SH53D:
Mass and Energy Transfer Between the Solar Photosphere and Corona II
SH53D:
Mass and Energy Transfer Between the Solar Photosphere and Corona II
Friday, 19 December 2014: 1:40 PM-3:40 PM
Chairs: Bart De Pontieu, Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States and Viggo H Hansteen, Institute for Theoretical Astrophysics, Oslo, Norway
Primary Conveners: Bart De Pontieu, Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States
Co-conveners: Viggo H Hansteen, Inst Theoretical Astrophysics, Oslo, Norway and Karel Schrijver, Lockheed Martin Adv Techn Ctr, Palo Alto, CA, United States
OSPA Liaisons: Bart De Pontieu, Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States
Abstracts Submitted to this Session:
2:14 PM
2:40 PM
3:06 PM
See more of: SPA-Solar and Heliospheric Physics