SH23C:
Coronal Magnetism II

Session ID#: 4406

Tuesday, 16 December 2014: 1:40 PM-3:40 PM
2012 (Moscone West)
Chairs:  Sarah E Gibson, National Center for Atmospheric Research, Boulder, CO, United States and Katharine Reeves, Center for Astrophysics | Harvard & Smithsonian, Cambridge, United States
Primary Convener:  Sarah E Gibson, National Center for Atmospheric Research, High Altitude Observatory, Boulder, CO, United States
Co-conveners:  Katharine Reeves, Center for Astrophysics | Harvard & Smithsonian, Cambridge, United States and Stephen M White, Air Force Research Laboratory Albuquerque, Albuquerque, NM, United States
OSPA Liaison:  Katharine Reeves, Center for Astrophysics | Harvard & Smithsonian, Cambridge, United States
Index Terms:

7509 Corona [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
7524 Magnetic fields [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
7594 Instruments and techniques [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
7974 Solar effects [SPACE WEATHER]
Virtual Option?: No

Abstracts Submitted to this Session:

SH23C-01
Coronal Extreme Ultraviolet (EUV) Waves and Their Seismological Applications (Invited) (3314)
Wei Liu, University of California Riverside, Riverside, CA, United States and Leon Ofman, Catholic University of America, Physics, Washington, DC, United States
SH23C-02
Coronal Modeling with Flux-Evolved Maps: Comparison with Observations (17391)
Jon Linker1, Cooper Downs1, Roberto Lionello1, Ronald M. Caplan2, Zoran Mikic1, Pete Riley1, Carl J Henney3 and Charles Nickolos Arge4, (1)Predictive Science Inc., San Diego, CA, United States, (2)Predictive Science Inc., San Diego, United States, (3)Air Force Research Laboratory Albuquerque, Albuquerque, NM, United States, (4)NASA Goddard Space Flight Center, Greenbelt, United States
SH23C-03
Combining Linear Polarization Measurements of both Forbidden/Permitted Coronal Emission Lines for measuring the Vector Magnetic Field in the Solar Corona (Invited) (3186)
Gabriel Ionel Dima1, Jeff R. Kuhn2 and Don Mickey1, (1)University of Hawaii at Manoa, Institute for Astronomy, Honolulu, HI, United States, (2)Institute for Astronomy, University of Hawaii, Makawao, United States
SH23C-04
Methods for estimating total open heliospheric magnetic flux (26492)
Samantha Wallace, Embry-Riddle Aeronautical University, Daytona Beach, FL, United States, Charles Nickolos Arge, NASA Goddard Space Flight Center, Greenbelt, 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 Albuquerque, Albuquerque, NM, United States
SH23C-05
Use of Magnetic Field Modeling and Topology Analysis in Understanding the Evolution and Eruption of Coronal Sigmoids (Invited) (4293)
Antonia Stefanova Savcheva, Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, United States
SH23C-06
SIMULATIONS OF FILAMENT CHANNEL FORMATION (17191)
Kalman Joshua Knizhnik, US Naval Research Laboratory, Washington, DC, United States, Spiro K Antiochos, NASA GSFC, Greenbelt, United States and C Richard DeVore, NASA Goddard Space Flight Center, Greenbelt, MD, United States
SH23C-07
Constraining Solar Coronal Magnetic Fields with New Radio Observing Techniques (Invited) (3825)
Bin Chen, Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, United States, Dale E Gary, New Jersey Institute of Technology, Center for Solar-Terrestrial Research, Newark, United States and Tim Bastian, National Radio Astronomy Observatory, Charlottesville, VA, United States
See more of: SPA-Solar and Heliospheric Physics