations of Yung et al. (1988), on the basis of their photochemical model, are found to be inconsistent with current theories for the evolution of the polar deposits on Mars. While the photochemical model predicts that about 95 percent of the Martian water has escaped over geologic time and the nonatmospheric reservoir is now only 02 m thick, the polar volatile theory suggest that polar deposits contain the equivalent of tens of meters of water, requiring a more rapid escape of H and D to space than predicted by the photochemical model to match the observed D/H ratio. The paper examines the behavior of the polar caps and the atmospheric water vapor over geologic time and the loss of H and D to space. It is concluded that, at present, it is premature to accept a specific history for water on Mars.

  19. The bioethical principles and Confucius' moral philosophy.

    PubMed

    Tsai, D F-C

    2005-03-01

    This paper examines whether the modern bioethical principles of respect for autonomy, beneficence, non-maleficence, and justice proposed by Beauchamp and Childress are existent in, compatible with, or acceptable to the leading Chinese moral philosophy-the ethics of Confucius. The author concludes that the moral values which the four prima facie principles uphold are expressly identifiable in Confucius' teachings. However, Confucius' emphasis on the filial piety, family values, the "love of gradation", altruism of people, and the "role specified relation oriented ethics" will inevitably influence the "specification" and application of these bioethical principles and hence tend to grant "beneficence" a favourable position that diminishes the respect for individual rights and autonomy. In contrast, the centrality of respect for autonomy and its stance of "first among equals" are more and more stressed in Western liberal viewpoints. Nevertheless, if the Confucian "doctrine of Mean" (chung-yung) and a balanced "two dimensional personhood" approach are properly employed, this will require both theorists and clinicians, who are facing medical ethical dilemmas, of searching to attain due mean out of competing moral principles thus preventing "giving beneficence a priority" or "asserting autonomy must triumph". PMID:15738437

  20. A first application of marine-controlled source method on gas-hydrate study off SW Taiwan

    NASA Astrophysics Data System (ADS)

    Chiang, C.; Hsu, S.; Chen, C.; Evans, R. L.

    2011-12-01

    Bottom simulating reflector (BSR), high methane flux, shallow sulfide/methane interface, fluid gushed from the seafloor, self-carbonate within sediment, methane reef, and self-biome are widely distributed in the offshore of the southwestern Taiwan. These geophysical and geochemistry signatures imply a high gas hydrate reservoir area. However, the upper bound of the gas hydrate and shallow section of the sediment are still unclear. This study shows the results of our first marine controlled-source electromagnetic survey in 2010 and provides the information of shallow sediment around the offshore of southwestern Taiwan. Three target areas were conducted: the southeast of Small Ryukyu Islands (seepage, G96), west of Yung-An Ridge (YAR) and northwest of Good Weather Ridge (GWR). In total, fourteen survey lines have been carried out, and the total survey length is about 72 km. Our preliminary result shows that the resistivity/porosity anomalies within pockmarks and seepages correspond to the features from the sub-bottom profilers. The range of porosity change is 4 % in G96 and YAR sites, while in the GWR site there is up to 8 % of porosity change and implies a high gas hydrate potential area.

  1. Isotopic fractionation of hydrogen in planetary exospheres due to ionosphere-exosphere coupling - Implications for Venus

    NASA Astrophysics Data System (ADS)

    Hodges, R. R.

    1993-06-01

    The paper considers isotopic hydrogen fractionation processes in the Venusian exosphere due to ionosphere-exosphere coupling by addressing two deficiencies in the present theory of differential escape. First, a set of D/H isotopic fractionation curves is derived for the ion-neutral interactions of charge and collisional momentum transfer, and these are compared with the results of Gurwell and Yung (1993) for hot O collisional ejection. Then, the question of the relative importance of collisional ejection in atmospheric escape is reexamined using two simple exosphere models. It is shown that O-O collisions suppress the high energy component of the hot O distribution by more than a factor of 10. Moreover, the ballistic trajectories of fast O atoms that reach the nighttime reservoir of exospheric hydrogen favor downward scatter of D and H rather than their escape. It is concluded that, due to severe limits placed on the effectiveness of collisional ejection, the differential escape of D and H from Venus is determined by charge exchange interactions rather than the collisional ejection.

  2. Isotopic fractionation of hydrogen in planetary exospheres due to ionosphere-exosphere coupling - Implications for Venus

    NASA Technical Reports Server (NTRS)

    Hodges, R. R., Jr.

    1993-01-01

    The paper considers isotopic hydrogen fractionation processes in the Venusian exosphere due to ionosphere-exosphere coupling by addressing two deficiencies in the present theory of differential escape. First, a set of D/H isotopic fractionation curves is derived for the ion-neutral interactions of charge and collisional momentum transfer, and these are compared with the results of Gurwell and Yung (1993) for hot O collisional ejection. Then, the question of the relative importance of collisional ejection in atmospheric escape is reexamined using two simple exosphere models. It is shown that O-O collisions suppress the high energy component of the hot O distribution by more than a factor of 10. Moreover, the ballistic trajectories of fast O atoms that reach the nighttime reservoir of exospheric hydrogen favor downward scatter of D and H rather than their escape. It is concluded that, due to severe limits placed on the effectiveness of collisional ejection, the differential escape of D and H from Venus is determined by charge exchange interactions rather than the collisional ejection.

  3. Tumor growth and angiogenesis are dependent on the presence of immature dendritic cells

    PubMed Central

    Fainaru, Ofer; Almog, Nava; Yung, Chong Wing; Nakai, Kei; Montoya-Zavala, Martin; Abdollahi, Amir; D'Amato, Robert; Ingber, Donald E.

    2010-01-01

    Dendritic cells (DCs)—immunomodulatory cells that initiate adaptive immune responses—have recently been shown to exert proangiogenic effects when infiltrating the tumor microenvironment. As tumors that escape immune surveillance inhibit DC maturation, we explored whether maturation status determines their ability to promote angiogenesis and whether angiogenesis depends on the presence of DCs. Using mouse xenograft models of human tumors, we show that fast-growing “angiogenic” tumors are infiltrated by a more immature DC population than respective dormant avascular tumors. Accordingly, supplementation of immature DCs, but not mature DCs, enhanced tumor growth. When DCs were mixed with Matrigel and injected subcutaneously into mice, only immature DCs promoted the ingrowth of patent blood vessels. Notably, depletion of DCs in a transgenic mouse model that allows for their conditional ablation completely abrogated basic fibroblast growth factor-induced angiogenesis in Matrigel plugs, and significantly inhibited tumor growth in these mice. Because immature DCs actively promote angiogenesis and tumor growth, whereas DC maturation or ablation suppresses this response, we conclude that angiogenesis is dependent on the presence of immature DCs. Thus, cancer immunotherapies that promote DC maturation may act by both augmenting the host immune response to the tumor and by suppressing tumor angiogenesis.—Fainaru, O., Almog, N., Yung, C. W., Nakai, K., Montoya-Zavala, M., Abollahi, A., D’Amato, R., Ingber, D. E. Tumor growth and angiogenesis are dependent on the presence of immature dendritic cells. PMID:20008545

  4. Corner detection and classification using anisotropic directional derivative representations.

    PubMed

    Shui, Peng-Lang; Zhang, Wei-Chuan

    2013-08-01

    This paper proposes a corner detector and classifier using anisotropic directional derivative (ANDD) representations. The ANDD representation at a pixel is a function of the oriented angle and characterizes the local directional grayscale variation around the pixel. The proposed corner detector fuses the ideas of the contour- and intensity-based detection. It consists of three cascaded blocks. First, the edge map of an image is obtained by the Canny detector and from which contours are extracted and patched. Next, the ANDD representation at each pixel on contours is calculated and normalized by its maximal magnitude. The area surrounded by the normalized ANDD representation forms a new corner measure. Finally, the nonmaximum suppression and thresholding are operated on each contour to find corners in terms of the corner measure. Moreover, a corner classifier based on the peak number of the ANDD representation is given. Experiments are made to evaluate the proposed detector and classifier. The proposed detector is competitive with the two recent state-of-the-art corner detectors, the He & Yung detector and CPDA detector, in detection capability and attains higher repeatability under affine transforms. The proposed classifier can discriminate effectively simple corners, Y-type corners, and higher order corners. PMID:23743776

  5. Helical Majorana fermions in d+id'-wave topological superconductivity of doped correlated quantum spin Hall insulators

    NASA Astrophysics Data System (ADS)

    Chung, Chung-Hou; Sun, Shih-Jye; Chang, Yung-Yeh; Tsai, Wei-Feng; Zhang, Fuchun

    Large Hubbard U limit of the Kane-Mele model on a zigzag ribbon of honeycomb lattice near half-filling is studied via a renormalized mean-field theory. The ground state exhibits time-reversal symmetry (TRS) breaking dx2 -y2 + idxy -wave superconductivity. At large spin-orbit coupling, the Z2 topological phase with non-trivial spin Chern number in the pure Kane-Mele model is persistent into the TRS broken state (called ``spin-Chern phase''), and has two pairs of counter-propagating helical Majorana modes at the edges. As the spin-orbit coupling is reduced, the system undergoes a topological quantum phase transition from the spin-Chern to chiral superconducting states. Possible relevance of our results to adatom-doped graphene and irridate compounds is discussed.Ref.:Shih-Jye Sun, Chung-Hou Chung, Yung-Yeh Chang, Wei-Feng Tsai, and Fu-Chun Zhang, arXiv:1506.02584. CHC acknowledges support from NSC Grant No. 98-2918-I-009-06, No. 98-2112-M-009-010-MY3, the NCTU-CTS, the MOE-ATU program, the NCTS of Taiwan, R.O.C.

  6. NOx in the atmospheres of aquaplanets as electron acceptors for life

    NASA Astrophysics Data System (ADS)

    Wong, M. L.; Yung, Y. L.; Russell, M. J.

    2014-12-01

    A high potential electron acceptor is required to drive the highly endergonic reactions at the entry points to the autotrophic metabolic pathways that would lead to life on any wet rocky world. Nitrate and nitrite in the earliest oceans are the most attractive candidates (Ducluzeau et al., 2009, 2014). It has been estimated that, given a CO2 and N2 atmosphere, lightning (a proportion of it volcanic), meteorite impacts and volcanic gases would have produced enough NOx in a million years or so (>1018 g) to generate micromolar amounts of NO3- and NO2- in the ocean (Yung and McElroy, 1979; Kasting, 1990; Navarro-González et al., 1998; Martin et al., 2007). It is notable that lightning has been detected on Venus and Mars along with evidence of atmospheric NO. Because a figure 1018 g of nitrate/nitrite is controversial, we will present new calculations based on 10 atmospheres of CO2, two atmospheres of N2 and stepped concentrations of water vapor dependent on surface temperatures.

  7. Exploring Chemical Equilibrium in Hot Jovians

    NASA Astrophysics Data System (ADS)

    Blumenthal, Sarah; Harrington, Joseph; Mandell, Avi; Hébrard, Eric; Venot, Olivia; Cubillos, Patricio; Blecic, Jasmina; Challener, Ryan

    2016-01-01

    It has been established that equilibrium chemistry is usually achieved deep in the atmosphere of hot Jovians where timescales are short (Line and Yung 2013). Thus, equilibrium chemistry has been used as a starting point (setting initial conditions) for evaluating disequilibrium processes. We explore parameters of setting these initial conditions including departures from solar metallicity, the number of species allowed in a system, the types of species allowed in a system, and different thermodynamic libraries in an attempt to create a standard for evaluating equilibrium chemistry. NASA's open source code Chemical Equilibrium and Applications (CEA) is used to calculate model planet abundances by varying the metallicity, in the pressure regime 0.1 to 1 bar. These results are compared to a variety of exoplanets(Teq between 600 and 2100K) qualitatively by color maps of the dayside with different temperature redistributions. Additionally, CEA (with an up-dated thermodynamic library) is compared with the thermochemical model presented in Venotet al. (2012) for HD 209458b and HD 189733b. This same analysis is then applied to the cooler planet HD 97658b. Spectra are generated and we compare both models' outputs using the open source codetransit (https://github.com/exosports/transit) using the opacities of 15 molecules. We make the updated CEA thermodyanamic library and supporting Python scripts to do the CEA analyses available open source. Thiswork was supported by NASA Planetary Atmospheres grant NNX12AI69G.

  8. The Critical Fugacity for Surface Adsorption of Self-Avoiding Walks on the Honeycomb Lattice is

    NASA Astrophysics Data System (ADS)

    Beaton, Nicholas R.; Bousquet-Mélou, Mireille; de Gier, Jan; Duminil-Copin, Hugo; Guttmann, Anthony J.

    2014-03-01

    In 2010, Duminil-Copin and Smirnov proved a long-standing conjecture of Nienhuis, made in 1982, that the growth constant of self-avoiding walks on the hexagonal (a.k.a. honeycomb) lattice is . A key identity used in that proof was later generalised by Smirnov so as to apply to a general O( n) loop model with (the case n = 0 corresponding to self-avoiding walks). We modify this model by restricting to a half-plane and introducing a surface fugacity y associated with boundary sites (also called surface sites), and obtain a generalisation of Smirnov's identity. The critical value of the surface fugacity was conjectured by Batchelor and Yung in 1995 to be . This value plays a crucial role in our generalized identity, just as the value of the growth constant did in Smirnov's identity. For the case n = 0, corresponding to self-avoiding walks interacting with a surface, we prove the conjectured value of the critical surface fugacity. A crucial part of the proof involves demonstrating that the generating function of self-avoiding bridges of height T, taken at its critical point 1/ μ, tends to 0 as T increases, as predicted from SLE theory.

  9. Tensile flow and work-hardening behavior of a Ti-modified austenitic stainless steel

    SciTech Connect

    Sivaprasad, P.V.; Venugopal, S.; Venkadesan, S.

    1997-01-01

    The flow-stress data of a 15Cr-15Ni-2.2Mo-Ti modified austenitic stainless steel in the temperature range 300 to 1,023 K was analyzed in terms of Ludwigson and Voce equations. The parameters of these equations were critically examined with respect to the effect of Ti/C ratio and test temperature. It was found that the Ludwigson equation described the flow behavior adequately up to the test temperature of 923 K, whereas the Voce equation could be employed in the full temperature range. The peaks/plateaus observed in the variation of these parameters as a function of temperature in the intermediate temperature range have been identified as one of the manifestations of dynamic strain aging (DSA). Also, the variation of these parameters with temperature clearly could bring out the different domains of DSA observed in this alloy. The work-hardening analysis of the flow-stress data revealed that in the DSA regime, the onset of stage III hardening is athermal.

