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- W1968318655 abstract "Changes of the H component observed by MAGSAT for equatorial dawn and dusk passes at seven altitude slabs equivalent to ~30 km each, viz. 340–370, 370–400, 400–430, 430–460, 460–490, 490–520 and 520–540 km, were compared with ground Dst. The correlation coefficients were generally high ( > + 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, ΔH0, i.e. the intercepts on the ΔH0 axis, were always negative for all slabs, indicating that, if a steady current existed, it should be above the ground, but below 340 km altitude." @default.
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- W1968318655 date "1990-07-01" @default.
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- W1968318655 title "Altitude dependence of H changes at magsat altitudes (325–550 km)" @default.
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- W1968318655 doi "https://doi.org/10.1016/0032-0633(90)90055-u" @default.
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