Abstract
During the period from 25 Feb. to 5 March, 1969 the Venus-5 and Venus-6 space probes detected an increase in solar cosmic ray protons with E p > 1 MeV and electrons with E e > 0.05 MeV. The increase had a complex form and was due to a series of solar flares occurring in a single active region. The main flares occurred on 24 and 27 Feb. 1969. A scheme for the development of a disturbance in the interplanetary medium caused by the above mentioned flares is considered on the basis of the analysis of the form of increase for various proton energies, anisotropy of protons with E p = 1 ÷ 4 MeV, and the increase in electrons with E e > 0.05 MeV together with solar and geophysical events.
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Vernov, S.N., Kontor, N.N., Lyubimov, G.P., Pereslegina, N.V., Chuchkov, E.A. (1970). Solar Cosmic Ray Increase on 25 February – 5 March, 1969 According to Measurements from Venus-5 and Venus-6 Space Probes. In: Manno, V., Page, D.E. (eds) Intercorrelated Satellite Observations Related to Solar Events. Astrophysics and Space Science Library, vol 19. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-3278-0_34
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