ENERGETIC PARTICLES IN THE SOLAR WIND: PROPAGATION, ACCELERATION, AND MODULATION

25th International Cosmic Ray Conference — Volume 8, pp. 135-150 (1998) No AccessENERGETIC PARTICLES IN THE SOLAR WIND: PROPAGATION, ACCELERATION, AND MODULATIONH. V. CaneH. V. CaneLaboratory for High Energy Astrophysics, NASA/GSFC, Greenbelt, MD 20771, U.S.APhysics Department, University of Tasmania, Hobart, Tasmania 7001, Australiahttps://doi.org/10.1142/9789814529044_0008Cited by:2 PreviousNext AboutSectionsPDF/EPUB ToolsAdd to favoritesDownload CitationsTrack CitationsRecommend to Library ShareShare onFacebookTwitterLinked InRedditEmail Abstract: This paper reviews the work presented at the XXV International Cosmic Ray Conference under the headings "Transport and Transient Phenomena in the Heliosphere" (SH2, SH3). Such research investigates the behaviour of solar particles and galactic cosmic rays in response to solar wind variations with timescales up to the order of days. Long term modulation forms part of SH4. The papers in the main discussed aspects of particle propagation, particle responses to corotating interaction regions and particle responses to coronal mass ejections and their associated shocks formed in the interplanetary medium. Most results referred to locations within 5 AU of the Sun. Although no dramatically new results were presented, continuous progress has been made. Topics of particular interest included 1) the role of perpendicular diffusion in explaining the Ulysses high latitude results, 2) comparisons between theory and observation in deriving diffusion coefficients and 3) the adequacy of diffusive shock acceleration to explain observations above about 10 MeV. FiguresReferencesRelatedDetailsCited By 2Energetic Particles and High-Energy Solar PhenomenaLeonty Miroshnichenko22 August 2014Solar Cosmic Rays in the Interplanetary SpaceLeonty Miroshnichenko22 August 2014 25th International Cosmic Ray Conference — Volume 8Metrics History PDF download