1 code implementation • 8 Sep 2017 • Makoto Uemura, Ryosuke Itoh, Ioannis Liodakis, Dmitry Blinov, Masanori Nakayama, Longyin Xu, Naoko Sawada, Hsiang-Yun Wu, Issei Fujishiro
The combined effect of the variation in $\delta$ and acceleration/cooling of electrons is probably responsible for the observed diversity of the polarization variations in the flares.
High Energy Astrophysical Phenomena Astrophysics of Galaxies
