Gallagher iaa 20121003_final
On going and planned activities by LAC group: Processing, Visualization and Analysis of Spatio-temporal Dynamics Reinaldo R. Rosa [email protected].
Observations. The SPIRIT sometimes observes in a high-temperature Mg XII 8.42 Å line large-scale features existing many hours high in the corona (Zhitnik.
Nobeyama Symposium 2004 Oct 29NJIT Center for Solar Terrestrial Research1 / 44 FASR Flare Science: Lessons from the Nobeyama Radioheliograph Dale E. Gary.
The Frequency Agile Solar Radiotelescope Current Status & Plans T. S. Bastian NRAO.
Electron Acceleration and Transport in Microwave Flaring Loops V. Melnikov (Radiophysical Research Institute, Russia) Nobeyama Symposium, 25-29 October.
Analysis of the polarization degree distribution along limb flaring loop of July 19, 2012 S. Kuznetsov 1, A. Morgachev 1 V. Melnikov 2 Radiophysical Research.
V.P. Maksimov, D.V. Prosovetsky, V.V. Grechnev, B.B. Krissinel
NoRH Observations of Prominence Eruption Masumi Shimojo Nobeyama Solar Radio Observatory NAOJ/NINS 2004/10/28 Nobeyama Symposium 2004 @ SeiSenRyo.
Conclusions. 1. Plasma parameters in the arcade: Ne ~10 10 cm -3 , Te ~6 MK.
NoRH Observations of Prominence Eruption
Altyntsev A. T., Kuznetsov A.A., Meshalkina N.S.
