Homogeneity of interplanetary space according to charged particle observations

K. Kecskemety, E. I. Daibog, Yu I. Logachev

Research output: Paper

Abstract

27-day variations of the fluxes of 0.25-10 MeV electrons, present in all the last four minima are studied on the basis of SOHO/COSTEP and IMP-8/CRNC data observed during the minimum of solar activity in 1996. Independent of the origin of particles, this means that during those periods some stable active structure existed on the Sun, providing quasi-stability of the interplanetary medium which manifested in the 27-day recurrence of electron fluxes.

Original languageEnglish
Pages184-186
Number of pages3
DOIs
Publication statusPublished - jan. 1 2011
Event32nd International Cosmic Ray Conference, ICRC 2011 - Beijing, China
Duration: aug. 11 2011aug. 18 2011

Other

Other32nd International Cosmic Ray Conference, ICRC 2011
CountryChina
CityBeijing
Period8/11/118/18/11

ASJC Scopus subject areas

  • Nuclear and High Energy Physics

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    Kecskemety, K., Daibog, E. I., & Logachev, Y. I. (2011). Homogeneity of interplanetary space according to charged particle observations. 184-186. Paper presented at 32nd International Cosmic Ray Conference, ICRC 2011, Beijing, China. https://doi.org/10.7529/ICRC2011/V02/0412