SH13A:
Coronal Magnetism I Posters

Monday, 15 December 2014: 1:40 PM-6:00 PM
Chairs:  Sarah E Gibson, National Center for Atmospheric Research, Boulder, CO, United States and Kathy Reeves, Smithsonian Institution, Cambridge, MA, United States
Primary Conveners:  Sarah E Gibson, NCAR, Boulder, CO, United States
Co-conveners:  Kathy Reeves, Smithsonian Institution, Cambridge, MA, United States and Stephen M White, Air Force Research Laboratory, Albuquerque, NM, United States
OSPA Liaisons:  Kathy Reeves, Smithsonian Institution, Cambridge, MA, United States

Abstracts Submitted to this Session:

4065
 
Coronal Magnetism and Forward Solarsoft Idl Package
Sarah E Gibson, National Center for Atmospheric Research, Boulder, CO, United States
4066
 
Coronal Magnetism: Hanle Effect in UV and IR Spectral Lines
Nour-Eddine Raouafi, Applied Physics Laboratory Johns Hopkins, Laurel, MD, United States and Pete Riley, Predictive Science Inc., San Diego, CA, United States
4067
 
Hinode, SDO AIA, and CoMP Observations of a Coronal Cavity with a Hot Core
Kathy Reeves and Patricia Jibben, Smithsonian Institution, Cambridge, MA, United States
4068
 
3D Coronal Density Reconstruction and Retrieving Coronal Magnetic Field Structures during Solar Minimum and Maximum
Maxim Kramar, Catholic University of America, Washington, DC, United States, Vladimir Airapetian, NASA Goddard Space Flight Center, Greenbelt, MD, United States and Joseph M Davila, NASA Goddard SFC, Greenbelt, MD, United States
4069
 
3D Coronal Magnetic Field Reconstruction Based on Infrared Polarimetric Observations
Haosheng Lin, Institute for Astronomy, Honolulu, HI, United States, Maxim Kramar, Catholic University of America, Washington, DC, United States and Steven Tomczyk, National Center for Atmospheric Research, Boulder, CO, United States
4070
 
Laboratory Evidence That Line-Tied Toroidal Magnetic Fields Can Suppress Loss-of-Equilibrium Flux Rope Eruptions in the Solar Corona
Clayton Edward Myers1,2, Masaaki Yamada1, Elena Belova1, Hantao Ji1,2, Jongsoo Yoo1, William R Fox II1,2 and Jonathan Jara-Almonte1,2, (1)Princeton Plasma Physics Laboratory, Princeton, NJ, United States, (2)Princeton University, Princeton, NJ, United States
4071
 
3-D Reconstruction of Structure and Dynamics of Coronal Twistors From STEREO and SDO Imagery
Gregory L Slater and Samuel L Freeland, Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States
4072
 
Interpreting Coronal-Loop Oscillations as the Modes of a 2D Waveguide
Bradley Hindman, Joint Institute for Laboratory Astrophysics, Boulder, CO, United States and Rekha Jain, University of Sheffield, Sheffield, United Kingdom
4073
 
Magnetic Energies in Solar Active Regions and Flares Calculated from Automated Coronal Loop Tracing
Markus J Aschwanden, Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States
4074
 
SDO/AIA Observation and Modeling of Flare-excited Slow Waves in Hot Coronal Loops
Tongjiang Wang1, Leon Ofman1, Elena Provornikova1, Xudong Sun2 and Joseph M Davila3, (1)Catholic University of America, Washington, DC, United States, (2)Stanford University, Los Altos Hills, CA, United States, (3)NASA Goddard SFC, Greenbelt, MD, United States
4075
 
Novel Approach to Construction Realistic Magnetic Field Configuration in the Lower Solar Atmosphere
Viktor Fedun, University of Sheffield, Sheffield, S10, United Kingdom, Frederick Gent, University of Sheffield, Sheffield, United Kingdom and Robert Erdelyi, University of Sheffield, School of Mathematics and Statistics, Sheffield, United Kingdom
4076
 
The Existence Condition for Magnetic Flux-Current Surfaces in Magnetohydrostatic Equilibria
Jincheol No, Gwang-Son Choe, Sunjung Kim and Minhwan Jang, Kyung Hee University, Yongin, South Korea
4077
 
How Much Can We Estimate the Magnetic Helicity Influx During a Magnetic Flux Emergence with a Footpoint Tracking Method?
Gwang-Son Choe and Sunjung Kim, Kyung Hee University, Yongin, South Korea
4078
 
Microwave Spectra and Coronal Magnetic Structure of Flaring Active Regions
Jeongwoo Lee, Chungnam National University, Daejeon, South Korea, Jung-Eun Hwangbo, Chungbuk National University, Cheongju, South Korea and Sung-Hong Park, National Observatory of Athens, IAASARS, Athens, Greece
4079
 
Magnetic Field Modeling of Complex, Flare Productive Active Regions
Sarah Catherine Millholland1,2, Antonia Stefanova Savcheva2 and Edward E DeLuca2, (1)University of Saint Thomas, Saint Paul, MN, United States, (2)Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, United States
4080
 
Reconstructing the 3D coronal magnetic field using a Potential Field Source Surface model comparing different magnetograph input data
Martin Alexander Kruse II, Thies Peleikis, Lars Berger and R F Wimmer-Schweingruber, University of Kiel, Kiel, Germany
4081
 
Solar Coronal Holes and Open Magnetic Flux
Chris Lowder, Jiong Qiu, Robert James Leamon and Dana W Longcope, Montana State University, Bozeman, MT, United States
4082
 
The Pre- and Post-Launch Configuration of a CME Flux Rope
Timothy A Howard, Southwest Research Institute Boulder, Boulder, CO, United States and Craig E DeForest, Southwest Research Institute, Boulder, CO, United States
 
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