77 FR 65361 - Xanthan Gum From Austria and the People's Republic of China: Postponement of Preliminary...

Federal Register 2010, 2011, 2012, 2013, 2014

2012-10-26

... Austria and the People's Republic of China: Postponement of Preliminary Determinations of Antidumping Duty...: October 26, 2012. FOR FURTHER INFORMATION CONTACT: Karine Gziryan (Austria) or Brandon Farlander (People's... of initiation of antidumping duty investigations of xanthan gum from Austria and the People's...

78 FR 24226 - Notice of Proposed Information Collection: Comment Request; FHA TOTAL (Technology Open to...

Federal Register 2010, 2011, 2012, 2013, 2014

2013-04-24

... Information Collection: Comment Request; FHA TOTAL (Technology Open to Approved Lenders) Mortgage Scorecard... proposed information collection requirement described below will be submitted to the Office of Management... Information Service (1-800-877-8339). FOR FURTHER INFORMATION CONTACT: Karin B. Hill, Director, Office of...

The End of the Six-Party Talks?

DTIC Science & Technology

2007-01-01

Pyongyang is wary of Beijing’s international influence, its ability to collaborate with the United States and South Korea, its willingness to foster ...Kenneth Quinones, “ Dualism in the Bush Administration’s North Korea Policy,” Asian Perspective, XXVII, no. 1, 2003, 197-224; Karin Lee and Adam Miles

Persistent Discourses in Physics Education: Gender Neutrality and the Gendering of Competence

ERIC Educational Resources Information Center

Gonsalves, Allison

2014-01-01

In her article, Karin Due presents us with a contradiction in physics: the construction of physics as a symbolically masculine discipline alongside a simultaneous discourse of the "gender-neutrality" of the discipline. Due's article makes an important contribution to the study of the gendering of physics practices, particularly in…

Schools That Succeed: How Educators Marshal the Power of Systems for Improvement

ERIC Educational Resources Information Center

Chenoweth, Karin

2017-01-01

Informed by years of research and on-the-ground reporting, "Schools That Succeed" is Karin Chenoweth's most inspiring and compelling book yet--an essential read for educators who seek to break the stubborn connection between academic achievement and socioeconomic status. Chenoweth draws on her decade-long journey into neighborhood…

Onboard Interferometric SAR Processor for the Ka-Band Radar Interferometer (KaRIn)

NASA Technical Reports Server (NTRS)

Esteban-Fernandez, Daniel; Rodriquez, Ernesto; Peral, Eva; Clark, Duane I.; Wu, Xiaoqing

2011-01-01

An interferometric synthetic aperture radar (SAR) onboard processor concept and algorithm has been developed for the Ka-band radar interferometer (KaRIn) instrument on the Surface and Ocean Topography (SWOT) mission. This is a mission- critical subsystem that will perform interferometric SAR processing and multi-look averaging over the oceans to decrease the data rate by three orders of magnitude, and therefore enable the downlink of the radar data to the ground. The onboard processor performs demodulation, range compression, coregistration, and re-sampling, and forms nine azimuth squinted beams. For each of them, an interferogram is generated, including common-band spectral filtering to improve correlation, followed by averaging to the final 1 1-km ground resolution pixel. The onboard processor has been prototyped on a custom FPGA-based cPCI board, which will be part of the radar s digital subsystem. The level of complexity of this technology, dictated by the implementation of interferometric SAR processing at high resolution, the extremely tight level of accuracy required, and its implementation on FPGAs are unprecedented at the time of this reporting for an onboard processor for flight applications.

Getting It Done: Leading Academic Success in Unexpected Schools

ERIC Educational Resources Information Center

Chenoweth, Karin; Theokas, Christina

2011-01-01

"Getting It Done" describes in clear and helpful detail what leaders of successful high-poverty and high-minority schools have done to promote and sustain student achievement. It follows two celebrated books by Karin Chenoweth: "It's Being Done," which established that the work of educating all children is possible, and "How It's Being Done,"…

Astronaut C. Michael Foale is briefed on use of Sky Genie

NASA Technical Reports Server (NTRS)

1994-01-01

Astronaut C. Michael Foale, STS-63 mission specialist, is briefed on the use of Sky Genie device by Karin L. Porter. The device would aid in emergency egress operations aboard a troubled Space Shuttle. Porter, an employee of Rockwell International, helps train astronauts in egress procedures at JSC's Shuttle mockup and integration laboratory.

Role of ets Oncogenes in the Progression of Breast Cancer

DTIC Science & Technology

1998-10-01

8217 References 167 Arias J, Alberts AS, Brindle P, Claret FX, Smeal T, Karin M, May WA, Lessnick SL, Braun BS, Klemsz M, Lewis BC, Feramisco J and Montminy M...0 and Shaw PE. (1994). Mol. Cell. Oncogene, 8, 3459-3464. Biol., 14, 4815-4824. Bories J, Willerford DM, Grevin D, Davidson L, Camus A, Lopez M

77 FR 36285 - Notice of Proposed Information Collection: Comment Request; Application for Fee or Roster...

Federal Register 2010, 2011, 2012, 2013, 2014

2012-06-18

... the FHA insurance fund. Agency form numbers, if applicable: HUD-92563I, HUD 92563A, HUD 92564-CN... to the proposal by name and/or OMB Control Number and should be sent to: Reports Liaison Officer... number for the Federal Information Relay Service (1-800-877-8339). FOR FURTHER INFORMATION CONTACT: Karin...

Adaptive Rules In Emergent Logistics (ARIEL) An Agent-Based Analysis Environment to Study Adaptive Route-Finding Constantly Changing Road-Networks

DTIC Science & Technology

2003-06-01

my wife Karin, my daughter Jasmin and my son Jan for their support and huge patience. Without the security and support of a loving home, none of...contains the trucks, which are the only moveable objects in the system. In essence they provide functionality and cannot act themselves. The layer

JPRS Report, West Europe.

DTIC Science & Technology

1987-08-11

11 AUGUST 1987 WEST EUROPE CONTENTS POLITICAL FEDERAL REPUBLIC OF GERMANY Greens Divided Over Defense Policy (SUEDDEUTSCHE ZEITUNG, 20, 21 Jun...Depopulation (Karin Henriksson, Emily von Sydow; SVENSKA DAGBLADET, 30 May 87) H /9986 - d - FEDERAL REPUBLIC OF GERMANY POLITICAL GREENS DIVIDED ...React Much More Vigorously to Threats to Freedom In this connection, I want to draw the attention of the National Conference to the seriousness and

Constitutive Activation of NF-kappaB in Prostate Carcinoma Cells Through a Positive Feedback Loop: Implication of Inducible IKK-Related Kinase (IKKi)

DTIC Science & Technology

2004-08-01

development in different tissues is strongly considered ( Greten and Karen, 2004). To assess the effect of w.t. IKKi and kinase inactive IKKi mutant...11: 1357-1362, 1999. 3. Greten FR, Karin M. The IKK/NF-kappaB activation pathway-a target for prevention and treatment of cancer. Cancer Lett. 206(2

Statements of IRAQI Communist Leaders.

DTIC Science & Technology

1960-07-19

Leader Abdul Karin Kassem J,.’l ; The Maintenance and Consolidation of Party Idfe Is a Deeply Sincere Policy of Cur Democratic Government STATEMENTS...OF IRAQI COMMUNIST LEADERS 1» Open Letter to His Excellency the Leader Abdul .Karflm Kassem /following is a ^translation of an article by the...they also exercised political influence and thus the fate of the feudalists was linked to the continued exploitation of our wealth, our natural

Perspectives on Positioning, Interaction, and Learning in Small-Group Discussion: Possibilities for Extending the Analytic Lens

ERIC Educational Resources Information Center

Kittleson, Julie M.; Wilson, Rachel E.

2014-01-01

In this forum piece, we respond to Karin Due's study of social dynamics in groups of students in physics class and gender issues that play out in this context. We discuss two threads that appear in Due's paper: one pertains to patterns of talk within groups and how these patterns open up possibilities for learning, the other pertains to…

Training Aide: Research and Guidance for Effective Training User Guide

DTIC Science & Technology

2013-12-01

Research Product 2014-02 Training Aide: Research and Guidance for Effective Training User Guide Beth Plott Shaun...Effective Training User Guide 5a. CONTRACT OR GRANT NUMBER W91WAW-07-C-0081 5b. PROGRAM ELEMENT NUMBER 611102 6. AUTHOR(S) Beth Plott...Representative and Subject Matter POC: Karin A. Orvis 14. ABSTRACT: This is a user guide for the web-based tool called Training Aide: Research and Guidance

Equitable PERSTEMPO - The Challenge for Long-Term Deployed Armed Forces

DTIC Science & Technology

2003-04-07

substantial impact on the operational effectiveness of the Bundeswehr of the future.  Rudolf Scharping Former Federal Minister of Defense The vision...Federal Minister of Defense, Rudolf Scharping, initiated a new force planning by means of the so-called "Cornerstones Paper" on 01 June 2000, the Chief of...Annex 1) 77 Rainer Marr, Timea Biro, and Karin Steiner , Vereinbarkeit von Familie und Beruf des Soldaten – Moeglichkeiten und Grenzen einer

Initial velocity V-shapes of young asteroid families

NASA Astrophysics Data System (ADS)

Bolin, Bryce T.; Walsh, Kevin J.; Morbidelli, Alessandro; Delbó, Marco

2018-01-01

Ejection velocity fields of asteroid families are largely unconstrained due to the fact that members disperse relatively quickly on Myr time-scales by secular resonances and the Yarkovsky effect. The spreading of fragments in a by the Yarkovsky effect is indistinguishable from the spreading caused by the initial ejection of fragments. By examining families <20 Myr old, we can use the V-shape identification technique to separate family shapes that are due to the initial ejection velocity field and those that are due to the Yarkovsky effect. Asteroid families that are <20 Myr old provide an opportunity to study the velocity field of family fragments before they become too dispersed. Only the Karin family's initial velocity field has been determined and scales inversely with diameter, D-1. We have applied the V-shape identification technique to constrain young families' initial ejection velocity fields by measuring the curvature of their fragments' V-shape correlation in semimajor axis, a, versus D-1 space. Curvature from a straight line implies a deviation from a scaling of D-1. We measure the V-shape curvature of 11 young asteroid families including the 1993 FY12, Aeolia, Brangane, Brasilia, Clarissa, Iannini, Karin, Konig, Koronis(2), Theobalda and Veritas asteroid families. We find that the majority of asteroid families have initial ejection velocity fields consistent with ∼D-1 supporting laboratory impact experiments and computer simulations of disrupting asteroid parent bodies.

Identifying and Leveraging Trust as a Key Element in the Development, Implementation and Sustainment of the Salt Lake City Fire Department’s Intelligence Program

DTIC Science & Technology

2014-09-01

this amazing adventure. An education in self-exploration balanced with relentless tests of my stamina and mettle. To my classmates: Thank you for...Karin and son Scott, thank you for providing the comic relief so needed throughout this process. And most importantly, to my husband, Jeff: There...development of a fire intelligence program.190191 In her NPS Masters Thesis, Terrorism Awareness and Education as a Prevention Strategy for First

Scanning the Horizon: Implications for Navy Strategy of National, Joint and Other Services’ Strategic Trends

DTIC Science & Technology

2012-02-01

CJCS’s) companion document, the Capstone Concept for Joint Operations (CCJO) (discussed below) "ibid., 28. "That said, it should be noted that it...Capstone Concept for Joint Operations (CCJO) The companion document to the JOE that answers the challenges of the future identified in the JOE (and...Karin E. Kitchens , Aaron Martin, A Review of the Army’s Modular Force Structure" (RAND National Defense Research Institute, Technical Report,Jun. 2011

Implications of Integrating Women into the Marine Corps Infantry

DTIC Science & Technology

2015-01-01

account by the research. 17 Guy L. Siebold, “The Essence of Military Group Cohesion,” Armed Forces and Society, Vol. 33, No. 2, January 1, 2007, pp...assignment of female personnel reveals a dearth of critical mass concepts: 24 Jasmin Joecks, Kerstin Pull, and Karin Vetter, “Gender Diversity in the...Personnel Psychology, Vol. 60, No. 2, 2007, pp. 303–335. 42 David M. Marx and Jasmin S. Roman, “Female Role Models: Protecting Women’s Math Test

Prevention of Breast Cell Transformation by Blockade of the AP-1 Transcription Factor.

DTIC Science & Technology

1997-09-01

Alto, CA) to normal for transfection efficiency. Both the CAT (from Dr. M . Karin) and Luciferase reporter plasmids used were: -73/+63 ColCAT, -73/+63...1. Table 1: HMECs used in this study. Cells Name Source Phenotype Normal HMECs: NHMEC Clonetics Senescent, anchorage-dependent 184 M . Stampfer...Immortal HMECs: 184A I N5 M . Stampfer Immortal, anchorage dependent 184B5 M . Stampfer MCF10A A. Russo Transformed HMECs: MCF1OAneoT (ras) A. Russo Immortal

Regulation of Estrogen Receptor Transcription in Breast Carcinoma.

DTIC Science & Technology

1998-10-01

E-cadherin 40 and HSP27 41. It is certainly plausible to hypothesize a role for ERF-1 in the coordinate regulation of a set of genes in hormonally...responsive carcinomas. This conjecture is supported by the fact that breast carcinoma cell lines that express E-cadherin and HSP27 are also ERF- 1...regulatory promoter elements of the hsp27 gene in human breast cancer cells. Biochem. Biophys. Res. Com. 222, 155-163 (1996). 42. Imagawa, M., Chiu, R. & Karin

To Investigate the Therapeutic Efforts of the COX-2 Inhibitor NS-398 as a Single Agent, and in Combination with Vitamin D, in Vitro and in Vivo

DTIC Science & Technology

2008-01-01

by immunoelectron microscopy. The Journal Of Biological Chemistry 1998;273:9886-93. 29. Iniguez M, Rodriguez A, Volpert O, Fresno M, Redondo J...controlled by local hypoxia that induces the synthesis of angio- genic factors that can activate signal pathways and transcrip- tion for endothelial...Helmberg,A. and Karin,M. (1995) Immunosuppression by glucocorticoids: inhibition of NF-kappa B activity through induction of I kappa B synthesis . Science

CPTAC Investigators Discuss Research Insights and Perspectives as part of ASBMB Journal Club - 12 Nov | Office of Cancer Clinical Proteomics Research

Cancer.gov

On Wednesday, November 12, 2014 from 2:00 PM to 3:00 PM EST, Daniel Liebler, PhD (Vanderbilt University) and Karin Rodland, PhD (Pacific Northwestern National Laboratory) and Ruedi Aebersold, PhD (Swiss Federal Institute of Technology) will share their research insight as part of the ASBMB Journal Club.  Both Doctors Liebler and Rodland are Principal Investigators in the NCI’s Clinical Proteomic Tumor Analysis Consortium.

A Comparison of the Compression Response of Thick (6.35mm) and Thin (1.60mm) Dry and Moisture Saturated AS4/3501-6 Laminates

DTIC Science & Technology

1990-10-01

of 1.27 mm/mm/min (0.05 in./in./min.) using a 60 kip Satec universal machine, with a spherically seated compression platen for alignment purposes. At...Task No. 6. AUTHOR(S) R3450SOS, ROOONOO, Work Karin Gipple Unit No. 2802-950 and 2844-220 7. PERFORMING ORGANIZATION NAME(S) AND ADDRESS( ES ) 8... ES ) 10. SPONSORING /MONITOR ING AGENCY REPORT NUMBER DTRC Materials Block, IR 11. SUPPLEMENTARY NOTES 12a. DISTRIBUTION /AVAILABILTY STATEMENT 12b

Chemotherapeutic Targeting of Fibulin-5 to Suppress Breast Cancer Invasion and Metastasis Stimulated by Transforming Growth Factor-Beta

DTIC Science & Technology

2012-10-22

Res. Commun 2004;316:997–1001. [PubMed: 15044083] 178. Karin M. NF-κB in cancer development and progression. Nature 2006;441:431. [PubMed: 16724054...of TWIST gene expression. Cancer Res 2007;67:9066–9076. [PubMed: 17909010] 199. Ali S, Coombes RC. Endocrine-responsive breast cancer and strategies...for combating resistance. Nat. Rev. Cancer 2002;2:101–112. [PubMed: 12635173] 200. Coombes RC, Gibson L, Hall E, Emson M, Bliss J. Aromatase

A Case Study in Security Sector Reform: Learning from Security Sector Reform/Building in Afghanistan (October 2002-September 2003)

DTIC Science & Technology

2009-11-01

Amb G (Ambassador-Italy)10. Mrs. G (ISAF Political Advisor)11. Amb K (Amb-Japan)12. Mr. K (ISAF PolAd)13. Mrs. M (Chargé-Netherlands)14. Mr. M ...DCM-Japan)15. BG M (Senior Military Advisor-Finland)16. Amb N (Amb-UK)17. Mr. S (DCM-Germany)18. Lt Col S (MilAd-GE)19. Amb T (Donor Asst-U.S...Building, Year One: From Bonn to Kabul.” Antonio Donini , Norah Niland, and Karin Wermester, eds., Nation Building Unraveled, pp. 39-60. Bloomfield, CT

Review of National Work Programme on the Long Term Effects of Sustained High G on the Cervical Spine (Analyse du programme de travail national : les effets long terme sur la colonne cervicale d’un nombre de G lev et prolong )

DTIC Science & Technology

2008-12-01

Prof. Karin Harms-Ringdahl, PhD, RPT Karolinska Institutet Department of Neurobiology, Care Sciences, and Society Division of Physiotherapy 23100...Äng Karolinska Institutet Department of Neurobiology, Care Sciences, and Society Division of Physiotherapy Alfred Nobels Allé 23100 SE-14183...report is in preparation. The RAF has an ongoing project (from August 2006 to September 2007) determining the need for physiotherapy for aircrew on the

The U.S. Navy in the World (1991-2000): Context for U.S. Navy Capstone Strategies and Concepts

DTIC Science & Technology

2012-03-01

D0026420.A2/Final March 2012 CNA ANALYSIS & SOLUTIONS CNA is a not-for-profit organization whose professional staff of over 700 provides in-depth...www.dtic.mil or contact CNA Document Control and Distribution Section at 703-824-2123. Copyright © 2012 CNA This work was created in the performance of...N00014-11-D-0323 5b. GRANT NUMBER 5c. PROGRAM ELEMENT NUMBER N/A 6. AUTHOR(S) Swartz, Peter M. Duggan, Karin 5d. PROJECT NUMBER N/A 5e. TASK

An Assessment of Spaceborne Near-Nadir Interferometric SAR Performance Over Inland Waters with Real

NASA Astrophysics Data System (ADS)

Tan, H.; Li, S. Y.; Liu, Z. W.

