GSTDTAP  > 气候变化
DOI10.1029/2021GL093879
Duration of Individual Relativistic Electron Microbursts: A Probe Into Their Scattering Mechanism
M. Shumko; L.W. Blum; A.B. Crew
2021-08-25
发表期刊Geophysical Research Letters
出版年2021
英文摘要

We used the Solar Anomalous and Magnetospheric Particle Explorer (SAMPEX) to identify and quantify the duration of relativistic, urn:x-wiley:00948276:media:grl62903:grl62903-math-0001 MeV, electron microbursts. A typical relativistic microburst has a urn:x-wiley:00948276:media:grl62903:grl62903-math-0002 millisecond (ms) duration, and the interquartile range of the duration distribution is 70-140 ms. We investigated trends in the microburst duration as a function of geomagnetic activity, L-shell, and magnetic local time (MLT). The clearest trend is in MLT: the median microburst duration doubles from 75 milliseconds at midnight to 140 milliseconds noon MLT. This trend is similar to the whistler mode chorus rising tone element duration trend, suggesting a possible relationship.

领域气候变化
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文献类型期刊论文
条目标识符http://119.78.100.173/C666/handle/2XK7JSWQ/336637
专题气候变化
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M. Shumko,L.W. Blum,A.B. Crew. Duration of Individual Relativistic Electron Microbursts: A Probe Into Their Scattering Mechanism[J]. Geophysical Research Letters,2021.
APA M. Shumko,L.W. Blum,&A.B. Crew.(2021).Duration of Individual Relativistic Electron Microbursts: A Probe Into Their Scattering Mechanism.Geophysical Research Letters.
MLA M. Shumko,et al."Duration of Individual Relativistic Electron Microbursts: A Probe Into Their Scattering Mechanism".Geophysical Research Letters (2021).
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