Study of Fluorine-Doped Tin Oxide (FTO) Thin Films for Photovoltaics Applications Shanting Zhang
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
March 21–25, 2016
FORTY-SEVENTH LUNAR AND PLANETARY SCIENCE CONFERENCE PROGRAM OF TECHNICAL SESSIONS MARCH 21–25, 2016 The Woodlands Waterway Marriott Hotel and Convention Center The Woodlands, Texas INSTITUTIONAL SUPPORT Universities Space Research Association Lunar and Planetary Institute National Aeronautics and Space Administration CONFERENCE CO-CHAIRS Stephen Mackwell, Lunar and Planetary Institute Eileen Stansbery, NASA Johnson Space Center PROGRAM COMMITTEE CHAIRS David Draper, NASA Johnson Space Center Walter Kiefer, Lunar and Planetary Institute PROGRAM COMMITTEE P. Doug Archer, NASA Johnson Space Center Nicolas LeCorvec, Lunar and Planetary Institute Katherine Bermingham, University of Maryland Yo Matsubara, Smithsonian Institute Janice Bishop, SETI and NASA Ames Research Center Francis McCubbin, NASA Johnson Space Center Jeremy Boyce, University of California, Los Angeles Andrew Needham, Carnegie Institution of Washington Lisa Danielson, NASA Johnson Space Center Lan-Anh Nguyen, NASA Johnson Space Center Deepak Dhingra, University of Idaho Paul Niles, NASA Johnson Space Center Stephen Elardo, Carnegie Institution of Washington Dorothy Oehler, NASA Johnson Space Center Marc Fries, NASA Johnson Space Center D. Alex Patthoff, Jet Propulsion Laboratory Cyrena Goodrich, Lunar and Planetary Institute Elizabeth Rampe, Aerodyne Industries, Jacobs JETS at John Gruener, NASA Johnson Space Center NASA Johnson Space Center Justin Hagerty, U.S. Geological Survey Carol Raymond, Jet Propulsion Laboratory Lindsay Hays, Jet Propulsion Laboratory Paul Schenk, -
DMAAC – February 1973
LUNAR TOPOGRAPHIC ORTHOPHOTOMAP (LTO) AND LUNAR ORTHOPHOTMAP (LO) SERIES (Published by DMATC) Lunar Topographic Orthophotmaps and Lunar Orthophotomaps Scale: 1:250,000 Projection: Transverse Mercator Sheet Size: 25.5”x 26.5” The Lunar Topographic Orthophotmaps and Lunar Orthophotomaps Series are the first comprehensive and continuous mapping to be accomplished from Apollo Mission 15-17 mapping photographs. This series is also the first major effort to apply recent advances in orthophotography to lunar mapping. Presently developed maps of this series were designed to support initial lunar scientific investigations primarily employing results of Apollo Mission 15-17 data. Individual maps of this series cover 4 degrees of lunar latitude and 5 degrees of lunar longitude consisting of 1/16 of the area of a 1:1,000,000 scale Lunar Astronautical Chart (LAC) (Section 4.2.1). Their apha-numeric identification (example – LTO38B1) consists of the designator LTO for topographic orthophoto editions or LO for orthophoto editions followed by the LAC number in which they fall, followed by an A, B, C or D designator defining the pertinent LAC quadrant and a 1, 2, 3, or 4 designator defining the specific sub-quadrant actually covered. The following designation (250) identifies the sheets as being at 1:250,000 scale. The LTO editions display 100-meter contours, 50-meter supplemental contours and spot elevations in a red overprint to the base, which is lithographed in black and white. LO editions are identical except that all relief information is omitted and selenographic graticule is restricted to border ticks, presenting an umencumbered view of lunar features imaged by the photographic base. -
Asteroid Regolith Weathering: a Large-Scale Observational Investigation
University of Tennessee, Knoxville TRACE: Tennessee Research and Creative Exchange Doctoral Dissertations Graduate School 5-2019 Asteroid Regolith Weathering: A Large-Scale Observational Investigation Eric Michael MacLennan University of Tennessee, [email protected] Follow this and additional works at: https://trace.tennessee.edu/utk_graddiss Recommended Citation MacLennan, Eric Michael, "Asteroid Regolith Weathering: A Large-Scale Observational Investigation. " PhD diss., University of Tennessee, 2019. https://trace.tennessee.edu/utk_graddiss/5467 This Dissertation is brought to you for free and open access by the Graduate School at TRACE: Tennessee Research and Creative Exchange. It has been accepted for inclusion in Doctoral Dissertations by an authorized