2018-04-01

Elevation measurements of the continental water surface have been poorly collected with in situ measurements or occasionally with conventional altimeters with low accuracy. Techniques using InSAR at near-nadir angles to measure the inland water elevation with large swath and with high accuracy have been proposed, for instance, the WSOA on Jason 2 and the KaRIn on SWOT. However, the WSOA was abandoned unfortunately and the SWOT is planned to be launched in 2021. In this paper, we show real acquisitions of the first spaceborne InSAR of such kind, the Interferometric Imaging Radar Altimeter (InIRA), which has been working on Tiangong II spacecraft since 2016. We used the 90-m SRTM DEM as a reference to estimate the phase offset, and then an empirical calibration model was used to correct the baseline errors.

Persistent discourses in physics education: gender neutrality and the gendering of competence

NASA Astrophysics Data System (ADS)

Gonsalves, Allison

2014-06-01

In her article, Karin Due presents us with a contradiction in physics: the construction of physics as a symbolically masculine discipline alongside a simultaneous discourse of the "gender-neutrality" of the discipline. Due's article makes an important contribution to the study of the gendering of physics practices, particularly in group dynamics, and how this serves to simultaneously reinforce the two competing discourses of physics as a masculine discipline, and the discourse of physics as a gender neutral discipline. Due also suggests that an implication of this contradiction is a limited number of available positions for girls in physics compared to those available to boys. I wish to take up this observation and discuss how available positions for boys and girls in physics are related quite closely to two other concepts discussed in Due's article: competence and recognition.

KARIN: The Ka-Band Radar Interferometer for the Proposed Surface Water and Ocean Topography (SWOT) Mission

NASA Technical Reports Server (NTRS)

Esteban-Fernandez, Daniel; Peral, Eva; McWatters, Dalia; Pollard, Brian; Rodriguez, Ernesto; Hughes, Richard

2013-01-01

Over the last two decades, several nadir profiling radar altimeters have provided our first global look at the ocean basin-scale circulation and the ocean mesoscale at wavelengths longer than 100 km. Due to sampling limitations, nadir altimetry is unable to resolve the small wavelength ocean mesoscale and sub-mesoscale that are responsible for the vertical mixing of ocean heat and gases and the dissipation of kinetic energy from large to small scales. The proposed Surface Water and Ocean Topography (SWOT) mission would be a partnership between NASA, CNES (Centre National d'Etudes Spaciales) and the Canadian Space Agency, and would have as one of its main goals the measurement of ocean topography with kilometer-scale spatial resolution and centimeter scale accuracy. In this paper, we provide an overview of all ocean error sources that would contribute to the SWOT mission.

John Martin Wood (1938-2008)--pioneering biochemist, educator and communicator.

PubMed

Tobin, Desmond J; Pittelkow, Mark R; Slominski, Andrzej

2008-07-01

John Martin Wood, Emeritus Professor of Medical Biochemistry at the University of Bradford died in Wieck by Greifswald, Germany after a short illness on February 5, 2008 - just short of his 70(th) year. John worked as a pioneering biochemist and educator in the US and in Britain across two research careers. He devoted the first twenty-five years to the role of transition metals in biology, and his last twenty-years to cutaneous enzymology and melanogenesis. Working together with his wife Professor Karin U. Schallreuter, his research on oxidative stress handling in skin and on the expression of a cutaneous catecholaminergic system will help direct research in these fields for many years to come. John impressed on his fellow cutaneous researchers and students the critical importance of appreciating the true role of enzymes in skin health and disease. This obituary aims to contextualize the significant contributions made by this remarkable man to experimental dermatology.

New insights on the Karoo shale gas potential from borehole KZF-1 (Western Cape, South Africa)

NASA Astrophysics Data System (ADS)

Campbell, Stuart A.; Götz, Annette E.; Montenari, Michael

2016-04-01

A study on world shale reserves conducted by the Energy Information Agency (EIA) in 2013 concluded that there could be as much as 390 Tcf recoverable reserves of shale gas in the southern and south-western parts of the Karoo Basin. This would make it the 8th-largest shale gas resource in the world. However, the true extent and commercial viability is still unknown, due to the lack of exploration drilling and modern 3D seismic. Within the framework of the Karoo Research Initiative (KARIN), two deep boreholes were drilled in the Eastern and Western Cape provinces of South Africa. Here we report on new core material from borehole KZF-1 (Western Cape) which intersected the Permian black shales of the Ecca Group, the Whitehill Formation being the main target formation for future shale gas production. To determine the original source potential for shale gas we investigated the sedimentary environments in which the potential source rocks formed, addressing the research question of how much sedimentary organic matter the shales contained when they originally formed. Palynofacies indicates marginal marine conditions of a stratified basin setting with low marine phytoplankton percentages (acritarchs, prasinophytes), good AOM preservation, high terrestrial input, and a high spores:bisaccates ratio (kerogen type III). Stratigraphically, a deepening-upward trend is observed. Laterally, the basin configuration seems to be much more complex than previously assumed. Furthermore, palynological data confirms the correlation of marine black shales of the Prince Albert and Whitehill formations in the southern and south-western parts of the Karoo Basin with the terrestrial coals of the Vryheid Formation in the north-eastern part of the basin. TOC values (1-6%) classify the Karoo black shales as promising shale gas resources, especially with regard to the high thermal maturity (Ro >3). The recently drilled deep boreholes in the southern and south-western Karoo Basin, the first since the SOEKOR exploration programmes of the 1960's and 1970's, provide new core material to determine the likely current potential for retention of shale gas with regard to the structural and thermal history of the basin. Thus, the KARIN research program will produce a valuable data set for future unconventional gas exploration and production in South Africa.

Recommended guidelines for uniform reporting of pediatric advanced life support: the pediatric Utstein style.

PubMed

Zaritsky, A; Nadkarni, V; Hazinski, M F; Foltin, G; Quan, L; Wright, J; Fiser, D; Zideman, D; O'Malley, P; Chameides, L

1995-10-01

This statement is the product of a task force meeting held June 8, 1994, in Washington DC in conjunction with the First International Conference on Pediatric Resuscitation and a follow-up task force writing group meeting held September 18, 1994, in Chicago. Draft versions of the statement were circulated for comment to all members of the task force, the American Heart Association Subcommittee on Pediatric Resuscitation, and several outside reviewers. This statement and the International Conference on Pediatric Resuscitation were cosponsored by the American Academy of Pediatrics and the American Heart Association. The development of this statement was authorized by the American Academy of Pediatrics; the American Heart Association National Subcommittees on Pediatric Resuscitation, Basic Life Support, and Advanced Cardiac Life Support, the Committee on Emergency Cardiac Care, the Science Advisory Committee; and the European Resuscitation Council. In addition to the writing group, members of the Pediatric Utstein Task Force are Paul Anderson, M Douglas Baker, Jane Ball, Desmond Bohn, Dena Brownstein, J Michael Dean, Niranjan Kissoon, Bruce Klein, Patrick Malone, Karin McCloskey, James McCrory, P Pearl O'Rourke, Mary Patterson, Charles Schleien, James Seidel, Joseph J Tepas III, and Becky Yano.

WatER: The proposed Water Elevation Recovery satellite mission

NASA Astrophysics Data System (ADS)

Alsdorf, D.; Mognard, N.; Rodriguez, E.; Participants, W.

2005-12-01

Surface fresh water is essential for life, yet we have surprisingly poor knowledge of the spatial and temporal dynamics of surface water storage and discharge globally. The core mission objective is to describe and understand the continental water cycle and the hydrological processes (e.g., floodplain hydraulics) at work in a river basin. The key question that will be answered by WatER is: "Where is water stored on Earth's land surfaces, and how does this storage vary in space and time?" WatER will facilitate societal needs by (1) improving our understanding of flood hazards; (2) freely providing water volume information to countries who critically rely on rivers that cross political borders; and (3) mapping the variations in water bodies that contribute to disease vectors (e.g., malaria). Conventional altimeter profiles are, without question, incapable of supplying the measurements needed to address scientific and societal questions. WatER will repeatedly measure the spatially distributed water surface elevations (h) of wetlands, rivers, lakes, reservoirs, etc. Successive h measurements yield dh/dt, (t is time), hence a volumetric change in water stored or lost. Individual images of h yield dh/dx (x is distance), hence surface water slope, which is necessary for estimating streamflow. WatER's main instrument is a Ka-band radar interferometer (KaRIN) which is the only technology capable of supplying the required imaging capability of h. KaRIN has a rich heritage based on (1) the many highly successful ocean observing radar altimeters, (2) the Shuttle Radar Topography Mission (SRTM), and (3) the development effort of the Wide Swath Ocean Altimeter (WSOA). The interferometric altimeter is a near-nadir viewing, 120 km wideswath based instrument that uses interferometric SAR processing of the returned pulses to yield single-look 5m azimuth and 10m to 70m range resolution, with an elevation accuracy of approximately 50 cm. Polynomial based averaging of heights along the water body increases the height accuracy to about 3 cm. The entire globe is covered twice every 16 days and orbit subcycles allow the average visit to be about half this time at low to mid-latitudes, and almost daily at high latitudes. The WatER mission is an international effort with a large, supporting scientific community. It is already proposed as an ESA Earth Explorer Core mission and will also be jointly submitted to NASA's Earth System Science Pathfinder program. WatER is designed to meet high priority targets for all nations and will provide essential data for the EU Water Framework Directive and the European Flood Alert System. WatER will meet the United Nations call for a "greater focus on water related issues", responds to the hydroclimatological needs of the International Working Group on Earth Observations, and answers the U.S. federal government call to focus on our "ability to measure, monitor, and forecast U.S. and global supplies of fresh water".

Discharge estimation in ungauged basins through variational data assimilation : The potential of the SWOT mission.

NASA Astrophysics Data System (ADS)

Oubanas, H.; Gejadze, I.; Malaterre, P. O.; Durand, M. T.; Wei, R.; Frasson, R. P. M.; Domeneghetti, A.

2017-12-01

This work investigates the estimation of river discharge from simulated observations of the forthcoming Surface Water and Ocean Topography (SWOT) mission, to be launched in 2021, using a variant of the standard variational data assimilation method `4D-Var'. The hydrology SWOT simulator, developed at the Jet Propulsion Laboratory (JPL) has been used to simulate the expected performance of the KaRIn instrument onboard the satellite, producing synthetic SWOT observations of height and width, at each satellite overpass. SWOT data products were synthesized at the spatial scale of 200 m along the river centerline. Using a 1.5D full Saint-Venant hydraulic model, variational data assimilation simultaneously estimates the inflow discharge, river bathymetry and bed roughness. The proposed method has been designed for an application to fully ungauged basins; therefore, the prior information is derived from the SWOT observations only and the globally available ancillary information. Two reaches of the Po and Sacramento Rivers of about 130 km and 150 km, respectively, have been considered in this study. Discharge was successfully recovered at the overpass time with a relative-root-mean-square error of 16% and 12.3% for the Po and Sacramento Rivers, respectively. The estimates of the bed level and the roughness coefficient demonstrate a local improvement; however they may not provide reliable global information of the river bathymetry and roughness.

New Techniques for Radar Altimetry of Sea Ice and the Polar Oceans

NASA Astrophysics Data System (ADS)

Armitage, T. W. K.; Kwok, R.; Egido, A.; Smith, W. H. F.; Cullen, R.

2017-12-01

Satellite radar altimetry has proven to be a valuable tool for remote sensing of the polar oceans, with techniques for estimating sea ice thickness and sea surface height in the ice-covered ocean advancing to the point of becoming routine, if not operational, products. Here, we explore new techniques in radar altimetry of the polar oceans and the sea ice cover. First, we present results from fully-focused SAR (FFSAR) altimetry; by accounting for the phase evolution of scatterers in the scene, the FFSAR technique applies an inter-burst coherent integration, potentially over the entire duration that a scatterer remains in the altimeter footprint, which can narrow the effective along track resolution to just 0.5m. We discuss the improvement of using interleaved operation over burst-more operation for applying FFSAR processing to data acquired by future missions, such as a potential CryoSat follow-on. Second, we present simulated sea ice retrievals from the Ka-band Radar Interferometer (KaRIn), the instrument that will be launched on the Surface Water and Ocean Topography (SWOT) mission in 2021, that is capable of producing swath images of surface elevation. These techniques offer the opportunity to advance our understanding of the physics of the ice-covered oceans, plus new insight into how we interpret more conventional radar altimetry data in these regions.

Using Sentinel-2A multispectral imagery to explore for deep groundwater resources in the Ceres-Tankwa Karoo, Western Cape, South Africa: Significance for the 'water-energy(-food) nexus' in an arid region

NASA Astrophysics Data System (ADS)

Hartnady, Chris; Wise, Edward; Hartnady, Michael; Olianti, Camille; Hay, E. Rowena

2017-04-01

The Ceres-Tankwa region is an arid region in the south-western part of the main Karoo Basin, underlain by folded and faulted strata of the Cape and lower Karoo Supergroups in the syntaxis zone between the Western and Southern branches of the Cape Fold Belt. Explored for oil in the mid-1960s, with the drilling of the >3000 m deep KL1/65 borehole, the area recently attracted attention as a potential shale-gas prospect with the drilling in 2015 of the 671 m-deep KZF-1 research borehole on the farm Zandfontein (de Kock et al, 2016). KZF-1 encountered no positive indication of methane gas in the carbonaceous shale target but intersected a strong flow of deep groundwater from fractures in the basal Dwyka tillite. The accidental discovery of deep artesian groundwater, probably originating from the underlying Cape Supergroup aquifers and of significantly better quality than the shallow aquifer utilised by local farmers, has important implications for future development here. Using 13-channel multispectral data from the European Space Agency satellite Sentinel-2A, a false-colour composite image, centred about the KZF-1 location, was assembled by combination of selected spectral band-ratios. Stratigraphic layering and associated folding within the hitherto undivided, pelitic Tierberg Formation (Ecca Group), is revealed in striking new detail, together with narrow lines of stratal offset corresponding to previously unmapped faults. KZF-1 is evidently sited within an anomalous NE/SW-striking belt, unlike the general NNW/SSE strike of Cape-Karoo sequence strata in the north-western part of the image. Associated with a notable strike change of a lower Tierberg marker unit, subparallel to and aligned with a similar trend in the Swartruggens mountain foothills to the SW, a deep-seated, controlling, NE/SW-striking fault structure may continue downwards from the lower Karoo units into the underlying Cape strata, providing hydraulic connection. With the looming threat of global warming and increasing water scarcity in semi-arid regions, deep artesian groundwater systems provide a long-term solution to future demands for water, food and power. In contrast to shale-gas development, which competes for the scarce water resource and poses a substantial pollution threat, an alternative, synergistic and conjunctive development of solar energy, specifically Concentrating Solar Power plants facilitated by the deep artesian groundwater resource, is envisaged for the Ceres-Tankwa and other parts of the Southern Karoo, in a proposed "Sores-Kamma (Sun-Water) Initiative". In this effort, Sentinel-2A-based lithological mapping is integrated with a new digital elevation model, providing geomorphometry and morphotectonic interpretations, and with the systematic monitoring of surface- and groundwater fluxes using a conjunction of radar satellite, Global Navigation Satellite Systems and microgravity approaches. Reference De Kock, M.O., Beukes, N.J., Götz, A.E., Cole, D., Birch, A., Withers, A. and Van Niekerk, H.S. 2016. Open file progress report on exploration of the southern Karoo Basin through CIMERA-KARIN borehole KZF-1 in the Tankwa Karoo, Witzenberg (Ceres) District. 12 pp. Available online at http://www.cimera.co.za/index.php/karin-feedback

2012 Aspen Winter Conference New Paradigms for Low-Dimensional Electronic Materials, February 5-10, 2012

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

Moore, Joel; Rabe, Karin; Nayak, Chetan

2012-05-01

Aspen Center for Physics Project Summary DOE Budget Period: 10/1/2011 to 9/30/2012 Contract # DE-SC0007479 New Paradigms for Low-Dimensional Electronic Materials The 2012 Aspen Winter Conference on Condensed Matter Physics was held at the Aspen Center for Physics from February 5 to 10, 2012. Seventy-four participants from seven countries, and several universities and national labs attended the workshop titled, New Paradigms for Low-Dimensional Electronic Materials. There were 34 formal talks, and a number of informal discussions held during the week. Talks covered a variety of topics related to DOE BES priorities, including, for example, advanced photon techniques (Hasan, Abbamonte, Orenstein,more » Shen, Ghosh) and predictive theoretical modeling of materials properties (Rappe, Pickett, Balents, Zhang, Vanderbilt); the full conference schedule is provided with this report. The week's events included a public lecture (Quantum Matters given by Chetan Nayak from Microsoft Research) and attended by 234 members of the public, and a physics caf© geared for high schoolers that is a discussion with physicists conducted by Kathryn Moler (Stanford University) and Andrew M. Rappe (University of Pennsylvania) and attended by 67 locals and visitors. While there were no published proceedings, some of the talks are posted online and can be Googled. The workshop was organized by Joel Moore (University of California Berkeley), Chetan Nayak (Microsoft Research), Karin Rabe (Rutgers University), and Matthias Troyer (ETH Zurich). Two organizers who did not attend the conference were Gabriel Aeppli (University College London & London Centre for Nanotechnology) and Andrea Cavalleri (Oxford University & Max Planck Hamburg).« less

The Praise and Price of Pokémon GO: A Qualitative Study of Children's and Parents' Experiences.

