On the causes of hard x-ray asymmetry in solar flares
Author:
Publisher
EDP Sciences
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://www.aanda.org/10.1051/0004-6361:20065670/pdf
Reference28 articles.
1. Difference between Spatial Distributions of the Hα Kernels and Hard X-Ray Sources in a Solar Flare
2. Deconvolution of Directly Precipitating and Trap‐precipitating Electrons in Solar Flare Hard X‐Rays. III.YohkohHard X‐Ray Telescope Data Analysis
3. Falewicz, R., Rudawy, P., & Siarkowski, M. 2005, ESA SP-600, 121
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