A possible explanation of the reduced temperature in coronal holes

Details A possible explanation of the reduced temperature in coronal holes A possible explanation of the reduced temperature in coronal holes

Apr 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980pazh....6..246k&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 6, Apr. 1980, p. 246-250.) Soviet Astronomy Letters, vol. 6, Mar.-Apr. 1980, p. 135-137

Astronomy and Astrophysics

Astronomy

Coronal Holes, Plasma Density, Solar Temperature, Solar Wind, Absorptivity, Electron Density (Concentration), Energy Absorption, Flow Geometry, Flux Density, Magnetohydrodynamic Flow, Solar Wind Velocity

Scientific paper

The dependence of the absorption coefficient on the coronal plasma density in the distance range r = 1.05-1.5 solar radius is established for various waves that heat the corona and the solar wind. The wave absorption coefficient depends more strongly on the density than does the coronal emission; it is this differential which causes the less dense coronal holes to appear cooler than quiet regions.

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