Physics
Scientific paper
Nov 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987p%26ss...35.1347t&link_type=abstract
Planetary and Space Science (ISSN 0032-0633), vol. 35, Nov. 1987, p. 1347-1358.
Physics
337
Cislunar Space, Earth Magnetosphere, Geomagnetism, Magnetic Field Configurations, Current Density, Geomagnetic Tail, Kp Index, Models
Scientific paper
A previously proposed model (Tsyganenko and Usmanov, 1982) is extended by the incorporation of a large amount of magnetotail field measurements obtained by IMP and HEOS spacecraft between 1966 and 1980 to produce a series of global quantitative magnetic field models valid throughout the entire cislunar region of earth's magnetosphre. The data cover a range of distances between 4 and 70 earth radii and contain a total of 36682 vector averages. The present results are divided into groups corresponding to a sequence of Kp-index intervals and to different conditions in the solar wind.
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