Heating and acceleration of minor ions in the solar wind

Details Heating and acceleration of minor ions in the solar wind Heating and acceleration of minor ions in the solar wind

Jul 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998a%26a...335..303c&link_type=abstract

Astronomy and Astrophysics, v.335, p.303-308 (1998)

Astronomy and Astrophysics

Astrophysics

22

Acceleration Of Particles, Polarization, Sun: Corona, Solar Wind

Scientific paper

We make use of the results of a one-ion model of McKenzie et al. (1997) to obtain the critical solution describing the acceleration of a two-ion solar wind. The model includes preferential heating of the heavy ion species and the temperature anisotropy expected if the heating is predominantly due to ion-cyclotron damping. The relationship of the model to the picture emerging from UVCS/SOHO observations is discussed.

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