SH23C:
Coronal Magnetism II

Tuesday, 16 December 2014: 1:40 PM-3:40 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:

1:40 PM
 
Coronal Extreme Ultraviolet (EUV) Waves and Their Seismological Applications
Wei Liu, Stanford University, Stanford, CA, United States and Leon Ofman, Catholic University of America, Washington, DC, United States
1:59 PM
 
Coronal Modeling with Flux-Evolved Maps: Comparison with Observations
Jon Linker1, Cooper Downs1, Roberto Lionello1, Ronald M. Caplan1, Zoran Mikic1, Pete Riley1, Carl J Henney2 and Charles Nickolos Arge3, (1)Predictive Science Inc., San Diego, CA, United States, (2)Air Force Research Laboratory Kirtland AFB, Kirtland AFB, NM, United States, (3)AFRL/RVBXS, Kirtland Afb, NM, United States
2:13 PM
 
Combining Linear Polarization Measurements of both Forbidden/Permitted Coronal Emission Lines for measuring the Vector Magnetic Field in the Solar Corona
Gabriel Ionel Dima, Jeff R. Kuhn and Don Mickey, University of Hawaii at Manoa, Institute for Astronomy, Honolulu, HI, United States
2:32 PM
 
Methods for estimating total open heliospheric magnetic flux
Samantha DeMarco, Embry-Riddle Aeronautical University, Daytona Beach, FL, United States, Charles Nickolos Arge, AFRL/RVBXS, Kirtland Afb, NM, United States, Marios Pattichis, University of New Mexico Main Campus, Department of Electrical and Computer Engineering, Albuquerque, NM, United States, Rachel A Hock, USAF/AFRL, Albuquerque, NM, United States and Carl J Henney, Air Force Research Laboratory Kirtland AFB, Kirtland AFB, NM, United States
2:46 PM
 
Use of Magnetic Field Modeling and Topology Analysis in Understanding the Evolution and Eruption of Coronal Sigmoids
Antonia Stefanova Savcheva, Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, United States
3:05 PM
 
SIMULATIONS OF FILAMENT CHANNEL FORMATION
Kalman Joshua Knizhnik, Johns Hopkins University, Baltimore, MD, United States, Spiro K Antiochos, NASA GSFC, Silver Spring, MD, United States and C Richard DeVore, NASA Goddard Space Flight Center, Greenbelt, MD, United States
3:19 PM
 
Constraining Solar Coronal Magnetic Fields with New Radio Observing Techniques
Bin Chen, Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, United States, Dale E Gary, New Jersey Institute of Technology, Newark, NJ, United States and Tim Bastian, National Radio Astronomy Observatory, Charlottesville, VA, United States