论文信息 - The prediction of coronal and interplanetary magnetic fields - 字舞流文

The prediction of coronal and interplanetary magnetic fields

Solar coronal structure and interplanetary magnetic fields prediction based on magnetic models, testing accuracy at solar eclipses

[1] G. Newkirk,et al. Magnetic fields and the structure of the solar corona , 1970 .

[2] W. Rusch,et al. The quasi-stationary coronal magnetic field and electron density as determined from a Faraday rotation experiment , 1970 .

[3] M. Waldmeier. Prediction and Observation of the Coronal Structure for the Solar Eclipse of March 7, 1970 , 1970, Nature.

[4] K. Schatten,et al. Preliminary Comparison of Predicted and Observed Structure of the Solar Corona at the Eclipse of March 7, 1970 , 1970, Nature.

[5] J. Wilcox,et al. Comparison of the mean photospheric magnetic field and the interplanetary magnetic field , 1970 .

[6] A. Severny. Is the Sun a Magnetic Rotator? , 1969, Nature.

[7] J. Wilcox,et al. A model of interplanetary and coronal magnetic fields , 1969 .

[8] L. Davis,et al. The angular momentum of the solar wind. , 1967 .

[9] J. Wilcox,et al. On the Solar Origin of the Interplanetary Magnetic Field , 1964 .

[10] Thomas Gold,et al. Plasma and Magnetic Fields in the Solar System , 1959 .

[11] E. Parker. Dynamics of the Interplanetary Gas and Magnetic Fields , 1958 .

[12] K. Schwarzschild,et al. The Observatory , 1886 .