Quantifying loss of current sheet scattered electrons during the substorm growth phase
Particles trapped in the magnetosphere are naturally accelerated by the exchange of electromagnetic and kinetic energy, resulting in relativistic plasma populations. Through a number of processes, these particles can be scattered into the atmosphere and lost to interactions. Such precipitating parti...
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| Language: | en_US |
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2021
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| Online Access: | https://hdl.handle.net/2144/42586 |