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• W3111412528 abstract "Fast magnetosonic (MS) waves are excited by the ring distribution of energetic protons preferably when the ring velocity (VR) is within a factor of 2 above or below the local Alfvén speed (VA). Here we examine the global distributions of MS waves and proton rings with 0.5VA ≤ VR ≤ 2VA based on 64 months (from October 25, 2012 to February 28, 2018) of Van Allen Probes observations. The statistical results show that MS waves are present over a broad region of L = 1.2–6.0 and 00–24 magnetic local time (MLT), with a higher occurrence rate at L = 2.5–5.5 on the dayside. Proton rings occur mainly on the dayside of L > 5.0. During active geomagnetic periods, both MS waves and proton rings occur more frequently and extend to low L-shells. The current results provide the further observational evidence that MS waves can be excited by proton rings at a distant region and propagate to low L-shells." @default.
• W3111412528 created "2020-12-21" @default.
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• W3111412528 date "2021-01-01" @default.
• W3111412528 modified "2023-10-17" @default.
• W3111412528 title "Correlated Observation on Global Distributions of Magnetosonic Waves and Proton Rings in the Radiation Belts" @default.
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• W3111412528 doi "https://doi.org/10.1029/2020ja028354" @default.
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