Insights into Cosmic-Ray Acceleration from the Study of Anomalous Cosmic Rays

被引:0
作者
J.R. Jokipii
机构
[1] The University of Arizona,
来源
Space Science Reviews | 1998年 / 86卷
关键词
Solar Wind; Current Sheet; Termination Shock; Sunspot Minimum; Diffusive Shock Acceleration;
D O I
暂无
中图分类号
学科分类号
摘要
Cosmic rays from many sources and in many locations exhibit similar, inverse-power-law energy spectra, which suggests a common origin for most cosmic rays. Diffusive shock acceleration appears at present to be this common accelerator. Hence, anomalous cosmic rays, thought to be accelerated at the solar-wind termination shock, provide a relatively accessible laboratory for the study of the mechanism of cosmic-ray acceleration. Observations showing a transition from singly-charged anomalous cosmic-ray oxygen to multiply-charged at an energy of some 250 MeV support the picture of acceleration at the quasi-perpendicular termination shock. Such acceleration may be important in other sources, as well. The basic physics of this acceleration process is discussed in some detail.
引用
收藏
页码:161 / 178
页数:17
相关论文
共 79 条
[1]  
Axford W. I.(1965)The Modulation of Galactic Cosmic Rays in the Interplanetary Medium Planetary Space. Sci. 13 115-undefined
[2]  
Chalov S. V.(1997)Spectra of Energized Pick-Up Ions Upstream of the Two-Dimensional Heliospheric Termination Shock. II. Acceleration by Alfvénic Fluctuations Astron. Astrophys. 320 659-undefined
[3]  
Fahr H. J.(1995)Observations of Anomalous Cosmic-Ray Hydrogen from the Voyager Spacecraft Astrophys. J. 446 L105-undefined
[4]  
Ismodenov V. T.(1987)Energy Spectra of Anomalous Cosmic-Ray Oxygen During 1977–1987 Proc. 20th Int. Cosmic Ray Conf., Moscow 3 421-undefined
[5]  
Christian E. R.(1987)Latitudinal and Radial Gradients of Anomalous and Galactic Cosmic Rays in the Outer Heliosphere Geophys. Res. Letters 14 174-undefined
[6]  
Cummings A. C.(1988)Computer Modeling of Test Particle Acceleration at Oblique Shocks Space Sci. Rev. 48 195-undefined
[7]  
Stone E. C.(1983)An Introduction to the Theory of Diffusive Shock Acceleration of Energetic Particles in Tenuous Plasmas Rept. Prog. Phys. 46 973-undefined
[8]  
Cummings A. C.(1974)An Interpretation of the Observed Oxygen and Nitrogen Enhancements in Low-Energy Cosmic Rays Astrophys. J. 190 L35-undefined
[9]  
Stone E. C.(1979)Time-Dependent Acceleration of Solar Wind Plasma to MeV Energies at Co-rotating Interplanetary Shocks Proc. 16th Int. Cosmic Ray Conf., Kyoto 5 328-undefined
[10]  
Cummings A. C.(1996)Perpendicular Transport in Shock Acceleration J. Geophys. Res. 101 11 095-undefined