PubMed

Lindqvist, Anna-Karin; Castelli, Darla; Hallberg, Josef; Rutberg, Stina

2018-01-03

Physical activity has multiple health benefits; however, the majority of children around the world do not attain the recommended levels of daily physical activity. Research has shown that the game Pokémon GO has increased the amount of physical activity of players and that the game has the potential to reach populations that traditionally have low levels of physical activity. Therefore, there is a need to understand which game components can promote initial and sustained physical activity. By using a qualitative research approach, it is possible to achieve rich descriptions and enhance a deep understanding of the components promoting physical activity among children in a game such as Pokémon GO. The objective of this study was to explore children's and parents' experiences playing Pokémon GO. Eight families comprising 13 children (aged 7-12 years) and 9 parents were selected using purposeful sampling. Data collected using focus groups were analyzed using qualitative latent content analysis. The following three themes were revealed: (1) exciting and enjoyable exploration; (2) dangers and disadvantages; and (3) cooperation conquers competition. The first centers around the present and possible future aspects of Pokémon GO that promote physical activity. The second focuses on unwanted aspects and specific threats to safety when playing the game. The third shows that cooperation and togetherness are highly valued by the participants and that competition is fun but less important. Components from Pokémon GO could enhance the efficacy of physical activity interventions. Cooperation and exploration are aspects of the game that preferably could be transferred into interventions aimed at promoting children's physical activity. ©Anna-Karin Lindqvist, Darla Castelli, Josef Hallberg, Stina Rutberg. Originally published in JMIR Serious Games (http://games.jmir.org), 03.01.2018.

Common Ground on Climate Change: Pairing Opposing Viewpoints for Conversations about Climate Change

NASA Astrophysics Data System (ADS)

Kirk, K. B.; Duggan-Haas, D.; Hayhoe, K.

2017-12-01

In American public discourse, people tend to strongly identify with the viewpoints held by their cultural and political tribes. However, entrenched positions do little to advance understanding, or work toward solving problems constructively. Worse yet, it has become commonplace to dismiss or demonize those coming from a different point of view - leading to the vitriolic stalemate that often characterizes social media and comment threads when it comes to climate change. One way to break this pattern is to invite people with opposing opinions to actually talk to one another. This presentation describes the lessons learned during the Common Ground on Climate Change project, in which people with contrasting views about climate change engage in a moderated interview with each other. Prior to the interview, participants complete a set of values-based questions. The goal is to reveal areas of common ground between apparent opposites, such as a sense of stewardship for Earth's resources, or an opinion that solutions to climate change will be more beneficial than harmful. The structure of the interviews is based on the hypothesis that if a conversation begins with an appreciation of common values, it becomes easier to broach areas of disagreement. Participants are matched up in one-on-one moderated interviews where they are encouraged to share their concerns, ideas, and priorities about the validity of climate science, the need for urgent action, and the types of solutions they find most tenable. Emerging themes from this series of interviews include the value of a diversity of outlooks, and the ability for moderated conversations to find surprising areas of agreement. Articles about the interviews also appear on the Yale Climate Connections website, https://www.yaleclimateconnections.org/author/karin/.

Controlling cytoplasmic c-Fos controls tumor growth in the peripheral and central nervous system.

PubMed

Gil, Germán A; Silvestre, David C; Tomasini, Nicolás; Bussolino, Daniela F; Caputto, Beatriz L

2012-06-01

Some 20 years ago c-Fos was identified as a member of the AP-1 family of inducible transcription factors (Angel and Karin in Biochim Biophys Acta 1072:129-157, 1991). More recently, an additional activity was described for this protein: it associates to the endoplasmic reticulum and activates the biosynthesis of phospholipids (Bussolino et al. in FASEB J 15:556-558, 2001), (Gil et al. in Mol Biol Cell 15:1881-1894, 2004), the quantitatively most important components of cellular membranes. This latter activity of c-Fos determines the rate of membrane genesis and consequently of growth in differentiating PC12 cells (Gil et al. in Mol Biol Cell 15:1881-1894, 2004). In addition, it has been shown that c-Fos is over-expressed both in PNS and CNS tumors (Silvestre et al. in PLoS One 5(3):e9544, 2010). Herein, it is shown that c-Fos-activated phospholipid synthesis is required to support membrane genesis during the exacerbated growth characteristic of brain tumor cells. Specifically blocking c-Fos-activated phospholipid synthesis significantly reduces proliferation of tumor cells in culture. Blocking c-Fos expression also prevents tumor progression in mice intra-cranially xeno-grafted human brain tumor cells. In NPcis mice, an animal model of the human disease Neurofibromatosis Type I (Cichowski and Jacks in Cell 104:593-604, 2001), animals spontaneously develop tumors of the PNS and the CNS, provided they express c-Fos (Silvestre et al. in PLoS One 5(3):e9544, 2010). Treatment of PNS tumors with an antisense oligonucleotide that specifically blocks c-Fos expression also blocks tumor growth in vivo. These results disclose cytoplasmic c-Fos as a new target for effectively controlling brain tumor growth.

Lunar and Planetary Science XXXVI, Part 18

NASA Technical Reports Server (NTRS)

2005-01-01

Topics discussed include: PoDS: A Powder Delivery System for Mars In-Situ Organic, Mineralogic and Isotopic Analysis Instruments Planetary Differentiation of Accreting Planetesimals with 26Al and 60Fe as the Heat Sources Ground-based Observation of Lunar Surface by Lunar VIS/NIR Spectral Imager Mt. Oikeyama Structure: First Impact Structure in Japan? Central Mounds in Martian Impact Craters: Assessment as Possible Perennial Permafrost Mounds (Pingos) A Further Analysis of Potential Photosynthetic Life on Mars New Insight into Valleys-Ocean Boundary on Mars Using 128 Pixels per Degree MOLA Data: Implication for Martian Ocean and Global Climate Change; Recursive Topography Based Surface Age Computations for Mars: New Insight into Surficial Processes That Influenced Craters Distribution as a Step Toward the Formal Proof of Martian Ocean Recession, Timing and Probability; Laser-induced Breakdown Spectroscopy: A New Method for Stand-Off Quantitative Analysis of Samples on Mars; Milk Spring Channels Provide Further Evidence of Oceanic, >1.7-km-Deep Late Devonian Alamo Crater, Southern Nevada; Exploration of Martian Polar Residual Caps from HEND/ODYSSEY Data; Outflow Channels Influencing Martian Climate: Global Circulation Model Simulations with Emplaced Water; Presence of Nonmethane Hydrocarbons on Pluto; Difference in Degree of Space Weathering on the Newborn Asteroid Karin; Circular Collapsed Features Related to the Chaotic Terrain Formation on Mars; A Search for Live (sup 244)Pu in Deep-Sea Sediments: Preliminary Results of Method Development; Some Peculiarities of Quartz, Biotite and Garnet Transformation in Conditions of Step-like Shock Compression of Crystal Slate; Error Analysis of Remotely-Acquired Mossbauer Spectra; Cloud Activity on Titan During the Cassini Mission; Solar Radiation Pressure and Transient Flows on Asteroid Surfaces; Landing Site Characteristics for Europa 1: Topography; and The Crop Circles of Europa.

Well-ordered science and Indian epistemic cultures: toward a polycentered history of science.

PubMed

Ganeri, Jonardon

2013-06-01

This essay defends the view that "modern science," as with modernity in general, is a polycentered phenomenon, something that appears in different forms at different times and places. It begins with two ideas about the nature of rational scientific inquiry: Karin Knorr Cetina's idea of "epistemic cultures," and Philip Kitcher's idea of science as "a system of public knowledge," such knowledge as would be deemed worthwhile by an ideal conversation among the whole public under conditions of mutual engagement. This account of the nature of scientific practice provides us with a new perspective from which to understand key elements in the philosophical project of Jaina logicians in the seventh, eighth, and ninth centuries C.E. Jaina theory seems exceptionally well targeted onto two of the key constituents in the ideal conversation--the classification of all human points of view and the representation of end states of the deliberative process. The Buddhist theory of the Kathāvatthu contributes to Indian epistemic culture in a different way: by supplying a detailed theory of how human dialogical standpoints can be revised in the ideal conversation, an account of the phenomenon Kitcher labels "tutoring." Thus science in India has its own history, one that should be studied in comparison and contrast with the history of science in Europe. In answer to Joseph Needham, it was not 'modern science' which failed to develop in India or China but rather non-well-ordered science, science as unconstrained by social value and democratic consent. What I argue is that this is not a deficit in the civilisational histories of these countries, but a virtue.

Bringing radical behaviorism to revolutionary Brazil and back: Fred Keller's Personalized System of Instruction and Cold War engineering education.

PubMed

Akera, Atsushi

2017-09-01

This article traces the shifting epistemic commitments of Fred S. Keller and his behaviorist colleagues during their application of Skinnerian radical behaviorism to higher education pedagogy. Building on prior work by Alexandra Rutherford and her focus on the successive adaptation of Skinnerian behaviorism during its successive applications, this study utilizes sociologist of science Karin Knorr Cetina's concept of epistemic cultures to more precisely trace the changes in the epistemic commitments of a group of radical behaviorists as they shifted their focus to applied behavioral analysis. The story revolves around a self-paced system of instruction known as the Personalized System of Instruction, or PSI, which utilized behaviorist principles to accelerate learning within the classroom. Unlike Skinner's entry into education, and his focus on educational technologies, Keller developed a mastery-based approach to instruction that utilized generalized reinforcers to cultivate higher-order learning behaviors. As it happens, the story also unfolds across a rather fantastic political terrain: PSI originated in the context of Brazilian revolutionary history, but circulated widely in the U.S. amidst Cold War concerns about an engineering manpower(sic) crisis. This study also presents us with an opportunity to test Knorr Cetina's conjecture about the possible use of a focus on epistemic cultures in addressing a classic problem in the sociology of science, namely unpacking the relationship between knowledge and its social context. Ultimately, however, this study complements another historical case study in applied behavioral analysis, where a difference in outcome helps to lay out the range of possible shifts in the epistemic commitments of radical behaviorists who entered different domains of application. The case study also has some practical implications for those creating distance learning environments today, which are briefly explored in the conclusion. © 2017 Wiley Periodicals, Inc.

Multiverse: Increasing Diversity in Earth and Space Science Through Multicultural Education

NASA Astrophysics Data System (ADS)

Peticolas, L. M.; Raftery, C. L.; Mendez, B.; Paglierani, R.; Ali, N. A.; Zevin, D.; Frappier, R.; Hauck, K.; Shackelford, R. L., III; Yan, D.; Thrall, L.

2015-12-01

Multiverse at the University of California, Berkeley Space Sciences Laboratory provides earth and space science educational opportunities and resources for a variety of audiences, especially for those who are underrepresented in the sciences. By way of carefully crafted space and earth science educational opportunities and resources, we seek to connect with people's sense of wonder and facilitate making personal ties to science and the learning process in order to, ultimately, bring the richness of diversity to science and make science discovery accessible for all. Our audiences include teachers, students, education and outreach professionals, and the public. We partner with NASA, the National Science Foundation, scientists, teachers, science center and museum educators, park interpreters, and others with expertise in reaching particular audiences. With these partners, we develop resources and communities of practice, offer educator workshops, and run events for the public. We will will present on our pedagogical techniques, our metrics for success, and our evaluation findings of our education and outreach projects that help us towards reaching our vision: We envision a world filled with science literate societies capable of thriving with today's technology, while maintaining a sustainable balance with the natural world; a world where people develop and sustain the ability to think critically using observation and evidence and participate authentically in scientific endeavors; a world where people see themselves and their culture within the scientific enterprise, and understand science within the context that we are all under one sky and on one Earth. Photo Caption: Multiverse Team Members at our Space Sciences Laboratory from left to right: Leitha Thrall, Daniel Zevin, Bryan Mendez, Nancy Ali, Igor Ruderman, Laura Peticolas, Ruth Paglierani, Renee Frappier, Rikki Shackelford, Claire Raftery, Karin Hauck, and Darlene Yan.

NASA Tech Briefs, December 2011

NASA Technical Reports Server (NTRS)

2011-01-01

Topics covered include: 1) SNE Industrial Fieldbus Interface; 2) Composite Thermal Switch; 3) XMOS XC-2 Development Board for Mechanical Control and Data Collection; 4) Receiver Gain Modulation Circuit; 5) NEXUS Scalable and Distributed Next-Generation Avionics Bus for Space Missions; 6) Digital Interface Board to Control Phase and Amplitude of Four Channels; 7) CoNNeCT Baseband Processor Module; 8) Cryogenic 160-GHz MMIC Heterodyne Receiver Module; 9) Ka-Band, Multi-Gigabit-Per-Second Transceiver; 10) All-Solid-State 2.45-to-2.78-THz Source; 11) Onboard Interferometric SAR Processor for the Ka-Band Radar Interferometer (KaRIn); 12) Space Environments Testbed; 13) High-Performance 3D Articulated Robot Display; 14) Athena; 15) In Situ Surface Characterization; 16) Ndarts; 17) Cryo-Etched Black Silicon for Use as Optical Black; 18) Advanced CO2 Removal and Reduction System; 19) Correcting Thermal Deformations in an Active Composite Reflector; 20) Umbilical Deployment Device; 21) Space Mirror Alignment System; 22) Thermionic Power Cell To Harness Heat Energies for Geothermal Applications; 23) Graph Theory Roots of Spatial Operators for Kinematics and Dynamics; 24) Spacesuit Soft Upper Torso Sizing Systems; 25) Radiation Protection Using Single-Wall Carbon Nanotube Derivatives; 26) PMA-PhyloChip DNA Microarray to Elucidate Viable Microbial Community Structure; 27) Lidar Luminance Quantizer; 28) Distributed Capacitive Sensor for Sample Mass Measurement; 29) Base Flow Model Validation; 30) Minimum Landing Error Powered-Descent Guidance for Planetary Missions; 31) Framework for Integrating Science Data Processing Algorithms Into Process Control Systems; 32) Time Synchronization and Distribution Mechanisms for Space Networks; 33) Local Estimators for Spacecraft Formation Flying; 34) Software-Defined Radio for Space-to-Space Communications; 35) Reflective Occultation Mask for Evaluation of Occulter Designs for Planet Finding; and 36) Molecular Adsorber Coating

Sustainable Seas Student Intertidal Monitoring Project at Duxbury Reef in Bolinas, CA (Invited)

NASA Astrophysics Data System (ADS)

Soave, K.; Dean, A.; Darakananda, K.; Ball, O.; Butti, C.; Yang, G.; Vetter, M.; Grimaldi, Z.

