Solar wind structure observed by interplanetary scintillation and spacecraft in 1985 and 1986

Details Solar wind structure observed by interplanetary scintillation and spacecraft in 1985 and 1986 Solar wind structure observed by interplanetary scintillation and spacecraft in 1985 and 1986

Mar 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987nuria..34....9o&link_type=abstract

Nagoya University, Research Institute of Atmospherics, Proceedings (ISSN 0077-264X), vol. 34, March 1987, p. 9-21.

Computer Science

Sound

Interplanetary Medium, Interplanetary Spacecraft, Japanese Spacecraft, Scintillation, Solar Wind, Wind Profiles, Leading Edges, Satellite Sounding, Solar Activity, Spacecraft Trajectories, Wind Velocity

Scientific paper

Solar wind speed maps on the source surface were derived from interplanetary scintillation observations and refined using Sakigake and Suisei data. During September-November of 1985, the leading edge of the northern high-speed region had a large latitudinal speed gradient of about 40 km/s/deg and inclined at a small angle to the longitudinal direction on the source surface. During January-April of 1986, the southern high-speed region did not have a sharp leading edge; a temperature increase was observed while a density increase was not.

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