动力Alfven波加热日冕和加速太阳风的耗散长度
摘要
动力Alfven波高频分支在冕洞中沿磁场方向传播时, 其Landau阻尼可以给出可观的加热效果. 从理论上计算出波能通量的耗散形式和耗散长度, 与经验模型给出的耗散长度一致, 从而给出经验模型中耗散长度的理论根据.
出处
《中国科学（A辑）》
CSCD
2000年第z1期51-53,共3页
Science in China(Series A)
参考文献8
-
11，Axford W I, Mckenzie J F. The origin of high speed solar wind streams. Solar Wind Seven, COSPAR Colloquia Series, 1992, 3: 1~ 5
-
22，Hollweg J V. Status of solar wind modeling from the transition region outward. Solar Wind Seven, COSPAR Colloquia Series, 1992, 3: 53~ 64
-
33，Withbore G L. The temperature, structure, mass and energy flow in the corona and inner solar wind. Astrophys J, 1988, 325(1): 442~ 467
-
44，Lopp R A, Holzer T E. Dynamics of coronal hole regions. Solar Physics, 1976, 49(1): 43~ 56
-
55，Bavassano B, Dobrowolny M, Mariani F, et al. Radial evolution of power spectra of interplanetary Alfvenic turbulence. J Geophy Res, 1982, 87(5): 3 617~ 3 622
-
66，Dobrowolny M, Mangeney A, Veltri P. Properties of magnetohydrodynamic turbulence in the solar wind. Astron and Astrophys, 1980, 83(1-2): 26~ 32
-
79，Leamon R J, Smith C W, Ness N F. Dissipation range dynamics: kinetic Alfven wave and the importance of . J Geophy Res, 1999, 104(10): 22 331~ 22 344
-
810，Kinney R M, Macwilliams J C. Turbulence cascade in anisotropic magnetohydrodynamics. Phys Rev, 1998, E57(6): 7 111~ 7 121
-
1日全食与日冕[J].科学,2009(5).
-
2李敬群,魏奉思.1996年12月非对称日冕多冕旒结构数值模拟[J].中国科学（A辑）,2000,30(z1):43-46.
-
3王荣伟.太阳风暴[J].大科技（科学之谜）（A）,2004(10).
-
4余恒.被遗忘的元素用字——氜、■、■[J].中国科技术语,2013,15(6):53-54.
-
5延三成.宏观和微观运动系统论[J].职大学报,1997(2):73-76. 被引量：2
-
6Ren-Xin Xu.A solution to the puzzling symbiotic X-ray system 4U 1700+24[J].Research in Astronomy and Astrophysics,2014,14(6):617-624.
-
7谢天.宇宙信息[J].天文爱好者,2009(10):14-17.
-
8汪景琇.关于扩展的太阳活动周期的概念[J].自然杂志,1991,14(7):489-492.
