Characteristics of Sudden Commencements Observed by Van Allen Probes in the Inner Magnetosphere

Characteristics of Sudden Commencements Observed by Van Allen Probes in the Inner Magnetosphere We have statistically studied sudden commencement (SC) by using the data acquired from Van Allen Probes (VAP) in the inner magnetosphere (L = 3.0–6.5) and GOES spacecraft at geosynchronous orbit (L =∼ 6.7) from October 2012 to September 2017. During the time period, we identified 85 SCs in the inner magnetosphere and 90 SCs at geosynchronous orbit. Statistical results of the SC events reveal the following characteristics. (1) There is strong seasonal dependence of the geosynchronous SC amplitude in the radial BV component at all local times. However, BV shows weak seasonal variation on the dayside in the inner magnetosphere. (2) The local time dependence of the SC amplitude in the compressional BH component at geosynchronous orbit is similar to that in the inner magnetosphere. (3) In a nightside region of L = 5.0–6.5, ∼19% of BH events are negative, while ∼58% of BH events are negative at geosynchronous orbit. (4) The amplitude of the SC‐associated Ey perturbations varies systematically with local time with a morning‐afternoon asymmetry near noon. These observations can be explained by spatial and/or temporal changes in the magnetopause and cross‐tail currents, which are caused by changes in the solar wind dynamic pressure, with respect to spacecraft positions. http://www.deepdyve.com/assets/images/DeepDyve-Logo-lg.png Journal of Geophysical Research: Space Physics Wiley

Characteristics of Sudden Commencements Observed by Van Allen Probes in the Inner Magnetosphere

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Publisher
Wiley Subscription Services, Inc., A Wiley Company
Copyright
©2018. American Geophysical Union. All Rights Reserved.
ISSN
2169-9380
eISSN
2169-9402
D.O.I.
10.1002/2017JA024770
Publisher site
See Article on Publisher Site

Abstract

We have statistically studied sudden commencement (SC) by using the data acquired from Van Allen Probes (VAP) in the inner magnetosphere (L = 3.0–6.5) and GOES spacecraft at geosynchronous orbit (L =∼ 6.7) from October 2012 to September 2017. During the time period, we identified 85 SCs in the inner magnetosphere and 90 SCs at geosynchronous orbit. Statistical results of the SC events reveal the following characteristics. (1) There is strong seasonal dependence of the geosynchronous SC amplitude in the radial BV component at all local times. However, BV shows weak seasonal variation on the dayside in the inner magnetosphere. (2) The local time dependence of the SC amplitude in the compressional BH component at geosynchronous orbit is similar to that in the inner magnetosphere. (3) In a nightside region of L = 5.0–6.5, ∼19% of BH events are negative, while ∼58% of BH events are negative at geosynchronous orbit. (4) The amplitude of the SC‐associated Ey perturbations varies systematically with local time with a morning‐afternoon asymmetry near noon. These observations can be explained by spatial and/or temporal changes in the magnetopause and cross‐tail currents, which are caused by changes in the solar wind dynamic pressure, with respect to spacecraft positions.

Journal

Journal of Geophysical Research: Space PhysicsWiley

Published: Jan 1, 2018

References

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