Consequences of a saturated convection electric field on the ring current

被引:26
作者
Liemohn, MW [1 ]
Kozyra, JU
Hairston, MR
Weimer, DR
Lu, G
Ridley, AJ
Zurbuchen, TH
Skoug, RM
机构
[1] Univ Michigan, Space Phys Res Lab, Ann Arbor, MI 48109 USA
[2] Univ Texas, Ctr Space Sci, Richardson, TX 75083 USA
[3] Mission Res Corp, Nashua, NH 03062 USA
[4] Natl Ctr Atmospher Res, High Altitude Observ, Boulder, CO 80307 USA
[5] Los Alamos Natl Lab, Los Alamos, NM 87545 USA
关键词
D O I
10.1029/2001GL014270
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
[1] Results from kinetic simulations of hot ion transport in the inner magnetosphere are used to show that the ring current energy content must have a nonlinear (asymptotic) coupling relationship to extreme solar wind conditions due to saturation of the near-Earth convection electric field E-y,E-conv (defined as a function of cross polar cap potential DeltaPhi(PC)). This study examines the Bastille Day magnetic storm (July 14-17, 2000), where the z-component of the interplanetary magnetic field reached -58 nT and the solar wind speed exceeded 1100 km s(-1). A large discrepancy in the modeled DeltaPhi(PC) confirms a nonlinear response of the high-latitude potential during this event. It is found that this nonlinearity of E-y,E-conv is necessary to obtain reasonable agreement between the simulation results and the observed geoeffectiveness (Dst) of the storm.
引用
收藏
页码:62 / 1
页数:4
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