administrator of TRACE: Tennessee Research and Creative Exchange. For more information, please contact [email protected]. To the Graduate Council: I am submitting herewith a dissertation written by Eric Michael MacLennan entitled "Asteroid Regolith Weathering: A Large-Scale Observational Investigation." I have examined the final electronic copy of this dissertation for form and content and recommend that it be accepted in partial fulfillment of the equirr ements for the degree of Doctor of Philosophy, with a major in Geology. Joshua P. Emery, Major Professor We have read this dissertation and recommend its acceptance: Jeffrey E. Moersch, Harry Y. McSween Jr., Liem T. Tran Accepted for the Council: Dixie L. Thompson Vice Provost and Dean of the Graduate School (Original signatures are on file with official studentecor r ds.) Asteroid Regolith Weathering: A Large-Scale Observational Investigation A Dissertation Presented for the Doctor of Philosophy Degree The University of Tennessee, Knoxville Eric Michael MacLennan May 2019 © by Eric Michael MacLennan, 2019 All Rights Reserved. -
Ancient Lamps in the J. Paul Getty Museum
ANCIENT LAMPS THE J. PAUL GETTY MUSEUM Ancient Lamps in the J. Paul Getty Museum presents over six hundred lamps made in production centers that were active across the ancient Mediterranean world between 800 B.C. and A.D. 800. Notable for their marvelous variety—from simple clay saucers GETTYIN THE PAUL J. MUSEUM that held just oil and a wick to elaborate figural lighting fixtures in bronze and precious metals— the Getty lamps display a number of unprecedented shapes and decors. Most were made in Roman workshops, which met the ubiquitous need for portable illumination in residences, public spaces, religious sanctuaries, and graves. The omnipresent oil lamp is a font of popular imagery, illustrating myths, nature, and the activities and entertainments of daily life in antiquity. Presenting a largely unpublished collection, this extensive catalogue is ` an invaluable resource for specialists in lychnology, art history, and archaeology. Front cover: Detail of cat. 86 BUSSIÈRE AND LINDROS WOHL Back cover: Cat. 155 Jean Bussière was an associate researcher with UPR 217 CNRS, Antiquités africaines and was also from getty publications associated with UMR 140-390 CNRS Lattes, Ancient Terracottas from South Italy and Sicily University of Montpellier. His publications include in the J. Paul Getty Museum Lampes antiques d'Algérie and Lampes antiques de Maria Lucia Ferruzza Roman Mosaics in the J. Paul Getty Museum Méditerranée: La collection Rivel, in collaboration Alexis Belis with Jean-Claude Rivel. Birgitta Lindros Wohl is professor emeritus of Art History and Classics at California State University, Northridge. Her excavations include sites in her native Sweden as well as Italy and Greece, the latter at Isthmia, where she is still active. -
Adams Adkinson Aeschlimann Aisslinger Akkermann
BUSCAPRONTA www.buscapronta.com ARQUIVO 27 DE PESQUISAS GENEALÓGICAS 189 PÁGINAS – MÉDIA DE 60.800 SOBRENOMES/OCORRÊNCIA Para pesquisar, utilize a ferramenta EDITAR/LOCALIZAR do WORD. A cada vez que você clicar ENTER e aparecer o sobrenome pesquisado GRIFADO (FUNDO PRETO) corresponderá um endereço Internet correspondente que foi pesquisado por nossa equipe. Ao solicitar seus endereços de acesso Internet, informe o SOBRENOME PESQUISADO, o número do ARQUIVO BUSCAPRONTA DIV ou BUSCAPRONTA GEN correspondente e o número de vezes em que encontrou o SOBRENOME PESQUISADO. Número eventualmente existente à direita do sobrenome (e na mesma linha) indica número de pessoas com aquele sobrenome cujas informações genealógicas são apresentadas. O valor de cada endereço Internet solicitado está em nosso site www.buscapronta.com . Para dados especificamente de registros gerais pesquise nos arquivos BUSCAPRONTA DIV. ATENÇÃO: Quando pesquisar em nossos arquivos, ao digitar o sobrenome procurado, faça- o, sempre que julgar necessário, COM E SEM os acentos agudo, grave, circunflexo, crase, til e trema. Sobrenomes com (ç) cedilha, digite também somente com (c) ou com dois esses (ss). Sobrenomes com dois esses (ss), digite com somente um esse (s) e com (ç). (ZZ) digite, também (Z) e vice-versa. (LL) digite, também (L) e vice-versa. Van Wolfgang – pesquise Wolfgang (faça o mesmo com outros complementos: Van der, De la etc) Sobrenomes compostos ( Mendes Caldeira) pesquise separadamente: MENDES e depois CALDEIRA. Tendo dificuldade com caracter Ø HAMMERSHØY – pesquise HAMMERSH HØJBJERG – pesquise JBJERG BUSCAPRONTA não reproduz dados genealógicos das pessoas, sendo necessário acessar os documentos Internet correspondentes para obter tais dados e informações. DESEJAMOS PLENO SUCESSO EM SUA PESQUISA. -
