Radiative Hydrodynamic Silumation of He 10830

Cheng Jianxia, jxcheng@nju.edu.cn, School of Astronomy and Space Science, Nanjing University
Ding Mingde, School of Astronomy and Space Science, Nanjing University
Fang Cheng, School of Astronomy and Space Science, Nanjing University

Abstract
It is well known that chromospheric lines in solar flares are often red asymmetric. Sometimes we also get blue shift in line asymmetries. Based on radiative hydrodynamic simulations, we study the role of non-thermal electron beams to He 10830 spectra. We vary the parameters of the electron beam and compare the results with the observational studies. Our calculations can explain most of the observational results.