Abstract
Basic conditions of observation of IMF tubular-loop structures are considered on the basis of experimental data of studying the fluxes of solar cosmic ray protons in the interplanetary medium. Lifetime of these structures, when their sources disappear on the Sun, is estimated.
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Original Russian Text © B.Ya. Shcherbovskii, E.A. Chuchkov, 2008, published in Kosmicheskie Issledovaniya, 2008, Vol. 46, No. 5, pp. 398–402.
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Shcherbovskii, B.Y., Chuchkov, E.A. Optimum conditions of observation of tubular-loop structures of the interplanetary magnetic field and estimation of their lifetime. Cosmic Res 46, 383–386 (2008). https://doi.org/10.1134/S001095250805002X
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DOI: https://doi.org/10.1134/S001095250805002X