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:

1:40 PM
 
The 2014 March 29 X-Flare: Results from the Best-Ever Flare Observation
Peter Young, George Mason University Fairfax, Fairfax, VA, United States
1:57 PM
 
Solar Flaring Activity and Coronal Heating.
Vasilis Archontis, University of St Andrews, St Andrews, KY16, United Kingdom and Viggo H Hansteen, Institute for Theoretical Astrophysics, Oslo, Norway
2:14 PM
 
Mass and energy of erupting plasma associated with coronal mass ejections in X-rays and EUV
Jin-Yi Lee1, John C Raymond2, Kathy Reeves2, Yong-Jae Moon1 and Kap-Sung Kim1, (1)Kyung Hee University, Yongin, South Korea, (2)Smithsonian Astrophysical Observatory, Cambridge, MA, United States
2:27 PM
 
Exploring He II 304 Å Spicules and Macrospicules at the Solar Limb
Alphonse C Sterling1, Ian Ross Snyder2, David Allen Falconer2 and Ronald L Moore1, (1)NASA Marshall Space Flight Center, Huntsville, AL, United States, (2)National Space Science and Technology Center, Huntsville, AL, United States
2:40 PM
 
Homologous Helical Jets: Observations by IRIS, SDO and Hinode and Data-Driven Simulations
Chun Ming Mark Cheung1, Bart De Pontieu1, Theodore D Tarbell1 and Yixing Fu2, (1)Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States, (2)University of California Berkeley, Berkeley, CA, United States
2:53 PM
 
Towards a Thermodynamic 3D MHD Model of Coronal Jets
Roberto Lionello1, Tibor Torok2, Jon Linker2 and Zoran Mikic2, (1)Predictive Science Incorporate, San Diego, CA, United States, (2)Predictive Science Inc., San Diego, CA, United States
3:06 PM
 
Investigating Alfven Wave Turbulence in Chromosphere and Corona Using Extreme Ultraviolet Imaging Spectrometer (EIS)
Mahboubeh Asgari-Targhi, Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, United States, Shinsuke Imada, Nagoya University, Solar-Terrestrial Environment Laboratory, Nagoya, Japan and Edward E DeLuca, SAO, Cambridge, MA, United States
3:23 PM
 
IRIS diagnostics of non-thermal particles in coronal loops heated by nanoflares
Paola Testa1, Bart De Pontieu2, Joel C Allred3, Mats Carlsson4, Fabio Reale5 and Adrian Nigel Daw3, (1)Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, United States, (2)Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States, (3)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (4)University of Oslo, Oslo, Norway, (5)University of Palermo, Dipartimento di Fisica & Chimica, Palermo, Italy