Numerical solution of the time-dependent kinetic equation for anisotropic pitch-angle scattering

被引:13
作者
Lu, JY [1 ]
Zank, GP
Webb, GM
机构
[1] Univ Delaware, Bartol Res Inst, Newark, DE 19716 USA
[2] Univ Arizona, Lunar & Planetary Lab, Tucson, AZ 85721 USA
[3] Chinese Acad Sci, Ctr Space Sci & Appl Res, Beijing, Peoples R China
关键词
acceleration of particles; cosmic rays; methods : numerical; plasmas;
D O I
10.1086/319722
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
A new powerful numerical method is developed for solving the time-dependent kinetic equation describing the anisotropic pitch-angle scattering of charged particles. The model includes the effects of adiabatic focusing in a radial magnetic field, adiabatic deceleration, anisotropic pitch-angle scattering, and convection in a magnetized plasma and significantly generalizes a model introduced by in Kota 1994. The pitch-angle scattering is assumed to scatter slowly through 90 degrees. By applying Legendre polynomial expansions to the particle transport equation, an infinite series of first-order differential equations for the harmonics of the distribution function is obtained. By means of a characteristic method (together with operator splitting), the solution of distributions at certain harmonics is computed. Solutions exhibiting coherent pulses are obtained, and these are identical to the exact analytic results obtained by Kota. However, the approach presented here allows for arbitrarily anisotropic initial data to be prescribed, and it can also be used to study the dependence of particle distribution on pitch angle. It is shown that the presence of adiabatic focusing results in highly asymmetric particle propagation in opposite directions with typically more particles in the sunward hemisphere than in the antisunward hemisphere, although two oppositely propagating initial beams are introduced symmetrically. An abrupt transition can be found between hemispheres, and the distribution within each hemisphere is quasi-isotropic. The model and approach discussed here lend themselves to the study of the propagation and transport of charged particles and pickup ions.
引用
收藏
页码:34 / 51
页数:18
相关论文
共 62 条
[1]  
[Anonymous], 1980, Plasma astrophysics. Nonthermal processes in diffuse magnetized plasmas-Vol.1: The emission
[2]   ANISOTROPIC DIFFUSION OF SOLAR COSMIC RAYS [J].
AXFORD, WI .
PLANETARY AND SPACE SCIENCE, 1965, 13 (12) :1301-&
[3]   PITCH ANGLE DISTRIBUTIONS OF SOLAR ENERGETIC PARTICLES AND THE LOCAL SCATTERING PROPERTIES OF THE INTERPLANETARY MEDIUM [J].
BEECK, J ;
WIBBERENZ, G .
ASTROPHYSICAL JOURNAL, 1986, 311 (01) :437-450
[4]  
BIBER JW, 1977, THESIS U MARYLAND
[5]   FOCUSING ANISOTROPY OF SOLAR COSMIC-RAYS [J].
BIEBER, JW ;
EVENSON, PA ;
POMERANTZ, MA .
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 1986, 91 (A8) :8713-8724
[6]   COSMIC-RAY STREAMING IN THE BORN APPROXIMATION [J].
BIEBER, JW ;
BURGER, RA .
ASTROPHYSICAL JOURNAL, 1990, 348 (02) :597-607
[7]   Dominant two-dimensional solar wind turbulence with implications for cosmic ray transport [J].
Bieber, JW ;
Wanner, W ;
Matthaeus, WH .
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 1996, 101 (A2) :2511-2522
[8]   PLANAR NUMERICAL COSMOLOGY .2. THE DIFFERENCE-EQUATIONS AND NUMERICAL TESTS [J].
CENTRELLA, J ;
WILSON, JR .
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 1984, 54 (02) :229-249
[9]   Signatures of the interplanetary helium cone reflected by pick-up ions [J].
Chalov, SV ;
Fahr, HJ .
SOLAR PHYSICS, 1999, 187 (01) :123-144
[10]   ION-CYCLOTRON HEATING AND ACCELERATION OF SOLAR-WIND MINOR IONS [J].
DUSENBERY, PB ;
HOLLWEG, JV .
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 1981, 86 (NA1) :153-164