A 16-moment Fast Solar Wind Model

Details A 16-moment Fast Solar Wind Model A 16-moment Fast Solar Wind Model

Jan 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999ssrv...87..253l&link_type=abstract

Space Science Reviews, v. 87, Issue 1/2, p. 253-256 (1999).

Physics

2

Scientific paper

A 16-moment fast solar wind model based on a bi-Maxwellian velocity
distribution is presented. Although the proton heat flux density is
found to be significantly smaller than the classical Spitzer-Härm
value, it still plays a significant role in shaping the proton
temperature anisotropy in the fast solar wind.

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