z-logo
open-access-imgOpen Access
What Are the Relative Roles of Heating and Cooling in Generating Solar Wind Temperature Anisotropies?
Author(s) -
B. A. Maruca,
J. C. Kasper,
S. D. Bale
Publication year - 2011
Publication title -
physical review letters
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 3.688
H-Index - 673
eISSN - 1079-7114
pISSN - 0031-9007
DOI - 10.1103/physrevlett.107.201101
Subject(s) - solar wind , physics , anisotropy , plasma , adiabatic process , isotropy , cyclotron , instability , computational physics , dissipation , electron temperature , atomic physics , mechanics , thermodynamics , optics , nuclear physics

The content you want is available to Zendy users.

Already have an account? Click here to sign in.
Having issues? You can contact us here
Accelerating Research

Address

John Eccles House
Robert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom