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Examination of Radiation Belt Dynamics During Substorm Clusters: Magnetic Local Time Variation and Intensity of Precipitating Fluxes.

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Title: Examination of Radiation Belt Dynamics During Substorm Clusters: Magnetic Local Time Variation and Intensity of Precipitating Fluxes.
Authors: Rodger, Craig J.1 (AUTHOR) craig.rodger@otago.ac.nz, Clilverd, Mark A.2 (AUTHOR), Hendry, Aaron T.1 (AUTHOR), Forsyth, Colin3 (AUTHOR)
Source: Journal of Geophysical Research. Space Physics. Dec2022, Vol. 127 Issue 12, p1-24. 24p.
Subject Terms: *Geomagnetism, Radiation belts, Low earth orbit satellites, Magnetic declination
Abstract: Substorms are short‐lived but significant reconfigurations of the geomagnetic field during which energetic particles are injected into the inner magnetosphere close to magnetic midnight. There is currently a need to quantify substorm‐driven energetic electron precipitation (EEP) to better understand its role in radiation belt dynamics and to quantify its impact on the atmosphere. As substorm injections trigger chorus waves, which have strong MLT, AE, and L‐shell dependence, we investigate the dependence of EEP in terms of these variables. We utilize many decades of low Earth orbit satellite observations to examine the typical statistical variability around substorm events identified by the Substorm Onsets and Phases from Indices of the Electrojet (SOPHIE) algorithm. In contrast to trapped flux enhancements, enhanced EEP is found to occur even for the quietest AE range of those considered (AE ≤ 100 nT, 100 nT < AE ≤ 300 nT, AE ≥ 300 nT). The MLT‐dependent analysis for all AE‐ranges shows a well‐defined variation in >30 keV EEP magnitude, with a distinct and deep minimum in the late afternoon sector (15–18 MLT), and maxima in the mid to late morning sector (6–12 MLT). The patterns show similarities to previously published whistler‐mode lower band chorus distributions with MLT. Clusters of substorms reliably produce enhancements in electron precipitation for >30 keV and >300 keV, with steadily increasing peak precipitation magnitudes with increasing AE. The peak precipitation flux L‐shell also moves inwards with increasing AE, in a similar way for the two energy ranges. Key Points: Magnetospheric substorm clusters produces energetic electron precipitation peaking in flux ∼2 hr after onsetThe precipitation of >30 keV electrons has a well‐defined pattern in Magnetic Local Time and L‐shell, peaking in the morning sectorIncreasing AE geomagnetic disturbance is found to be a good proxy of both >30 and > 300 keV peak precipitation flux for these events [ABSTRACT FROM AUTHOR]
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Abstract:Substorms are short‐lived but significant reconfigurations of the geomagnetic field during which energetic particles are injected into the inner magnetosphere close to magnetic midnight. There is currently a need to quantify substorm‐driven energetic electron precipitation (EEP) to better understand its role in radiation belt dynamics and to quantify its impact on the atmosphere. As substorm injections trigger chorus waves, which have strong MLT, AE, and L‐shell dependence, we investigate the dependence of EEP in terms of these variables. We utilize many decades of low Earth orbit satellite observations to examine the typical statistical variability around substorm events identified by the Substorm Onsets and Phases from Indices of the Electrojet (SOPHIE) algorithm. In contrast to trapped flux enhancements, enhanced EEP is found to occur even for the quietest AE range of those considered (AE ≤ 100 nT, 100 nT < AE ≤ 300 nT, AE ≥ 300 nT). The MLT‐dependent analysis for all AE‐ranges shows a well‐defined variation in >30 keV EEP magnitude, with a distinct and deep minimum in the late afternoon sector (15–18 MLT), and maxima in the mid to late morning sector (6–12 MLT). The patterns show similarities to previously published whistler‐mode lower band chorus distributions with MLT. Clusters of substorms reliably produce enhancements in electron precipitation for >30 keV and >300 keV, with steadily increasing peak precipitation magnitudes with increasing AE. The peak precipitation flux L‐shell also moves inwards with increasing AE, in a similar way for the two energy ranges. Key Points: Magnetospheric substorm clusters produces energetic electron precipitation peaking in flux ∼2 hr after onsetThe precipitation of >30 keV electrons has a well‐defined pattern in Magnetic Local Time and L‐shell, peaking in the morning sectorIncreasing AE geomagnetic disturbance is found to be a good proxy of both >30 and > 300 keV peak precipitation flux for these events [ABSTRACT FROM AUTHOR]
ISSN:21699380
DOI:10.1029/2022JA030750