1 Plasma flows during solar flares A. Berlicki Observatoire de Paris, Section de Meudon, LESIA (Astronomical Institute of the Wrocław University, Poland)
What can helicity redistribution in solar eruptions tell us about reconnection in these events? by Brian Welsch, JSPS Fellow (Short-Term ), Space Sciences.
Magnetic Reconnection Rate and Energy Release Rate Jeongwoo Lee 2008 April 1 NJIT/CSTR Seminar Day.
Particle acceleration and plasma heating in the chromosphere Alexander Stepanov, Pulkovo Observatory, St.Petersburg, Russia Valery Zaitsev Institute of.
Michael L. Kaiser STEREO Project Scientist NASA/Goddard Space Flight Center
Magnetic Reconnection Rate and Energy Release Rate
Observations of Eruptive Events with Two Radioheliographs, SSRT and NoRH
Plasma flows during solar flares
2010 August 04
Challenges in Understanding 3D Magnetic Reconnection in Observations and Simulations Session organizers: Peter Wyper (NASA Goddard Space Flight Center/Oak.
Flare Energy Build-Up in a Decaying Active Region Near a Coronal Hole
Department of Astronomy, Nanjing University, Nanjing 210093, China C. Fang, M. D. Ding, P. F. Chen Possible collaboration between Solar-B and the facilities.
