Constraints on high frequency wave heating of coronal holes and the fast solar wind

Details Constraints on high frequency wave heating of coronal holes and the fast solar wind Constraints on high frequency wave heating of coronal holes and the fast solar wind

May 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001agusm..sh41b04v&link_type=abstract

American Geophysical Union, Spring Meeting 2001, abstract #SH41B-04

Mathematics

Logic

2149 Mhd Waves And Turbulence, 7509 Corona

Scientific paper

We present numerical simulations as well as model calculations of ion heating via interaction with a spectrum of outward propagating Alfven waves and compare them with phenomenological models of the solar wind. Approximations for the total maximm amount of energy that may be absorbed by minor ions, as well as the overall absorption spectrum are given and compared to predictions from quasi-linear theory. The simulations use the previously developed Expandng Box Model to provide limits on the efficiency of cyclotron heating.

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