Transition region, corona, and solar wind in coronal holes

Details Transition region, corona, and solar wind in coronal holes Transition region, corona, and solar wind in coronal holes

Apr 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986jgr....91.4111h&link_type=abstract

Journal of Geophysical Research (ISSN 0148-0227), vol. 91, April 1, 1986, p. 4111-4125.

Physics

201

Coronal Holes, Magnetohydrodynamic Waves, Plasma Heating, Solar Temperature, Solar Wind Velocity, Conductive Heat Transfer, Energy Dissipation, Plasma Turbulence

Scientific paper

The formation of wind-driven solar model based on a new hypothesis for nonlinear wave dissipation is described. The equations and solutions used to derive the model are examined. The corona and solar wind are analyzed. The model is applied to observations and it is detected that it displays the proper steep temperature rise to a maximum coronal temperature in excess of 10 to the 6th K, a solar wind flux in excess of 3.5 x 10 to the 8th/sq cm per sec at 1 AU, and nonthermal velocities are observed at the bases of coronal holes; however, the model does not produce enough detail.

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