LERMA REPORT V1.1 PART II
LERMA 2007-2012 Contractualisation vague D Results vol. 3 Bibliography (version 1.1) Conception graphique S. Cabrit Sect. 3. Bibliography Sect. 3. Bibliography A detailed analysis of the lab's production would need a huge investment to be truly meaningful, so we better stay with simple facts. The table below shows the distribution among years and thematic poles of refereed and non refereed publications during the reporting period. Year ACL Publ. Pole 1 Pole 2 Pole 3 Pole 4 Overlap 2007 119 37 45 27 18 8 2008 133 40 57 25 21 10 2009 116 27 59 17 17 4 2010 214 50 112 25 87 60 2011 197 81 71 53 51 59 2012 77 31 29 15 10 8 Total 856 266 373 162 204 149 Table 2: Count of refereed publications from the ADS database Year Publis ACL Pôle 1 Pôle 2 Pôle 3 Pôle 4 Overlap 2007 2409 988 798 220 502 99 2008 2239 633 1166 222 290 72 2009 1489 341 852 119 196 19 2010 3283 1394 1412 213 1548 1284 2011 3035 2331 637 1345 1434 2712 2012 239 183 62 20 2 28 Totaux 12694 5870 4927 2139 3972 4214 Table 3: Count of the citations to the refereed publications from the ADS database. Beware the incompleteness of citations to plasma physics, molecular physics, remote sensing and engineering papers in this database Year ACL Publ. Pole 1 Pole 2 Pole 3 Pole 4 2007 20 27 18 8 28 2008 17 16 20 9 14 2009 13 13 14 7 12 2010 15 28 13 9 18 2011 15 29 9 25 28 2012 3 6 2 1 0 Totaux 15 22 13 13 19 Table 4: Average citation rate for the same publications Sect. -
2015 Spring Commencement Metropolitan State University of Denver
2015 SPRING COMMENCEMENT METROPOLITAN STATE UNIVERSITY OF DENVER SATURDAY, MAY 16, 2015 SPRING COMMENCEMENT SATURDAY, MAY 16, 2015 Letter from the President .......................... 2 MSU Denver: Transforming Lives, Communities and Higher Education .... 3 Marshals, Commencement Planning Committee, Retirees ............ 4 In Memoriam, Board of Trustees ............. 5 Academic Regalia ....................................... 6 Academic Colors ......................................... 7 Provost’s Award Recipient ......................... 8 Morning Ceremony Program .................... 9 President’s Award Recipient ................... 10 Afternoon Ceremony Program ................ 11 Morning Ceremony Candidates School of Education and College of Letters, Arts and Sciences ........................................ 12 Afternoon Ceremony Candidates College of Business and College of Professional Studies ..........20 Seating Diagrams ................................….27 1 DEAR 2015 SPRING GRADUATION CANDIDATES: Congratulations to you, our newest graduates! And welcome to your families and friends who have anticipated this day — this triumph — with immense pride. Each of our more than 80,000 graduates is unique, but all have one thing in common: Their lives were transformed by the education they received at MSU Denver. Most have stayed in Colorado, where they teach our children, own small businesses, create beautiful works of art, counsel families in crisis and design cutting-edge products that improve our lives. They are role models who have infused our state and their neighborhoods with economic growth, civic responsibility and culture. They have seized the opportunity to transform their families and their communities. Now it is your time to begin making the most of all that you have learned! MSU Denver transformed higher education in Colorado when, 50 years ago in the fall of 1965, we opened our doors with six majors, 1,187 students and a mission to give the opportunity to earn a college degree to almost anyone willing to take on the challenge. -
Explosion of Comet 17P/Holmes As Revealed by the Spitzer Space Telescope