  10. Hierarchical clustering of 54 races and strains of the mulberry silkworm, Bombyx mori L: Significance of biochemical parameters.

    PubMed

    Chatterjee, S N; Datta, R K

    1992-12-01

    A detailed analysis was undertaken to test the efficacy of hierarchical agglomerative clustering (UPGMA method) in grouping the races and strains of the mulberry silkworm, Bombyx moti L., and to ascertain the importance of biochemical parameters in the clustering process. The analysis was based on data from two rearing seasons with 54 selected races/strains of different geographic origin and varying yield potentials. The results indicate that seven clusters can be realised with yield parameters alone, whereas the inclusion of biochemical parameters in clustering resulted into two broad groups: one having all the breeds with high cocoon weight and shell weight, the other having all the low-yielding silkworm strains both from India and from other countries. Further sub-grouping under these two groups highlights genetical differences associated with the differentiation of various groups of races in temperate and tropical areas as well as their significance for silkworm breeding. Estimates of all ten variables were further subjected to 'quick clustering' and the results showed that cluster 5, constituted by 38 lowyielding strains of India, China and Europe, had the highest values of the final cluster centre for amylase and the effective rate of rearing (ERR), while clusters 1 and 4 had the highest values for invertase and alkaline phosphatase. The evolutionary aspect of the genetic channelisation of silkworm races from various countries is discussed against the background of differences in the biochemical parameters and yield variables. PMID:24197452

  11. SCC of austenitic stainless steel, Ni-21Cr-13.5Mo alloy, and 0.3Mo-0.8Ni-Ti in 350 C synthetic, NO{sub 2}2-NO{sub 3}-OH tank waste

    SciTech Connect

    Pednekar, S.P.

    1998-12-31

    A necessary step in preparation of high-level radioactive tank waste for sate disposal is removal of non radioactive organic and inorganic components from washed waste. The oxidizing and alkaline nature of most wastes allows the removal of the organic components as water vapor, carbon dioxide, and ammonia gas merely by heating the wastes to no more than 350 C. Type 3 16L stainless steel (UNS S3 1603) a 21Cr-13.5Mo-Ni alloy (UNS N06022), and 0.8Ni-0.3Mo-Ti alloy (UNS R53400) were candidate materials for reactors in which the oxidation could be performed. Slow-strain-rate tests were performed on these three materials at a strain rate of 10{sup {minus}6}sec{sup {minus}1} in a diluted waste type solution containing 4.1% NO{sub 2}, 3.7% NO{sub 3}, 1% OH, and 0.22% TIC. All three materials showed intergranular stress corrosion cracking with substantial losses in ductility and strength.

  12. The FlgT Protein Is Involved in Aeromonas hydrophila Polar Flagella Stability and Not Affects Anchorage of Lateral Flagella

    PubMed Central

    Merino, Susana; Tomás, Juan M.

    2016-01-01

    Aeromonas hydrophila sodium-driven polar flagellum has a complex stator-motor. Consist of two sets of redundant and non-exchangeable proteins (PomA/PomB and PomA2/PomB2), which are homologs to other sodium-conducting polar flagellum stator motors; and also two essential proteins (MotX and MotY), that they interact with one of those two redundant pairs of proteins and form the T-ring. In this work, we described an essential protein for polar flagellum stability and rotation which is orthologs to Vibrio spp. FlgT and it is encoded outside of the A. hydrophila polar flagellum regions. The flgT was present in all mesophilic Aeromonas strains tested and also in the non-motile Aeromonas salmonicida. The A. hydrophila ΔflgT mutant is able to assemble the polar flagellum but is more unstable and released into the culture supernatant from the cell upon completion assembly. Presence of FlgT in purified polar hook-basal bodies (HBB) of wild-type strain was confirmed by Western blotting and electron microscopy observations showed an outer ring of the T-ring (H-ring) which is not present in the ΔflgT mutant. Anchoring and motility of proton-driven lateral flagella was not affected in the ΔflgT mutant and specific antibodies did not detect FlgT in purified lateral HBB of wild type strain. PMID:27507965

  13. Comparison of a Simple Patched Conic Trajectory Code to Commercially Available Software

    NASA Technical Reports Server (NTRS)

    AndersonPark, Brooke M.; Wright, Henry S.

    2007-01-01

    Often in spaceflight proposal development, mission designers must eva luate numerous trajectories as different design factors are investiga ted. Although there are numerous commercial software packages availab le to help develop and analyze trajectories, most take a significant amount of time to develop the trajectory itself, which isn't effectiv e when working on proposals. Thus a new code, PatCon, which is both q uick and easy to use, was developed to aid mission designers to condu ct trade studies on launch and arrival times for any given target pla net. The code is able to run quick analyses, due to the incorporation of the patched conic approximation, to determine the trajectory. PatCon provides a simple but accurate approximation of the four body moti on problem that would be needed to solve any planetary trajectory. P atCon has been compared to a patched conic test case for verification, with limited validation or comparison with other COTS software. This paper describes the patched conic technique and its implementation i n PatCon. A description of the results and comparison of PatCon to ot her more evolved codes such as AGI#s Satellite Tool Kit and JAQAR As trodynamics# Swingby Calculator is provided. The results will include percent differences in values such as C3 numbers, and Vinfinity at a rrival, and other more subjective results such as the time it takes to build the simulation, and actual calculation time.

  14. Microstructural Characterization of U-Nb-Zr, U-Mo-Nb, and U-Mo-Ti Alloys via Electron Microscopy

    SciTech Connect

    A. Ewh; D. D. Keiser, Jr.; Y. H. Sohn

    2010-06-01

    Ternary uranium molybdenum alloys are currently being investigated for use as dispersion and monolithic nuclear fuels in research reactors. In this study, two such ternary alloys, with compositions U-8Mo-3Nb and U-7Mo-3Ti in wt.%, were examined using scanning electron microscopy (SEM), X-ray diffraction (XRD), and transmission electron microscopy (TEM) with high angle annular dark field (HAADF) imaging via scanning transmission electron microscopy (STEM) to identify phase constituents. These alloys were homogenized at 950°C for 96 hours and were expected to be single-phase bcc-!-U. However, upon examination, it was determined that despite homogenization, each of the alloys contained a small volume fraction precipitate phase. Through SEM and XRD, it was confirmed that the matrix retained the bcc-!-U phase, but the precipitate phases could not be identified using these methods. TEM specimens were prepared using site-specific focused ion beam (FIB) in situ lift out (INLO) technique to include at least one precipitate from each alloy. By electron diffraction, the precipitate phases for the U- 8Mo-3Nb and U-7Mo-3Ti alloys were identified as bcc-(Mo,Nb) solid solution and bcc- (Mo,Ti) solid solution, respectively.

  15. NASA Tech Briefs, July 2007

    NASA Technical Reports Server (NTRS)

    2007-01-01

    Topics covered include: Miniature Intelligent Sensor Module; "Smart" Sensor Module; Portable Apparatus for Electrochemical Sensing of Ethylene; Increasing Linear Dynamic Range of a CMOS Image Sensor; Flight Qualified Micro Sun Sensor; Norbornene-Based Polymer Electrolytes for Lithium Cells; Making Single-Source Precursors of Ternary Semiconductors; Water-Free Proton-Conducting Membranes for Fuel Cells; Mo/Ti Diffusion Bonding for Making Thermoelectric Devices; Photodetectors on Coronagraph Mask for Pointing Control; High-Energy-Density, Low-Temperature Li/CFx Primary Cells; G4-FETs as Universal and Programmable Logic Gates; Fabrication of Buried Nanochannels From Nanowire Patterns; Diamond Smoothing Tools; Infrared Imaging System for Studying Brain Function; Rarefying Spectra of Whispering-Gallery-Mode Resonators; Large-Area Permanent-Magnet ECR Plasma Source; Slot-Antenna/Permanent-Magnet Device for Generating Plasma; Fiber-Optic Strain Gauge With High Resolution And Update Rate; Broadband Achromatic Telecentric Lens; Temperature-Corrected Model of Turbulence in Hot Jet Flows; Enhanced Elliptic Grid Generation; Automated Knowledge Discovery From Simulators; Electro-Optical Modulator Bias Control Using Bipolar Pulses; Generative Representations for Automated Design of Robots; Mars-Approach Navigation Using In Situ Orbiters; Efficient Optimization of Low-Thrust Spacecraft Trajectories; Cylindrical Asymmetrical Capacitors for Use in Outer Space; Protecting Against Faults in JPL Spacecraft; Algorithm Optimally Allocates Actuation of a Spacecraft; and Radar Interferometer for Topographic Mapping of Glaciers and Ice Sheets.

  16. "Tinni" rice (Oryza rufipogon Griff.) production: an integrated sociocultural agroecosystem in eastern Uttar Pradesh of India.

    PubMed

    Singh, Ranjay K; Turner, Nancy J; Pandey, C B

    2012-01-01

    This study reports how Traditional Ecological Knowledge (TEK) and informal cultural institutions have conserved key varieties of the wildgrowing rice, 'tinni' (red rice, or brownbeard rice, Oriza rufipogon Griff.), within the Bhar community of eastern Uttar Pradesh, India. The study was conducted, using conventional and participatory methods, in 10 purposively selected Bhar villages. Two distinct varieties of tinni ('tinni patali' and 'tinni moti') with differing habitats and phenotypic characters were identified. Seven microecosystems (Kari, Badaila, Chammo, Karmol, Bhainsiki, Bhainsala and Khodailia) were found to support these varieties in differing proportions. Tinni rice can withstand more extreme weather conditions (the highest as well as lowest temperatures and rainfall regimes) than the 'genetically improved' varieties of rice (Oriza sativa L.) grown in the region. Both tinni varieties are important bioresources for the Bhar's subsistence livelihoods, and they use distinctive conservation approaches in their maintenance. Bhar women are the main custodians of tinni rice agrobiodiversity, conserving tinni through an institution called Sajha. Democratic decision-making at meetings organized by village elders determines the market price of the tinni varieties. Overall, the indigenous institutions and women's participation seem to have provided safeguards from excessive exploitation of tinni rice varieties. The maintenance of tinni through cultural knowledge and institutions serves as an example of the importance of locally maintained crop varieties in contributing to people's resilience and food security in times of rapid social and environmental change. PMID:21959872

  17. MotX, the channel component of the sodium-type flagellar motor.

    PubMed Central

    McCarter, L L

    1994-01-01

    Thrust for propulsion of flagellated bacteria is generated by rotation of a propeller, the flagellum. The power to drive the polar flagellar rotary motor of Vibrio parahaemolyticus is derived from the transmembrane potential of sodium ions. Force is generated by the motor on coupling of the movement of ions across the membrane to rotation of the flagellum. A gene, motX, encoding one component of the torque generator has been cloned and sequenced. The deduced protein sequence is 212 amino acids in length. MotX was localized to the membrane and shown to interact with MotY, which is the presumed stationary component of the motor. Overproduction of MotX, but not that of a nonfunctional mutant MotX, was lethal to Escherichia coli. The rate of lysis caused by induction of motX was proportional to the sodium ion concentration. Li+ and K+ substituted for Na+ to promote lysis, while Ca2+ did not enhance lysis. Protection from the lethal effects of induction of motX was afforded by the sodium channel blocker amiloride. The data suggest that MotX forms a sodium channel. The deduced protein sequence for MotX shows no homology to its ion-conducting counterpart in the proton-driven motor; however, in possessing only one hydrophobic domain, it resembles other channels formed by small proteins with single membrane-spanning domains. Images PMID:7928960

  18. Cytotoxicity of Metal and Ceramic Particles in Different Sizes

    NASA Astrophysics Data System (ADS)

    Yoshida, Kazuhiro; Morita, Masafumi; Mishina, Hiroshi

    The wear debris caused by joint prosthesis is well known to induce an inflammation in the peripheral tissue. The authors carried out two kinds of experiments, to clarify the phagocytable size of wear particles and the cytotoxicity of macrophage related to the size and materials. The test materials were Al2O3, SiO2, TiO2 fine particles and Ti-6Al-4V, Co-28Cr-6Mo wear particles. The results showed that the phagocytable particle size was less than 11.9±11.2µm. It appears that the cytotoxicity did not depend on the particle size, even if the particles were phagocytable size. In the relationship between material type and inflammation, damage levels were found to be different between SiO2 and TiO2 particles, even if neither material released metal ions. The cells were damaged more severely by SiO2 particles than by Co-28Cr-6Mo for which the eluted ion could not be ignored (damage levels; SiO2>Co-28Cr-6Mo>Ti-6Al-4V>Al2O3≧TiO2). For these reasons, it was confirmed that there was a factor in addition to the toxicity of the eluted metal ion (i. e., the implant material's corrosion resistance ability), which influenced the inflammation.

  19. Tuning Electronic and magnetic properties of phosphorene by vacancies and adatoms

    NASA Astrophysics Data System (ADS)

    Srivastava, Pooja; Hembram, K. P. S. S.; Mizuseki, Hiroshi; Lee, Kwang-Ryeol; Han, Sang Soo; Kim, Seungchul

    2015-03-01

    In the search of novel materials, phosphorene (2D layers of black phosphorus) has been synthesized recently. Intrinsic bandgap, hydrophilicity and anisotropic electron mobility make phosphorene different from graphene and also, its hole mobility is higher than that in MoS2. All these properties make it a very promising material for electronics and optoelectronics applications. As with other as-synthesized materials, phosphorene exhibits defects such as vacancies, and these defects can affect the properties of the material significantly. The present work provides a detailed understanding of various vacancy defects (mono- and di-vacancies) and their effect on the electronic and magnetic properties of phosphorene. We have also studied the effects of omnipresent non-metallic C/N/O and transition metal (TM) Fe/Co/Ni on the electronic and magnetic properties of phosphorene. We show that, for various adatom adsorbed pristine/defected phosphorene structures the magnetic moment can be tuned via the control of Fermi level. The magnetism for non-metallic adatom adsorbed pristine/defective phosphorene systems can be switch ON/OFF. TM adatoms provide extra flexibility by tuning the magnitude as well. We acknowledge support from KIST Institutional project (Grant No. 2E24630) and Industrial Strategic Technology Development Program (Grant No. 10041589) funded by the MOTIE, Korea.