2009-12-01

Sustainable Seas Student Intertidal Monitoring Project at Duxbury Reef in Bolinas, CA Kathy Soave, Amy Dean, Olivia Ball, Karin Darakananda, Matt Vetter, Grant Yang, Charlotte Butti, Zoe Grimaldi The Sustainable Seas Student Monitoring Project at the Branson School in Ross, CA has monitored Duxbury Reef in Bolinas, CA since 1999, in cooperation with the Farallones Marine Sanctuary Association and the Gulf of Farallones National Marine Sanctuary. Goals of the project include: 1) To monitor the rocky intertidal habitat and develop a baseline database of invertebrates and algal density and abundance; 2) To contribute to the conservation of the rocky intertidal habitat through education of students and visitors about intertidal species and the requirements for maintaining a healthy, diverse intertidal ecosystem; 3) To increase stewardship in the Gulf of the Farallones National Marine Sanctuary; and 4) To contribute abundance and population data on key algae and invertebrate species to the national database, LiMPETS (Long Term Monitoring Program & Experiential Training for Students). Student volunteers complete an intensive training course on the natural history of intertidal invertebrates and algae, identification of key species, rocky intertidal monitoring techniques, and history of the sanctuary. Students identify and count key invertebrate and algae species along two permanent transects (A and B) and using randomly determined points within a permanent 100 m2 area, three times per year (fall, winter, and late spring). Using the data collected since 2004, we will analyze the population densities, seasonal abundance and long-term population trends of key algal and invertebrate species. Future analyses and investigations will include intertidal abiotic factors (including water temperature and human foot-traffic) to enhance insights into the workings of the Duxbury Reef ecosystem, in particular, the high intertidal zone which experiences the greatest amount of human impacts. Kathy Soave The Branson School 39 Fernhill Rd. Ross, CA 94957 (415) 454-3612 x 323 Amy Dean Farallones Marine Sanctuary Association, PO Box 29386 San Francisco, CA 94129, 415-561-6625 x 303 AGU Sponsor, Ines Cifuentes, AGU membership number 10189667

Festive Nebulas Light Up Milky Way Galaxy Satellite

NASA Image and Video Library

2017-12-08

NASA’s Hubble Space Telescope captured two festive-looking nebulas, situated so as to appear as one. They reside in the Small Magellanic Cloud, a dwarf galaxy that is a satellite of our Milky Way galaxy. Intense radiation from the brilliant central stars is heating hydrogen in each of the nebulas, causing them to glow red. The nebulas, together, are called NGC 248. They were discovered in 1834 by the astronomer Sir John Herschel. NGC 248 is about 60 light-years long and 20 light-years wide. It is among a number of glowing hydrogen nebulas in the dwarf satellite galaxy, which is located approximately 200,000 light-years away in the southern constellation Tucana. The image is part of a study called Small Magellanic Cloud Investigation of Dust and Gas Evolution (SMIDGE). Astronomers are using Hubble to probe the Milky Way satellite to understand how dust is different in galaxies that have a far lower supply of heavy elements needed to create dust. The Small Magellanic Cloud has between a fifth and a tenth of the amount of heavy elements that the Milky Way does. Because it is so close, astronomers can study its dust in great detail, and learn about what dust was like earlier in the history of the universe. “It is important for understanding the history of our own galaxy, too,” explained the study’s principal investigator, Dr. Karin Sandstrom of the University of California, San Diego. Most of the star formation happened earlier in the universe, at a time where there was a much lower percentage of heavy elements than there is now. “Dust is a really critical part of how a galaxy works, how it forms stars,” said Sandstrom. Credit: NASA, ESA, STScI, K. Sandstrom (University of California, San Diego), and the SMIDGE team NASA image use policy. NASA Goddard Space Flight Center enables NASA’s mission through four scientific endeavors: Earth Science, Heliophysics, Solar System Exploration, and Astrophysics. Goddard plays a leading role in NASA’s accomplishments by contributing compelling scientific knowledge to advance the Agency’s mission. Follow us on Twitter Like us on Facebook Find us on Instagram

Lunar and Planetary Science XXXV: Asteroids, Meteors, Comets

NASA Technical Reports Server (NTRS)

2004-01-01

Reports included:Long Term Stability of Mars Trojans; Horseshoe Asteroids and Quasi-satellites in Earth-like Orbits; Effect of Roughness on Visible Reflectance Spectra of Planetary Surface; SUBARU Spectroscopy of Asteroid (832) Karin; Determining Time Scale of Space Weathering; Change of Asteroid Reflectance Spectra by Space Weathering: Pulse Laser Irradiation on Meteorite Samples; Reflectance Spectra of CM2 Chondrite Mighei Irradiated with Pulsed Laser and Implications for Low-Albedo Asteroids and Martian Moons; Meteorite Porosities and Densities: A Review of Trends in the Data; Small Craters in the Inner Solar System: Primaries or Secondaries or Both?; Generation of an Ordinary-Chondrite Regolith by Repetitive Impact; Asteroid Modal Mineralogy Using Hapke Mixing Models: Validation with HED Meteorites; Particle Size Effect in X-Ray Fluorescence at a Large Phase Angle: Importance on Elemental Analysis of Asteroid Eros (433); An Investigation into Solar Wind Depletion of Sulfur in Troilite; Photometric Behaviour Dependent on Solar Phase Angle and Physical Characteristics of Binary Near-Earth-Asteroid (65803) 1996 GT; Spectroscopic Observations of Asteroid 4 Vesta from 1.9 to 3.5 micron: Evidence of Hydrated and/or Hydroxylated Minerals; Multi-Wavelength Observations of Asteroid 2100 Ra-Shalom: Visible, Infrared, and Thermal Spectroscopy Results; New Peculiarities of Cometary Outburst Activity; Preliminary Shape Modeling for the Asteroid (25143) Itokawa, AMICA of Hayabusa Mission; Scientific Capability of MINERVA Rover in Hayabusa Asteroid Mission; Characteristics and Current Status of Near Infrared Spectrometer for Hayabusa Mission; Sampling Strategy and Curation Plan of Hayabusa Asteroid Sample Return Mission; Visible/Near-Infrared Spectral Properties of MUSES C Target Asteroid 25143 Itokawa; Calibration of the NEAR XRS Solar Monitor; Modeling Mosaic Degradation of X-Ray Measurements of 433 Eros by NEAR-Shoemaker; Scattered Light Remediation and Recalibration of near Sheomaker s NIS Global Dataaset at 433 Eros; Evaluation of Preparation and Measuring Techniques for Interplanetary Dust Particles for the MIDAS Experiment on Rosetta; Chiron: a Proposed Remote Sensing Prompt Gamma Ray Activation Analysis Instrument for a Nuclear Powered Prometheus Mission;From Present Surveying to Future Prospecting of the Asteroid Belt; Asteroid Physical Properties Probe Microgravity Testing of a Surface Sampling System for Sample Return from Small Solar System Bodies;and Penetrator Coring Apparatus for Cometary Surfaces.

On Hilbert-Huang Transform Based Synthesis of a Signal Contaminated by Radio Frequency Interference or Fringes

NASA Technical Reports Server (NTRS)

Kizhner, Semion; Shiri, Ron S.; Vootukuru, Meg; Coletti, Alessandro

2015-01-01

Norden E. Huang et al. had proposed and published the Hilbert-Huang Transform (HHT) concept correspondently in 1996, 1998. The HHT is a novel method for adaptive spectral analysis of non-linear and non-stationary signals. The HHT comprises two components: - the Huang Empirical Mode Decomposition (EMD), resulting in an adaptive data-derived basis of Intrinsic Mode functions (IMFs), and the Hilbert Spectral Analysis (HSA1) based on the Hilbert Transform for 1-dimension (1D) applied to the EMD IMF's outcome. Although paper describes the HHT concept in great depth, it does not contain all needed methodology to implement the HHT computer code. In 2004, Semion Kizhner and Karin Blank implemented the reference digital HHT real-time data processing system for 1D (HHT-DPS Version 1.4). The case for 2-Dimension (2D) (HHT2) proved to be difficult due to the computational complexity of EMD for 2D (EMD2) and absence of a suitable Hilbert Transform for 2D spectral analysis (HSA2). The real-time EMD2 and HSA2 comprise the real-time HHT2. Kizhner completed the real-time EMD2 and the HSA2 reference digital implementations respectively in 2013 & 2014. Still, the HHT2 outcome synthesis remains an active research area. This paper presents the initial concepts and preliminary results of HHT2-based synthesis and its application to processing of signals contaminated by Radio-Frequency Interference (RFI), as well as optical systems' fringe detection and mitigation at design stage. The Soil Moisture Active Passive (SMAP mission (SMAP) carries a radiometer instrument that measures Earth soil moisture at L1 frequency (1.4 GHz polarimetric - H, V, 3rd and 4th Stokes parameters). There is abundant RFI at L1 and because soil moisture is a strategic parameter, it is important to be able to recover the RFI-contaminated measurement samples (15% of telemetry). State-of-the-art only allows RFI detection and removes RFI-contaminated measurements. The HHT-based analysis and synthesis facilitates recovery of measurements contaminated by all kinds of RFI, including jamming [7-8]. The fringes are inherent in optical systems and multi-layer complex contour expensive coatings are employed to remove the unwanted fringes. HHT2-based analysis allows test image decomposition to analyze and detect fringes, and HHT2-based synthesis of useful image.

Ridge interaction features of the Line Islands

NASA Astrophysics Data System (ADS)

Konter, J. G.; Koppers, A. A. P.; Storm, L. P.

2016-12-01

The sections of Pacific absolute plate motion history that precede the Hawaii-Emperor and Louisville chains are based on three chains: the Line Islands-Mid-Pacific Mountains, the Hess Rise-Shatsky Rise, and the Marshall Islands-Wake Islands (Rurutu hotspot). Although it has been clear that the Line Islands do not define a simple age progression (e.g. Schlanger et al., 1984), the apparent similarity to the Emperor Seamount geographic trend has been used to extend the overall Hawaii-Emperor track further into the past. However, we show here that plate tectonic reconstructions suggest that the Mid-Pacific Mountains (MPMs) and Line Islands (LIs) were erupted near a mid-ocean ridge, and thus these structures do not reflect absolute plate motion. Moverover, the morphology and geochemistry of the volcanoes show similarities with Pukapuka Ridge (e.g. Davis et al., 2002) and the Rano Rahi seamounts, presumed to have a shallow origin. Modern 40Ar/39Ar ages show that the LIs erupted at various times along the entire volcanic chain. The oldest structures formed within 10 Ma of plate formation. Given the short distance to the ridge system, large aseismic volcanic ridges, such as Necker Ridge and Horizon Guyot may simply reflect a connection between MPMs and the ridge, similar to the Pukapuka Ridge. The Line Islands to the south (including Karin Ridge) define short subchains of elongated seamounts that are widespread, resembling the Rano Rahi seamount field. During this time, the plate moved nearly parallel to the ridge system. The change from few large ridges to many subchains may reflect a change in absolute plate motion, similar to the Rano Rahi field. Here, significant MPMs volcanism is no longer connected to the ridge along plate motion. Similar to Pukapuka vs. Rano Rahi, the difference in direction between plate motion and the closest ridge determines whether larger ridges or smaller seamount subchains are formed. The difference between the largest structures (MPMs and LIs ridge south of Clarion fracture zone) may result from their formation near microplate triple junctions, above the edges of the LLSVPs, during increased spreading rates of the Cretaceous. Unusually strong passive upwelling may have sampled dense fertile material (Korenaga, 2005) from the LLSVP generating a LIP without a hotspot chain.

"Wish You Were Here": Examining Characteristics, Outcomes, and Statistical Solutions for Missing Cases in Web-Based Psychotherapeutic Trials.

PubMed

Karin, Eyal; Dear, Blake F; Heller, Gillian Z; Crane, Monique F; Titov, Nickolai

2018-04-19

Missing cases following treatment are common in Web-based psychotherapy trials. Without the ability to directly measure and evaluate the outcomes for missing cases, the ability to measure and evaluate the effects of treatment is challenging. Although common, little is known about the characteristics of Web-based psychotherapy participants who present as missing cases, their likely clinical outcomes, or the suitability of different statistical assumptions that can characterize missing cases. Using a large sample of individuals who underwent Web-based psychotherapy for depressive symptoms (n=820), the aim of this study was to explore the characteristics of cases who present as missing cases at posttreatment (n=138), their likely treatment outcomes, and compare between statistical methods for replacing their missing data. First, common participant and treatment features were tested through binary logistic regression models, evaluating the ability to predict missing cases. Second, the same variables were screened for their ability to increase or impede the rate symptom change that was observed following treatment. Third, using recontacted cases at 3-month follow-up to proximally represent missing cases outcomes following treatment, various simulated replacement scores were compared and evaluated against observed clinical follow-up scores. Missing cases were dominantly predicted by lower treatment adherence and increased symptoms at pretreatment. Statistical methods that ignored these characteristics can overlook an important clinical phenomenon and consequently produce inaccurate replacement outcomes, with symptoms estimates that can swing from -32% to 70% from the observed outcomes of recontacted cases. In contrast, longitudinal statistical methods that adjusted their estimates for missing cases outcomes by treatment adherence rates and baseline symptoms scores resulted in minimal measurement bias (<8%). Certain variables can characterize and predict missing cases likelihood and jointly predict lesser clinical improvement. Under such circumstances, individuals with potentially worst off treatment outcomes can become concealed, and failure to adjust for this can lead to substantial clinical measurement bias. Together, this preliminary research suggests that missing cases in Web-based psychotherapeutic interventions may not occur as random events and can be systematically predicted. Critically, at the same time, missing cases may experience outcomes that are distinct and important for a complete understanding of the treatment effect. ©Eyal Karin, Blake F Dear, Gillian Z Heller, Monique F Crane, Nickolai Titov. Originally published in JMIR Mental Health (http://mental.jmir.org), 19.04.2018.

Social Health Inequalities and eHealth: A Literature Review With Qualitative Synthesis of Theoretical and Empirical Studies.

PubMed

Latulippe, Karine; Hamel, Christine; Giroux, Dominique

2017-04-27

eHealth is developing rapidly and brings with it a promise to reduce social health inequalities (SHIs). Yet, it appears that it also has the potential to increase them. The general objective of this review was to set out how to ensure that eHealth contributes to reducing SHIs rather than exacerbating them. This review has three objectives: (1) identifying characteristics of people at risk of experiencing social inequality in health; (2) determining the possibilities of developing eHealth tools that avoid increasing SHI; and (3) modeling the process of using an eHealth tool by people vulnerable to SHI. Following the EPPI approach (Evidence for Policy and Practice of Information of the Institute of Education at the University of London), two databases were searched for the terms SHIs and eHealth and their derivatives in titles and abstracts. Qualitative, quantitative, and mixed articles were included and evaluated. The software NVivo (QSR International) was employed to extract the data and allow for a metasynthesis of the data. Of the 73 articles retained, 10 were theoretical, 7 were from reviews, and 56 were based on empirical studies. Of the latter, 40 used a quantitative approach, 8 used a qualitative approach, 4 used mixed methods approach, and only 4 were based on participatory research-action approach. The digital divide in eHealth is a serious barrier and contributes greatly to SHI. Ethnicity and low income are the most commonly used characteristics to identify people at risk of SHI. The most promising actions for reducing SHI via eHealth are to aim for universal access to the tool of eHealth, become aware of users' literacy level, create eHealth tools that respect the cultural attributes of future users, and encourage the participation of people at risk of SHI. eHealth has the potential to widen the gulf between those at risk of SHI and the rest of the population. The widespread expansion of eHealth technologies calls for rigorous consideration of interventions, which are not likely to exacerbate SHI. ©Karine Latulippe, Christine Hamel, Dominique Giroux. Originally published in the Journal of Medical Internet Research (http://www.jmir.org), 27.04.2017.

