The Effects of Field Line Curvature (FLC) Scattering on Ring Current Dynamics and Isotropic Boundary

被引:26
|
作者
Yu, Yiqun [1 ,2 ]
Tian, Xingbin [1 ]
Jordanova, Vania K. [3 ]
机构
[1] Beihang Univ, Sch Space & Environm, Beijing, Peoples R China
[2] Minist Ind & Informat Technol, Key Lab Space Environm Monitoring & Informat Proc, Beijing, Peoples R China
[3] Los Alamos Natl Lab, Space Sci & Applicat, Los Alamos, NM USA
关键词
ENERGETIC PROTON PRECIPITATION; PITCH-ANGLE SCATTERING; CURRENT SHEET; INNER MAGNETOSPHERE; RAM-SCB; MODEL; PLASMA; CONDUCTANCES; ENVIRONMENT; CONFIGURATION;
D O I
10.1029/2020JA027830
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In the ring current dynamics, various loss mechanisms contribute to the ring current decay, including losses to the upper atmosphere through particle precipitation. This study implements the field line curvature (FLC) scattering mechanism in a kinetic ring current model and investigates its role in precipitating ions into the ionosphere during the 17 March 2013 storm. Simulation results indicate that (1) the FLC scattering process exerts on energetic ions on the nightside where the magnetospheric configuration is more stretching. It is more effective on heavy ions (e.g., O+\). These ion losses thereafter lead to a faster recovery of the ring current. (2) The FLC-associated ion precipitation mainly occurs in the outer region (L > 5 for protons and L > 4.5 for oxygen ions) on the nightside. The O+ precipitation takes places in a wider region than protons although its intensity is much lower. Comparisons with POES observations suggest that more proton precipitation is needed in the inner region. This is probably caused by the less stretched configuration in the simulation that prevents more precipitation. It may also imply that other loss process is required in the model such as wave-particle interactions. (3) The storm time precipitating proton flux of tens of keV due to the FLC scattering sometimes becomes comparable to that of electrons on the nightside, although electrons usually dominate the ionospheric energy deposition from the midnight eastward toward the dayside. (4) The FLC scattering process seems to be capable of explaining the formation of isotropic boundary in the ionosphere during the investigated event.
引用
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页数:17
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