PARTICLE ENERGIZATION DURING SOLAR MAXIMUM: DIFFUSIVE SHOCK ACCELERATION AT MULTIPLE SHOCKS

被引:4
|
作者
Parker, L. Neergaard [1 ,2 ]
Zank, G. P. [1 ,3 ]
机构
[1] Univ Alabama, CSPAR, Huntsville, AL 35899 USA
[2] Univ Alabama, Dept Phys, Huntsville, AL 35899 USA
[3] Univ Alabama, Dept Space Sci, Huntsville, AL 35899 USA
来源
ASTROPHYSICAL JOURNAL | 2014年 / 790卷 / 02期
关键词
acceleration of particles; plasmas; shock waves; EJECTION-DRIVEN SHOCKS; CORONAL MASS EJECTIONS; COSMIC-RAYS; CHARGED-PARTICLES; DEPENDENCE; TRANSPORT; ENSEMBLE; EVENTS; ENERGY;
D O I
10.1088/0004-637X/790/2/153
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present a model for the acceleration of particles at multiple shocks using an approach related to box models. A distribution of particles is diffusively accelerated inside the box while simultaneously experiencing decompression through adiabatic expansion and losses from the convection and diffusion of particles out of the box by either the method used in Melrose & Pope and Pope & Melrose or by the approach introduced in Zank et al. where we solve the transport equation by a method analogous to operator splitting. The second method incorporates the additional loss terms of convection and diffusion and allows for the use of a variable time between shocks. We use a maximum injection energy (E-max) appropriate for quasi-parallel and quasi-perpendicular shocks. We provide a preliminary application of the diffusive acceleration of particles by multiple shocks with frequencies appropriate for solar maximum.
引用
收藏
页数:10
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