Obituary: Einar A. Tandberg-Hanssen (1921-2011)

NASA Astrophysics Data System (ADS)

Gary, G.; Emslie, A.; Hathaway, David; Moore, Ronald

2011-12-01

Dr. Einar Andreas Tandberg-Hanssen was born on 6 August 1921, in Bergen, Norway, and died on July 22, 2011, in Huntsville, AL, USA, due to complications from ALS (Amyotrophic lateral sclerosis, often referred to as Lou Gehrig's disease). His parents were administrator Birger Tandberg-Hanssen (1883-1951) and secretary Antonie "Mona" Meier (1895-1967). He married Erna Rönning (27 October 1921 - 22 November 1994), a nurse, on 22 June 1951. She was the daughter of Captain Einar Rönning (1890-1969) and Borghild Lyshaug (1897-1980). Einar and Erna had two daughters, Else Biesman (and husband Allen of Rapid City, SD, USA) and Karin Brock (and husband Mike of Gulf Shores, AL, USA). At the time of his death Einar had eight grandchildren and eight great-grandchildren. Dr. Tandberg-Hanssen was an internationally-known member of the solar physics community, with over a hundred published scientific papers and several books, including Solar Activity (1967), Solar Prominences (1974), The Physics of Solar Flares (1988) and The Nature of Solar Prominences (1995). Einar grew up in Langesund and Skien, Norway, where he took the qualifying exams at Skien High School in 1941. After the war he studied natural sciences at the University of Oslo and received his undergraduate degree in astronomy in 1950. He worked as a research assistant in the Institute of Theoretical Astrophysics at the University of Oslo for three intervals in the 1950s, interspersed by fellowships at the Institut d'Astrophysique in Paris, Caltech in Pasadena, CA, the High Altitude Observatory in Boulder, CO, and the Cavendish Laboratory in the UK (at the invitation of British radio-astronomer Sir Martin Ryle). He earned a doctorate in astrophysics at the University in Oslo in 1960 with a dissertation titled "An Investigation of the Temperature Conditions in Prominences with a Special Study of the Excitation of Helium." From 1959-61, Tandberg-Hanssen was a professor at the University in Oslo. He then traveled back to the High Altitude Observatory in Boulder, Colorado, where he was employed until 1974. He was then employed at the Space Science Laboratory at NASA's Marshall Space Flight Center (MSFC) in Huntsville, Alabama. There, he was a Senior Research Scientist and later Deputy Director of the Laboratory. He served as Lab Director from 1987 until his retirement from NASA in 1993. He promptly took a part-time post within the Center for Space Plasma and Aeronomic Research at The University of Alabama in Huntsville, where he worked until his death. During his tenure at NASA, he, along with Dr. Mona Hagyard and Dr. S. T. Wu, built up a substantial, internationally-based group of solar physicists at MSFC and UA Huntsville. He was a lead investigator on two instruments aboard NASA spacecraft: the S-056 X-Ray Event Analyzer on the Skylab Apollo Telescope Mount (which provided pioneering, high-time-cadence temperature and density information on solar X-ray-emitting regions) and the Ultraviolet Spectrometer and Polarimeter on the Solar Maximum Mission (which carried out sweeping new studies of EUV emission from solar active regions and flares). Dr. Tandberg-Hanssen's books about various aspects of solar activity, viz.Solar Activity (Blaisdell, 1967), Solar Prominences (Reidel, 1974), The Physics of Solar Flares (with A. G. Emslie) (Cambridge, 1988), and The Nature of Solar Prominences (Reidel, 1995), have become international standard works within the discipline of solar physics. In 1982, Dr. Tandberg-Hanssen was elected to membership in the Norwegian Academy of Science and Letters. From 1979-82 and 1982-85, respectively, he served as vice-president and president of Commission 10 of the International Astronomical Union (IAU). He served as president of the Federation of Astronomical and Geophysical Data Analysis Services from 1990-1994. He has received the NASA Exceptional Service Medal. He was also a long time editor of the journal Solar Physics. Dr. Tandberg-Hanssen's Solar Physics Memoir paper, entitled Solar Prominences - An Intriguing Phenomenon http://www.springerlink.com/content/1166j74k577kv332/ was published shortly before his death. The article starts with an autobiographical account, where the author relates how his several study-trips abroad gradually led him to the study of solar physics in general, and prominences particularly. Einar's residence as a research fellow at the Institut d'Astrophysique in Paris in the 1950s laid the foundation for a lifelong interest in France and French culture. His great interest in and knowledge of French mediaeval churches, as well as the Norwegian stave churches, is reflected in two books, Letters to My Daughters (Ivy House Pub. Group, 2004), and The Joy of Travel: More Letters to My Daughters (Pentland Press, 2007), which serve as a review, tourist guide and history book, shaped in the form of letters home to his two daughters, from his many travels in Norway and France. Einar was a true gentleman and a true scholar. As evidenced by his papers, his books, and his dealings with others, he was always seeking not only to expand his own knowledge and understanding, but also to find new ways of communicating his remarkable insight to others. He is survived by his daughters, Else and Karin, and their families.

Biological soil crusts in Chile along the precipitation gradient

NASA Astrophysics Data System (ADS)

Samolov, Elena; Glaser, Karin; Baumann, Karen; Leinweber, Peter; Jung, Patrick; Büdel, Burkhard; Mikhailyuk, Tatiana; Karsten, Ulf

2017-04-01

Biological soil crusts in Chile along a precipitation gradient Elena Samolov* (1), Karin Glaser (1), Karen Baumann (2), Peter Leinweber (2), Patrick Jung (3), Burkhard Büdel (3), Tatiana Mikhailyuk (4) and Ulf Karsten (1) (1) Institute of Biological Sciences - Applied Ecology and Phycology, University of Rostock, Rostock, Germany, (2) Faculty of Agricultural and Environmental Sciences - Soil Sciences, University of Rostock, Rostock, Germany (3) University of Kaiserslautern, Kaiserslautern, Germany (4) M.H. Kholodny Institute of Botany, National Academy of Science of Ukraine, Kyiv, Ukraine * elena.samolov@uni-rostock.de Biological soil crusts (BSCs) are an association of different microorganisms and soil particles in the top millimeters of the soil. They are formed by algae, cyanobacteria, microfungi, bacteria, bryophytes and lichens in various compositions; together with their by-products they create a micro-ecosystem that performs important ecological functions, e.g. primary production, nitrogen fixation, mineralization and stabilization of soils. These top-soil assemblages are almost unstudied in South America (Büdel et al. 2016). Therefore, our aim is to investigate for the first time biodiversity of the key photosynthetic organisms, green algae and cyanobacteria following a precipitation gradient along the west coast of Chile. We are applying polyphasic approach - a combination of microscopy, culture dependent (16S and 18S rRNA, ITS) and culture independent molecular techniques (NGS). First results, based on culturing and light microscopy, showed high diversity of eukaryotic algae in biocrusts from humid regions, followed by semi-arid regions. Lichen dominated biocrusts from arid regions were characterized by a high diversity of green algae, while cyanobacteria were scarcely present. The functional role of the BSCs in the biogeochemical cycle of phosphorous (P) was evaluated using state of the art analytical methods including 31P-NMR (nuclear magnetic resonance) spectroscopy and P K-edge XANES (x-ray absorbance near edge structures). Total P as well as P fractions were quantified in all BSCs, adjacent soil underneath and comparable nearby soil of BSC-free areas, revealing a slight accumulation of total phosphorous and a distinct pattern of P fractions in the crust. Our study describes for the first time the diversity of photosynthetic organisms in BSCs along a precipitation gradient in South America and their functional role in biogeochemical cycle of phosphorus as an important macronutrient. Reference: Büdel et al. "Cyanobacteria and Algae of Biological soil crusts". In B. Weber et al. (eds.), Biological Soli Crusts: An Organizing Principle in Drylands, Ecological Studies 226, Springer International Publishing Switzerland: 2016. (pp. 55-80).

Adherence to Report and Patient Perception of an Interactive App for Managing Symptoms During Radiotherapy for Prostate Cancer: Descriptive Study of Logged and Interview Data.

PubMed

Langius-Eklöf, Ann; Christiansen, Mats; Lindström, Veronica; Blomberg, Karin; Hälleberg Nyman, Maria; Wengström, Yvonne; Sundberg, Kay

2017-10-31

Patients undergoing radiotherapy for prostate cancer experience symptoms related to both the cancer itself and its treatment, and it is evident that patients with prostate cancer have unmet supportive care needs related to their disease. Over the past decade, there has been an increase in the amount of research within the field of mobile health and the use of apps as tools for managing illness. The main challenge is to develop a mobile technology to its full potential of being interactive in real time. The interactive app Interaktor, which aims to identify and manage symptoms in real time includes (1) a function for patients' assessment of the occurrence, frequency, and distress of symptoms; (2) a connection to a monitoring Web interface; (3) a risk assessment model that sends alerts via text message to health care providers; (4) continuous access to evidence-based self-care advice and links to relevant websites for more information; and (5) graphs for the patients and health care providers to view the history of symptom reporting. The aim of the study was to investigate user behavior, adherence to reporting, and the patients' experiences of using Interaktor during radiotherapy for localized advanced prostate cancer. The patients were instructed to report daily during the time of treatment and then for an additional 3 weeks. Logged data from patients' use of the app were analyzed with descriptive statistics. Interview data about experiences of using the app were analyzed with content analysis. A total of 66 patients participated in the study. Logged data showed that adherence to daily reporting of symptoms was high (87%). The patients used all the symptoms included in the app. Of the reports, 15.6% generated alerts to the health care providers. Overall, the patients found that it was easy and not particularly time-consuming to send a daily report, and many described it as becoming a routine. Reporting symptoms facilitated reflection on their symptoms and gave them a sense of security. Few technological problems were reported. The use of Interaktor increased patients' sense of security and their reflections on their own well-being and thereby served as a supportive tool for the self-management of symptoms during treatment of prostate cancer. Some further development of the app's content might be beneficial for future use. ©Ann Langius-Eklöf, Mats Christiansen, Veronica Lindström, Karin Blomberg, Maria Hälleberg Nyman, Yvonne Wengström, Kay Sundberg. Originally published in JMIR Cancer (http://cancer.jmir.org), 31.10.2017.

Universal Versus Conditional Third Day Follow-Up Visit for Children With Nonsevere Unclassified Fever at the Community Level in Ethiopia: Protocol for a Cluster Randomized Noninferiority Trial.

PubMed

Källander, Karin; Alfven, Tobias; Workineh, Ayalkibet Abebe; Hailemariam, Abreham; Petzold, Max; Getachew, Dawit; Barat, Lawrence; Steinhardt, Laura C; Gutman, Julie R

2018-04-12

Under the World Health Organization's integrated community case management strategy, febrile children seen by community health workers (on day 1) without a diagnosable illness and without danger signs are advised to return on day 3, regardless of symptom resolution. This advice might be unnecessary and place additional time and cost burdens on caregivers and community health workers. However, the safety of not following up with respect to children with unclassified fever is unknown. The objective of this study is to establish the safety of conditional follow-up of nonsevere unclassified fever, that is, nonsevere illness with fever, no malaria, pneumonia, diarrhea, or danger signs, compared with universal follow-up on day 3, through a 2-arm cluster randomized controlled noninferiority trial. The study is being conducted in 3 districts in southwest Ethiopia. A total of 25 health facilities are randomized to one of the 2 intervention arms; all 144 health posts and 284 community health workers are included. All enrolled children are followed-up after 1 week (on day 8) for re-assessment. If still sick on day 8, additional follow-up takes place after 2 weeks (day 15) and 1 month (day 29). To demonstrate that there is no significant increase in the percentage of children deteriorating clinically, the sample size needed for a noninferiority margin of 4%, a power of 80%, an alpha of 5%, and a design effect of 3 is 4284 children with unclassified fever. Main outcome is treatment failure on day 8, defined as death, hospitalization, one or more danger signs, or persistent fever. The project was funded in 2015 and enrollment was completed 2016. Data analysis is currently under way, and the first results are expected to be submitted for publication in 2018. This study addresses the question as to whether there is any benefit in recommending universal follow-up among children seen for nonsevere unclassified fever, or whether parents can be counseled to return in the event of persistent fever, using a cluster randomized controlled trial design embedded in a national program. Outcomes will be relevant for policy makers and are important for the evaluation of current and future World Health Organization guidelines for the management of children with fever. ClinicalTrials.gov NCT02926625; https://clinicaltrials.gov/ct2/show/NCT02926625 (Archived by WebCite at http://www.webcitation.org/6xrQWn50t). ©Karin Källander, Tobias Alfven, Ayalkibet Abebe Workineh, Abreham Hailemariam,, Max Petzold, Dawit Getachew, Lawrence Barat, Laura C Steinhardt, Julie R Gutman. Originally published in JMIR Research Protocols (http://www.researchprotocols.org), 12.04.2018.

The Epital Care Model: A New Person-Centered Model of Technology-Enabled Integrated Care for People With Long Term Conditions.

PubMed

Phanareth, Klaus; Vingtoft, Søren; Christensen, Anders Skovbo; Nielsen, Jakob Sylvest; Svenstrup, Jørgen; Berntsen, Gro Karine Rosvold; Newman, Stanton Peter; Kayser, Lars

2017-01-16

There is worldwide recognition that the future provision of health care requires a reorganization of provision of care, with increased empowerment and engagement of patients, along with skilled health professionals delivering services that are coordinated across sectors and organizations that provide health care. Technology may be a way to enable the creation of a coherent, cocreative, person-centered method to provide health care for individuals with one or more long-term conditions (LTCs). It remains to be determined how a new care model can be introduced that supports the intentions of the World Health Organization (WHO) to have integrated people-centered care. To design, pilot, and test feasibility of a model of health care for people with LTCs based on a cocreative, iterative, and stepwise process in a way that recognizes the need for person-centered care, and embraces the use of digital technology. The overall research method was inspired by action research and used an agile, iterative approach. In 2012, a living lab was established in a Danish municipality which allowed for the freedom of redesigning health care processes. As the first step, a wide group of stakeholders was gathered to create a layout for the reorganization of services and development of technology, based on established principles for innovative management of people with chronic conditions. The next three steps were (1) a proof of concept in 2012, (2) a pilot study, and (3) a feasibility study from 2013 to 2015, in which a total of 93 chronic obstructive pulmonary disease (COPD) patients were enrolled. Citizens were provided a tablet-based solution for remote follow-up and communication purposes, and access to a 24/7 response and coordination center that coordinated both virtual and face-to-face support for COPD management. In step five the initial model was extended with elements that support continuity of care. Beginning in the autumn of 2013, 1102 frail elderly individuals were included and offered two additional services: an outgoing acute medical team and a local subacute bed function. Based on the findings from the iterative process, and evolving technology and workflow solutions, we propose a robust and feasible model that can provide a framework for developing solutions to support an active life with one or more LTCs. The resulting Epital Care Model (ECM) consists of six stages, and serves as a template for how a digitally-enhanced health service can be provided based on patients' medical needs. The model is designed to be a proactive, preventive, and monitoring health care system that involves individuals in the management of their own health conditions. The ECM is in accordance with WHO's framework for integrated people-centered health services, and may serve as a framework for the development of new technologies and provide a template for future reorganization. ©Klaus Phanareth, Søren Vingtoft, Anders Skovbo Christensen, Jakob Sylvest Nielsen, Jørgen Svenstrup, Gro Karine Rosvold Berntsen, Stanton Peter Newman, Lars Kayser. Originally published in JMIR Research Protocols (http://www.researchprotocols.org), 16.01.2017.

Reach and Acceptability of a Mobile Reminder Strategy and Facebook Group Intervention for Weight Management in Less Advantaged Adolescents: Insights From the PRALIMAP-INÈS Trial.

PubMed

Saez, Laura; Langlois, Johanne; Legrand, Karine; Quinet, Marie-Hélène; Lecomte, Edith; Omorou, Abdou Y; Briançon, Serge

2018-05-18

Although information and communication technology interventions appear to be a promising means of reducing the health inequality gap in overweight and obesity prevention, research on information and communication technology interventions is lacking outside the Anglo-Saxon world. The aim of this study was to assess the reach and acceptability of 2 information and communication technology interventions delivered as part of a French nutritional program: an SMS text messaging (short message service, SMS) attendance-reminder for collective sessions strategy and a Facebook challenge group. This study sample comprised 262 socially less advantaged overweight adolescents aged between 13 and 18 years. The information and communication technology interventions were carried out during the 2013-2014 academic year in 33 French state-run schools. For the SMS attendance-reminder for collective sessions strategy, at the start of the academic year, adolescents were asked to give their mobile number. SMS attendance-reminders were sent shortly before each of the 5 collective sessions. For the Facebook challenge group, adolescents were invited to join a closed Facebook group in which challenges on physical activity and on diet were posted weekly. Process data and 2 sets of face-to-face interviews were also used to interpret participation rates and access to Facebook. Appreciation for both interventions was evaluated by a questionnaire at the end of the academic year. Of the recruited adolescents, 79.0% (207/262) gave their mobile number, reflecting high access to a mobile phone. Giving a number was significantly more likely for girls (odds ratio [OR] 2.1, 95% CI 1.1-3.9; P=.02) and adolescents in a vocational or general high school as opposed to middle school (OR 1.0, 95% CI 0.4-2.7; OR 0.2, 95% CI 0.1-0.5; P<.001). Indicating a mobile number at the start of the year was not significantly associated with participation in collective sessions. Of the adolescents seen at the start-of-year face-to-face interviews, 78.1% (153/196) declared an interest in the Facebook challenge group, which implies having a Facebook account or being able to have access to one. However, only 21 adolescents went through the process of joining the group. Although there was satisfaction with the Facebook group among the participants, the low participation rate in the Facebook group does not allow conclusions to be drawn with confidence. The results are in line with the claim that using information and communication technologies in health programs is unlikely to widen health inequalities. However, in this population of French adolescents, mobile phone strategies seem more adapted to a high school context, and caution should be exercised with a younger audience. Although there is positive appreciation of the SMS attendance-reminders and a Facebook intervention is initially highly appealing to less advantaged adolescents, no evidence of impact could be demonstrated. These results highlight the difficulty in assessing the impact of specific interventions in complex health programs. Clinicaltrials.gov NCT01688453; https://clinicaltrials.gov/ct2/show/NCT01688453 (Archived by WebCite at http://www.webcitation.org/6yy6EQ0SM). ©Laura Saez, Johanne Langlois, Karine Legrand, Marie-Hélène Quinet, Edith Lecomte, Abdou Y Omorou, Serge Briançon, PRALIMAP-INÈS Trial Group. Originally published in JMIR Mhealth and Uhealth (http://mhealth.jmir.org), 18.05.2018.

The Hawaii trails project: comet-hunting in the main asteroid belt

NASA Astrophysics Data System (ADS)

Hsieh, H. H.

