Power of the solar wind in the acceleration region according to radio-occultation data

Details Power of the solar wind in the acceleration region according to radio-occultation data Power of the solar wind in the acceleration region according to radio-occultation data

Feb 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990pazh...16..163i&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 16, Feb. 1990, p. 163-168. In Russian. In Russian.

Astronomy and Astrophysics

Astronomy

1

Magnetohydrodynamic Waves, Radio Occultation, Solar Wind Velocity, Spatial Dependencies, Supersonic Speed, Velocity Distribution, Wave Propagation

Scientific paper

Results of measurements of solar wind velocity are presented for heliocentric distances between 3 and 80 solar radii. It is shown that, as the distance increases from 8 to 20 solar radii, the velocity increases from 40 km/s to 250 km/s and the power increases from 10 to the 18th to 3 x 10 to the 19th W. It is confirmed that the solar wind velocity becomes supersonic in this region.

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