Dependence of the Spectrum of Shock-Accelerated Ions on the Dynamics at the Shock Crossing

被引:6
作者
Gedalin, M. [1 ]
Drge, W. [2 ]
Kartavykh, Y. Y. [2 ]
机构
[1] Ben Gurion Univ Negev, Dept Phys, IL-8410501 Beer Sheva, Israel
[2] Univ Wurzburg, Inst Theoret Phys & Astrophys, D-97074 Wurzburg, Germany
基金
以色列科学基金会;
关键词
PARTICLE-ACCELERATION; ASTROPHYSICAL SHOCKS; ENERGETIC PARTICLES; CHARGED-PARTICLES; MAGNETIC-FIELD; FAST MODE; FRONT; ANGLE; DRIFT;
D O I
10.1103/PhysRevLett.117.275101
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
Diffusive shock acceleration (DSA) of ions occurs due to pitch-angle diffusion in the upstream and downstream regions of the shock and multiple crossing of the shock by these ions. The classical DSA theory implies continuity of the distribution at the shock transition and predicts a universal spectrum of accelerated particles, depending only on the ratio of the upstream and downstream fluid speeds. However, the ion dynamics at the shock front occurs within a collision-free region and is gyrophase dependent. The ions fluxes have to be continuous at the shock front. The matching conditions for the gyrophase-averaged distribution functions at the shock transition are formulated in terms of the transition and reflection probabilities. These probabilities depend on the shock angle and the magnetic compression as does the power spectrum of accelerated ions. Their spectral index is expressed in terms of the reflectivity. The spectrum is typically harder than the spectrum predicted by the classical DSA theory.
引用
收藏
页数:5
相关论文
共 23 条
[1]  
Axford W. I., 1978, INT COSM RAY C BULG, P13
[2]   ACCELERATION OF COSMIC-RAYS IN SHOCK FRONTS .1. [J].
BELL, AR .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1978, 182 (01) :147-156
[3]   PARTICLE-ACCELERATION AT ASTROPHYSICAL SHOCKS - A THEORY OF COSMIC-RAY ORIGIN [J].
BLANDFORD, R ;
EICHLER, D .
PHYSICS REPORTS-REVIEW SECTION OF PHYSICS LETTERS, 1987, 154 (01) :1-75
[4]   PARTICLE ACCELERATION BY ASTROPHYSICAL SHOCKS [J].
BLANDFORD, RD ;
OSTRIKER, JP .
ASTROPHYSICAL JOURNAL, 1978, 221 (01) :L29-L32
[6]   DYNAMICS OF HIGH ENERGY IONS AT A STRUCTURED COLLISIONLESS SHOCK FRONT [J].
Gedalin, M. ;
Droege, W. ;
Kartavykh, Y. Y. .
ASTROPHYSICAL JOURNAL, 2016, 825 (02)
[7]   SCATTTERING OF HIGH-ENERGY PARTICLES AT A COLLISIONLESS SHOCK FRONT: DEPENDENCE ON THE SHOCK ANGLE [J].
Gedalin, M. ;
Droege, W. ;
Kartavykh, Y. Y. .
ASTROPHYSICAL JOURNAL, 2015, 807 (02)
[8]   Ion dynamics in quasi-perpendicular collisionless interplanetary shocks: a case study [J].
Gedalin, Michael ;
Droege, Wolfgang .
FRONTIERS IN PHYSICS, 2013, 1
[9]   Cosmic-Ray Transport and Interaction with Shocks [J].
Giacalone, Joe .
SPACE SCIENCE REVIEWS, 2013, 176 (1-4) :73-88
[10]   COSMIC-RAY PROPAGATION .1. CHARGED PARTICLES IN A RANDOM MAGNETIC FIELD [J].
JOKIPII, JR .
ASTROPHYSICAL JOURNAL, 1966, 146 (02) :480-&