JpGU-AGU Joint Meeting 2017

講演情報

[EE] 口頭発表

セッション記号 P (宇宙惑星科学) » P-EM 太陽地球系科学・宇宙電磁気学・宇宙環境

[P-EM16] [EE] Physics of Inner Magnetosphere Coupling

2017年5月23日(火) 15:30 〜 17:00 A02 (東京ベイ幕張ホール)

コンビーナ:Danny Summers(Memorial University of Newfoundland)、Jichun Zhang(University of New Hampshire Main Campus)、海老原 祐輔(京都大学生存圏研究所)、桂華 邦裕(東京大学大学院理学系研究科地球惑星科学専攻)、Aleksandr Y Ukhorskiy(Johns Hopkins University Applied Physics Laboratory)、Dae-Young Lee(Chungbuk Natl Univ)、Yiqun Yu(Beihang University)、三好 由純(名古屋大学宇宙地球環境研究所)、座長:Ukhorskiy Aleksandr(Johns Hopkins University Applied Physics Laboratory)

16:00 〜 16:15

[PEM16-15] Nature's Grand Experiment: Linkage Between Magnetospheric Convection, Substorms, and the Radiation Belts

*Craig J Rodger1Kathy Cresswell-Moorcock1Mark A. Clilverd2 (1.Department of Physics, University of Otago, Dunedin 9016, New Zealand、2.British Antarctic Survey (NERC), Madingley Road, Cambridge, CB3 0ET, United Kingdom)

キーワード:outer radiation belt, electron acceleration, coupling processes, whistler mode chorus

The solar minimum of 2007-2010 was unusually deep and long-lived. In the later stages of this period the electron fluxes in the radiation belts dropped to extremely low levels. The flux of relativistic electrons (>1 MeV) was significantly diminished, and at times were below instrument thresholds both for spacecraft located in geostationary orbits and also those in low-Earth orbit. This period has been described as a natural "grand experiment" allowing us to test our understanding of basic radiation belt physics and in particular the acceleration mechanisms which lead to enhancements in outer belt relativistic electron fluxes.
Here we test the hypothesis [1] that processes driven by magnetospheric convection initiate repetitive substorm onsets, which in turn triggers enhancement in whistler mode chorus that accelerates radiation belt electrons to relativistic energies. Conversely, individual substorms would not be associated with radiation belt acceleration. Contrasting observations from multiple satellites of energetic and relativistic electrons with substorm event lists, as well as chorus measurements, shows that the data are consistent with the hypothesis.
We show that repetitive substorms are associated with enhancements in the flux of energetic and relativistic electrons and enhanced whistler mode wave intensities. Our finding is consistent with the recent RBSP case studies [2], which suggested that substorms were the trigger for chorus which lead to acceleration of radiation belt electrons to relativistic energies. However, in our study we see a two stage chorus wave power enhancement, the first starts slightly before the repetitive substorm epoch onset, suggesting that magnetospheric convection leading the chorus activity may be the trigger. This conclusion requires some care, as the second and strongest enhancement in chorus is very slightly after the onset, complicating the picture.
During the 2009/2010 period the only relativistic electron flux enhancements that occurred were preceded by repeated substorm onsets, consistent with enhanced magnetospheric convection and repetitive substorms as a trigger for outer radiation belt electron acceleration. This work has been recently published in JGR [3].

References
Lyons, L. R., D.-Y. Lee, R. M. Thorne, R. B. Horne, and A. J. Smith, J. Geophys. Res., 110, A11202, doi:10.1029/2005JA011254 (2005)
Jaynes, A. N., et al., J. Geophys. Res. Space Physics, 120, 7240–7254, doi:10.1002/2015JA021234 (2015).
Rodger, C. J., K. Cresswell-Moorcock, and M. A. Clilverd, J. Geophys. Res. Space Physics, 121, 171–189, doi:10.1002/2015JA021537 (2016).