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H. Nieuwenhuijzen F. P. Israel C. Slottje L. B. F. M. Waters J. Kleczek K. Werner M. Barylak Patricia Whitelock Ľ Kresák G. Meynet K. A. van der Hucht D. Stickland 《Space Science Reviews》1992,61(3-4):393-417
The general significance of streamers of the solar corona is discussed in the frame of our knowledge of the solar wind phenomenon and the large-scale solar magnetic structure. Thermodynamical and geometric parameters of streamers observed and measured at total solar eclipses are reviewed. Both the low part (in the form of a helmet with a cusp) and the external part (in the form of a stalk extended at many solar radii) are considered. The modelling of streamers starts with the analysis of effects produced by the solar wind flow on a magnetic structure. Facts and arguments are presented in favor of a model with a current sheet and reconnection processes going on along the axis of the streamer, especially in the non-collisional part of the radially extended streamer. Further development of the Pneuman and Kopp (1971) model is discussed, including difficulties occurring in the interpretation of a stationary solution. An empirical model satisfying observations is presented. Future researchs on streamers were discussed with emphasis on observations to be done with the space-borne coronagraphs on the SOHO spacecraft. 相似文献
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Space Science Reviews - 相似文献
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P. S. Thé L. Matveyenko J. Kleczek L. M. Gindilis G. M. Rudnitskij J. Arbocz J. Schuve J. A. Steketee W. de Graaff K. A. van der Hucht Wayne G. Roberge G. Kockarts R. H. van Gent E. Dekker T. S. van Albada D. de Hoop H. Nieuwenhuijzen Josip Kleczek J. L. van Ingen P. Hellings A. Achterberg 《Space Science Reviews》1985,41(1-2):201-213
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V. Icke K. F. Wakker A. Journet P. C. van der Kruit H. Nieuwenhuijzen R. Mewe 《Space Science Reviews》1992,62(1-2):205-212
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