Format

Send to

Choose Destination
Phys Rev Lett. 2011 Nov 11;107(20):201102. Epub 2011 Nov 11.

Modified temperature-anisotropy instability thresholds in the solar wind.

Author information

1
Institut für Theoretische Physik, Lehrstuhl IV: Weltraum- und Astrophysik, Ruhr-Universität Bochum, Germany.

Abstract

The proton and electron temperature anisotropies in the solar wind are constrained by the instability thresholds for temperature-anisotropy-driven kinetic plasma instabilities. The modifications to the marginal instability conditions from accounting for the influence of damping connected with the collisional effects in the solar wind plasma are calculated for right- and left-handed polarized parallel propagating Alfvén waves and mirror and firehose fluctuations. These modifications provide tighter threshold constraints compared to the marginal thresholds but do not fully explain the observations at small values of the parallel plasma beta.

Supplemental Content

Full text links

Icon for American Physical Society
Loading ...
Support Center