Our Quantitative Understanding of the Coronal Expansion

作者: Thomas E. Holzer

DOI: 10.1029/SP007P0366

关键词:

摘要:

参考文章(62)
G. Alazraki, P. Couturier, SOLAR-WIND ACCELERATION CAUSED BY THE GRADIENT OF ALFVEN-WAVE PRESSURE. Astron. Astrophys. 13: No. 3, 380-9(Aug 1971).. ,vol. 13, pp. 380- ,(1971)
F. Q. Orrall, R. A. Kopp, Temperature and density structure of the corona and inner solar wind Astronomy and Astrophysics. ,vol. 53, pp. 363- 375 ,(1976)
R. G. EDWARDS, Problems of artificial fertilization. Nature. ,vol. 233, pp. 23- 25 ,(1971) , 10.1038/233023A0
Aaron Barnes, Theoretical Studies of the Large-Scale Behavior of the Solar Wind Advances in Electronics and Electron Physics. ,vol. 36, pp. 1- 56 ,(1975) , 10.1016/S0065-2539(08)61117-8
Michael D. Montgomery, Solar Wind Observations Throughout the Solar System Physics of Solar Planetary Environments. ,vol. 1, pp. 304- 318 ,(2013) , 10.1029/SP007P0304
J.T. Gosling, Transient Phenomena in the Solar Atmosphere and Solar Wind pspe. ,vol. 1, pp. 286- 303 ,(1976) , 10.1029/SP007P0286
J. W. Belcher, ALFVÉNIC Wave Pressures and the Solar Wind The Astrophysical Journal. ,vol. 168, pp. 509- ,(1971) , 10.1086/151105
A. S. Krieger, A. F. Timothy, E. C. Roelof, A coronal hole and its identification as the source of a high velocity solar wind stream Solar Physics. ,vol. 29, pp. 505- 525 ,(1973) , 10.1007/BF00150828