Modulation of galactic cosmic ray intensities by coronal mass ejections into interplanetary spaceстатья
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Дата последнего поиска статьи во внешних источниках: 5 июня 2017 г.
Аннотация:The data on the measurements of the intensities of galactic cosmic rays with proton energies greater than 30 MeV are compared with the data on the solar wind and interplanetary magnetic field measured on board the Vega-1 and Vega-2 automated interplanetary stations. Modulation structures with characteristic shapes and durations, namely quasi-symmetric ("bays") short-term Forbush decreases of intensity, are revealed. It is shown that these Forbush decreases were recorded due to the stations flying through coronal mass-ejection regions.