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  • 1
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    Unknown
    In:  Other Sources
    Publication Date: 2019-06-27
    Description: Observation of a systematic increase in the mean energy of auroral electrons as the total precipitated energy increases. The change in 4278-A N2(+) intensity from about 50 R to about 10 kR correlates better with the change in mean energy of the precipitating electrons than with the change in number flux. Nightside aurora that exhibit this property superimpose on a wide region of soft (less than or about equal to 1 keV) precipitation that extends from the equatorial boundary of aurora to well poleward of normal visible aurora. On the dayside, the soft 'cusp' precipitation generates the statistical oval, although there may be larger energy inputs equatorward of the oval.
    Keywords: SPACE RADIATION
    Type: Journal of Geophysical Research; 77; Feb. 1
    Format: text
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  • 2
    Publication Date: 2019-07-13
    Keywords: SPACE RADIATION
    Type: Magnetosphere-ionosphere interactions; Advanced Study Institute; Apr 14, 1971 - Apr 23, 1971; Dalseter; Norway
    Format: text
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  • 3
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    Unknown
    In:  Other Sources
    Publication Date: 2019-07-13
    Description: Auroral electron and proton precipitation patterns, measuring airglow emissions
    Keywords: SPACE RADIATION
    Type: THE RADIATING ATMOSPHERE SYMPOSIUM; Aug 03, 1970 - Aug 14, 1970; KINGSTON, ONTARIO; CANADA
    Format: text
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