  20. A new algorithm for fluid simulation of high density plasma discharges

    NASA Astrophysics Data System (ADS)

    Oh, Seon-Geun; Lee, Young-Jun; Choe, Heehwan; Jeon, Jae-Hong; Seo, Jong-Hyun

    2013-10-01

    Low temperature, high density plasma sources are widely used for the electronic device fabrications such as semiconductor, flat panel display, and solar cell. The inductively coupled plasma or the capacitively coupled plasma reactors are typical ones in these processes. Fluid simulation is one of the methods for transport modeling of high density discharge, because the profiles of plasma quantities are easily obtained. The short shielding time scale of an electric field perturbation is a major restriction on the simulation time step. In most cases, the simulation time step in the explicit method is less than 10-13 sec. To overcome this limitation, a new method for steady-state fluid simulation of high density plasma discharge is suggested. Following the physical origin of restriction on simulation time step, a new method is developed using both analytic and numerical methods. A simple application of the new method with previously known one is given to study the validity of the method. This work was supported in part by the International collaborative R&D program (N0000678), and by the Industrial Strategic Technology Development Program (10041681) funded by the Ministry of Trade, Industry and Energy (MOTIE, Korea).

  1. Aging behavior and mechanical properties of maraging steels in the presence of submicrocrystalline Laves phase particles

    SciTech Connect

    Mahmoudi, A.; Ghavidel, M.R. Zamanzad; Nedjad, S. Hossein; Heidarzadeh, A.; Ahmadabadi, M. Nili

    2011-10-15

    Cold rolling and annealing of homogenized Fe-Ni-Mn-Mo-Ti-Cr maraging steels resulted in the formation of submicrocrystalline Fe{sub 2}(Mo,Ti) Laves phase particles. Optical and scanning electron microscopy, X-ray diffraction, tensile and hardness tests were used to study the microstructure, aging behavior and mechanical properties of the annealed steels. The annealed microstructures showed age hardenability during subsequent isothermal aging at 753 K. Ultrahigh fracture stress but poor tensile ductility was obtained after substantial age hardening in the specimens with 2% and 4% chromium. Increasing chromium addition up to 6% toughened the aged microstructure at the expense of the fracture stress by increasing the volume fraction of retained austenite. The Laves phase particles acted as crack nucleation sites during tensile deformation. - Highlights: {yields} Laves phases dispersed in a BCC iron matrix by annealing of cold rolled samples. {yields} The samples showed age hardenability during subsequent isothermal aging at 753 K. {yields} Ultrahigh fracture stress but poor ductility was obtained after age hardening. {yields} Increasing chromium addition toughened the aged microstructure. {yields} Laves phase particles acting as crack nucleation sites during tensile deformation.

  2. S3 and S4 abundances and improved chemical kinetic model for the lower atmosphere of Venus

    NASA Astrophysics Data System (ADS)

    Krasnopolsky, Vladimir A.

    2013-07-01

    Mixing ratios of S3 and S4 are obtained from reanalysis of the spectra of true absorption in the visible range retrieved by Maiorov et al. (Maiorov, B.S. et al. [2005]. Solar Syst. Res. 39, 267-282) from the Venera 11 observations. These mixing ratios are fS3 = 11 ± 3 ppt at 3-10 km and 18 ± 3 ppt at 10-19 km, fS4 = 4 ± 4 ppt at 3-10 km and 6 ± 2 ppt at 10-19 km, and show a steep decrease in both S3 and S4 above 19 km. Photolysis rates of S3 and S4 at various altitudes are calculated using the Venera 11 spectra and constant photolysis yields as free parameters. The chemical kinetic model for the Venus lower atmosphere (Krasnopolsky, V.A. [2007]. Icarus 191, 25-37) has been improved by inclusion of the S4 cycle from Yung et al. (Yung, Y.L. et al. [2009]. J. Geophys. Res. 114, E00B34), reduction of the H2SO4 and CO fluxes at the upper boundary of 47 km by a factor of 4 in accord with the recent photochemical models for the middle atmosphere, by using a closed lower boundary for OCS instead of a free parameter for this species at the surface, and some minor updates. Our model with the S4 cycle but without the SO3 + 2 OCS reaction suggested by Krasnopolsky and Pollack (Krasnopolsky, V.A., Pollack, J.B. [1994]. Icarus 109, 58-78) disagrees with the observations of OCS, CO, S3, and S4. However, inclusion of the S4 cycle improves the model fit to all observational constraints. The best-fit activation energy of 7800 K for thermolysis of S4 supports the S4 enthalpy from Mills (Mills, K.C. [1974]. Thermodynamic Data for Inorganic Sulfides, Selenides and Tellurides. Butterworths, London). Chemistry of the Venus lower atmosphere is initiated by disequilibrium products H2SO4 and CO from the middle atmosphere, photolysis of S3 and S4, and thermochemistry in the lowest scale height. The chemistry is mostly driven by sulfur that is formed in a slow reaction SO + SO, produces OCS, and results in dramatic changes in abundances of OCS, CO, and free sulfur allotropes. The SX + OCS

  3. SOIR/VEX mesospheric aerosols observations and modelling

    NASA Astrophysics Data System (ADS)

    Wilquet, Valérie; Carine Vandaele, Ann; Drummond, Rachel; Mahieux, Arnaud; Robert, Séverine; Daerden, Frank; Neary, Lori; Bertaux, Jean-Loup

    2013-04-01

    , A. Mahieux, A.A. Fedorova, O.I. Korablev., E. Marcq, Y.L. Yung, X. Zhang. Icarus, 217, 740-751 (2012). Sandor, B.J., R.T. Clancy, G. Moriarty-Schieven, F.P. Mills. Icarus, 208, 49-60 (2010). Wilquet, V., A. Fedorova, F. Montmessin, R. Drummond, A. Mahieux, A.C. Vandaele, E. Villard, O. Korablev, and J.-L. Bertaux. J. Geophys. Res., 114 (E00B42), doi:10.1029/2008JE003186 (2009). Wilquet, V., R. Drummond, A. Mahieux, S. Robert, A.C. Vandaele, J.-L. Bertaux. Icarus 217, 875-881 (2012). Zhang, X., M. Chang Liang, F.P. Mills, D.A. Belyaev, Y.L. Yung. Icarus, 217, 714-739 (2012).

  4. a New Hybrid Program for Fitting Rotationally Resolved Spectra of Methylamine-Like Molecules: Application to 2-METHYLMALONALDEHYDE

    NASA Astrophysics Data System (ADS)

    Kleiner, Isabelle; Hougen, Jon T.

    2015-06-01

    A new hybrid-model fitting program for methylamine-like molecules has been developed, based on an effective Hamiltonian in which the ammonia-like inversion motion is treated using a tunneling formalism, while the internal-rotation motion is treated using an explicit kinetic energy operator and potential energy function. The Hamiltonian in the computer program is set up as a 2x2 partitioned matrix, where each diagonal block consists of a traditional torsion-rotation Hamiltonian (as in the earlier program BELGI), and the two off-diagonal blocks contain all tunneling terms. This hybrid formulation permits the use of the permutation-inversion group G6 (isomorphic to C3v) for terms in the two diagonal blocks, but requires G12 for terms in the off-diagonal blocks. Our first application of the new program is to 2-methylmalonaldehyde. Microwave data for this molecule were previously fit (essentially to experimental measurement error) using an all-tunneling Hamiltonian formalism to treat both large-amplitude-motions. For 2-methylmalonaldehyde, the hybrid program achieves a fit of nearly the same quality as that obtained by the all-tunneling program, but fits with the hybrid program eliminate a large discrepancy between internal rotation barriers in the OH and OD isotopologues of 2-methylmalonaldehyde that arose in fits with the all-tunneling program. Other molecules for application of the hybrid program will be mentioned. V.V. Ilyushin, E.A. Alekseev, Yung-Ching Chou, Yen-Chu Hsu, J. T. Hougen, F.J. Lovas, L. Picraux, J. Mol. Spectrosc. 251 (2008) 56-63

  5. Evaluation of the models available for the prediction of pressure drop in venturi scrubbers.

    PubMed

    Gonçalves, J A; Alonso, D F; Costa, M A; Azzopardi, B J; Coury, J R

    2001-01-29

    The major running cost derived from the operation of venturi scrubbers is pressure drop. In the present study, the predictions of different models are compared to experimental data from venturi scrubbers of different sizes (throat diameter from 1.9 to 16cm), geometries, operating variables and liquid injection arrangements. As a result, it is concluded that most of the models must be used with caution. Much attention must be paid to the validity of the assumptions employed in the mathematical models. The equations proposed by Calvert [Scrubbing, Air Pollution, 3rd Edition, Vol. IV, Academic Press, New York, 1982], Yung et al. [JAPCA 27 (1977) 348] or Hesketh [Atomization and cloud behaviour in wet scrubbers, in: Proceedings of the US-USSR Symposium Control Fine Particulate Emissions 1974, San Francisco, 15-18 January 1974] produce good results only in very specific situations. The model proposed by Boll [Ind. Eng. Chem. Fundam. 12 (1973) 40] is simple, easy to compute and agrees reasonably well with the experimental data. Unfortunately, it cannot predict the effect of different liquid injection arrangements. The model by Azzopardi and coworkers [Filtr. Sep. 21 (1984) 196; Trans. IchemE. 69B (1991) 237; Chem Eng. J. 67 (1997) 9] was the only one to give good predictions for all the range of variables studied. On the other hand, this model is not simple and requires from the engineer an additional effort in terms of computation. In order to apply this model to the rectangular geometry, the concept of hydraulic equivalent diameter was used. PMID:11118688

  6. Comparison Studies on the Observation of Raindrop Size Distribution in Strong Precipitation Frontal Case in Northern Taiwan

    NASA Astrophysics Data System (ADS)

    Lin, Pay-Liam; Chen, Ying-Jhen

    2015-04-01

    In the nighttime of 11th June 2012, a mature Mai-Yu front passed through northern Taiwan. The leading edge of front associated with southwesterly flow produced strong precipitation in a short time. The extreme rainfall event caused multiple areas flooding. In order to investigate the characteristic of drop size distribution (DSD) accompanied with this heavy rainfall event, we used an impact type Joss-Waldgovel disdrometer (JWD), a laser-optical OTT Parsivel disdrometer (Parsivel) and a two dimensional video disdrometer (2DVD) collocated at NCU, and we also used three JWDs in FeiCui, NanGang and XiaYung to investigate the frontal precipitation. In the weak precipitation period, we found the concentration of small raindrops would be underestimated because the velocity detected by Parsivel is faster than the real situation. But we also made sure that before the strong precipitation happens, the three type disdrometers (JWD, 2DVD and Parsivel) operate consistently.During strong precipitation period, we found a significant DSD variation characteristic. As a convective cell passes, the concentration of medium to large drops increases in Parsivel, while decreases in JWD. Due to the limitation of instrument, Parsivel tended to overestimate the concentration of medium to large drops in the strong rainfall intensity. Comparing the rain drops concentration with the rain rate varies with time, Parsivel showed a good agreement but JWD even did not get the most significant characteristic as the strongest rainfall occurred. The rain rates of JWD and Parsivel varied in the same trend, but compared the rain rates with the rain gauge observation in the 10 m tower at NCU, both of them showed obvious underestimation. We suspected the limitation of instrument made the rain rate underestimated.

  7. On the one-dimensional chemistry-diffusion model in planetary atmospheres

    NASA Astrophysics Data System (ADS)

    Zhang, Xi; Showman, Adam

    Most of the current atmospheric chemistry models for planets (e.g., Krasnopolsky & Parshev 1981; Yung et al., 1984; Lavvas et al., 2008) and exo-planets (e.g., Moses et al., 2011; Line et al., 2011; Hu et al., 2012) adopt a one-dimensional (1D) chemistry-diffusion approach in the vertical coordinate such as pressure or altitude. Although only a crude approximation, these 1D models have succeeded in explaining the global-averaged vertical profiles of many chemical species in observations. One of the important assumptions of these models is that, all chemical species are transported via the same eddy diffusion profile. Here we show that, as also noticed in the Earth community (e.g., Holton 1986), in the presence of horizontal transport driven by eddies in the middle atmospheres such as the stratospheres on Earth and Titan, this “homogenous eddy diffusion” assumption generally breaks down. Instead, the eddy diffusion should depend both on the horizontal eddy mixing and the chemical lifetime of the species. It implies that the long-lived species and short-lived species could have significantly different eddy diffusion profiles. We show analytically why this new approach is more physically based. We also show numerically why the old approach fails compared with the globally averaged results from a more realistic two-dimensional (2D) simulation using the state-of-art Caltech/JPL 2D chemistry-diffusion-advection model (Zhang et al., 2013), and discuss the possible consequences. This research was supported by the Bisgrove Scholar Program in the University of Arizona.

  8. Observations of Altitude Dependence and Temporal Variation of ClO in the Venus Mesosphere

    NASA Astrophysics Data System (ADS)

    Sandor, Brad J.; Clancy, R. Todd

    2015-11-01

    Analysis of the first observations of ClO in the Venus mesosphere indicate ClO is present above 85 +/-3 km altitude and not below. The retrieved nightside mean abundances show a factor of 2 decrease between observation dates Oct. 23 and Nov. 11, 2015, with change between the two dates evident at more than two sigma confidence. Abundances and altitude distributions are retrieved from submm spectroscopic observations of the 352.88 GHz line of 35ClO (made with the James Clerk Maxwell Telescope - JCMT - located an Mauna Kea, Hawaii).Detection of ClO in the Venus atmosphere confirms a theory put forward by Yung and DeMore (1982) that the Venus atmosphere is stabilized as CO2 due to chlorine catalytic recombination of CO and O. (Without some form of catalysis, the Venus atmosphere would have 10s of percent CO and O2, but it is in fact 97% CO2 and 3% N2, with only trace amounts of CO and O2.) Detailed retrieval of ClO abundances and altitude distributions (the focus of this talk) provides greater insight to the catalytic process, and to other aspects of Venus atmospheric chlorine chemistry. We compare findings of our quantitave retrieval with predictions of photochemical models, and discuss the implications for chlorine photochemisty of the Venus atmosphere. We also discuss retrieved ClO temporal variation with that of upper mesospheric HCl (Sandor and Clancy, 2012).[We acknowledge funding of this project by NASA grants NNX10AB33G, NNX12AI32G, and NNX14AK05G, as well as NSF grant AST-1312985.

  9. Pluto Photochemical Models for the New Horizons Flyby

    NASA Astrophysics Data System (ADS)

    Gladstone, R.; Wong, M. L.; Yung, Y. L.

