Some features of the solar microwave emission and their connection with geomagnetic activity
暂无分享,去创建一个
[1] J. Wilcox. The interplanetary magnetic field. Solar origin and terrestrial effects , 1968 .
[2] T. Velusamy,et al. Lunar Occupation of a Solar Active Region at 4 cm Wavelength , 1968, Nature.
[3] G. Newkirk. Structure of the Solar Corona , 1967 .
[4] T. Tsubaki. A New Model of Coronal Condensation , 1967 .
[5] J. Roosen,et al. The distribution of the 9 cm radio emission over the solar disk during the sunspot minimum , 1967 .
[6] Donald E. Billings,et al. A Guide to the Solar Corona , 2013 .
[7] R. P. Basler. The nature of solar M-regions , 1966 .
[8] G. Pneuman. INTERACTION OF THE SOLAR WIND WITH A LARGE-SCALE SOLAR MAGNETIC FIELD , 1966 .
[9] R. Howard,et al. A Note on the Identification of "m" Regions , 1966 .
[10] H. J. Hagger,et al. Solar Radio Astronomy , 1965 .
[11] J. Wilcox,et al. Extension of the photospheric magnetic field into interplanetary space. , 1965 .
[12] D. E. Billings,et al. Polarimetric Observations of a Coronal Condensation. , 1964 .
[13] U. R. Rao,et al. The solar wind velocity and its correlation with cosmic-ray variations and with solar and geomagnetic activity , 1963 .
[14] R. E. Marshak,et al. Interplanetary Dynamical Processes , 1963 .
[15] T. Kakinuma,et al. A MODEL FOR THE SOURCES OF THE SLOWLY VARYING COMPONENT OF MICROWAVE SOLAR RADIATION , 1962 .
[16] G. A. Harvey,et al. Selected High-Resolution Strip Scans of the 10.7-CM Sun. , 1962 .
[17] T. Saemundsson. Statistics of Geomagnetic Storms and Solar Activity , 1961 .
[18] G. Newkirk. The Solar Corona in Active Regions and the Thermal Origin of the Slowly Varying Component of Solar Radio Radiation. , 1961 .
[19] R. Bracewell. Paris Symposium on Radio Astronomy , 1959 .
[20] H. Babcock,et al. The Sun's Magnetic Field, 1952-1954. , 1955 .
[21] J. Alden Wier,et al. The Sun: , 1939, Nature.