Manuscript Pages: 51, Tables: 4, Figures: 18 Explosion of Comet 17P/Holmes as revealed by the Spitzer Space Telescope William T. Reach Infrared Processing and Analysis Center, MS 220-6, California Institute of Technology, Pasadena, CA 91125 [email protected] Jeremie Vaubaillon Institut de M´ecanique C´elesteet de Calcul des Eph´em´erides,77´ avenue Denfert-Rochereau, 75014 Paris, France Carey M. Lisse Johns Hopkins Applied Physics Laboratory, SD/SRE-MP3/E167, 11100 Johns Hopkins Road, Laurel, MD 20723 Mikel Holloway Holloway Comet Observatory, Van Buren, AR Jeonghee Rho Spitzer Science Center, MS 220-6, California Institute of Technology, Pasadena, CA 91125 Proposed running head: Explosion of comet Holmes arXiv:1001.4161v2 [astro-ph.EP] 25 Jan 2010 { 2 { Abstract An explosion on comet 17P/Holmes occurred on 2007 Oct 23, projecting particulate debris of a wide range of sizes into the interplanetary medium. We observed the comet using the mid- infrared spectrograph (5{40 µm), on 2007 Nov 10 and 2008 Feb 27, and the imaging photometer (24 and 70 µm), on 2008 Mar 13, on board the Spitzer Space Telescope. The 2007 Nov 10 spectral mapping revealed spatially diffuse emission with detailed mineralogical features, primarily from small crystalline olivine grains. The 2008 Feb 27 spectra, and the central core of the 2007 Nov 10 spectral map, reveal nearly featureless spectra, due to much larger grains that were ejected from the nucleus more slowly. Optical images were obtained on multiple dates spanning 2007 Oct 27 to 2008 Mar 10 at the Holloway Comet Observatory and 1.5-m telescope at Palomar Observatory. -
A'ana WILLIAM JARRET, 62, of Honolulu, Died March 15, 1993. He
A’ANA WILLIAM JARRET, 62, of Honolulu, died March 15, 1993. He was born in Honolulu. He worked for Oahu Transport Co. and Dole of Castle & Cookie. Survived by wife. Mary E. A’ana; sons, John, Bruce and Keith; daughter, Mrs. Mike (Wilette) Walter; five grandchildren; two great-grandsons; sisters, Beatrice Ogate, Angeline Paikai, and Penny Hajiwara; brother, Charles. Friends may call 6 to 9 p.m. Monday at Borthwick Mortuary; service 7:30 p.m. Cremation. No flowers. Aloha attire. [Honolulu Advertiser 19 March 2010] AARONA, ANNIE KUULEIOKEALALOA, 67, of Honolulu, died Nov. 20, 1993. She was born in Eleele, Kauai, and was a full-blooded Hawaiian retired from Tripler Army Medical Center. Survived by brother, William “Bucky”; sisters, Elizabeth Kepilino, Mrs. Joseph (Bertha K.) Huihui and Mrs. Larry (Isabelle N.) Mariano; aunt and uncle; nieces and nephews; cousins. Friends may call 6 to 9 p.m. Monday at Co-Cathedral of Saint Theresa; Mass 7:30 p.m. Or call 8 a.m. to noon Tuesday. Burial at Diamond Head Memorial Park. Arrangements by Nuuanu Memorial Park Mortuary. [Honolulu Advertiser 27 November 1993] AAU, ITUMALO FALEPULE, 74, of American Samoa, died June 25, 1993. He was born in Faleasao, Manu’atele, American Samoa and was a school teacher and judge in American Samoa. Survived by wife, Vavaifono; son, Iotamo; daughters, Tafaifa, Mataina A.; sisters, Atoaolemasina A. Gordon of American Samoa, Vaeaolemasina, Aofia A. Matautia; nieces and nephews. Friends may call 8 to 9 a.m. Friday at Mililani Downtown Mortuary; service 9 a.m. Burial at Valley of the Temples. -
Nasa'suniversityprogram
NASA TM X-74142 NASA'SUNIVERSITYPROGRAM /'_lkjI^r'T,_lCIVL ni:}AklTq%.41t_,• , _ & ..........RF.qFARCH CONTRACTS _77-13891 Unclas G3/_l 582o0 , / j National Aeronautics and Space Administration Office of University Affairs Washington, D. C. 20546 FISCAL YEAR 1 976 IMPORTANT NOTICE This report is compiled primarily from information obtained from two internal NASA sources: 1. "CASE Report on Support of Colleges and Universities" (NASA Form 1356). 2. "Individual Procurement Action Report" (NASA Form 507). Therefore, other sources should be used for completing Forms 507 or 1356. # NASA'S UNIVERSITY PROGRAM ACTIVE GRANTS AND RESEARCH CONTRACTS FISCAL YEAR 1976 National Aeronautics and Space Administration Oifice of University Affairs Washington, D.C. 20546 I Acknowledgements This report was developed in the Policy Coordination Division of the Office of University Affairs under the guidance of W. A. Greene, Chief. Preparation of the input data for processing was accomplished by Doris J. Goodwin, Management Information Systems Officer. The Scientific and Technical Information Office produced the reproduction masters on the Phdton Computer. Additional Copies This publication is available from the National Technical Information Service (NTIS), 5285 Port Royal Rd., Springfield, Virginia 22161 for $4.75. FOREV¢ORD AsbasicpolicyNASAbelievesthatcollegesand universities should be encouraged to participate in the nation's space and aeronautics program to the maximum extent ........ ,-,4 111 _lUt_,, 1.1, Ulll v_,| ol_l_o are considered as partners with government and industry in the nation's aerospace program. NASA's objective is to have them bring their scientific, engineering, and social research competence to bear on aerospace problems and on the broader social, economic, and international i/nplications of NASA's technical and scientific programs. -
User Guide To
USER GUIDE TO 1 2 5 0 , 000 S CA L E L U NA R MA P S DANNY C. KINSLER Lunar Science Institute 3303 NASA Road #1 Houston, TX 77058 Telephone: 713/488-5200 Cable Address: LUNSI The Lunar Science Institute is operated by the Universities Space Research Association under Contract No. NSR 09-051-001 with the National Aeronautics and Space Administration. This document constitutes LSI Contribution No. 206 March 1975 USER GUIDE TO 1 : 250 , 000 SCALE LUNAR MAPS GENERAL In 1 972 the NASA Lunar Programs Office initiated the Apoll o Photographic Data Analysis Program. The principal point of this program was a detail ed scientific analysis of the orbital and surface experiments data derived from Apollo missions 15, 16, and 17 . One of the requirements of this program was the production of detailed photo base maps at a useabl e scale . NASA in conjunction with the Defense Mapping Agency (DMA) commenced a mapping program in early 1973 that would lead to the production of the necessary maps based on the need for certain areas . This paper is desi gned to present in outline form the neces- sary background information for users to become familiar with the program. MAP FORMAT The scale chosen for the project was 1:250,000* . The re- search being done required a scale that Principal Investigators (PI's) using orbital photography could use, but would also serve PI's doing surface photographic investigations. Each map sheet covers an area four degrees north/south by five degrees east/west. The base is compiled from vertical Metric photography from Apollo missions 15, 16, and 17. -
Quantitative and Qualitative Factors for PSPS Decision-Making
Quantitative and Qualitative Factors for PSPS Decision-Making Appendix May 2021 Contents Appendix A: Quantitative and Qualitative Factors for PSPS Decision-making, May 2021 Version.............. 3 Appendix B: PSPS Wind Speed Thresholds by Circuit as of 04/01/21 ...................................................... 15 Appendix A: Quantitative and Qualitative Factors for PSPS Decision- making, May 2021 Version SCE’s Quantitative and Qualitative Factors for PSPS Decision-making was revised in August of 2021 to include updated information on SCE’s new Fire Potential Index (FPI) thresholds and on the new In-Event Risk Calculation tool. The original version, published in May 2021, is produced below. QUANTITATIVE AND QUALITATIVE FACTORS FOR PSPS DECISION-MAKING May 2021 As the severity and frequency of wildfires in California continues to grow,1 the state’s utilities, including Southern California Edison, have implemented Public Safety Power Shutoffs (PSPS) to reduce the risk of electrical infrastructure igniting a significant wildfire. SCE’s core objective is to keep customers safely energized, which is why PSPS remains a tool of last resort. We forecast with as much granularity as possible and then work to reduce the number of customers impacted. Customer impacts are reduced by de-energizing only when necessary, based on real-time weather reporting; isolating only those circuits that present REDUCING THE NEED FOR significant risk; moving customers between circuits PUBLIC SAFETY POWER (sectionalization) and turning off specific segments SHUTOFFS while keeping other segments of the same circuit Concurrent with the work that SCE is doing energized (segmentation). to reduce the number of customer impacts from PSPS, we are increasing grid resiliency We use preset thresholds for dangerous wind in high fire risk areas through grid hardening speeds, low humidity and dry fuels as the basis of measures.