Ray tracing of penetrating chorus and its implications for the radiation belts

被引:68
作者
Bortnik, J. [1 ]
Thorne, R. M.
Meredith, N. P.
Santolik, O.
机构
[1] Univ Calif Los Angeles, Dept Atmospher & Ocean Sci, Los Angeles, CA 90095 USA
[2] British Antarctic Survey, NERC, Cambridge CB3 0ET, England
[3] Charles Univ Prague, Fac Math & Phys, Prague, Czech Republic
[4] IAP ASCR, Prague, Czech Republic
基金
英国自然环境研究理事会;
关键词
D O I
10.1029/2007GL030040
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
Using ray tracing and suprathermal electron distributions from CRRES, the final propagation latitudes of typical chorus rays are calculated as a function of L, MLT, AE, and initial wave normal angle. Rays initiated within a certain range of wave normals psi(P) similar to -0.8 psi(G) to -0.6 psi(G) ( where psi(G) is the Gendrin angle) propagate to very high latitudes, largely avoiding Landau damping whilst remaining roughly field-aligned for large portions of their propagation paths. The relative wave power of such penetrating chorus may increase above its initial value due to the low damping rates and magnetic field line convergence. By considering 4 representative rays with f = 0.3f(ce), and calculating the resonant energies at the edge of the loss-cone, it is shown that penetrating chorus readily interacts with electrons in the > 1 MeV energy range, and may thus contribute to the previously reported relativistic electron microbursts.
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页数:5
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