Место издания:GSU, GA: Georgia State University, Atlanta, GA, USA Atlanta, GA, USA
Аннотация:Stellar/solar flares are usually connected with magnetic reconnection around chromosphere and corona, but impacts of comet-like bodies, FEBs, with the Sun/stars will also be accompanied by generation of a hot (around 10^7 K) plasma and high-temperature thin layer near photosphere, i.e., photospheric stellar flares, due to strong aerodynamic effects within chromosphere.