Wave-Trains in the Solar Wind. I: General Theory and Its Application to an Ideal, Isotropic, One-Fluid Plasma

Details Wave-Trains in the Solar Wind. I: General Theory and Its Application to an Ideal, Isotropic, One-Fluid Plasma Wave-Trains in the Solar Wind. I: General Theory and Its Application to an Ideal, Isotropic, One-Fluid Plasma

Feb 1973

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1973ap%26ss..20..373o&link_type=abstract

Astrophysics and Space Science, Volume 20, Issue 2, pp.373-389

Astronomy and Astrophysics

Astrophysics

4

Scientific paper

The main results of Whitham's averaged Lagrangian method for the
treatment of linear wave-trains in a weakly inhomogeneous, moving medium
are presented briefly. This method is then applied to an ideal,
isotropic, one-fluid plasma which can be taken for the lowest order
approximation for the interplanetary solar wind expansion.

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