2009-10-01

Context: The mysterious solar system object 133P/(7968) Elst-Pizarro is dynamically asteroidal, yet displays recurrent comet-like dust emission. Two scenarios were hypothesized to explain this unusual behavior: 1) 133P is a classical comet from the outer solar system that has evolved onto a main-belt orbit or 2) 133P is a dynamically ordinary main-belt asteroid on which subsurface ice has recently been exposed. If 1) is correct, the expected rarity of a dynamical transition onto an asteroidal orbit implies that 133P could be alone in the main belt. In contrast, if 2) is correct, other icy main-belt objects should exist and could also exhibit cometary activity. Aims: Believing 133P to be a dynamically ordinary, yet icy main-belt asteroid, I set out to test the primary prediction of the hypothesis: that 133P-like objects should be common and could be found by an appropriately designed observational survey. Methods: I conducted just such a survey - the Hawaii Trails Project - of selected main-belt asteroids in a search for objects displaying cometary activity. Optical observations were made of targets selected from among the Themis, Koronis, and Veritas asteroid families, the Karin asteroid cluster, and low-inclination, kilometer-scale outer-belt asteroids, using the Lulin 1.0 m, small and moderate aperture research telescope system (SMARTS) 1.0 m, University of Hawaii 2.2 m, southern astrophysical research (SOAR) 4.1 m, Gemini North 8.1 m, Subaru 8.2 m, and Keck I 10 m telescopes. Results: I made 657 observations of 599 asteroids, discovering one active object now known as 176P/LINEAR, leading to the identification of the new cometary class of main-belt comets (MBCs). These results suggest that there could be ~100 currently active MBCs among low-inclination, kilometer-scale outer-belt asteroids. Physically and statistically, MBC activity is consistent with initiation by meter-sized impactors. The estimated rate of impacts and sizes of resulting active sites, however, imply that 133P-sized bodies should become significantly devolatilized over Gyr timescales, suggesting that 133P, and possibly the other MBCs as well, could be secondary, or even multigenerational, fragments from recent breakup events. Some of the data presented herein were obtained at the W. M. Keck Observatory, the Gemini Observatory, Subaru Telescope, National Optical Astronomy Observatory (NOAO) facilities at the Cerro Tololo Inter-American Observatory, and Lulin Observatory. Keck is operated as a scientific partnership among the California Institute of Technology, the University of California, and the National Aeronautics and Space Administration, and was made possible by the generous financial support of the W. M. Keck Foundation. Gemini is operated by the Association of Universities for Research in Astronomy, Inc., under a cooperative agreement with the National Science Foundation (NSF) on behalf of the Gemini partnership. Subaru is operated by the National Astronomical Observatory of Japan. NOAO and Cerro Tololo are operated by the Association of Universities for Research in Astronomy, Inc., under co-operative agreement with the NSF. Lulin is supported and was made possible by the National Science Council of Taiwan, the Ministry of Education of Taiwan, and National Central University. Table [see full textsee full textsee full text] is available in its entirety in electronic form at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsweb.u-strasbg.fr/cgi-bin/qcat?J/A+A/505/1297 Table 2 is only available in electronic form at http://www.aanda.org

NASA Announces 2009 Astronomy and Astrophysics Fellows

NASA Astrophysics Data System (ADS)

2009-02-01

WASHINGTON -- NASA has selected fellows in three areas of astronomy and astrophysics for its Einstein, Hubble, and Sagan Fellowships. The recipients of this year's post-doctoral fellowships will conduct independent research at institutions around the country. "The new fellows are among the best and brightest young astronomers in the world," said Jon Morse, director of the Astrophysics Division in NASA's Science Mission Directorate in Washington. "They already have contributed significantly to studies of how the universe works, the origin of our cosmos and whether we are alone in the cosmos. The fellowships will serve as a springboard for scientific leadership in the years to come, and as an inspiration for the next generation of students and early career researchers." Each fellowship provides support to the awardees for three years. The fellows may pursue their research at any host university or research center of their choosing in the United States. The new fellows will begin their programs in the fall of 2009. "I cannot tell you how much I am looking forward to spending the next few years conducting research in the U.S., thanks to the fellowships," said Karin Oberg, a graduate student in Leiden, The Netherlands. Oberg will study the evolution of water and ices during star formation when she starts her fellowship at the Smithsonian Astrophysical Observatory in Cambridge, Mass. People Who Read This Also Read... Milky Way's Super-efficient Particle Accelerators Caught in The Act Cosmic Heavyweights in Free-for-all Galaxies Coming of Age in Cosmic Blobs Cassiopeia A Comes Alive Across Time and Space A diverse group of 32 young scientists will work on a wide variety of projects, such as understanding supernova hydrodynamics, radio transients, neutron stars, galaxy clusters and the intercluster medium, supermassive black holes, their mergers and the associated gravitational waves, dark energy, dark matter and the reionization process. Other research topics include searching for transits among hot Neptunes and super-Earths, microlensing planets through modeling algorithms, conducting high-contrast imaging surveys to detect planetary-mass companions, interferometrically imaging of the inner regions of protoplanetary disks, and modeling of super-Earth planetary atmospheres. The 10 fellows in the Einstein program conduct research broadly related to the mission of NASA's Physics of the Cosmos Program. Its science goals include understanding the origin and destiny of the universe, the nature of gravity, phenomena near black holes, and extreme states of matter. The Chandra X-ray Center in Cambridge, Mass., administers the Einstein Fellowships for NASA. The 17 awardees of the Hubble Fellowship pursue research associated with NASA's Cosmic Origins Program. The missions in this program examine the origins of galaxies, stars, and planetary systems, and the evolution of these structures with cosmic time. The Space Telescope Science Institute in Baltimore, Md., administers the Hubble Fellowships for NASA. The Sagan Fellowship, created in September 2008, supports five scientists whose research is aligned with NASA's Exoplanet Exploration Program. The primary goal of this program is to discover and characterize planetary systems and Earth-like planets around other stars. The NASA Exoplanet Science Institute, which is operated at the California Institute of Technology in coordination with NASA's Jet Propulsion Laboratory in Pasadena, Calif., administers the Sagan Fellowship Program

Young People, Adult Worries: Randomized Controlled Trial and Feasibility Study of the Internet-Based Self-Support Method "Feel the ViBe" for Adolescents and Young Adults Exposed to Family Violence.

PubMed

van Rosmalen-Nooijens, Karin; Lo Fo Wong, Sylvie; Prins, Judith; Lagro-Janssen, Toine

2017-06-12

Adolescents and young adults (AYAs) are of special interest in a group of children exposed to family violence (FV). Past-year prevalence of exposure to FV is known to be highest in AYAs and has severe consequences. Peer support is an effective approach to behavior change and the Internet is considered suitable as a mode of delivery. The study aimed to evaluate both effectiveness and feasibility of a randomized controlled trial (RCT) and feasibility study of the Internet-based self-support method "Feel the ViBe" (FtV) using mixed-methods approach to fully understand the strengths and weaknesses of a new intervention. AYAs aged 12-25 years and exposed to FV were randomized in an intervention group (access to FtV + usual care) and a control group (minimally enhanced usual care) after they self-registered themselves. From June 2012 to July 2014, participants completed the Impact of Event Scale (IES) and Depression (DEP) and Anxiety (ANX) subscales of the Symptom CheckList-90-R (SCL-90) every 6 weeks. The Web Evaluation Questionnaire was completed after 12 weeks. Quantitative usage data were collected using Google analytics and content management system (CMS) logs and data files. A univariate analysis of variance (UNIANOVA) and mixed model analysis (intention-to-treat [ITT], complete case) were used to compare groups. Pre-post t tests were used to find within-group effects. Feasibility measures structurally address the findings. The CONsolidated Standards Of Reporting Trials of Electronic and Mobile HEalth Applications and onLine TeleHealth (CONSORT-EHEALTH) checklist was closely followed. In total, 31 out of 46 participants in the intervention group and 26 out of 47 participants in the control group started FtV. Seventeen participants (intervention: n=8, control: n=9) completed all questionnaires. Mixed model analysis showed significant differences between groups on the SCL-90 DEP (P=.04) and ANX (P=.049) subscales between 6 and 12 weeks after participation started. UNIANOVA showed no significant differences. Pre-post paired sample t tests showed significant improvements after 12 weeks for the SCL-90 DEP (P=.03) and ANX (P=.046) subscales. Reported mean Web-based time per week was 2.83 with a session time of 36 min. FtV was rated a mean 7.47 (1-10 Likert scale) with a helpfulness score of 3.16 (1-5 Likert scale). All participants felt safe. Two-thirds of the intervention participants started regular health care. No changes on the IES were found. SCL-90 DEP and ANX showed promising results; however, the calculated sample size was not reached (n=18). FtV functions best as a first step for adolescents and young adults in an early stage of change. FtV can be easily implemented without extensive resources and fits best in the field of public health care or national governmental care. Netherlands National Trial Register (NTR): NTR3692; http://www.trialregister.nl/trialreg/admin/ rctview.asp?TC=3692 (Archived by WebCite at http://www.webcitation.org/6qIeKyjA4). ©Karin van Rosmalen-Nooijens, Sylvie Lo Fo Wong, Judith Prins, Toine Lagro-Janssen. Originally published in the Journal of Medical Internet Research (http://www.jmir.org), 12.06.2017.

Voluminous low-T granite: fluid present partial melting of the crust?

NASA Astrophysics Data System (ADS)

Hand, Martin; Barovich, Karin; Morrissey, Laura; Bockmann, Kiara; Kelsey, David; Williams, Megan

2017-04-01

Voluminous low-T granite: fluid present partial melting of the crust? Martin Hand(1), Karin Barovich(1), Laura Morrissey(1), Vicki Lau(1), Kiara Bockmann(1), David Kelsey(1), Megan Williams(1) (1) Department of Earth Sciences, University of Adelaide, Adelaide, Australia Two general schools of thought exist for the formation of granites from predominantly crustal sources. One is that large-scale anatexis occurs via fluid-absent partial melting. This essentially thermal argument is based on the reasonable premise that the lower crust is typically fluid depleted, and experimental evidence which indicates that fluid-absent partial melting can produce significant volumes of melt, creating compositionally depleted residua that many believe are recorded by granulite facies terranes. The other school of thought is that large-scale anatexis can occur via fluid-fluxed melting. This essentially compositional-based contention is also supported by experimental evidence which shows that fluid-fluxed melting is efficient, including at temperatures not much above the solidus. However, generating significant volumes of melt at low temperatures requires a large reservoir of fluid. If fluid-fluxed melting is a realistic model, the resultant granites should be comparatively low temperature compared to those derived from predominantly fluid-absent partial melting. Using a voluminous suite of aluminous granites in the Aileron Province in the North Australian Craton together with metasedimentary granulites as models for source behaviour, we evaluate fluid-absent verse fluid-present regimes for generating large volumes of crustally-derived melt. The central Aileron Province granites occupy 32,500km2, and in places are in excess of 8 km thick. They are characterised by abundant zircon inheritance that can be matched with metasedimentary successions in the region, suggesting they were derived in large part from melting of crust similar to that presently exposed. A notable feature of many of the granites is their enriched Th concentrations compared to typical Aileron Province sub solidus metapelitic successions. However, based on continuous transects within metasedimentary rocks from a number of different regions that record transitions from sub-solidus assemblages to supra-solidus rocks petrologically characterised by typical fluid-absent peritectic assemblages (central Aileron Province, Broken Hill Zone, Ivrea-Verbano Zone), fluid-absent partial melting does not deplete Th concentrations in the residuum with respect to their sub-solidus protoliths. If these compositional transects are used as a guide to the general behaviour of Th during fluid-absent partial melting, the voluminous Th-enriched granites in the Aileron Province are unlikely to be the products of fluid-absent partial melting. This contention is supported by phase equilibria modelling of sub-solidus metasedimentary units whose detrital zircons match in age the granite-hosted xenocrysts, which indicate that temperatures in excess of 840°C are required to generate significant volumes (ie ≥ 30%) of melt under fluid-absent conditions. However, zircon saturation temperatures for the granites have a weighted mean of 776 ± 4 °C (n = 220). Because the granites contain abundant inheritance, this is an upper-T limit that also suggests fluid-absent partial melting was not the primary mechanism for granite formation. We suggest that voluminous granite formation in the Aileron Province occurred in a fluid-rich regime that was particularly effective at destabilising monazite and liberating Th into melt. Because of the propensity of monazite to destabilise in the presence of fluid, we suggest that high-grade metasedimentary terrains that are notably depleted in Th may be residuum associated with fluid-fluxed melt loss.

a Passage to the Universe

NASA Astrophysics Data System (ADS)

1995-11-01

Exciting Week Ahead for Winners of Unique Astronomy Contest Following the very successful events of 1993 and 1994 [1], ESO again opens its doors for an `educational adventure' next week. It takes place within the framework of the `Third European Week for Scientific and Technological Culture', initiated and supported by the European Commission. On Tuesday, November 14, 1995, about forty 16-18 year old students and their teachers will converge towards Munich from all corners of Europe. They are the happy winners of a Europe-wide astronomy contest (`Europe Towards the Stars') that took place during the summer and early autumn. Their prize is a free, week-long stay at the Headquarters of the European Southern Observatory. During this time they will work with professional astronomers and get a hands-on experience within modern astronomy and astrophysics at one of the world's foremost international centres. In particular, the participants will be exposed to the scientific method by carrying through a research programme of their own, all the way from conception to interpretation of the data. The culmination of the stay will be the opportunity to perform remote observations via a satellite link with two major telescopes at the ESO La Silla observatory in Chile, including the very advanced 3.5-metre New Technology Telescope (NTT). The European Contest This year's EU/ESO programme was devised as a contest between joint teams of secondary school students and their teachers. The teams had to choose between four different subjects requiring either practical or theoretical work, and all with strong scientific and technological components. One subject was to devise an observational programme with an existing telescope and instrument and to discuss the resulting data in order to arrive at a scientific conclusion. This was the preferred subject by many teams. For instance, the winning German team observed the moons of Jupiter and the Danish team studied a star cluster in order to derive its age and other characteristics. The second subject, to build and test an astronomical instrument, posed a welcome challenge to teams with a particular interest in technology. Some of the instruments were quite advanced; in France, for instance, the winning team built a working solar radio interferometer. In the same direction, but with a more theoretical touch, some teams chose the third subject, to design on paper an instrument for a future space mission to the outer Solar System for the exploration of Pluto and the newly discovered Transneptunian Objects. The last subject, which secured the first prize for the Dutch winning team, concerned the study of a hypothetical, stable planetary system around another star, its properties and the technical requirements for observing this system from the Earth. With the recent discovery of a planet around the nearby star 51 Pegasi, this theme has unexpectedly gained added relevance. During the past few weeks, the work by the teams was evaluated by specially established, national juries, consisting of scientists, educators and ministerial representatives (addresses below). The establishment of the European Association for Astronomy Education (EAAE) last year contributed to the Europe-wide interest in these matters and many EAAE members have been involved in the present contest, as participants or in its organisation. The national winners have now been selected; their names are listed below. In most countries, the award ceremonies have already taken place. Media Coverage The main event, i.e. the stay of the winning teams at the ESO Headquarters in Garching (Germany) from November 14 - 20, 1995, will be covered by the various media in the appropriate ways. More information, including a detailed programme of the many (day and night) activities during this event, may be obtained at request from the ESO Education and Public Relations Department at the Headquarters. In this connection, ESO is also pleased to invite the media to a concluding Press Conference , during which the outcome of this unique event will be summarized by the participants and the organisers: Monday, November 20, 1995, 15:30 pm, at the ESO Headquarters, Karl-Schwarzschild-Strasse 2, D-85748 Garching, Germany List of National First-Prize Winners Belgium: Mr. Freddy Allemeersch (Teacher), Mr. Pieter De Ceuninck, Mr. Jeroen Staelens (Onze-Lieve-Vrouwecollege, Brugge) Denmark: Mr. Joern C. Olsen, Mr. Henrik Struckmann, Mr. Uffe A. Hansen, Mr. Mogens Winther (Teacher) (Soenderborg Amtsgymnasium) Finland: Mr. Reima Eresmaa, Ms. Laura Elina Nykyri, Ms. Reetamaija Janhonen (Cygnaeues-Lukeo, Jyvaeskylae and Jyvaeskylaen Lyseon Lukeo) France: Mr. Rene Cavaroz (Teacher), Mr. Vincent Hardy, Mr. Antoine Lesuffleur (Lycee Chartier, Bayeux) Germany: Ms. Dorothee Barth, Mr. Walter Czech (Teacher), Mr. Uwe Kranz, Ms. Karin Wieland (Immanuel-Kant-Gymnasium, Leinfelden-Echterdingen, Baden-Wuerttemberg) Greece: Ms. Agni Ioannidi, Ms. Elena Katifori, Mr. Vassilis Samiotis, Mr. Vassillos Tzotzes (Teacher) (Second Varvakelo Experimental Lyceum, Athens) Ireland: Mr. Declan Maccuarta (Teacher), Mr. Colm Mcloughlin (St. Peter's College, Wexford, Co. Wexford) Italy: Mr. Pasquale Ciarletta, Ms. Francesca D'elia, Ms. Ada Fortugna (Teacher), Mr. Alfredo Pudano (Liceo Scientifico `Leonardo da Vinci', Reggio Calabria) The Netherlands: Mr. Alex De Beer, Mr. Klaas Huijbregts, Mr. Ruud Nellen (Norbertuscollege, Rosendaal) Spain: Mr. Aritz Atela Aio, Mr. Julen Sarasola Manich (Teacher), Mr. Jon Huertas Rodriquez (Txorierri Batxilergoko Institua, Derio Bizkaia) Sweden: Mr. Rahman Amanullah, Mr. Kjell L. Bonander (Teacher), Mr. Tomas Oppelstrup, Ms. Christin Wiedemann (Saltsjoebadens Samskola, Saltsjoebaden) United Kingdom: Mr. Michael Ching, Dr. Richard Field (Teacher) (Oundle School, Peterborough) National Committees Further information about the national contests may be obtained from the National Committees: Belgium: Dr. C. Sterken, Vrije Universiteit Brussel, Campus Ofenplein, Pleinlaan 2, B-1050 Brussels, Tel. 0032-2-6293469, Fax 0032-9-3623976, E-mail csterken@is1.vub.ac.be Denmark: Mr. B. F. Joergensen, Tycho Brahe Planetariet, Gl. Kongevej 10, DK-1610 Copenhagen V, Tel. 0045-33-144888, Fax 0045-33-142888, E-mail tycho@inet.uni-c.dk Finland: Mr. M. Hotakainen, Taehtitieteellinen Yhdistys Ursa, Laivanvarustajankatu 9C 54, FIN-00140 Helsinki, Tel. 00358-0-174048, Fax 00358-0-657728 France: Mr. B. Pellequer, Geospace d'Aniane, Boite Postale 22, F-34150 Aniane, Tel. 0033-6-7034949, Fax 0033-6-7752864 Germany: Dr. K.-H. Lotze, Friedrich-Schiller-Universitaet, Max-Wien-Platz 1, D-07743 Jena, Germany, Tel. +49-3641-635904/636654, Fax +49-3641-636728 Greece: Dr. D. Simopoulos, Eugenides Foundation, Astronomy Department, 387 Sygrou Avenue, Palaio Faliro, GR-175 64 Athens, Tel. 0030-1-941-1181, Fax 0030-1-941-7372 Ireland: Dr. I. Elliot, Dunsink Observatory (Dublin Institute for Advanced Studies), Castleknock, Dublin 15, Tel. 00353-1- 838-7911/7959, Fax 00353-1-8387090, E-mail ie@dunsink.dias.ie Italy: Dr. B. Monsignori Fossi, Osservatorio Astrofisico di Arcetri, Largo Enrico Fermi 5, I-50125 Florence, Tel. 0039-55-2752246, Fax 0039-55-220039, E-mail bmonsignori@arcetri.astro.it The Netherlands: Dr. M. Drummen, Stichting `De Koepel', Zonnenburg 2, NL-3512 NL Utrecht, Tel. 0031-30-311360, Fax 0031-30-342852, E-mail dekoepel@knoware.nl Spain: Dr. A. Sanchez/Dr. T. Fernandez, Planetario de Madrid, Parque Tierno Galvan, E-28045 Madrid, Tel. 0034-1-4673578, Fax 0034-1-4681154, E-mail tfc@vilspa.esa.es Sweden: Dr. K. Loden, Stockholms Observatorium, S-133 36 Saltsjoebaden, Tel. 0046-8-164454, Fax 0046-8-7174719, E-mail lodenk@astro.su.se United Kingdom: Dr. A. M. Cohen, c/o The Association for Astronomy Education, 9 Hurst Lane, Bollington, Macclesfield, Cheshire SK10 5LN, England Notes: [1] See ESO Press Releases 08/93 of 5 November 1993 and 17/94

