Lu, Li, McKenna-Lawlor, Susan, Cao, JinBin, Kudela, K. and Balaz, J. (2016) The causal sequence investigation of the ring current ion-flux increasing and the magnetotail ion injection during a major storm. Science China Earth Sciences, 59 (1). pp. 129-144. ISSN 1674-7313
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Abstract
Comprehensive records are available in ENA data of ring current activity recorded by the NUADU instrument
aboard TC-2 on 15 May, 2005 during a major magnetic storm (which incorporated a series of substorms). Ion fluxes at 4-min
temporal resolution derived from ENA data in the energy ranges 50–81 and 81–158 keV are compared with in situ particle
fluxes measured by the LANL-SOPA instruments aboard LANL-01, LANL-02, LANL-97, and LANL-84 (a series of
geostationary satellites that encircle the equatorial plane at ~6.6 RE). Also, magnetic fields measured simultaneously by the
magetometers aboard GOES-10 and GOES-12 (which are also geostationary satellites) are compared with the particle data. It
is demonstrated that ion fluxes in the ring current were enhanced during geomagnetic field tailward stretching in the growth
phases of substorms rather than after Earthward directed dipolarization events. This observation, which challenges the existing
concept that ring current particles are injected Earthward from the magnetotail following dipolarization events, requires further
investigation using a large number of magnetic storm events.
Item Type: | Article |
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Keywords: | Energetic neutral atoms; Ring current; Energetic particles; Energetic ions injection; |
Academic Unit: | Faculty of Science and Engineering > Experimental Physics |
Item ID: | 20564 |
Identification Number: | 10.1007/s11430-015-5121-7 |
Depositing User: | IR Editor |
Date Deposited: | 16 Sep 2025 11:50 |
Journal or Publication Title: | Science China Earth Sciences |
Publisher: | Springer |
Refereed: | Yes |
Related URLs: | |
URI: | https://mural.maynoothuniversity.ie/id/eprint/20564 |
Use Licence: | This item is available under a Creative Commons Attribution Non Commercial Share Alike Licence (CC BY-NC-SA). Details of this licence are available here |
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