Solar and Heliospheric Physics General Contributions II Sun and Corona

Friday, 18 December 2015: 10:20-12:20
2011 (Moscone West)
Primary Conveners:  Todd Hoeksema, Stanford University, Stanford, CA, United States
Conveners:  Robyn M Millan, Dartmouth College, Hanover, NH, United States and Anja Stromme, SRI International Menlo Park, Menlo Park, CA, United States
Chairs:  Todd Hoeksema, Stanford University, Stanford, CA, United States and Shadia R Habbal, Institute for Astronomy, Honolulu, HI, United States
OSPA Liaisons:  Todd Hoeksema, Stanford University, Stanford, CA, United States
On solar oblateness measurements during the current solar cycle 24 (58255)
Mustapha Meftah1,2, Alain Hauchecorne2, Abdenour Irbah2 and Rock I Bush3, (1)CNRS, Paris Cedex 16, France, (2)LATMOS/IPSL/CNRS/UVSQ, Guyancourt, France, (3)Stanford University, Stanford, CA, United States
Fred Sigernes1,2, Pål Gunnar Ellingsen1,2, Silje Eriksen Holmen1,2, Pal Brekke1,3, Arne Danielsen4, Bernt Olsen5, Mikko Syrjäsuo1,2, Xiangcai Chen1,2, Margit Elisabet Dyrland1,2, Noora Partamies1,2, Lisa J Baddeley1,2, Dag A Lorentzen1,2, Marcus Aleksander Krogtoft6, Torstein Dragland6, Hans Mortensson6, Lisbeth Smistad6, Kjellmar Oksavik1,2, Craig J Heinselman7 and Shadia R Habbal8, (1)University Centre in Svalbard, Longyearbyen, Norway, (2)University of Bergen, Birkeland Centre for Space Science, Bergen, Norway, (3)Norwegian Space Centre, Oslo, Norway, (4)Brages 2, 1540 Vestby, Akershus, Norway, (5)Norwegian Broadcasting Corporation, Troms and Finnmark, Tromsø, Norway, (6)Lufttransport AS, Svalbard, Longyearbyen, Norway, (7)IRF Swedish Institute of Space Physics Kiruna, Kiruna, Sweden, (8)Institute for Astronomy, Honolulu, HI, United States
Full-sun synchronic EUV and coronal hole mapping using multi-instrument images: Data and software made available (81470)
Ronald M. Caplan, Cooper Downs and Jon Linker, Predictive Science Inc., San Diego, CA, United States
The Unusual Event of October 26, 2010: An “Almost” Coronal Hole (65621)
William Dean Pesnell, NASA / GSFC, Greenbelt, MD, United States and Rachel O'Connor, Smith College, Northampton, MA, United States
SDO/HMI -- RHESSI White-Light Flare Catalog: Matsushita Analysis (74335)
Juan Carlos Martinez Oliveros1, Hugh S Hudson1,2 and Sam Krucker1,3, (1)Space Sciences Laboratory, Berkeley, CA, United States, (2)University of Glasgow, Glasgow, United Kingdom, (3)University of Applied Sciences and Arts Northwestern Switzerland, Windisch, Switzerland
Energetic electrons and photospheric electric currents during solar flares (80254)
Sophie Musset, Paris Observatory, Paris, France
Why and How do Solar Eruptions Occur? Studies based on SDO/HMI Vector Magnetograms and Data-Driven MHD Simulations (Invited) (66633)
Chaowei Jiang, Chinese Academy of Sciences, SIGMA Weather Group, State Key Laboratory of Space Weather, National Space Science Center, Beijing, China; University of Alabama in Huntsville, Center for Space Plasma & Aeronomic Research, Huntsville, AL, United States
How Much Energy Can Be Stored in Solar Active Region Magnetic Fields? (81459)
Jon Linker, Cooper Downs, Tibor Torok, Viacheslav S Titov, Roberto Lionello, Zoran Mikic and Pete Riley, Predictive Science Inc., San Diego, CA, United States