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Shock drift electron acceleration and generation of waves |
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| Authors: | M Karlický M Vandas |
| Institution: | aAstronomical Institute, Academy of Sciences, 251 65 Ond?ejov, Czech Republic bAstronomical Institute, Academy of Sciences, Bo?ní II 1401, 141 31 Praha 4, Czech Republic |
| Abstract: | An analytically derived distribution function of reflected and accelerated electrons at a nearly perpendicular shock is presented. Then this distribution in a simplified form is introduced into a 1.5-D relativistic electromagnetic particle-in-cell (PIC) model and a generation of waves is studied. Numerical modeling shows not only a generation of Langmuir and high-frequency electromagnetic waves as expected, but also an efficient generation of whistler waves. Their role in emission processes of type II solar radio bursts is discussed. |
| Keywords: | Electrons: beam Electromagnetic waves Sun: radio bursts Simulation |
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