Volume 478, Number 3, February II 2008
|Page(s)||889 - 895|
|Published online||04 December 2007|
Collisionless transport of energetic electrons in the solar corona at current-free double layers
Max-Planck-Institut für Sonnensystemforschung, Germany e-mail: email@example.com
2 Institute of Space Science, NCU, Taiwan
3 Keldysh Institute for Applied Mathematics, Russia
Accepted: 9 November 2007
Context.Impinging electron beams in the solar chromosphere generate hard X-ray radiation (HXR) through the collisional Bremstrahlung thick target model. The deduced electron distributions usually exhibit a broken-power-law. Assuming that the initial distribution function was a drift-Maxwellian, this indicates that the distribution of energetic electrons changes in the course of their propagation, from the looptop acceleration site to the high density chromosphere, via a collisionless scattering mechanism.
Aims. The formation of a broken-power-law spectrum via the particle interaction with the current-free weak double layers (DLs) in a reverse current beam plasma system.
Methods. The unstable waves generated in current-free coronal plasmas are first studied by means of a linear instability analysis. For most probable coronal plasma parameters, a one-dimensional electrostatic Vlasov-code simulation is performed to understand the nonlinear evolution of the instabilities and their influences on the electron distribution.
Results. DL structures cause a dissipation of low energy beam electrons and a stagnation of return-current electrons. Fast electron holes are formed, a secondary two-stream instability, caused by the DL-accelerated electrons. Electron and ion heating by DLs also takes place.
Conclusions. The plasma distributions of energetic electrons in the solar corona evolve via their interactions with nonlinear large-amplitude phase-space structures. At the late stage of evolution, the low-energy electrons are slowed down while the high energy part stays uninfluenced after the appearance of DLs. A major part of the return-current electrons change their direction to that of the injected beam. As a result the distribution becomes a broken-power-law as observed by chromospheric HXR radiation.
Key words: plasmas / waves / Sun: corona / Sun: flares
© ESO, 2008
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