THE EFFECT OF THE SHOCK OF 15/43 UT MARCH 23, 1991 ON 50 KEV TO 5 MEV IONS AT ULYSSES

被引:4
作者
ARMSTRONG, TP
CHOO, TH
ROELOF, EC
SIMNETT, GM
SARRIS, ET
机构
[1] DEMOCRITOS UNIV,ATHENS,GREECE
[2] JOHNS HOPKINS UNIV,APPL PHYS LAB,LAUREL,MD 20707
[3] UNIV BIRMINGHAM,SCH PHYS & SPACE RES,BIRMINGHAM B15 2TT,W MIDLANDS,ENGLAND
关键词
D O I
10.1029/92GL00777
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
The intensities, angular distributions, and energy spectra of 50 keV to 5 MeV ions are examined in the several hour time interval when an interplanetary shock passed the Ulysses spacecraft. The increase in intensity, evolution of Pitch angle distribution from upstream flow away from the shock to a post-shock "pancake" distribution, the earlier arrival of more energetic particles, and the presence of non-gyrotropic effects at the time of shock passage all can be understood in terms of kinematical behavior of the particles crossing the shock.
引用
收藏
页码:1247 / 1250
页数:4
相关论文
共 8 条
[1]  
Armstrong T. P., 1977, Study of Travelling Interplanetary Phenomena 1977. Astrophysics and Space Science Library, vol.71, P367
[2]  
Armstrong T.P., 1985, GMS, V35, P271, DOI [10.1029/GM035p0271, DOI 10.1029/GM035P0271]
[3]  
BALOGH A, 1991, 1991 AGU FALL M PROG, P379
[4]  
DECKER RB, 1988, SPACE SCI REV, V48, P195, DOI 10.1007/BF00226009
[5]  
GIACALONE J, 1991, THESIS U KANSAS LAWR
[6]   ACCELERATION OF 0.29-MEV TO 0.5-MEV PROTONS BY INTERPLANETARY SHOCKS [J].
KESSEL, RL .
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 1988, 93 (A6) :5525-5540
[7]  
LANZEROTTI LJ, 1992, IN PRESS ASTRON ASTR
[8]  
ROELOF EC, 1992, IN PRESS GEOPHYS RES