    2014-12-01

    During the New Horizons flyby of the Pluto system on July 14, 2015 a number of observations will be made to determine the structure, composition, and variability of Pluto's atmosphere. A key observation of this type is the Alice solar occultation, which will measure the full disk ultraviolet (52-187 nm) spectral flux from the Sun through ingress and egress behind Pluto, about one hour after closest approach. This observation will be used to determine the temperature and vertical density profiles of N2, CH4, and various minor species above two regions of very different surface albedo. Nearly simultaneous Earth ingress and egress occultations observed in X-band uplink will provide profiles of temperature and pressure in Pluto's lower atmosphere, and electron densities in the ionosphere. Wave structures in both the solar and radio occultation data will provide constraints on atmospheric dynamics. In order to interpret and understand these data sets, we have modified a 1-D Titan photochemical model to Pluto, for the epoch of the New Horizons flyby. The model uses a similar, but updated reaction list to that of Krasnopolsky and Cruikshank [1999] and Wong et al. [2014], and adopts the results of Zhu et al. [2014] for the background atmosphere. We present here initial results for several assumed eddy diffusion profiles. Krasnopolsky, V. A., and D. P. Cruikshank, J. Geophys. Res., 104, 21,979, 1999. Wong, M. L., Y. L. Yung, and G. R. Gladstone, Icarus, in press, 2014. Zhu, X., D F. Strobel, and J. T. Erwin, Icarus, 228, 301, 2014.

  10. Variability of CO, OCS And H2O Below The Clouds of Venus From VIRTIS-HNight-side Spectra

    NASA Astrophysics Data System (ADS)

    Marcq, Emmanuel; Bezard, B.; Drossart, P.; Piccioni, G.; VIRTIS Team

    2007-10-01

    The VIRTIS imaging spectrometer has provided numerous spectra of Venus since the beginning of the Venus Express mission in April 2006. The high resolution of the H-channel (R 2000) enables the investigation of the composition below the clouds using the thermal emission from the night side of the planet, since several absorption of minor components (CO, OCS, H2O, HDO, SO2, HF) are located in the 2.3 µm transparency window of CO2. Using a radiative transfer computer model, we were able to derive constraints on the vertical profiles of CO, OCS and H2O in the 30-40 km altitude range up to areas unreacheable with Earth-based instruments (0° - 60°S). Our findings extend the latitudinal trends already noticed from both space (Collard et al., 1993, using Galileo/NIMS) and Earth (Marcq et al. 2005,2006, using IRTF/SpeX): an increase of CO towards high latitudes (30 ± 10 % between 60°S and 0°), a correlated decrease of OCS in the same region and a constant abundance of 28 ± 4 ppmv at 35 km for H2O. The latitudinal variations of CO are in good agreement with the VIRTIS-M observations from Tsang et al. (private communication). The quantitative interpretation of CO and OCS variations in terms of global-scale vertical circulation is in progress, using circulation models such as Yung et al's (private communication) in 2D and Lebonnois et al.'s (38th DPS meeting, #19.04) in 3D, thus helping in precising the understanding of both dynamics and chemistry in the deep atmopshere of Venus. This work has been funded by the CNES space agency.

  11. Coupled Sulfur and Chlorine Chemistry in Venus' Upper Cloud Layer

    NASA Astrophysics Data System (ADS)

    Mills, Franklin P.

    2006-09-01

    Venus' atmosphere likely contains a rich variety of sulfur and chlorine compounds because HCl, SO2, and OCS have all been observed. Photodissociation of CO2 and SO2 in the upper cloud layer produces oxygen which can react directly or indirectly with SO2 to form SO3 and eventually H2SO4. Photodissociation of HCl within and above the upper cloud layer produces chlorine which can react with CO and O2 to form ClCO and ClC(O)OO. These two species have been identified as potentially critical intermediaries in the production of CO2. Much less work has been done on the potential coupling between sulfur and chlorine chemistry that may occur within the upper cloud layer. Several aspects have been examined in recent modeling: (1) linkage of the CO2 and sulfur oxidation cycles (based on ideas from Yung and DeMore, 1982), (2) reaction of Cl with SO2 to form ClSO2 (based on ideas from DeMore et al., 1985), and (3) the chemistry of SmCln for m,n = 1,2 (based on preliminary work in Mills, 1998). Initial results suggest the chemistry of SmCln may provide a pathway for accelerated production of polysulfur, Sx, if the oxygen abundance in the upper cloud layer is as small as is implied by the observational limit on O2 (Trauger and Lunine, 1983). Initial results also suggest that ClSO2 can act as a buffer which helps increase the scale height of SO2 and decrease the rate of production of H2SO4. This presentation will describe the results from this modeling; discuss their potential implications for the CO2, sulfur oxidation, and polysulfur cycles; and outline key observations from Venus Express that can help resolve existing questions concerning the chemistry of Venus' upper cloud. Partial funding for this research was provided by the Australian Research Council.

  12. A Theoretical Model of the Photolysis of Nitrous Oxide Isotopomers and Isotopologues

    NASA Astrophysics Data System (ADS)

    Johnson, M. S.; Feilberg, K. L.; von Hessberg, P.; Billing, G. D.; Janssen, M. H.

    2002-05-01

    Nitrous oxide (N2O) plays an important role in radiative forcing and ozone depletion. Yung and Miller's zero point energy (ZPE) model for the photolysis of N2O was able to explain atmospheric isotopomer distributions without invoking in situ chemical sources. Unexpectedly, subsequent experiments showed enrichment factors greater than predicted by the ZPE model. We have calculated the UV spectrum of the key N2O isotopomers and isotopologues to quantify the influence of factors not included in the ZPE model, namely the transition dipole surface, bending vibrational excitation, dynamics on the excited state potential surface, and factors related to isotopic substitution itself. The relative cross-sections are calculated as the Fourier transform of the correlation function of the initial vibrational wavefunction and the time-propagated wavefunction, using a Hermite expansion of the time evolution operator. The model makes several predictions. (1) The absolute values of the enrichment factors decrease with increasing temperature. (2) Photolysis of N2O will produce 'mass independent' enrichment in the remaining sample. (3) Much of the enrichment is due to decreased heavy isotopomer cross section over the entire absorption band, in contrast to the wavelength shift predicted by the ZPE model. Consequently to within the error of the calculation we predict only minor enrichments at wavelengths less than 182 nm. The smaller bending excursion of heavy isotopomers combines with the transition dipole surface to produce a smaller integrated cross section. This effect is partially countered by the larger fraction of heavy isotopomers in excited bending states; the first three bending states have an integrated intensity ratio of ca. 1:3:6. The model agrees with experimental enrichment factors and stratospheric enrichment data to within the estimated error.

  13. Isotopic Fractionation of Atmospheric Nitrous Oxide

    NASA Astrophysics Data System (ADS)

    Morgan, C. G.; Yung, Y. L.; Allen, M. A.; Blake, G. A.; Liang, N. C.

    2002-05-01

    Nitrous oxide (N2O) is an important greenhouse gas in the Earth's atmosphere, with both natural and anthropogenic sources. Much effort has been made in using isotopic signatures as a way to constrain the magnitudes of the various sources of N2O. A necessary part of this task is to understand what effect the atmosphere, which is the major sink of N2O, has on these isotopic signatures. Using a two-dimensional (2-D) chemical transport model, we investigated the isotopic fractionation of N2O in the Earth's atmosphere, and we compared the results of our model with laboratory experiments and atmospheric observations. Isotopic fractionation of N2O can occur through photolytic destruction and through a reaction with singlet oxygen. We used three different methods of calculating photolytic cross-sections for each of the major isotopomers of N2O. We found that although the Yung and Miller approach (Science, 278, 1778 (1997)), which postulates that changes in the zero point energies between the isotopomers causes shifts in their respective absorption profiles, can model the pattern of enrichment factors for each isotopomer relative to each other, this approach underestimates the magnitude of the enrichment factors. The ab initio approach by Johnson et al. (JPCA, 105, 8672 (2001)) provided a better fit to the magnitudes of the enrichment factors, with the notable exception of the 15N14N16O isotopomer. A simpler, semi-empirical approach by Blake et al. (2002, in preparation) was able to model the magnitude of all the enrichment factors, including the one for the 15N14N16O isotopomer. We also explored the contributions and effects that the singlet oxygen reaction, climatology and transport have on atmospheric isotopic fractionation.

  14. [From influence to confluence : positioning the history of pre-modern Korean medicine in East Asia].

    PubMed

    Suh, Soyoung

    2010-12-31

    This article surveys studies focusing on pre-modern Korean medicine, which are both written in English and analyzed primary sources up to 1876. Overall, the history of pre-modern Korean medicine is an unknown filed in Anglophone academia. Yung Sik Kim's, James Palais's, and Carter Ecart's problematization of the nationalist framework of Korean scholarship partially explains the marginality of the field. Addressing these criticisms, this review argues that pre-modern Korean medicine's uneasy task lies in both elaborating Korea's own experience of medicine, while simultaneously avoiding making the "Korean" category itself essential. Korean narratives of premodern medicine need to go beyond the mere territorilalization of Korean medicine against its Chinese, Japanese, or Western counterparts, thereby to tackle the field's own boundary of research objects. The existing scholarship in English responds to this challenge by primarily examining the way in which Korea has shared textual tradition with China. Sirhak scholars' innovation in medicine, visual representation of Tongŭi bogam, Korean management of epidemics in the eleventh century, and Korean indexing of local botanicals, engages not only native achievements, but also the process of modifying medicine across geographical and political boundaries. More to the point, the emerging native narratives, although written in Korean, are implicitly resonant with those currently present in Anglophone academia. Taking "tension," "intertextuality," and "local traits" as a lens, this article assesses a series of current research in Korea. Aiming to go beyond appeals for a "distinctively" Korean experience of medicine, the future study of Korean pre-modern medicine will further elucidate confluences of different flows, such as "Chinese and Korean," "universal and local," "center and periphery," and "native and foreign," which will eventually articulate a range of Korean techniques of creating a bricolage in medicine. PMID

  15. WE-G-18A-07: Clinical Evaluation of Normalized Metal Artifact Reduction in KVCT Using MVCT Prior Images (MVCT-NMAR) Technique in Radiotherapy

    SciTech Connect

    Paudel, M; MacKenzie, M; Fallone, B; Rathee, S

    2014-06-15

    Purpose: To evaluate the metal artifacts in diagnostic kVCT images of patients that are corrected using a normalized metal artifact reduction method with MVCT prior images, MVCT-NMAR. Methods: An MVCTNMAR algorithm was developed and applied to five patients: three with bilateral hip prostheses, one with unilateral hip prosthesis and one with dental fillings. The corrected images were evaluated for visualization of tissue structures and their interfaces, and for radiotherapy dose calculations. They were also compared against the corresponding images corrected by a commercial metal artifact reduction technique, O-MAR, on a Phillips™ CT scanner. Results: The use of MVCT images for correcting kVCT images in the MVCT-NMAR technique greatly reduces metal artifacts, avoids secondary artifacts, and makes patient images more useful for correct dose calculation in radiotherapy. These improvements are significant over the commercial correction method, provided the MVCT and kVCT images are correctly registered. The remaining and the secondary artifacts (soft tissue blurring, eroded bones, false bones or air pockets, CT number cupping within the metal) present in O-MAR corrected images are removed in the MVCT-NMAR corrected images. Large dose reduction is possible outside the planning target volume (e.g., 59.2 Gy in comparison to 52.5 Gy in pubic bone) when these MVCT-NMAR corrected images are used in TomoTherapy™ treatment plans, as the corrected images no longer require directional blocks for prostate plans in order to avoid the image artifact regions. Conclusion: The use of MVCT-NMAR corrected images in radiotherapy treatment planning could improve the treatment plan quality for cancer patients with metallic implants. Moti Raj Paudel is supported by the Vanier Canada Graduate Scholarship, the Endowed Graduate Scholarship in Oncology and the Dissertation Fellowship at the University of Alberta. The authors acknowledge the CIHR operating grant number MOP 53254.

  16. Potential Impact of the National Plan for Future Electric Power Supply on Air Quality in Korea

    NASA Astrophysics Data System (ADS)

    Shim, C.; Hong, J.

    2014-12-01

    Korean Ministry of Trade, Industry and Energy (MOTIE) announced the national plan for Korea's future electric power supply (2013 - 2027) in 2013. According to the plan, the national demand for electricity will be increased by 60% compared to that of 2010 and primary energy sources for electric generation will still lean on the fossil fuels such as petroleum, LNG, and coal, which would be a potential threat to air quality of Korea. This study focused on two subjects: (1) How the spatial distribution of the primary air pollutant's emissions (i.e., NOx, SOx, CO, PM) will be changed and (2) How the primary emission changes will influence on the national ambient air quality including ozone in 2027. We used GEOS-Chem model simulation with modification of Korean emissions inventory (Clean Air Policy Support System (CAPSS)) to simulate the current and future air quality in Korea. The national total emissions of CO, NOx, SOx, PM in year 2027 will be increased by 3%, 8%, 13%, 2%, respectively compared to 2010 and there are additional concern that the future location of the power plants will be closer to the Seoul Metropolitan Area (SMA), where there are approximately 20 million population vulnerable to the potentially worsened air quality. While there are slight increase of concentration of CO, NOx, SOx, and PM in 2027, the O3 concentration is expected to be similar to the level of 2010. Those results may imply the characteristics of air pollution in East Asia such as potentially severe O3 titration and poorer O3/CO or O3/NOx ratio. Furthermore, we will discuss on the impact of transboundary pollution transport from China in the future, which is one of the large factors to control the air quality of Korea.

