The spatial structure of the solar wind transition region

Details The spatial structure of the solar wind transition region The spatial structure of the solar wind transition region

Sep 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991raf....34..971l&link_type=abstract

Radiofizika (ISSN 0021-3462), vol. 34, no. 9, p. 971-974.

Computer Science

Sound

Heliosphere, Mapping, Solar Wind, Supersonic Flow, Latitude, Solar Corona, Sounding

Scientific paper

The subsonic-to-supersonic transition area of the solar wind flow is
studied via five natural radio sounding sources used simultaneously. The
observations were performed in June 1988 at a 2.9-m wavelength. As the
sources passed different heliolatitudes, a 2D mapping of the solar wind
transonic region was obtained.

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