SH53D:
Mass and Energy Transfer Between the Solar Photosphere and Corona II
SH53D:
Mass and Energy Transfer Between the Solar Photosphere and Corona II
Mass and Energy Transfer Between the Solar Photosphere and Corona II
Session ID#: 4414
Friday, 19 December 2014: 1:40 PM-3:40 PM
2016 (Moscone West)
Chairs: Bart De Pontieu, Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States and Viggo Haraldson Hansteen, Institute for Theoretical Astrophysics, University of Oslo, Oslo, Norway
Primary Convener: Bart De Pontieu, Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States
Co-conveners: Viggo Haraldson Hansteen, Inst Theoretical Astrophysics, Oslo, Norway and Karel Schrijver, Lockheed Martin Adv Techn Ctr, Palo Alto, CA, United States
OSPA Liaison: Bart De Pontieu, Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States
Index Terms:
7507 Chromosphere [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
7509 Corona [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
7529 Photosphere [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
7546 Transition region [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
Virtual Option?: No
Abstracts Submitted to this Session:
See more of: SPA-Solar and Heliospheric Physics