  17. Geotechnical and rheological characteristics of waste materials taken from abandoned mine deposit

    NASA Astrophysics Data System (ADS)

    Jeong, Sueng-Won; Ji, Sang Woo; Fukuoka, Hiroshi

    2014-05-01

    According to the Ministry of Trade, Industry & Energy in Korean (MOTIE), approximately 5,000 metal mines are spread in the Republic of Korea, but almost 80% mines are still left without any proper remediation and cleanup. The physic-chemical properties of waste materials in the mountainous area are strongly affected by heavy rainfall. Failed sediments pose the largest threat to the mountain communities and environments. In particular, a significant amount of heavy metals, such as arsenic, cadmium, copper, zinc, lead etc., is introduced to soil systems. This study examined the geotechnical and rheological characteristics of waste rock materials collected from mine deposits, located in Imgi-ri, Busan Metropolitan City, Korea. We used a ring shear apparatus for geotechnical properties and a rheometer for rheological properties. The materials collected from mines are classified as gravelly sand soils. A series of drained and undrained ring shear tests were performed to examine the stress characteristics with regard to (i) shearing time dependency, (ii) shear speed dependency, and (iii) normal stress dependency. In addition, the grain crushing in the shear zone was examined to explain a high mobile failed masses. This work is also concerned with post-failure characteristics of rainfall-induced debris flows. From the rheological tests, the materials examined exhibited the shear-thinning behavior, which is the viscosity decreases with increasing shear rates. In the relationship between shear stress and shear rate, one of simplest rheological models, i.e., the ideal Bingham fluid model, is selected to examine the debris flow potential. There are positive relationships between the volumetric concentration of sediment ranging from 50% to 65% and rheological values (i.e., yield stress and viscosities). However, the difference in rheological parameters is of significance for given shear rates. The effect of wall-slip in different geometries between ball and vane

  18. SU-E-J-217: Accuracy Comparison Between Surface and Volumetric Registrations for Patient Setup of Head and Neck Radiation Therapy

    SciTech Connect

    Kim, Y; Li, R; Na, Y; Jenkins, C; Xing, L; Lee, R

    2014-06-01

    Purpose: Optical surface imaging has been applied to radiation therapy patient setup. This study aims to investigate the accuracy of the surface registration of the optical surface imaging compared with that of the conventional method of volumetric registration for patient setup in head and neck radiation therapy. Methods: Clinical datasets of planning CT and treatment Cone Beam CT (CBCT) were used to compare the surface and volumetric registrations in radiation therapy patient setup. The Iterative Closest Points based on point-plane closest method was implemented for surface registration. We employed 3D Slicer for rigid volumetric registration of planning CT and treatment CBCT. 6 parameters of registration results (3 rotations and 3 translations) were obtained by the two registration methods, and the results were compared. Digital simulation tests in ideal cases were also performed to validate each registration method. Results: Digital simulation tests showed that both of the registration methods were accurate and robust enough to compare the registration results. In experiments with the actual clinical data, the results showed considerable deviation between the surface and volumetric registrations. The average root mean squared translational error was 2.7 mm and the maximum translational error was 5.2 mm. Conclusion: The deviation between the surface and volumetric registrations was considerable. Special caution should be taken in using an optical surface imaging. To ensure the accuracy of optical surface imaging in radiation therapy patient setup, additional measures are required. This research was supported in part by the KIST institutional program (2E24551), the Industrial Strategic technology development program (10035495) funded by the Ministry of Trade, Industry and Energy (MOTIE, KOREA), and the Radiation Safety Research Programs (1305033) through the Nuclear Safety and Security Commission, and the NIH (R01EB016777)

  19. Diverse interface effects on ferroelectricity and magnetoelectric coupling in asymmetric multiferroic tunnel junctions: the role of the interfacial bonding structure.

    PubMed

    Liu, X T; Chen, W J; Jiang, G L; Wang, B; Zheng, Yue

    2016-01-28

    Interface and size effects on electric/magnetic orders and magnetoelectric coupling are vital in the modern application of quantum-size functional devices based on multiferroic tunnel junctions. In order to give a comprehensive study of the interface and size effects, the properties of a typical asymmetric multiferroic tunnel junction, i.e., Fe/BaTiO3/Co, have been calculated using the first-principles simulations. Most importantly, all of the eight possible structures with four combinations of electrode/ferroelectric interfaces (i.e., Fe/BaO, Fe/TiO2, Co/BaO and Co/TiO2) and a series of barrier thicknesses have been taken into account. In this work, the equilibrium configurations, polarization, charge density, spin density and magnetic moments, etc., have been completely simulated and comprehensively analyzed. It is found that the ferroelectric stability is determined as a competition outcome of the strength of short-range chemical bondings and long-range depolarization/built-in fields. M/BaO (M = magnetic metal) terminations show an extraordinary enhancement of local polarization near the interface and increase the critical thickness of ferroelectricity. The bistability of polarization is well kept at the M/TiO2 interface. At the same time, the induced magnetic moment on atoms at the interfaces is rather localized and dominated by the local interfacial configuration. Reversing electric polarization can switch the induced magnetic moments, wherein atoms in M-O-Ti and M-Ti-O chains show preference for being magnetized. In addition, the difference between the sum of the interfacial magnetic moments is also enlarged with the increase of the barrier thickness. Our study provides a comprehensive and detailed reference to the manipulation and utilization of the interface, size and magnetoelectric effects in asymmetric multiferroic tunnel junctions. PMID:26732894

  20. Stable and very sensitive gas sensor based on novel mixed-metal oxides

    NASA Astrophysics Data System (ADS)

    Comini, Elisabetta; Faglia, Guido; Sberveglieri, Giorgio

    2004-03-01

    The material properties of the nano-structured materials show remarkable improvement or deviation from the properties exhibited by the coarser grained material. These unique properties are attributed to the significant increase in grain boundary area due to the small grain size. The possibility to manipulate the properties of a nanosized thin film simply through annealing appears to be of widespread interest for material science. In the gas sensing field of application there is a great effort in reducing the grain dimension and increasing the surface area exposed to the interaction with gaseous species. One of the strategies used is the addition of a second element, which can inhibit the grain growth. Furthermore, there may be a coexistence of two phases and one phase can act as a receptor while the other can act as transducers and an effect on film porosity is also expected, depending on the extent of oxide segregation from the nanosized film. Thin films made of Mo-Ti, Mo-W, Ti-W, Ti-Nb mixed oxides were achieved by reactive sputtering, assisted by thermal treatments. These layers were characterized by means of the electrical measurements in presence of different pollutants and alcohols and with the Kelvin probe at different working temperatures; the good sensing capabilities registered with these mixed oxide compared to their single oxides have to be ascribed to the nanosized structure of these layers. In particular different p-type sensing materials were produced, the opposite behavior of these layer is attractive to ease data processing in sensors arrays.

  1. The new large-area wide-angle ground-based cosmic-ray and gamma-ray detector SCORE

    NASA Astrophysics Data System (ADS)

    Tluczykont, Martin; Hampf, Daniel; Horns, Dieter; Kneiske, Tanja; Rowell, Gavin

    We propose to explore the so-far poorly measured cosmic-ray and gamma-ray sky (accelerator sky) in the energy range from 10 TeV to 1 EeV with the new large-area (10 square-km) wide-angle (1 sr) air Cherenkov detector SCORE (Study for a Cosmic ORigin Explorer). The SCORE detector concept is based on non-imaging Cherenkov light-front sampling with sensitive large-area (order of square-m) detector modules, distributed over an array covering a total area of at least 10 square-kilometers. The lateral intensity and arrival-time distribu-tions will be sampled with high sensitivity up to large distances from the shower core. An extension of the SCORE detector to HiSCORE (Hundred Square-km Cosmic ORigin Explorer) is planned. With SCORE (and HiSCORE) fundamental physics questions can be addressed, including the origin of charged Galactic cosmic rays, diffuse gamma-ray emission from the Galactic plane and the local super-cluster, attenuation by Galactic interstellar radiaton fields and the cosmic microwave background and studies of possible effects on this attenuation by photon/axion conversion, hidden-sector photon oscillations or violation of Lorentz invariance. Further motivations are spectral and chemical composition measurements of charged cosmic rays from 100 TeV to 1 EeV and independent measurements of the proton-proton inelastic cross-section overlapping with and exceeding LHC energies. First simulations show that already SCORE has the potential to be competitive with existing and planned experiments above 10 TeV and outperforming above 100 TeV. The physics moti-vations, the detector concept / performance expectations and the status of our project will be presented.

  2. Corrosion resistance of weldable super 13Cr stainless steel in H{sub 2}S containing CO{sub 2} environments

    SciTech Connect

    Ueda, M.; Amaya, H.; Kondo, K.; Ogawa, K.; Mori, T.

    1996-08-01

    The weldable super 13Cr stainless steel was investigated because of the application for flow line in CO{sub 2} environments with a little amount of H{sub 2}S. TIG welding in the condition of no post weld heat treatment (PWHT) was used as the welding technique. The lowering of C content less than 0.01 mass% in the weldable steel decreased a maximum hardness in the heat-affected zone(HAZ) and mitigated the sulfide stress cracking (SSC) susceptibility. The increasing of Mo content from 2.0 mass% of the super 13Cr stainless steel OCTG (0.02C-12Cr-5.5Ni-2Mo) to 2.5 mass% improved SSC resistance in the HAZ. Based on these results, the weldable super 13Cr stainless steel, which consisted of 0.007C-12Cr-6Ni-2.5Mo-Ti, has been developed. The welded-joint with the yield strength of 550 MPa (80 ksi) and enough corrosion resistance was completed by using the welding material of super duplex stainless steel which had 25Cr-9Ni-3Mo-2W-0.3N. The corrosion resistance to SSC at room temperatures and localized-corrosion at elevated temperatures of the welded-joint was the same as the super 13Cr stainless steel OCTG. The improvement effect of the corrosion resistance by means of Mo addition was discussed based on the stability of Cr oxide passive film, the analysis results of the surface film formed in the CO{sub 2} environment containing H{sub 2}S, and calculated-solubility of oxides, FeCO{sub 3} and sulfides in that environment. It was clarified that Mo assisted the formation of the Cr oxide passive film in the inner layer of the surface film and the formation of Mo sulfide in the outer layer.

  3. Continuous-flow IRMS technique for determination of Δ17O in (stratospheric) CO2 using complete oxygen isotope exchange with cerium oxide

    NASA Astrophysics Data System (ADS)

    Mrozek, D. J.; Roeckmann, T.

    2012-12-01

    Isotope studies of carbon dioxide (CO2) play an important role in understanding of the global carbon cycle. Stratospheric CO2 is known to undergo an isotopic exchange reaction with ozone (Yung et all 1991). Therefore, stratosphere CO2 shows a mass independent fractionation (MIF) which is a deviation in the 17O content from a purely mass-dependent pattern (MDF): for MDF processes δ17O = 0.52 δ18O, for MIF phenomena Δ17O = δ17O - 0.52 δ18O ≠ 0. The detailled mechanism that controls the 17O anomalies in stratospheric CO2 is not fully understood. Interest in this field has caused innovations in analytical techniques based on Isotope Ratio Mass Spectrometry (IRMS). Our approach was to design an analytical system that allows analysis of δ17O on nanomolar quantities of CO2 suitable for measuring oxygen isotope anomalies in stratospheric air samples. Based on complete oxygen isotope exchange with CeO2 at 650°C (Assonov et al. 2001) we have established an online measurement system for δ17O in CO2. Due to isotopic equilibration with CeO2 the CO2 samples loose their mass independent fractionation information and from the difference between the exchanged and non-exchanged sample Δ17O in the original CO2 can be calculated. The technique is fast and efficient due to its fully automation. A single measurement takes 15 minutes and 2 ml of air (plus flushing of the lines). Analytical precision can be improved by performing multiple measurements on one sample, and the analytical precision for a package of ten measurements is 0.7 ‰ for Δ17O. The new technique is a valuable tool to study the isotopic exchange mechanism between O3 and CO2 in the stratosphere. As a first application, we have determined the isotopic composition of stratospheric CO2 on air samples obtained during the EU project RECONCILE in the Arctic winter/spring season with the high-altitude aircraft Geophysica.

  4. IUSSP activities. Committee on Historical Demography. Report: Conference on Asian Population History, Taipei, Taiwan, 4-8 January 1996.

    PubMed

    Osirike, A B

    1996-05-01

    This article presents an overview of the Asian Population History Conference held in Taipei, Taiwan, January 4-8, 1996. 41 papers were presented on seven themes: Asian population growth, epidemiological transition and public health, mortality trends in pretransitional populations, marriage patterns and demographic systems, fertility levels and trends in pretransitional Asian populations, migration and population distribution, and family systems. Papers were presented by Anthony Reid; Chris Wilson; Bruce Fetter; Sumit Guha; Sheila Zurbrigg; Timothy Dyson and Monica Das Gupta; Cameron Campbell; Robert Shepherd; Ann Jannetta; Chai-Bin Park, Eise Yokoyama, and Sadahiko Nozaki; Peter Boomgaard; Jose Antonio Ortega Osona; Osamu Saito; Ts'ui-jung Liu and Shi-yung Liu; Wen Shang Yang; Dallas Fernando; Bruce Caldwell; A. Francis Gealogo; S. Irudaya Rajan; Kiyoshi Hamano; Guo Songyi; Wang Feng and James Lee; Christopher Langford; Terence H. Hull; Paul K.C. Liu; Xizhe Peng and Yangfang Hou; Ken'ichi Tomobe; Nokiro O. Tsuya; Peter Xenos; Daniel Doeppers; Chaonan Chen and Su-fen Liu; Jiang Tao; Akira Hayami and Emiko Ochiai; Arthur P. Wolf and Chuang Ying-chang; Myron L. Cohen; Burton Pasternak; Zhongwei Zhao; Li-shou Yang, Arland Thornton, and Tamara Hareven; Chi-chun Yi and Yu-hsia Lu; Lai Huimin; Ding Yizhuang; and John Caldwell, who chaired the concluding session. John Caldwell concluded that the conference provided an impressive collection of findings on Asian population history. There was much more research possible, particularly research based on India's rich historical data archives. Research was needed to confirm the assertion that Asian mortality transition began after the two world wars. A focus on natural family planning methods used prior to the transition was suggested. International Union for Scientific Study of Population Committee Chairman David Reher suggested multidisciplinary research on Asian differences in fertility, mortality, and migration. Hayami and Ts

  5. NOTE: On the Deuterium Abundance on Mars and Some Related Problems

    NASA Astrophysics Data System (ADS)

    Krasnopolsky, Vladimir

    2000-12-01

    Strong fractionation of deuterium in photolysis of H 2O and above the hygropause reduces the production of HD relative to H 2 on Mars by a factor of 3.7 total. The model by Y. L. Yung et al. (1988, Icarus76, 146-159) for deuterium fractionation in chemical reactions on Mars corrected for this factor results in (HD/H 2)/(HDO/H 2O)=0.43. This value may fit the deuterium abundance observed by V. A. Krasnopolsky et al. (1998, Science 280, 1576-1580) if the eddy diffusion coefficient does not depend on solar activity: K=1.4×10 13n-1/2 cm 2 s -1 (model 2). The Mariner 9 observations show very low variability of atomic oxygen at the 1.2 n bar pressure level (h˜125 km) with solar activity. This requires eddy diffusion to be proportional to the solar activity index F10.7: K=( F10.7 cm/30)×10 13n-1/2 cm 2 s -1 (model 1). The fractionation factor for escape of hydrogen isotopes is equal to 0.016 and 0.135 for models 1 and 2. These values have been averaged over the solar cycle. The three-reservoir model for hydrogen isotope fractionation suggested by Krasnopolsky et al. (1998) involves a reservoir composed primarily of water ice in the polar caps that isotopically interacts with the atmosphere. Assuming that water ice is half of the total volume of the polar caps and the polar-layered deposits, the total loss of water from Mars is equal to 65 and 120 m for models 1 and 2, respectively. Along with thermal and nonthermal escape, these values may include the loss of water by oxidation of regolith, if the released hydrogen escaped with isotopic fractionation. Although the solar-wind α particles are the main source of He on Mars, capture of the solar-wind H + and D + ions by Mars has a negligible effect on the thermospheric abundances of H and D. Improved observations of minor components in Mars' thermosphere may resolve the problem of eddy diffusion at various solar activity and choosing between the models.

