How are storm time injections different from nonstorm time injections? |
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| Authors: | D-Y Lee JA Hwang ES Lee KW Min WY Han UW Nam |
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| Institution: | aDepartment of Astronomy and Space Science, College of Natural Sciences and Institute for Basic Science Research, Chungbuk National University, 48 Gaeshin-dong, Heungduk-gu, Cheongju 361-763, Chungbuk, Korea;bPhysics Department, Korea Advanced Institute of Science and Technology, Taejon 305-701, Korea;cKorea Astronomical Observatory, Taejon 305-348, Korea |
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| Abstract: | One of the key elements of storms and substorms is the injection of energetic particles into the region of near geosynchronous orbit, that is, the sudden flux enhancement in the energy range of tens to hundreds of keV. This paper reports the observational results on how such injection features during storm times are different from those of nonstorm times. We particularly focus on the difference between proton injections and electron injections. Based on a number of storm time injection events that meet our strict selection criteria, we find a notable difference between proton injections and electron injections in the energy-spectral dependence of the flux enhancement averaged over the first 30 min after the injection onset: The average flux enhancement of many protons injections tends to be bigger at higher energy channels than at lower energy channels, but electron injections exhibit the opposite tendency for the energy-spectral dependence of flux enhancement, i.e., average flux enhancement decreasing with increasing energy. We show that this feature is almost unique only for the injection events during the storm main and early recovery phase. It is suggested that any successful scenario intended to model storm time injections should be able to explain this difference between proton injections and electron injections. |
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| Keywords: | Storm Substorm Energetic particle Injection |
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