Altitude dependence of H changes at Magsat altitudes (325-550 km)

Details Altitude dependence of H changes at Magsat altitudes (325-550 km) Altitude dependence of H changes at Magsat altitudes (325-550 km)

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990p%26ss...38..883k&link_type=abstract

Planetary and Space Science (ISSN 0032-0633), vol. 38, July 1990, p. 883-888.

Computer Science

1

Geomagnetism, Magsat Satellites, Upper Ionosphere, Atmospheric Radiation, Slabs

Scientific paper

Changes of the H component observed by Magsat for equatorial dawn and dusk passes at seven altitude slabs equivalent to about 30 km each, viz 340-370, 370-400, 400-430, 430-460, 460-490, 490-520, and 520-540 km, were compared with ground D(st). The correlation coefficients were generally high (greater than + 0.90) except for some slabs in some longitude belts, when correlations were lower, indicating these slabs as possible sources of some stray, transient currents. However, Delta H(0) were always negative for all slabs, indicating that, if a steady current existed, it should be above the ground, but below 340 km altitude.

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