  6. Inhibition of Janus kinase signaling during controlled mechanical ventilation prevents ventilation-induced diaphragm dysfunction

    PubMed Central

    Smith, Ira J.; Godinez, Guillermo L.; Singh, Baljit K.; McCaughey, Kelly M.; Alcantara, Raniel R.; Gururaja, Tarikere; Ho, Melissa S.; Nguyen, Henry N.; Friera, Annabelle M.; White, Kathy A.; McLaughlin, John R.; Hansen, Derek; Romero, Jason M.; Baltgalvis, Kristen A.; Claypool, Mark D.; Li, Wei; Lang, Wayne; Yam, George C.; Gelman, Marina S.; Ding, Rongxian; Yung, Stephanie L.; Creger, Daniel P.; Chen, Yan; Singh, Rajinder; Smuder, Ashley J.; Wiggs, Michael P.; Kwon, Oh-Sung; Sollanek, Kurt J.; Powers, Scott K.; Masuda, Esteban S.; Taylor, Vanessa C.; Payan, Donald G.; Kinoshita, Taisei; Kinsella, Todd M.

    2014-01-01

    Controlled mechanical ventilation (CMV) is associated with the development of diaphragm atrophy and contractile dysfunction, and respiratory muscle weakness is thought to contribute significantly to delayed weaning of patients. Therefore, therapeutic strategies for preventing these processes may have clinical benefit. The aim of the current study was to investigate the role of the Janus kinase (JAK)/signal transducer and activator of transcription 3 (STAT3) signaling pathway in CMV-mediated diaphragm wasting and weakness in rats. CMV-induced diaphragm atrophy and contractile dysfunction coincided with marked increases in STAT3 phosphorylation on both tyrosine 705 (Tyr705) and serine 727 (Ser727). STAT3 activation was accompanied by its translocation into mitochondria within diaphragm muscle and mitochondrial dysfunction. Inhibition of JAK signaling during CMV prevented phosphorylation of both target sites on STAT3, eliminated the accumulation of phosphorylated STAT3 within the mitochondria, and reversed the pathologic alterations in mitochondrial function, reduced oxidative stress in the diaphragm, and maintained normal diaphragm contractility. In addition, JAK inhibition during CMV blunted the activation of key proteolytic pathways in the diaphragm, as well as diaphragm atrophy. These findings implicate JAK/STAT3 signaling in the development of diaphragm muscle atrophy and dysfunction during CMV and suggest that the delayed extubation times associated with CMV can be prevented by inhibition of Janus kinase signaling.—Smith, I. J., Godinez, G. L., Singh, B. K., McCaughey, K. M., Alcantara, R. R., Gururaja, T., Ho, M. S., Nguyen, H. N., Friera, A. M., White, K. A., McLaughlin, J. R., Hansen, D., Romero, J. M., Baltgalvis, K. A., Claypool, M. D., Li, W., Lang, W., Yam, G. C., Gelman, M. S., Ding, R., Yung, S. L., Creger, D. P., Chen, Y., Singh, R., Smuder, A. J., Wiggs, M. P., Kwon, O.-S., Sollanek, K. J., Powers, S. K., Masuda, E. S., Taylor, V. C., Payan, D. G

  7. A model for the chemical deposition of minerals in an evaporation basin on early Mars

    NASA Astrophysics Data System (ADS)

    Catling, David C.

    1998-09-01

    Mars, Oxford University Press. [2] J. B. Pollack et al. (1987) Icarus, 71, 203-224. [3] J. F. Kasting (1991), Icarus, 94, 1-13. [4] F. Forget and R. T. Pierrehumbert (1997) Science, 278, 1273. [5] Y. L. Yung et al. (1997) Icarus, 136, 222-224. [6] R. D. Forsythe and J. R. Zimbelman (1995) J. Geophys. Res., 100, 5553-5563. [7] D. C. Catling (1998), LPSC XXIX, 1568-1569. [8] J. C. Bridges and M. M. Grady (1998) LPSC XXIX, 1399-1400. [9] P. H. Warren (1998) J. Geophys. Res., 103, 16759-16773. [10] D. Anderson et al. (1998) Antarctic Science, 10, 124-133.

  8. The sensitivity of Titan's current atmosphere to variations in solar EUV flux and implications for the evolution of the atmosphere

    NASA Astrophysics Data System (ADS)

    Mandt, K.; Bell, J. M.; Waite, J. H.

    2010-12-01

    K. E. Mandt, J. Bell, J. H. Waite, Jr. Southwest Research Institute, San Antonio, TX Stable isotope ratios are an important tool for tracing the evolution of an atmosphere. By carefully evaluating processes that fractionate the isotopes (e.g. escape and photochemistry), the inventory of a constituent can be tracked over geological time scales. For Saturn’s largest moon, Titan, the 14N/15N in N2 and the 12C/13C in CH4 can be used to constrain the initial size of the atmosphere and the amount of time that has passed since the current inventory of methane began outgassing into the atmosphere (see Lunine et al. [1999] and Mandt et al. [2009]). Because the processes that fractionate the isotopes are directly tied to the amount of solar EUV/UV energy deposited in the upper atmosphere, it is important to understand the sensitivity of the atmosphere to varying solar EUV flux. On short time scales, the EUV flux can vary by as much as a factor of two during the eleven-year solar cycle. On geologic time scales, the solar EUV flux is believed to have been about 2.5 times greater than the current flux about 2.5 billion years ago, and 6 times the current flux 3.5 billion years ago [Ribas et al. 2005]. Using a 1D version of the 3D Titan Global Ionosphere-Thermosphere Model (T-GITM), we will explore the impact of the eleven-year solar cycle variations on Titan’s upper atmosphere, focusing on the key fractionating processes of photochemistry and escape. We will then discuss the implications of these results for modeling the evolution of the atmosphere over geological time scales. Lunine, J. I., Y. L. Yung and R. D. Lorenz, 1999. On the volatile inventory of Titan from isotopic abundances in nitrogen and methane. Planetary and Space Science, 47, 1291-1303. Mandt, K. E., J. H. Waite, Jr., B. A. Magee, J. Bell, J. Lunine, O. Mousis, D. Cordier, 2009, Isotopic evolution of Titan’s main atmospheric constituents, Planetary and Space Science, 57, 1917-1930. Ribas, I., E. F. Guinan

  9. Evolutionary implications of a steady-state water abundance on Venus

    NASA Technical Reports Server (NTRS)

    Grinspoon, David H.

    1993-01-01

    In 1987, Grinspoon proposed that the data on hydrogen abundance, isotopic composition, and escape rate were consistent with the hypothesis that water on Venus might be in steady-state rather than monotonic decline since the dawn of time. This conclusion was partially based on a derived water lifetime against nonthermal escape of approximately 10(exp 8) years. Others have questioned this conclusion. De Bergh et al. found H2O lifetimes of greater than 10(exp 9) years. Donahue and Hodges derived H2O lifetimes of 0.4 - 5 x 10(exp 9) years. The most sophisticated analysis to date of near-IR radiation from Venus' nightside reveals a water mixing ratio of approximately 30 ppm. Recent re-analysis of Pioneer Venus Mass Spectrometer Data are consistent with a water abundance of 30 ppm. Hodges and Tinsley found an escape flux due to charge exchange with hot H(+) of 2.8 x 10(exp 7) cm(exp -2) s(exp -1). Gurwell and Yung estimated an escape flux of 3.5 x 10(exp 6) cm(exp -2) s(exp -1) from collisions with hot O produced by dissociative recombination of O2(+). Brace et al. estimated an escape flux of 5 x 10(exp 6) cm(exp -2) s(exp -1) from ion escape from the ionotail of Venus. The combined estimated escape flux from all of these processes is 3.7 x 10(exp 7) cm(exp -2) s(exp -1), suggesting a lifetime against escape for water of less than 10(exp 8) years. A recent estimate of H escape flux employing a different ionospheric model and using Pioneer Venus reentry data to estimate the response of the escape flux to the solar cycle finds a somewhat lower escape flux of 1.4 x 10(exp 7) cm(exp -2) s(exp -1), suggesting a water lifetime closer to 2 x 10(exp 8) years, significantly less than the age of the planet. Large uncertainties remain in these quantities, yet the data suggest that a source of water more recent than primordial sources is required and that a steady-state is likely. To obvious candidates for this source water are cometary impact and volcanic outgassing. Other aspects

  10. Up-regulation of the mammalian target of rapamycin complex 1 subunit Raptor by aldosterone induces abnormal pulmonary artery smooth muscle cell survival patterns to promote pulmonary arterial hypertension.

    PubMed

    Aghamohammadzadeh, Reza; Zhang, Ying-Yi; Stephens, Thomas E; Arons, Elena; Zaman, Paula; Polach, Kevin J; Matar, Majed; Yung, Lai-Ming; Yu, Paul B; Bowman, Frederick P; Opotowsky, Alexander R; Waxman, Aaron B; Loscalzo, Joseph; Leopold, Jane A; Maron, Bradley A

    2016-07-01

    Activation of the mammalian target of rapamycin complex 1 (mTORC1) subunit Raptor induces cell growth and is a downstream target of Akt. Elevated levels of aldosterone activate Akt, and, in pulmonary arterial hypertension (PAH), correlate with pulmonary arteriole thickening, which suggests that mTORC1 regulation by aldosterone may mediate adverse pulmonary vascular remodeling. We hypothesized that aldosterone-Raptor signaling induces abnormal pulmonary artery smooth muscle cell (PASMC) survival patterns to promote PAH. Remodeled pulmonary arterioles from SU-5416/hypoxia-PAH rats and monocrotaline-PAH rats with hyperaldosteronism expressed increased levels of the Raptor target, p70S6K, which provided a basis for investigating aldosterone-Raptor signaling in human PASMCs. Aldosterone (10(-9) to 10(-7) M) increased Akt/mTOR/Raptor to activate p70S6K and increase proliferation, viability, and apoptosis resistance in PASMCs. In PASMCs transfected with Raptor-small interfering RNA or treated with spironolactone/eplerenone, aldosterone or pulmonary arterial plasma from patients with PAH failed to increase p70S6K activation or to induce cell survival in vitro Optimal inhibition of pulmonary arteriole Raptor was achieved by treatment with Staramine-monomethoxy polyethylene glycol that was formulated with Raptor-small interfering RNA plus spironolactone in vivo, which decreased arteriole muscularization and pulmonary hypertension in 2 experimental animal models of PAH in vivo Up-regulation of mTORC1 by aldosterone is a critical pathobiologic mechanism that controls PASMC survival to promote hypertrophic vascular remodeling and PAH.-Aghamohammadzadeh, R., Zhang, Y.-Y., Stephens, T. E., Arons, E., Zaman, P., Polach, K. J., Matar, M., Yung, L.-M., Yu, P. B., Bowman, F. P., Opotowsky, A. R., Waxman, A. B., Loscalzo, J., Leopold, J. A., Maron, B. A. Up-regulation of the mammalian target of rapamycin complex 1 subunit Raptor by aldosterone induces abnormal pulmonary artery smooth

  11. Variations of carbon monoxide in the martian lower atmosphere

    NASA Astrophysics Data System (ADS)

    Krasnopolsky, Vladimir A.

    2015-06-01

    Our observations of variations of CO on Mars by means of the ground-based spatially-resolved high-resolution spectroscopy (Krasnopolsky, V.A. [2003]. J. Geophys. Res. 108(E2), 5010; Krasnopolsky, V.A. [2007]. Icarus 190, 93-102) have been significantly improved using the 13CO lines near 4148 cm-1 and the CO2 lines near 4570 cm-1. These lines are of optimal strength, of low sensitivity to variations of temperature, and covered by the ATMOS solar spectrum that makes it possible to use the synthetic spectra technique for retrieval of CO and CO2 to get CO mixing ratios. The CO2 line strengths from Toth et al. (2008) were also essential to improve accuracy of the results. The 13CO/CO ratio of 1.023 times the terrestrial carbon isotope ratio was calculated using the known 13CO2/CO2 = 1.046 in the martian atmosphere (Webster, C.R., et al. [2013]. Science 341, 260-263), the photo-induced isotope fractionation (Miller, C.E., Yung, Y.L. [2000]. J. Geophys. Res. 105(D23), 29039-29051) in the CO2 photolysis, and isotope fractionation in the reaction between CO and OH (Feilberg, K.L., Johnson, M.S., Nielsen, C.J. [2005]. Phys. Chem. Chem. Phys. 7, 2318-2323). The observations were conducted at LS = 60°, 89°, 110°, and 145° and extend over the maximum of CO in the southern hemisphere during the northern summer. The CO mixing ratio was observed to be constant over the 55°S-90°N latitudinal range to within 7%, for each observed LS period. Therefore our observations show that the enrichment of incondensable gases by condensation of CO2 in the southern polar regions does not significantly extend to the middle and low latitudes. This behavior agrees with the Mars Climate Database (Lefevre, F., Forget, F. [2009]. Nature 460, 720-722), whereas most other observations exhibit much larger latitudinal gradients and seasonal variations. Our measurements do not show the CO depletion at high northern latitudes predicted by MCD of ∼20% at LS≈ 60-150° and observed as much stronger

  12. Effects of Induced Sputtering on delta (13) C and AR in the Martian Atmosphere

    NASA Astrophysics Data System (ADS)

    Kass, D. M.; Yung, Y. L.

