Solar proton magnetosphere penetration

Received April 20, ; in final form, September 2, Parasitic resonance with VLF emissions, generated by. Figure 1 shows the lati-. The BP shift during magnetic storms was studied in. It is shown that observed Different levels of the IE.

From Wikipedia, the free encyclopedia. Recommended articles Citing articles 0. Main goal of presented work was to find the possibility to estimate the extreme the most low latitude solar particle penetration boundary location during the strong magnetic storms using geomagnetic indices using CORONAS-F and "Universitetskiy-Tatiana" satellites measurements. The g ood agreement of experimental measured on.

Unable to display preview. The present analysis suggests either that a regular pulsing by high-speed solar wind streams makes the magnetosphere an efficient relativistic electron accelerator or else that the Jovian magnetosphere is a recurrent source of a significant electron population in the outer terrestrial magnetosphere. The region around an astronomical object in which charged particles are affected by its magnetic field. Download full-text PDF.

Peak intensities of the SEP fluxes inside and outside the magnetosphere were compared for each event. Ryumin, and Y u. The correlation coefficient for protons with energies from 1 to 5 MeV is higher in the nightside sector as compared to the dayside sector. Data from the Russian space experiments. The collimator selects an observational cone of. W e should note that the PB motion is not smooth.