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Oxygen torus and its coincidence with EMIC wave in the deep inner magnetosphere: Van Allen Probe B and Arase observations.

Authors :
Nosé, M.
Matsuoka, A.
Kumamoto, A.
Kasahara, Y.
Teramoto, M.
Kurita, S.
Goldstein, J.
Kistler, L. M.
Singh, S.
Gololobov, A.
Shiokawa, K.
Imajo, S.
Oimatsu, S.
Yamamoto, K.
Obana, Y.
Shoji, M.
Tsuchiya, F.
Shinohara, I.
Miyoshi, Y.
Kurth, W. S.
Source :
Earth, Planets & Space; 8/3/2020, Vol. 72 Issue 1, p1-17, 17p
Publication Year :
2020

Abstract

We investigate the longitudinal structure of the oxygen torus in the inner magnetosphere for a specific event found on 12 September 2017, using simultaneous observations from the Van Allen Probe B and Arase satellites. It is found that Probe B observed a clear enhancement in the average plasma mass (M) up to 3–4 amu at L = 3.3–3.6 and magnetic local time (MLT) = 9.0 h. In the afternoon sector at MLT ~ 16.0 h, both Probe B and Arase found no clear enhancements in M. This result suggests that the oxygen torus does not extend over all MLT but is skewed toward the dawn. Since a similar result has been reported for another event of the oxygen torus in a previous study, a crescent-shaped torus or a pinched torus centered around dawn may be a general feature of the O<superscript>+</superscript> density enhancement in the inner magnetosphere. We newly find that an electromagnetic ion cyclotron (EMIC) wave in the H<superscript>+</superscript> band appeared coincidently with the oxygen torus. From the lower cutoff frequency of the EMIC wave, the ion composition of the oxygen torus is estimated to be 80.6% H<superscript>+</superscript>, 3.4% He<superscript>+</superscript>, and 16.0% O<superscript>+</superscript>. According to the linearized dispersion relation for EMIC waves, both He<superscript>+</superscript> and O<superscript>+</superscript> ions inhibit EMIC wave growth and the stabilizing effect is stronger for He<superscript>+</superscript> than O<superscript>+</superscript>. Therefore, when the H<superscript>+</superscript> fraction or M is constant, the denser O<superscript>+</superscript> ions are naturally accompanied by the more tenuous He<superscript>+</superscript> ions, resulting in a weaker stabilizing effect (i.e., larger growth rate). From the Probe B observations, we find that the growth rate becomes larger in the oxygen torus than in the adjacent regions in the plasma trough and the plasmasphere. [ABSTRACT FROM AUTHOR]

Details

Language :
English
ISSN :
13438832
Volume :
72
Issue :
1
Database :
Complementary Index
Journal :
Earth, Planets & Space
Publication Type :
Academic Journal
Accession number :
144920908
Full Text :
https://doi.org/10.1186/s40623-020-01235-w