    1996-09-01

    Given the possibility of life having developed on Mars, it becomes important to know the environment that it evolved in. There is geomorphological evidence that the ancient climate was wetter and warmer. This environment was presumably created by a dense CO_2 atmosphere, but it leaves the fundamental question of what happened to the atmosphere. One possibility is that the atmosphere escaped to space. The main method for removing CO_2 is indirect sputtering, a process where the solar wind accelerates O(+) to high energies and then has them impact the upper atmosphere, causing them to eject other particles (see Luhmann and Kozyra, { \\sl JGR}, 1991). The primary constraint on sputtering and its effect on the atmosphere is the isotopic signature. We have updated our Monte-Carlo model for sputtering (Kass and Yung, Science, 1995) with improved cross sections (from Johnson and Liu, Science, in press) and a more realistic handling of the dissociation of CO_2. Using our new model, we find that Mars could have lost as much as a bar of CO_2 in the last 3.5 Gyr. This is sufficient CO_2 to allow a warmer and wetter climate to have existed during the early part of Mars' history. While there are large errors associated with the calculation due to uncertainties in modeling the evolution of the Sun, our modeling indicates (unlike Luhmann et al., \\sl JRL, 1992) that sputtering can play a significant role in the evolution of the Martian atmosphere. Using our new model, we considered the effects of the sputtering on the delta (13) C and (36) Ar /(38) Ar ratio of the Martian atmosphere. Using a simple model combining the effects of sputtering, outgassing (taken from Jakosky et al., \\sl Icarus, 1994), carbonate formation (Stephens, Caltech Thesis, 1995) and polar reservoirs, we find that the model predicts values for the two isotopic systems in agreement with the current measurements for Mars. These two systems were chosen both because they are affected by relatively few processes

  13. A physical model of Titan's aerosols.

    PubMed

    Toon, O B; McKay, C P; Griffith, C A; Turco, R P

    1992-01-01

    Microphysical simulations of Titan's stratospheric haze show that aerosol microphysics is linked to organized dynamical processes. The detached haze layer may be a manifestation of 1 cm sec-1 vertical velocities at altitudes above 300 km. The hemispherical asymmetry in the visible albedo may be caused by 0.05 cm sec-1 vertical velocities at altitudes of 150 to 200 km, we predict contrast reversal beyond 0.6 micrometer. Tomasko and Smith's (1982, Icarus 51, 65-95) model, in which a layer of large particles above 220 km altitude is responsible for the high forward scattering observed by Rages and Pollack (1983, Icarus 55, 50-62), is a natural outcome of the detached haze layer being produced by rising motions if aerosol mass production occurs primarily below the detached haze layer. The aerosol's electrical charge is critical for the particle size and optical depth of the haze. The geometric albedo, particularly in the ultraviolet and near infrared, requires that the particle size be near 0.15 micrometer down to altitudes below 100 km, which is consistent with polarization observations (Tomasko and Smith 1982, West and Smith 1991, Icarus 90, 330-333). Above about 400 km and below about 150 km Yung et al.'s (1984, Astrophys. J. Suppl. Ser. 55, 465-506) diffusion coefficients are too small. Dynamical processes control the haze particles below about 150 km. The relatively large eddy diffusion coefficients in the lower stratosphere result in a vertically extensive region with nonuniform mixing ratios of condensable gases, so that most hydrocarbons may condense very near the tropopause rather than tens of kilometers above it. The optical depths of hydrocarbon clouds are probably less than one, requiring that abundant gases such as ethane condense on a subset of the haze particles to create relatively large, rapidly removed particles. The wavelength dependence of the optical radius is calculated for use in analyzing observations of the geometric albedo. The lower

  14. Greenhouse Gases and Gas-Water-Rock Interactions at the Surface of Early Mars

    NASA Astrophysics Data System (ADS)

    Murphy, W. M.; Bass, D. S.

    1998-09-01

    other constraints as a paleo-CO2 barometer for Mars. 1. Pollack et al., 1987 Icarus 71, p. 203-224. 2. Kasting, 1991 Icarus 94, p. 1-13. 3. Yung et al., 1997. Icarus 130, p. 222-224. 4. Gooding et al., 1991. Meteoritics 26, p. 135-143.

  15. SU-E-I-92: Is Photon Starvation Preventing Metal Artifact Reduction Algorithm From Working in KVCT?

    SciTech Connect

    Paudel, M; MacKenzie, M; Fallone, B; Rathee, S

    2014-06-01

    hip implants. Moti Raj Paudel is supported by the Vanier Canada Graduate Scholarship, the Endowed Graduate Scholarship in Oncology and the Dissertation Fellowship at the University of Alberta. The authors acknowledge the CIHR operating grant number MOP 53254.

  16. Strong Local-Nonlocal Coupling for Integrated Fracture Modeling

    SciTech Connect

    Littlewood, David John; Silling, Stewart A.; Mitchell, John A.; Seleson, Pablo D.; Bond, Stephen D.; Parks, Michael L.; Turner, Daniel Z.; Burnett, Damon J.; Ostien, Jakob; Gunzburger, Max

    2015-09-01

    dramatically improved consistency at domain boundaries, and an enhancement to the meshfree discretization applied to peridynamic models that removes irregularities at the limit of the nonlocal length scale and dramatically improves conver- gence behavior. Finally, a novel approach for modeling ductile failure has been developed, moti- vated by the desire to apply coupled local-nonlocal models to a wide variety of materials, including ductile metals, which have received minimal attention in the peridynamic literature. Software im- plementation of the partial-stress coupling strategy, the position-aware peridynamic constitutive models, and the strategies for improving the convergence behavior of peridynamic models was completed within the Peridigm and Albany codes, developed at Sandia National Laboratories and made publicly available under the open-source 3-clause BSD license.

  17. Swell effect correction for the high-resolution marine seismic data acquired using an airgun and an 8-channel streamer cable

    NASA Astrophysics Data System (ADS)

    Lee, Ho-Young; Koo, Nam-Hyung; Kim, Wonsik; Kim, Byoung-yeop; Cheong, Snons; Kim, Young-Jun

    2015-04-01

    Energy Technology Innovation (ETI) Project of the Korea Institute of Energy Technology Evaluation and Planning (KETEP), funded by the Ministry of Trade, Industry and Energy (MOTIE). The authors thank the officers and crew of the R/V Tamhae II for their efforts in the field survey.

  18. SU-E-I-64: Transverse Relaxation Time in Methylene Protons of Non-Alcoholic Fatty Liver Disease Rats

    SciTech Connect

    Song, K-H; Lee, D-W; Choe, B-Y

    2015-06-15

    Purpose: The aim of this study was to evaluate transverse relaxation time of methylene resonance compared to other lipid resonances. Methods: The examinations were performed using a 3.0 T scanner with a point — resolved spectroscopy (PRESS) sequence. Lipid relaxation time in a lipid phantom filled with canola oil was estimated considering repetition time (TR) as 6000 msec and echo time (TE) as 40 — 550 msec. For in vivo proton magnetic resonance spectroscopy ({sup 1}H — MRS), eight male Sprague — Dawley rats were given free access to a normal - chow (NC) and eight other male Sprague-Dawley rats were given free access to a high — fat (HF) diet. Both groups drank water ad libitum. T{sub 2} measurements in the rats’ livers were conducted at a fixed TR of 6000 msec and TE of 40 – 220 msec. Exponential curve fitting quality was calculated through the coefficients of determination (R{sup 2}). Results: A chemical analysis of phantom and liver was not performed but a T{sub 2} decay curve was acquired. The T{sub 2} relaxation time of methylene resonance was estimated as follows: NC rats, 37.07 ± 4.32 msec; HF rats, 31.43 ± 1.81 msec (p < 0.05). The extrapolated M0 values were higher in HF rats than in NC rats (p < 0.005). Conclusion: This study of {sup 1}H-MRS led to sufficient spectral resolution and signal — to — noise ratio differences to characterize all observable resonances for yielding T{sub 2} relaxation times of methylene resonance. {sup 1}H — MRS relaxation times may be useful for quantitative characterization of various liver diseases, including fatty liver disease. This study was supported by grant (2012-007883 and 2014R1A2A1A10050270) from the Mid-career Researcher Program through the NRF funded by Ministry of Science. In addition, this study was supported by the Industrial R&D of MOTIE/KEIT (10048997, Development of the core technology for integrated therapy devices based on real-time MRI-guided tumor tracking)

  19. SU-C-207-01: Four-Dimensional Inverse Geometry Computed Tomography: Concept and Its Validation

    SciTech Connect

    Kim, K; Kim, D; Kim, T; Kang, S; Cho, M; Shin, D; Suh, T

    2015-06-15

    Purpose: In past few years, the inverse geometry computed tomography (IGCT) system has been developed to overcome shortcomings of a conventional computed tomography (CT) system such as scatter problem induced from large detector size and cone-beam artifact. In this study, we intend to present a concept of a four-dimensional (4D) IGCT system that has positive aspects above all with temporal resolution for dynamic studies and reduction of motion artifact. Methods: Contrary to conventional CT system, projection data at a certain angle in IGCT was a group of fractionated narrow cone-beam projection data, projection group (PG), acquired from multi-source array which have extremely short time gap of sequential operation between each of sources. At this, for 4D IGCT imaging, time-related data acquisition parameters were determined by combining multi-source scanning time for collecting one PG with conventional 4D CBCT data acquisition sequence. Over a gantry rotation, acquired PGs from multi-source array were tagged time and angle for 4D image reconstruction. Acquired PGs were sorted into 10 phase and image reconstructions were independently performed at each phase. Image reconstruction algorithm based upon filtered-backprojection was used in this study. Results: The 4D IGCT had uniform image without cone-beam artifact on the contrary to 4D CBCT image. In addition, the 4D IGCT images of each phase had no significant artifact induced from motion compared with 3D CT. Conclusion: The 4D IGCT image seems to give relatively accurate dynamic information of patient anatomy based on the results were more endurable than 3D CT about motion artifact. From this, it will be useful for dynamic study and respiratory-correlated radiation therapy. This work was supported by the Industrial R&D program of MOTIE/KEIT [10048997, Development of the core technology for integrated therapy devices based on real-time MRI guided tumor tracking] and the Mid-career Researcher Program (2014R1A2A1A

  20. Comparison of misfit functions for phase-only inversion in the frequency domain

    NASA Astrophysics Data System (ADS)

    Jeong, G.; Jeong, W.; Min, D. J.

    2014-12-01

    results than the logarithmic and conventional II methods. Acknowledgements This work was supported by the Human Resources Development program (No. 20134010200510) of the KETEP grant funded by the Korean government MOTIE and by the "Development of Technology for CO2 Marine Geological Storage" grant funded by the MOF of Korea.

  1. Presolar Graphite from AGB Stars: Microstructure and s-Process Enrichment

    NASA Astrophysics Data System (ADS)

    Croat, Thomas K.; Stadermann, Frank J.; Bernatowicz, Thomas J.

    2005-10-01

    Correlated transmission electron microscopy and secondary ion mass spectrometry with submicron spatial resolution (NanoSIMS) investigations of the same presolar graphites spherules from the Murchison meteorite were conducted, to link the isotopic anomalies with the mineralogy and chemical composition of the graphite and its internal grains. Refractory carbide grains (especially titanium carbide) are commonly found within the graphite spherules, and most have significant concentrations of Zr, Mo, and Ru in solid solution, elements primarily produced by s-process nucleosynthesis. The effect of chemical fractionation on the Mo/Ti ratio in these carbides is limited, and therefore from this ratio one can infer the degree of s-process enrichment in the gas from which the graphite condensed. The resulting s-process enrichments within carbides are large (~200 times solar on average), showing that most of the carbide-containing graphites formed in the mass outflows of asymptotic giant branch (AGB) stars. NanoSIMS measurements of these graphites also show isotopically light carbon (mostly in the 100<12C/13C<400 range). The enrichment of these presolar graphites in both s-process elements and 12C considerably exceeds that astronomically observed around carbon stars. However, a natural correlation exists between 12C and s-process elements, as both form in the He intershell region of thermally pulsing AGB stars and are dredged up together to the surface. Their observation together suggests that these graphites may have formed in chemically and isotopically inhomogeneous regions around AGB stars, such as high-density knots or jets. As shown in the companion paper, a gas density exceeding that expected for smooth mass outflows is required for graphite of the observed size to condense at all in circumstellar environments, and the spatially inhomogeneous, high-density regions from which they condense may also be incompletely mixed with the surrounding gas. We have greatly expanded

  2. SU-E-I-60: Quality Assurance Testing Methods and Customized Phantom for Magnetic Resonance Imaging and Spectroscopy

    SciTech Connect

    Song, K-H; Lee, D-W; Choe, B-Y

    2015-06-15

    factors simultaneously. This study was supported by grant (2012-007883 and 2014R1A2A1A10050270) from the Mid-career Researcher Program through the NRF funded by Ministry of Science. In addition, this study was supported by the Industrial R&D of MOTIE/KEIT (10048997, Development of the core technology for integrated therapy devices based on real-time MRI-guided tumor tracking)

  3. Oxygen Isotopic Analyses of Water Extracted from the Martian Meteorite NWA 7034

    NASA Astrophysics Data System (ADS)

    Nunn, M.; Agee, C. B.; Thiemens, M. H.

    2012-12-01

    isotopic composition of atmospheric CO2 [5]. This anomaly is transferred by exchange from CO2 to water and subsequently to secondary minerals. The much larger CO2 to water ratio on Mars could allow this process to introduce a measurable oxygen isotopic anomaly to sulfates, carbonates, and water. The magnitude and variability of this anomaly would depend on the formation mechanism of the species (particularly the source of oxygen), as is consistent with measurements to date of phases in SNCs. References: [1] Franchi, I.A., et al. (1999) MAPS 34, 657-661. [2] Rumble, D. and Irving, A.J. (2009) LPSC XXXX, #2293 [3] Karlsson, H.R., et al. (1992) Science 255, 1409-1411. [4] Farquhar, J. and Thiemens, M.H. (2000) J. Geophys. Res. 105, 11991-11997. [5] Yung, Y.L., et al. (1991) Geophys. Res. Lett. 18, 13-16.

  4. The potential impact of hydrogen energy use on the atmosphere

    NASA Astrophysics Data System (ADS)

    van Ruijven, B. J.; Lamarque, J. F.; van Vuuren, D. P.; Kram, T.; Eerens, H.

    2009-04-01

    ., Hess, P. G., Collins, W. D., Emmons, L. K., Ginoux, P., Luo, C. and Tie, X. X. (2005). "Response of a coupled chemistry-climate model to changes in aerosol emissions: Global impact on the hydrological cycle and the tropospheric burdens of OH, ozone and NOx." Geophysical Research Letters 32(16). Lamarque, J.-F., Kinnison, D. E., Hess, P. G. and Vitt, F. (2008). "Simulated lower stratospheric trends between 1970 and 2005: identifying the role of climate and composition changes." Journal of Geophysical Research 113(D12301). Price, H., Jaegle, L., Rice, A., Quay, P., Novelli, P. C. and Gammon, R. (2007). "Global budget of molecular hydrogen and its deuterium content: constraints from ground station, cruise, and aircraft observations." Journal of Geophysical Research 112(D22108). Sanderson, M. G., Collins, W. J., Derwent, R. G. and Johnson, C. E. (2003). "Simulation of Global Hydrogen Levels Using a Lagrangian Three-Dimensional Model." Journal of Atmospheric Chemistry 46(1): 15-28. Schultz, M. G., Diehl, T., Brasseur, G. P. and Zittel, W. (2003). "Air Pollution and Climate-Forcing Impacts of a Global Hydrogen Economy." Science 302(5645): 624-627. Tromp, T. K., Shia, R. L., Allen, M., Eiler, J. M. and Yung, Y. L. (2003). "Potential environmental impact of a hydrogen economy on the stratosphere." Science 300(5626): 1740-1742. van Ruijven, B., Hari, L., van Vuuren, D. P. and de Vries, B. (2008). "The potential role of hydrogen in India and Western Europe." Energy Policy 36(5): 1649-1665. van Ruijven, B., van Vuuren, D. P. and de Vries, B. (2007). "The potential role of hydrogen in energy systems with and without climate policy." International Journal of Hydrogen Energy 32(12): 1655-1672. van Vuuren, D. P. (2007). Energy systems and climate policy. Dept. of Science, Technology and Society, Faculty of Science. Utrecht, Utrecht University: 326.

