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- W14110958 abstract "The characteristics of erupting protons in the near-midnight MLT sector in the auroral zone are considered from measurements carried out on the Kosmos 348 artificial earth satellite. An analysis of the results demonstrates that a maximum of proton eruption with mean energy E/sub p/ greater than or equal to 6 keV with nearly isotropic pitch angle distribution near the equatorial boundary of the averaged H/sub ..cap alpha../ hydrogen emission glow zone is observed during magnetically quiescent periods. The eruption zone during the substorm of June 26, 1970 was divided into two regions at latitude ..lambda..-bar, a wide latitude region where longitudinal fluxes of low energy (E-bar/sub p/ approximately 0.5 to 1.5 keV) protons was observed, and a low latitude region, where E-bar/sub p/ approximately 4 to 8 keV with isotropic pitch angle distribution was observed. The results are interpreted on the basis of theoretical concepts on plasma convection under the effect of an electric field in the tail of the magnetosphere and on the formation of a neutral line with X-type point during a substorm." @default.
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- W14110958 date "1976-01-01" @default.
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- W14110958 title "Structure of the bursts of auroral protons" @default.
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