Multi-spacecraft observations of heliographic structure of the solar wind speed

Details Multi-spacecraft observations of heliographic structure of the solar wind speed Multi-spacecraft observations of heliographic structure of the solar wind speed

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988p%26ss...36.1329m&link_type=abstract

Planetary and Space Science (ISSN 0032-0633), vol. 36, Dec. 1988, p. 1329-1342.

Computer Science

10

Interplanetary Medium, Satellite Observation, Solar Wind Velocity, Velocity Distribution, Explorer 50 Satellite, Giotto Mission, High Speed, Low Speed, Space Plasmas

Scientific paper

Multispacecraft observations in the interplanetary space are used to build up a picture of the distribution of solar wind velocities in heliographic latitude and longitude. Analyses are made for the solar wind data obtained by Sakigake, Suisei, IMP-8 and Giotto between late 1985 and early 1987. Until January 1986, high-speed streams were extended across the equator from the high latitudes of the heliosphere. After March 1986, high-speed streams were rarely seen on the equator. Although there remained a slight wavy pattern in latitude-longitude structure, low-speed streams were basically ranged along the equator. After January 1987, the amplitude of this wavy pattern was further diminished and low-speed regions were completely aligned to the equator.

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