Modeling of an interplanetary disturbance event tracked by the interplanetary scintillation method. Scientific Report No. 5
暂无分享,去创建一个
[1] A. Hewish,et al. A new method of forecasting geomagnetic activity and proton showers , 1987 .
[2] S. Akasofu,et al. A method for determining corotating interaction regions in the equatorial plane of the heliosphere from solar wind velocity data , 1986 .
[3] D. Simpson,et al. Seismic domains within the Gissar‐Kokshal Seismic Zone, soviet central Asia , 1986 .
[4] S. Akasofu,et al. A first generation numerical geomagnetic storm prediction scheme , 1986 .
[5] Z. Smith,et al. Calibration of the kinematic method of studying solar wind disturbances on the basis of a one-dimensional MHD solution and a simulation study of the heliosphere disturbances between 22 november and 6 december 1977 , 1985 .
[6] S. Akasofu,et al. One-dimensional kinematics of particle stream flow with application to solar wind simulation , 1985 .
[7] A. Hewish,et al. Origin of strong interplanetary shocks , 1985, Nature.
[8] A. Hewish,et al. Tracking a major interplanetary disturbance , 1983 .
[9] R. Howard,et al. Associations between coronal mass ejections and soft X-ray events , 1983 .
[10] R. Stone,et al. Type II solar radio events observed in the interplanetary medium , 1982 .
[11] K. Hakamada,et al. Simulation of three-dimensional solar wind disturbances and resulting geomagnetic storms , 1982 .
[12] P. McIntosh,et al. Disappearing solar filaments: A useful predictor of geomagnetic activity , 1981 .
[13] H. E. Taylor. Sudden commencement associated discontinuities in the interplanetary magnetic field observed by IMP 3 , 1969 .
[14] S. Akasofu,et al. ON THE THREE-DIMENSIONAL STRUCTURE OF THE SOLAR PLASMA FLOW GENERATED BY SOLAR FLARES. , 1967 .