Book Review: Beitraege zur Astronomiegeschichte, Band 5 (Acta Historica Astronomiae Vol. 15)

NASA Astrophysics Data System (ADS)

Duerbeck, H. W.; Dick, W. R.; Hamel, J.

2002-12-01

The 15th volume of the Acta Historica Astronomiae is at the same time the fifth collection of essays on the history of astronomy (Beitraege zur Astronomiegeschichte, Band 5), edited by the historians of astronomy W.R. Dick (Potsdam) and J. Hamel (Berlin). Besides a few short notices and book reviews, the book contains 11 major articles, which deal with astronomical topics covering the time from the 16th to the 20th centuries. The first article, on the analysis and interpretation of historical horoscopes as a source of the history of science, is based on the inaugural lecture of its author, Guenther Oestmann. After a general introduction, which deals with the principles of horoscope making, the author discusses the horoscope of Count Heinrich Ranzau (1526-1598), the Danish governor of Schleswig-Holstein, who was a friend of Tycho Brahe. Oestmann shows that the astronomical-mathematical basis of such a horoscope can be reconstructed and interpreted. However, it is hardly possible to gain an insight in the process how the interpretation of a horoscope was done in detail. The second and third articles, by Franz Daxecker, deal with Athanasius Kircher and Christoph Scheiner, two catholic astronomers of the 17th century. Kircher's Organum Mathematicum is a calculating device that can be used in the fields of arithmetic, geometry, chronology, astronomy, astrology and others. The author provides extracts of the description of the Organum taken from a book by Caspar Schott, which deal with chronology and astronomy. A photograph of the Organum indicates that this tool consists of a set of tables glued on wooden or cardboard, but details of its contents and applications remain pretty obscure for the reader - a few elaborated examples would have been helpful. The second paper deals with the life of Christoph Scheiner SJ, the co-discoverer of sunspots (next to Galileo), after leaving Rome in 1633 - the year of the Galileo trial. Scheiner spent his later years in the Austrian and Bohemian (Jesuit) provinces, mainly in Vienna and Neisse (the present Nysa in Silesia, Poland), but no traces of further astronomical activity have survived, if they ever existed. The fourth article, by Hans Gaab, is a very thoroughly researched biography of Johann Philipp von Wurzelbau (1651-1725), an merchant turned astronomer from Nuremberg. Wurzelbau started his activities at Christoph Eimmart's (the director of the painters' academy in Nuremberg) private observatory, and his first published work deals with observations of the great comet of 1680. Furthermore, he observed solar eclipses, Mercury transits, and determined the geographical latitude of Nuremberg. The article also contains a detailed description of Wurzelbau's observatory and its instruments. The fifth paper, by Klaus-Dieter Herbst, deals with Gottfried Kirch's idea of founding an astronomical society - being a vehicle to publishing astronomical observations. Kirch (1639-1710) was a well-known astronomer and calendar manufacturer. Around 1700, Kirch was appointed first astronomer at the Brandenburg society of sciences, and director of the observatory that was to be established with the new Berlin Academy. Herbst shows that Kirch's religious attitude that converged on pietism was a driving force to establish a scientific society. However, the final failure of such a project is due to the emergence of the scientific journal Acta Eruditorum, issued since 1682 in Leipzig, which could serve as an outlet for the publication of astronomical data by Kirch and others, thus fulfilling an essential task of the projected academy. Kirch's occupation with the composition of calendars, which took most of his time, was another reason. The following three shorter articles deal with 19th century astronomy. Peter Brosche describes an early visual photometer employed by Johann Gottfried Koehler (1745-1801) in Dresden, Alberto Meschiari edits and comments letters by Franz Xaver von Zach (1754-1832) to the physicist Gerbi in Pisa and the librarian Pozzetti at Bologna, and Karin Reich describes and edits Bessel's book critique of Gauss' Theoria Motus. How many one-time astronomers have to earn their living in other ways, become distracted from astronomical research, and vanish from the horizon of astronomical history? In the ninth paper, Hans-Joachim Ilgauds has traced the life of Georg Koch (1851-1905), who started his career as an astronomer at Leipzig Observatory in 1874. Later Koch worked at Hamburg Observatory, and then became an employee at the statistical office in Kiel, and finally director of the statistical office of the Hamburg revenue service. He was a collaborator for the statistical yearbook of German cities, and also contributed to a book investigating the causes and the impact of the cholera epidemic of 1892 in Hamburg. The last two papers deal with the circumstances of the discovery of the first Near-Earth asteroid (433) Eros. It was recorded on photographic plates taken at the Urania-Sternwarte Berlin and at Nice Observatory. The Berlin observer Witt announced the discovery, and only later, the Nice observer Charlois published a position of Eros. While all plates have disappeared, the authors Hans Scholl and Lutz D. Schmadel could prove that the Nice plate was poorly guided and Charlois would have been unable to discover the object. From a copy of the Berlin plate, published 50 years after the discovery by Witt's co-observer F. Linke, the exact position was determined, and the time of observation (which had not been published) was derived. The second article, by Lutz D. Schmadel, deals with the life of the Eros co-discoverer Felix Linke (1879-1959), who later worked in statistic offices, was a frequent writer of popular scientific articles, and later the editor of a journal, "Technik im Hotel'', and author of a book of the same title. As can be seen from the summaries given above, this collection of essays deals mainly with historical events that occurred in Germany and neighboring countries, and is focussed mainly on events in the 17th to 19th centuries. Except for the Eros article by Scholl and Schmadel, which is written in English, all contributions are written in German. The editors have taken care that generally a high standard was kept. The series appears to be a complement to the Journal for the History of Astronomy, in spite of the fact that its scope is somewhat narrower and somewhat less international. Of course, the use of the German language and the Germany-based small publishing company hampers a wide distribution of this series (but an all-English edition would turn away potential German readers). Nevertheless, it should be noted that English is not necessarily the "lingua franca'' in all cultural fields, and students of the history of science should have at least a cursory knowledge of several languages at their command. It would be nice to see that such a history of astronomy series would also be published in other countries, focussing on the historical events in these regions (French, Italian, Spanish - it should be mentioned that a series Istoriko-astronomicheskie issledovaniia has appeared since 1955 in Moscow). In any case, the editors should be congratulated in having established (with a lot of personal engagement) a flourishing book series. I hope that their venture may serve as an example for others.

Congratulations to Carey King

NASA Astrophysics Data System (ADS)

Hall, Charles A. S.

2012-03-01

I first came across Carey King when, out of the blue, he invited me to a special session of the annual meeting of the American Association for the Advancement of Science (the largest and most prestigious US scientific meeting) where he was developing a special session on energy return on investment (EROI). At that meeting and since, I have found Carey to be a refreshing new colleague, extremely intelligent, very knowledgeable about many diverse aspects of energy and other things, able to take criticism and to dish it out, and very ambitious, which is mostly a good thing. He is becoming a leader in thinking about EROI and its implications, and I am delighted to see him honored by Environmental Research Letters. This is important because in the US, there is little insight about energy or, especially, its potential physical limitations except when gas prices increase. There is also little awareness of the very strong historical connection in both the US and the world between increased affluence and increased use of energy, especially petroleum. It is not understood by all that many of the economic problems we have now (such as the budgetary problems faced by most of our State governments, pension plans and universities) have substantial origin in the fact that oil and other energy production no longer increase reliably year after year, as they once did (Murphy and Hall 2011). Many economists have argued in the past that energy is not important because it constituted only 5 per cent or so of GDP, or because they believe that market forces and innovations will substitute for any shortage (e.g. Barnett and Morse 1963, Passell et al 1972, Solow 1974, Denison 1989). One problem with that view is that if you remove that five per cent the economy comes to a dead stop, as Cuba found out in 1989 when Russia removed its oil subsidy. Additionally if that five per cent goes up to 10 or 15 per cent, as it did in the early 1980s, and again in 2008, recession steps in (Murphy and Hall 2011). In fact, the US economy and our energy use increased almost lockstep from 1900 until 1984 (Cleveland et al 1984). The economy has grown more rapidly than energy use since 1984. Most economists think that this is due to our cleverness at increasing efficiency, but Robert Kaufmann (2004) and others find that instead most of the increase has been due to, essentially, the outsourcing of our heavy industry (think steel imported from Korea or Brazil, petroleum refined in Trinidad etc). An additional issue is that there is considerable evidence (e.g. Shadow Government Statistics) that the official US government inflation corrections have been deliberately underestimated since about 1985. If this is true then GDP growth has been exaggerated and there has been little or no increase in efficiency. Thus our gain in actual national energy efficiency is probably much less than most economists believe, and may be close to zero. Obviously some few of us think a great deal about energy, and for those who are willing to undertake some personal research (for example on the ASPO (aspo-usa.com) or The Oil Drum (www.theoildrum.com) websites), there is much to be concerned about. First on the list of concerns is 'peak oil'; the concept that there comes a time over the life cycle of the extraction of a non-renewable resource when there will be maximum production. This concept, derived by geologist M K Hubbert in the 1950s, assumes that this peak will occur when roughly 50 per cent of the resource has been exploited. Hubbert famously predicted in 1955 that this would occur for the United States in 1970. Initially he was derided by most in the oil industry, but in fact peak oil for the US did occur in 1970, just as he had predicted. Oil production has declined essentially every year since then. 'Peak oil' has now occurred for something like three quarters of all oil producing nations, although not yet for most of the largest producers. Second on my list of energy concerns is declining EROI. EROI is a term I had developed in the early 1980s based on the net energy concepts of Howard Odum (Odum 1973, Hall 1972). It is simply the ratio of the energy returned from an energy extraction process divided by the energy to get that energy. The concept had a certain amount of traction in the 1980s (Hall and Cleveland 1981, Cleveland et al 1984) but as gasoline prices fell and memories of the 'energy crises' of the 1970s faded, interest in energy matters also declined. A few of us 'energy nuts' kept plugging away at trying to get better numbers (Hall and Klitgaard 2011). In contrast to most people and certainly most economists, Carey King is someone who has thought about energy, peak oil and EROI a lot, and in very sophisticated ways. Early in his career Carey deduced that EROI appeared to be having a new day because of, for example, questions about the EROI of corn-based ethanol for transportation fuels and because of the declining productivity and profitability of many Texas and other oil fields. For many, including Carey and myself, it made no sense to trade one Joule of fossil energy to run tractors, make fertilizers, distill mash and so on to generate about one Joule of corn-based ethanol, which the US is doing on a vast, federally-subsidized scale. Carey has had some quite original ideas about coming up with a shortcut to deriving a proxy measurement for EROI, which is quite difficult to calculate, and about the importance of EROI for financial issues. For example Carey has found that the inflation-adjusted prices of oil and coal are basically predicable over the last century from the EROI at that time (King 2010). He has also worked with others at attempting to get at a more comprehensive EROI that would include the energy cost of supporting all of the money spent developing the resource, including the energy associated with giving meaning to laborers' pay checks and the energy associated with financial services. We do not yet understand the importance of these more comprehensive EROIs but we do understand that our usual methods of including only energy used directly (e.g. to run a pump) or indirectly (e.g. to manufacture the steel forms used) greatly underestimates the total amount of energy needed to produce energy. In conclusion, Carey King appears to be one of the real rising energy stars as energy becomes again much more important. He is very bright, original and is a very hard worker. I look forward to much exciting, innovative and important work from his endeavors. References Barnett H and Morse C 1963 Scarcity and Growth: The Economics of Natural Resource Availability (Baltimore, MD: Johns Hopkins Press) Cleveland C J, Costanza R, Hall C A S and Kaufmann R 1984 Energy and the United States economy: a biophysical perspective Science 225 890-7 Denison E F 1989 Estimates of Productivity Change by Industry, an Evaluation and an Alternative (Washington, DC: The Brookings Institution) Hall C A S 1972 Migration and metabolism in a temperate stream ecosystem Ecology 53 585-604 Hall C A S and Cleveland C J 1981 Petroleum drilling and production in the United States: yield per effort and net energy analysis Science 211 576-9 Hall C A S and Klitgaard K 2011 Energy and the Wealth of Nations: Understanding the Biophysical Economy (New York: Springer) Kaufmann R 2004 The mechanisms for autonomous energy efficiency increases: a cointegration analysis of the US Energy/GDP Ratio The Energy Journal 25 63-86 King C W 2010 Energy intensity ratios as net energy measures of United States energy production and expenditures Environ. Res. Lett. 5 044006 Murphy D J and Hall C A S 2011 Energy return on investment, peak oil, and the end of economic growth in 'Ecological Economics Reviews' ed Robert Costanza, Karin Limburg and Ida Kubiszewski Ann. N.Y. Acad. Sci. 1219 52-72 Solow R M 1974 The economics of resources or the resources of economics American Economic Review 66 1-14 Odum H T 1973 Environment, Power and Society (New York: Wiley Interscience) Passell P, Roberts M and Ross L 1972 Review of 'Limits to Growth' New York Times Book Review 2 April 1972

Young Astronomers' Observe with ESO Telescopes

NASA Astrophysics Data System (ADS)

