Electron acceleration to high energies at quasi-parallel shock waves in the solar corona.

Details Electron acceleration to high energies at quasi-parallel shock waves in the solar corona. Electron acceleration to high energies at quasi-parallel shock waves in the solar corona.

Dec 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995a%26a...304..576m&link_type=abstract

Astronomy and Astrophysics, v.304, p.576

Astronomy and Astrophysics

Astrophysics

18

Acceleration Of Particles, Shocks, Sun: Corona, Magnetic Fields, Radio Radiation

Scientific paper

In the solar corona shock waves are generated by flares and/or coronal mass ejections. They manifest themselves in solar type II radio bursts appearing as emission stripes with a slow drift from high to low frequencies in dynamic radio spectra. Their nonthermal radio radiation indicates that electrons are accelerated to suprathermal and/or relativistic velocities at these shocks. As well known by extraterrestrial in-situ measurements supercritical, quasi-parallel, collisionless shocks are accompanied by so-called SLAMS (short large amplitude magnetic field structures). These SLAMS can act as strong magnetic mirrors, at which charged particles can be reflected and accelerated. Thus, thermal electrons gain energy due to multiple reflections between two SLAMS and reach suprathermal and relativistic velocities. This mechanism of accelerating electrons is discussed for the solar corona and may be responsible for the so-called "herringbones" observed in solar type II radio bursts.

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