Transition region of the solar wind

Details Transition region of the solar wind Transition region of the solar wind

Jun 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ge%26ae..26..369l&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 26, May-June 1986, p. 369-372. In Russian.

Physics

Plasma Physics

9

Interplanetary Medium, Multiphase Flow, Nonuniform Plasmas, Plasma Physics, Solar Wind Velocity, Transition Points, Anomalies, Heliosphere, Plasma Jets

Scientific paper

The most significant acceleration of the solar wind (SW) and the
mixed-flow regime arise in the transition region of the SW. The
mixed-flow concept is based on data concerning the jet structure of the
flow in the interplanetary medium. An analysis is made of
interplanetary-plasma anomalies identified with the transition region.

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