  5. The influence of photochemical fractionation on the evolution of the nitrogen isotope ratios - detailed analysis of current photochemical loss rates

    NASA Astrophysics Data System (ADS)

    Mandt, K. E.; Waite, J. H., Jr.; Westlake, J.; Magee, B.; Liang, M. C.; Bell, J.

    2012-04-01

    . Robertson, and S. Lebonnois: " Coupled ion and neutral rotating model of Titan’s upper atmosphere". Icarus, Vol. 197, pp. 236-262, 2008. Liang M., A. N. Heays, B. R. Lewis, S. T. Gibson and Y. L. Yung: “Source of nitrogen isotope anomaly in HCN in the atmosphere of Titan”. Astrophys. J., Vol. 664, pp. L115-L118, 2007. Mandt, K. E., J. H. Waite, Jr., B. A. Magee, J. Bell, J. Lunine, O. Mousis and D. Cordier: “Isotopic evolution of Titan’s main atmospheric constituents”. Planetary and Space Science, Vol. 57, pp. 1917-1930, 2009. Niemann, H.B., S.K. Atreya, J.E. Demick, D. Gautier, J.A. Haberman, D.N. Harpold, W.T. Kasprzak, J.I. Lunine, T.C. Owen and F. Raulin: “The composition of Titan’s lower atmosphere and simple surface volatiles as measured by the Cassini-Huygens probe gas chromatograph mass spectrometer experiment”. J. Geophys. Res., Vol. 115, pp. E12006, 2010. Vinatier, S., et al.: “Vertical abundance profiles of hydrocarbons in Titan’s atmosphere at 15o S and 80o N retrieved from Cassini/CIRS spectra”. Icarus, Vol. 188, pp. 120-138, 2007.

  6. Two formation regions for Titan's hazes: indirect clues and possible synthesis mechanisms

    NASA Astrophysics Data System (ADS)

    Chassefière, E.; Cabane, M.

    1995-02-01

    It is suggested that aerosol particles forming the detached and main haze layers of Titan's atmosphere do not originate in the same atmospheric levels. Particles present above ≈350 km could be formed of polyacetylenes synthetized in the 500-800 km altitude range through successive insertion reactions involving the C 2H radical under the action of solar ultraviolet photons (Yung et al., Astrophys. J. Suppl.55, 465, 1984). They might contain CN oligomers in comparable amounts, as well as CHN oligomers synthetized at high altitude (900-1000 km) by the action of suprathermal Saturn plasma electrons. Physically, they are expected to consist of fluffy aggregates of density ≈0.01-0.1 g cm -3. Their mass production rate is small (10 -15-10 -14 kg m -2 s -1), that is typically 10% or less of the main haze production rate. Due to their low fall velocity, they are very sensitive to large scale horizontal motions and one substantial part of them may be swept away by meridional circulation at the detached haze level. The altitude range where these aerosols are created is well above the range proposed by Cabane et al. ( Planet. Space Sci.41, 257, 1993) for aerosols of the main haze layer, on the basis of a new fractal microphysical modeling of Titan's aggregates, that is ≈ 350-400 km. A natural outcome of this apparent discrepancy is to suppose that there is a second formation region, below ≈400 km altitude, giving rise to the main haze layer. The aim of the present paper is to review the different possible formation mechanisms of this main haze layer and assess their ability to account for the observed characteristics of the haze Several conditions are established. The first one, called "condition A", concerns the formation altitude range imposed by fractal modeling. Possible chemical and energy sources are examined. Two additional constraints, relative to the minimum gas mass ("condition B") and input energy ("condition C") required for efficient conversion of

  7. Accidental Predissociation: A Special Case of Photo-Induced Isotope Fractionation Effect and Possible Occurrence in Nature

    NASA Astrophysics Data System (ADS)

    Chakraborty, S.; Thiemens, M. H.

    2009-12-01

    light of these data, anomalous isotopic fractionations associated with accidental predissociation will be discussed for the CO and N2. These fractionations are important as VUV-photodissociation of CO and N2 have been invoked in solar nebula (self-shielding, (9-10)) to explain the observed iso-topic signatures in different solar system objects neglecting these isotope effects during photo-dissociation. References: 1. Y. L. Yung, C. E. Miller, Science 278, 1778 (1997). 2. S. Chakraborty, S. K. Bhattacharya, J. Chem. Phys. 118, 2164 (2003). 3. H. Lefebvre-Brion, R. W. Field, The Spectra and Dynamics of Diatomic Molecules. (Elsevier Academic Press, 2004). 4. A. J. Lorquet, J. C. Lorquet, Chem. Phys. Lett. 26, 138 (1974). 5. W. Ubachs, I. Velchev, P. Cacciani, J. Chem. Phys. 113, 547 (2000). 6. H. Lefebvre-Brion, R. Colin, J. Mol. Spectrosc. 65, 33 (1977). 7. S. Chakraborty, M. Ahmed, T. L. Jackson, M. H. Thiemens, Science 321, 1328 (2008). 8. S. Chakraborty, M. Ahmed, T. L. Jackson, M. H. Thiemens, Science 324, 4 (2009). 9. R. N. Clayton, Nature 415, 860 (2002). 10. J. R. Lyons, E. D. Young, Nature 435, 317 (2005).

  8. D/H Ratios and Water Contents of Amphiboles in Magmatic Inclusions in Chassigny and Shergotty

    NASA Astrophysics Data System (ADS)

    Watson, L. L.; Hutcheon, I. D.; Epstein, S.; Stolper, E. M.

    1993-07-01

    delta-D value could reflect martian interior water that has a very similar delta-D to the bulk Earth, consistent with predictions of formation of the terrestrial planets from material with similar bulk D/H. Ion microprobe measurement of the H+/Si+ secondary ion ratio allows estimation of the total water content of the kaersutites. Both the Chassigny and Shergotty kaersutites contain only ~0.5 wt% water, indicating that they contain a significant oxyamphibole component, similar to terrestrial kaersutites. Water contents of the kaersutites have been previously assumed to be between 1.5 and 2 wt%. These high values have been used to infer the amount of water in the melt inclusion magma at the time they were trapped [8,9] and to constrain the depth of kaersutite crystallization on Mars. Since the kaersutites are much less hydrous than previously assumed, these estimates may need revision, although little is known about the effect of water fugacity on the incorporation of a Ti-coupled oxyamphibole component, so that a kaersutite with low hydroxyl abundance does not necessarily imply a less hydrous melt. References: [1] Bjoraker G. L. et al. (1989) In Proc. 4th Int. Conf. Mars, Tucson, 69-70. [2] Owen T. et al. (1988) Science, 240, 1767-1770. [3] Yung Y. L. et al. (1988) Icarus, 76, 146159. [4] Watson L. L. et al. (1993) In LPSC XXIV, 1493-1494. [5] Deloule E. et al. (1991) In Stable Isotope Geochemistry: A Tribute to Samuel Epstein, 53-62. [6] Kerridge J. F. (1988) In LPSC XIX, 599-600. [7] Watson L. L. et al. (1991) In LPI Tech. Rept. 92-02, 156-166. [8] Johnson et al. (1990) GCA, 55, 349366. [9] McSween H. Y. Jr. and Harvey R. P. (1993) Science, 259, 1890-1892.

  9. Wave propagation, scattering and emission in complex media

    NASA Astrophysics Data System (ADS)

    Jin, Ya-Qiu

    propagation in forested environment / K. Sarabandi, I. Koh. Angle-of-arrival fluctuations due to meteorological conditions in the diffraction zone of C-band radio waves, propagated over the ground surface / T. A. Tyufilina, A. A. Meschelyakov, M. V. Krutikov. Simulating radio channel statistics using ray based prediction codes / H. L. Bertoni. Measurement and simulation of ultra wideband antenna elements / W. Sörgel, W. Wiesbeck. The experimental investigation of a ground-placed radio complex synchronization system / V. P. Denisov ... [et al.] -- VII. Computational electromagnetics. Analysis of 3-D electromagnetic wave scattering with the Krylov subspace FFT iterative methods / R. S. Chen ... [et al.]. Sparse approximate inverse preconditioned iterative algorithm with block toeplitz matrix for fast analysis of microstrip circuits / L. Mo, R. S. Chen, E. K. N. Yung. An Efficient modified interpolation technique for the translation operators in MLFMA / J. Hu, Z. P. Nie, G. X. Zou. Efficient solution of 3-D vector electromagnetic scattering by CG-MLFMA with partly approximate iteration / J. Hu, Z. P. Nie. The effective constitution at interface of different media / L. G. Zheng, W. X. Zhang. Novel basis functions for quadratic hexahedral edge element / P. Liu ... [et al.]. A higher order FDTD method for EM wave propagation in collision plasmas / S. B. Liu, J. J. Mo, N. C. Yuan. Attenuation of electric field eradiated by underground source / J. P. Dong, Y. G. Gao.

  10. PREFACE: XIV International Conference on Calorimetry in High Energy Physics

    NASA Astrophysics Data System (ADS)

    Wang, Yifang

    2011-03-01

    (Texas Tech University), Weidong Li (IHEP) 3) Readout techniques - Gerald Eigen (University of Bergen), Zheng Wang (IHEP) 4) Operating calorimeters and calibration - Marat Gataullin (CERN), Francesco Lanni (BNL) 5) Future calorimetry - Tohru Takeshita (Shinshu University), Lei Xia (Argonne National Laboratory) 6) Astrophysics and neutrino calorimetry - Giuliana Fiorillo (INFN), Hiro Tajima (SLAC) List of Participants AKCHURIN, NuralTexas Tech University AN, ZhenghuaIHEP AUFFRAY, EtiennetteCERN BANFI, DaniloUniversità degli Studi di Milano, INFN BASHARINA-FRESHVILLE, AnastasiaUniversity College London BEAUCHEMIN, Pierre-HuguesUniversity of Oxford BENAGLIA, Andrea DavideUniversity of Milano - Bicocca and INFN BIAN, JianminIHEP BIINO, CristinaINFN BILKI, BurakUniversity of Iowa BLAHA, JanLAPP BOUDRY, VincentLLR / CNRS-IN2P3 CAI, XiaoIHEP CAPONE, AntonioPhysics Department University "La Sapienza" and INFN CAVALLARI, FrancescaCERN and INFN Rome CECCHI, ClaudiaUniversity di Perugia e INFN CHANG, JinfanIHEP CHEN, HuchengBrookhaven National Laboratory CHILDERS, TaylorUniversität Heidelberg - Kirchhoff-Institut für Physik DAO, ValerioGeneva University - DPNC DE LA TAILLE, ChristopheIN2P3/OMEGA-LAL DIEMOZ, MarcellaINFN Roma DOTTI, AndreaCERN EIGEN, GeraldUniversity of Bergen EPIFANOV, DenisBudker Institute of Nuclear Physics FAIVRE, JulienLPSC Grenoble France FANG, JianIHEP FANG, ShuangshiIHEP FANTONI, AlessandraINFN - LNF FERRI, FedericoCEA/Saclay Irfu/SPP FERRONI, FernandoSapienza University & INFN Roma FISK, Henry EugeneFermilab GABALDON, CarolinaCERN GARUTTI, ErikaDESY GAUDIO, GabriellaIstituto Nazionale di Fisica Nucleare - Sezione di Pavia GILLBERG, DagCarleton University GIOVANNINI, PaolaMax-Planck-Institut für Physik GLAZOV, AlexanderDESY GRACHOV, OlegUniversity of Kansas HAPPACHER, FabioINFN HE, MiaoIHEP HORI, YasutoUniversity of Tokyo, CNS HU, TaoIHEP HULTH, Per-OlofStockholm University JUN, Soon YungCarnegie Mellon University JURK, StefanISEG Spezialelektronik gmb

  11. Poster Session B

    PubMed Central

    2014-01-01

    that the most significantly enriched molecular function categories for SSG-modified proteins were free radical scavenging and cell death/survival. This preliminary result provides some insights on protein SSG modification as a potential regulatory mechanism of nanomaterial-induced oxidative stress. B.11 O-GlcNAc Regulates SOX2 Activity in Embryonic Stem Cells by Altering Protein-SOX2 Interactions Samuel Myers1, Sailaja Pedadda, Tara Freidrich, Sean Thomas, Gregor Krings, Michael Lopez, Marena Trinidad, Barbara Panning, Al Burlingame University of California, San Francisco, CA, USA SOX2 is a versatile transcription factor that maintains embryonic stem cell (ESC) pluripotency and self-renewal, and is important for proper lineage specification and adult stem cell maintenance. This versatility is likely due to post-translational modifications (PTMs) as SOX2 has been reported to be modified by numerous chemical moieties in a variety of cell types. One such PTM is O-GlcNAc, the dynamic and regulatory glycosylation of intracellular proteins. Global O-GlcNAc is essential for ESC self-renewal though the function of SOX2 O-GlcNAcylation in ESC is not understood. Here, we show that SOX2 is O-GlcNAc modified in the transactivation domain and alterations of self-renewing signals induce changes in SOX2 O-GlcNAc stoichiometry. Replacement of wild-type SOX2 with an O-GlcNAc-deficient mutant SOX2 in ESCs increases the pluripotency transcriptional network while down-regulating genes involved in differentiation. Analysis of SOX2-interacting proteins from ESCs revealed that the WT and mutant SOX2 interact with distinct subsets of transcriptional regulatory complexes. Thus, SOX2 O-GlcNAcylation modulates the transcriptional landscape of ESCs by modulating SOX2 activity and interactions with epigenetic regulatory complexes. B.12 Development of Multiplexed Assays for Oral Cancer Biomarker Verification by Peptide Immunoaffinity Enrichment and Targeted Mass Spectrometry Yung-Chin Hsiao1, Lang