A model of solar wind and corona driven by high-frequency Alfvén waves

Chinese Astronomy and Astrophysics

Volumn 22, Issue 1, 1998, Pages 76-82

  Zhu, Xiao mei ^a   Tu, Chuan yi ^a   Hu, You qiu ^b  

^a PEKING UNIVERSITY   (China)

^b UNIVERSITY OF SCIENCE AND TECHNOLOGY OF CHINA   (China)

Author keywords

Alfv n waves; Solar corona; Solar wind

Indexed keywords

EID: 0031606356     PISSN: 02751062     EISSN: None     Source Type: Journal    
DOI: 10.1016/S0275-1062(98)00011-3     Document Type: Article

References (6)

1. [1] Marsch E., Adv. Space Res., 1994, 14(4), 103
2. [2] Tu C. Y., Marsch E., MHD Structures, Waves and Turbulence in the Solar Wind: observations and Theories, Dordrecht:Kluwer, 1995, 1
3. [3] Axford .. In: E. Marsch and R. Schwerin, eds., Solar Wind Seven, Oxford: Pergamon, 1992, 1
4. [4] Tu C. Y., Marsch E., Solar Phys., 1997
5. [5] Habbal S. R., Hu Y. Q., Esser R., J. Geophys. Res., 1994, 99(A5), 8465
6. [6] Habbal S. R., Esser R., Geophys. Res. Lett., 1995, 22(13), 1465