1995-11-01

Today, forty 16-18 year old students and their teachers are concluding a one-week, educational `working visit' to the ESO Headquarters in Garching (See ESO Press Release 14/95 of 8 November 1995). They are the winners of the Europe-wide contest `Europe Towards the Stars', organised by ESO with the support of the European Union, under the auspices of the Third European Week for Scientific and Technological Culture. From November 14-20, they have worked with professional ESO astronomers in order to get insight into the methods and principles of modern astronomy and astrophysics, as carried out at one of the world's foremost international centres. This included very successful remote observations with the ESO 3.5-m New Technology Telescope (NTT) and the 1.4-m Coude Auxiliary Telescope (CAT) via a satellite link between the ESO Headquarters and the La Silla observatory in Chile, 12,000 kilometres away. After a general introduction to modern astronomy on the first day of the visit, the participants divided into six teams, according to their interests. Some chose to observe distant galaxies, others prefered to have a closer look on binary stars, and one team decided to investigate a star which is thought to be surrounded by a proto-planetary system. Each team was supported by an experienced ESO astronomer. Then followed the observations at the remote consoles during three nights, the first at the NTT and the following at the CAT. Each team had access to the telescope during half a night. Although the work schedule - exactly as in `real' science - was quite hard, especially during the following data reduction and interpretative phase, all teams managed extremely well and in high spirits. The young astronomers' observations were favoured by excellent atmospheric conditions. At the NTT, the seeing was better than 0.5 arcsecond during several hours, an exceptional value that allows very good images to be obtained. All observations represent solid and interesting science, and some of the new results are indeed at the frontline. Together with the team leaders, this will be followed up during the next months, with the likely result in the form of one or more scientific papers. It is difficult to think of an experience for young people that brings them closer to real science. The stay at ESO is concluded today with the formal presentation of the team's reports, followed by a Press Conference. There will be a closing dinner this evening and tomorrow the participants will return to the respective countries and revert to normal life at the schools. The entire event has been covered by assisting journalists and has also been documented by the ESO Video Team; a corresponding video film will become available shortly. This experience has been very positive, both in terms of human relations, education and science. With their widely different cultural backgrounds and common interest in astronomy, the young people and their teachers have demonstrated the many virtues of international collaboration and thereby also made this event a valuable contribution to the integration of Europe. The two Addenda to this Press Release contain information about the winning projects, and also, in a very provisional form, about the outcome of the work carried out at ESO. Addendum 1 The Projects of the National first-prize winners Belgium: Mr. Freddy Allemeersch (Teacher), Mr. Pieter De Ceuninck, Mr. Jeroen Staelens (Onze-Lieve-Vrouwecollege, Brugge) This project aims at the theoretical description of a stable planetary system around another star and the possibilities to observe it from the Earth. A star of 0.8 solar mass is placed at the centre, surrounded with 3 terrestrial (Earth-like) planets and 4 planets of the gaseous, Jovian type. The distance from the Earth is 10 parsec, i.e. about 33 light-years. The project provides a very detailed description of these planets, their inner constitution, surface conditions and atmospheres. Many different observational approaches are described, but in the end it is appears that only infrared astrometry and astrometry would allow to detect the presence of the planets around this star. Denmark: Mr. Joern C. Olsen, Mr. Henrik Struckmann, Mr. Uffe A. Hansen, Mr. Mogens Winther (Teacher) (Soenderborg Amtsgymnasium) This team performed extensive CCD-observations with the school telescope of three stellar clusters. The goal was to determine their HR-diagrammes (colour-magnitude) and other characteristics. Among others, the team succeeded to measure quite accurate B (blue) and V (green-yellow) colours of 40, 12-16-magnitude stars in the open stellar cluster NGC 6939. This allowed a determination of the distance (2500 parsec) to this cluster and its age (1800 million years), quite similar to the `professionally' determined values. As a side-result, and illustrating the faintness of starlight, a calculation showed that it would take no less than 437,236 years for the brightest star in the sky, Sirius, to heat a cup of coffee to the boiling point ! Finland: Mr. Reima EresmA, Ms. Laura Elina Nykyri, Ms. Reetamaija Janhonen (Cygnaeues-Lukeo, Jyvaeskylae and Jyvaeskylae Lyseon Lukeo) This group used a 50-cm amateur telescope in their home town to observe the spectra of galaxies. A CCD spectrograph recorded the data which were then image-processed in the computer. For this programme, five galaxy pairs were selected and their velocities were measured. This allowed to calculate the distance to the galaxies by means of Hubble's law and also to determine the velocity difference between the two galaxies in a binary system. This in turn makes it possible to estimate the galaxies' total mass. When comparing these numbers with the mass of the visible objects, the group finally determined that the visible mass is only about 8 percent of the total mass, i.e. there must be much `dark matter' in these galaxies. France: Mr. Rene Cavaroz (Teacher), Mr. Vincent Hardy, Mr. Antoine Lesuffleur (Lycee Chartier, Bayeux) This project concerned the actual construction of a working solar radio interferometer, a rather complex instrument that allows measurements of the long-wavelength radiation from the Sun and to map the locations in the solar corona where this radiation originates. The antennae and receiver were designed for frequences around 550 and 750 MHz and were built by the team members themselves. Radio signals from the Sun (as interference fringes) were effectively observed with this instrument, documenting the excellent functioning of this advanced equipment. Germany: Ms. Dorothee Barth, Mr. Walter Czech (Teacher), Mr. Uwe Kranz, Ms. Karin Wieland (Immanuel-Kant-Gymnasium, Leinfelden-Echterdingen, Baden-Wurttemberg) Following a careful planning phase, systematic observations of the 14-magnitude planet Pluto were made with a CCD camera and a 30-cm telescope during 18 nights in the spring and summer of this year. Five nearby stars were used to calibrate the resulting photometric measurements. In the end, this programme was shown to achieve a very good photometric accuracy of about +- 0.2 magnitude per measurement. The variation of Pluto's brightness was found to be about 0.7 magnitude for this particular instrumental combination (no filtre). It was thus possible to draw the lightcurve which was found to be in complete agreement with the established 6.4 day rotation period. Greece: Ms. Agni Ioannidi, Ms. Elena Katifori, Mr. Vassilis Samiotis, Mr. Vassillos Tzotzes (Teacher) (Varvakio Experimental Lyceum, Athens) The project starts out from a star of 1.56 solar mass and a certain density. From this, its size, luminosity, temperature, pressure and other parameters are calculated. With an analogue to the Titius-Bode law for planetary distances, a new planetary system is constructed. It has 5 planets, 3 of which are of the terrestrial type and the other 2 are giant gas planets, larger than Jupiter. Their physical characteristics are calculated. One planet (the 3rd from the central star) is somewhat similar to the Earth, but it is too cold for life as we know it, and because of its comparatively small size, the atmospheric pressure is very low. It would in principle be possible to detect the outermost planet with the HST, if the distance to this planetary system was less than about 30 light-years. Ireland: Mr. Declan MacCuarta (Teacher), Mr. Colm McLoughlin (St. Peter's College, Wexford, Co. Wexford) The nearest star, Alpha Centauri, is a double star and a hypothetical planetary system around the A-component, a solar-type star, is studied in some detail. The presence of the companion star makes some planetary orbits unstable. In this project, 4 planets are placed within 2 AU (300 million km) of the central star; 3 of these are terrestrial (no. 3 is Earth-like) and the outermost is a small gaseous planet. Cometary orbits may be very complex in this gravitatinal field. A planetary system like the one described may be barely observable with the Hubble Space Telescope, and only if one of the planets passes in front of the star (an `occultation') and its light diminishes accordingly. Italy: Mr. Pasquale Ciarletta, Ms. Francesca D'elia, Ms. Ada Fortugna (Teacher), Mr. Alfredo Pudano (Liceo Scientifico `Leonardo da Vinci', Reggio Calabria) This group built a spectrograph from scratch, with a grating and all the usual optical parts. They were able to calibrate the solar spectrum with the help of standard lamps and in this way, they observed several prominent, solar absorption lines. Among them were the H-alpha line at 6562 A, the sodium D-lines at 5890--96 And the magnesium triplet near 5175 A. These observations were made with the eye and also with the photographic recording technique. They were planning to observe the spectra of some stars also, but in the end time was too short and they had to hurry to send in the report. The Netherlands: Mr. Alex De Beer, Mr. KlAs Huijbregts, Mr. Ruud Nellen (Norbertuscollege, RosendAl) This team has designed their own planetary system (with the name `Ngnz'i'!), consisting of a central star that is somewhat larger than the Sun and situated at the same distance as the Sun from the centre of the Milky Way System (31,700 light-years). The distance from the Sun is twice as large, 63,400 light-years. Circling the central star at a distance of 300 million kilometres, there is a double planet with a revolution period of just over 3 years. The conditions on another planet further out is suitable for life and it harbours frog-like intelligent beings. Two outer, gaseous planets complete this system. Spain: Mr. Aritz Atela Aio, Mr. Julen Sarasola Manich (Teacher), Mr. Jon Huertas Rodriquez (Txorierri Batxilergoko Institua, Derio Bizkaia) The group built its own f/8 Newtonian reflector with a main mirror of 20 cm diameter. They tested it on various astronomical objects and found that it produced quite good images. Then they put together their own CCD camera from spare parts; the frame size is about 5 x 4 mm with a total of 300,000 pixels. With this special equipment, they have observed the major Jovian moons as they revolve around Jupiter. They projected the image on a TV-screen and measured the exact positions of the moons, relative to Jupiter, on this screen. In this way, they were able to determine the periods of revolution of the moons and from the diameters of the orbits and Jupiter's size, they could determine Jupiter's mass and mean density. Sweden: Mr. Rahman Amanullah, Mr. Kjell L. Bonander (Teacher), Mr. Tomas Oppelstrup, Ms. Christin Wiedemann (Saltsjoebadens Samskola, Saltsjoebaden) In another Universe, three heroes meet on a far-away planet, named Magrathea. They check the computerized data archive available there, discovering a reference to the planetary system Ikaros III, and a description of its formation and evolution. At the centre is an A-type star, Ikaros; the temperature is 9700 K, and its lifetime is about 500 million years. It is surrounded by three planets, whose physical characteristics are listed in great detail. Two are small and dense and the outermost is gaseous. It turns out that the distance to our Earth is 26 light-years and that it would be not be too easy to observe the Ikaros system from here. It is unlikely that life can develop in this planetary system during the relatively short lifetime of the central star. United Kingdom: Mr. Michael Ching, Mr. Richard Field (Teacher) (Oundle School, Peterborough) This project is directed towards variable stars of the pulsating type. It discusses the theory for these pulsations and the peculiar location of these types of stars in the HR-diagramme, as well as the technique to determine distances by means of measurements of the period. Once the period has been found observationally, the Period-Luminosity diagram makes is possible to find the luminosity and hence the distance to the star. The project also involved real measurements of an RR Lyr-type variable with a period of about 1/3 day. For this, a phototransitor and a registering device were used. The expected light variations were clearly seen. Addendum 2 A brief summary of the results obtained at ESO This brief description is based on the provisional data reduction and subsequent interpretation by the six teams, as presented during a final session on November 20, 1995. Further work will allow to quantify the results in greater detail. Each team was guided by a young ESO astronomer as Team Leader and was also provided support during the observations by ESO-astronomers Lex Kaper and Marcus Kissler, as well as by night assistants Vicente Reyes and Jesus Rodriguez (Garching), Hernan Nunez, Jorge Miranda and Victor Merino at (La Silla). For the data reduction, the teams used the MIDAS image processing system; the introduction was provided by Rein Warmels, one of ESO's experts on these matters. Since the teams that were observing during the last night (3A and 3B) had very little time to reduce and interpret their data, it was not possible to carry these investigations to the same level of completeness as the others. Team 1a: Participants: Amanullah, De Beer, Huertas Rodriguez, Huijbregts, Kranz, Olsen, Oppelstrup; Team leaders: Jari Ronnback and Frederic Courbin This team used the multi-mode EMMI instrument at the 3.5-m NTT to observe so called `Interacting Galaxies'. These are galaxies which are so close to each other that their shapes are distorted by the action of their gravitational fields. Some of them are actually in a state of collision. Direct CCD images were obtained of a total of 8 galaxies; 7 of these were observed in one colour (red) and 1 in two (red and yellow-green). The programme comprises a selection of different types of galaxies (Elliptical + Elliptical; Elliptical + Spiral; etc.) and different types of interactions (direct collision; fly-by; etc.). The observing conditions were quite good, with seeing from 0.5--1.2 arcseconds and some of the images obtained are probably the best ever made of these particular objects. The team classified the types of involved, heavily distorted galaxies and attempted to decide what type of interaction is occurring. A very nice and instructive pictorial Atlas will be produced from this material. Team 1b: Participants: Barth, Bonander, Ching, Ciarletta, EresmA, Wiedemann, Wieland; Team leaders: Paul Goudfrooij and Frederic Courbin This team obtained short-exposure direct images and long-exposure long-slit spectra with NTT + EMMI of two peculiar galaxies, the edge-on distorted spiral NGC 1448 and the elliptical NGC 1947 which has a crossing dust lane. One IRAS superluminous galaxy was also observed. The latter part of the night was characterized by exceptionally good seeing (down to 0.3 arcsecond!), permitting to see many details in these galaxies, which have never been perceived before. For instance, several hitherto unknown dust lanes were found in the outer regions of NGC 1947 ! The slits were placed through the central part of the galaxies and along the major axis (NGC 1448) and the dust lane (NGC 1947), respectively. Strong emission lines of H-alpha, ionized nitrogen [N II] and ionized sulphur [S II] were seen in both galaxies; they originate in interstellar gas clouds within their confines. From the exact wavelengths of these lines, the velocity of the galaxies can be measured. The team found values near 1100-1200 km/sec for both galaxies, in full agreement with the published values. Moreover, the variations of these line wavelengths at increasing distance from the galaxy centres allow to determine the rotation curves with good accuracy. A total amplitude of about 400 km/sec was observed in both galaxies. The velocity gradient is very steep at the centre, indicating the presence of a large mass in this area. Indeed, total masses of the order of 10e9 or even 10e10 solar masses were calculated for the innermost region of the galaxies. Team 2a: D'elia, Hardy, Janhonen, Lesuffleur, Nellen, Nykyri, Pudano; Team leader: Jacco van Loon This team obtained high-dispersion spectra (resolution about 80,000) with the Coude Echelle Spectrometer and the 1.4-m Coude Auxiliary Telescope (CAT) of 5 late-type gaint and supergiant stars. These stars have arrived at a late phase of their lives. The heaviest, i.e. the supergiants may soon become supernovae, while the less heavy, the giants, may develop into a White Dwarf via the intermediate Planetary Nebula stage. The team wanted to find out which of these stars would develop which way by classifying them. The spectra covered two spectral regions, at the hydrogen H-alpha 6562 A line and at the ionized calcium Ca II 8542 A line. The calcium line serves for spectral classification; the deeper and broader this line is, the higher is the luminosity of the star. Of the five stars, T Microscopis and nu Eridanis were found to have a rather weak and narrow Ca II line and are therefore giants; the others had higher luminosity, in particular Alpha Orionis. In astronomical terms, the latter may in fact soon reach the supernova phase. One unknown emission line was found in the spectrum of this star; it will be interesting to try to identify it later. Team 2b: Participants: Allermeersch, Cavaroz, Czech, De Ceuninck, Ioannidi, Katifori; Team Leader: George Dudziak The object of the CAT observations by this team was the famous 4th-magnitude star Beta Pictoris which is known to have a surrounding disk of dust and gas. Recent observations indicate that planets may be forming in this disk at the present moment. Comparatively rapid changes in some spectral lines have been reported; the origin is unknown but may be infalling matter (comets?) on the star. The team decided to take a closer look at this. A total of 12 spectra (1 a 5 min and 11 a 15 min exposure) were obtained at very high spectral resolution and high signal-to-noise ratio (better than 200). They cover the spectral region that includes the Ca II 8542 A absorption line. This line has a very complex structure in Beta Pictoris. At the bottom of the line is seen the sharp dip that results from absorption in the part of the disk that is in front of the star. Two H2O-lines from the terrestrial atmosphere also fall within this line profile. All spectra were carefully calibrated and compared. For this, a mean spectrum was derived, and each of the 11 spectra was then divided by this. Deviations from the mean spectrum were present, in particular just redward of the disk absorption, and they were definitively larger than the very low observational noise. They may very well represent infalling bodies, but this is difficult to say on the basis of a preliminary data reduction. It will clearly be most interesting to continue the study of these spectra. Team 3a: Participants: Atela Aio, Fortugno, Hansen, Sarasalo Manich. Staelens, Winther; Team leader: Rene Mendez This team decided to study two planetary nebula by means of high-dispersion CAT spectra. In these objects, most of the light is emitted in a small number of emission lines and the accurate determination of the shape and wavelength of these lines will allow to measure various parameters of the nebulae. For instance, the internal motion os the gas can be derived. The first nebula was the well-known NGC 7293. The first spectra obtained showed splitting of the [S II] line; the two line components correspond to emission from the gas in the front and rear side of the nebula. The difference is 13 km/sec. This is important supplementary information to the observed geometric expansion of this nebula. It supports the derived age of about 50,000 years. The distance is found to be about 120 parsec, close to the nominal value. The other object observed, NGC 1535, is even younger, only about 3,500 years. It will take some time to exploit the full information available in these very detailed spectra. Team 3b: Participants: Field, MacCuarta, McLoughlin, Samiotis, Struckman, Tzotzes; Team leader: Fernando Comeron This team, which observed during the second half of the last night at the CAT, decided to look at spectroscopic binary stars. These stars are detectable as such by temporal changes in their spectra. For instance, the orbital motion of the two components causes changes in the measured radial velocity. Moreover, the different temperatures of the components are reflected in the combined spectrum and it may also be possible to detect gaseous streams from one star to the other. Two spectra were obtained of the suspected W Ursa Majoris type binary star Gamma Doradus with an internval of about 3 hours. This type of binary star consists of two components which are almost in contact and the rotation periods are short. Nevertheless, no changes were seen at all, casting some doubt on this proposed classification. Seven more spectra were obtained of 4 Beta Lyrae type binaries; four covered the region of H-alpha and three the He I 6678 A line. After a preliminary reduction of the data, the binary nature of three of them could be confirmed because of the presence of double lines, but for one, PU Puppis, only a single line was seen. Clear signs of circumstellar streams were not detected in any of them.