Now showing items 1-4 of 4

    • Comparison of astrospheres around cool and hot stars 

      Scherer, K.; Ferreira, S.E.S.; Strauss, R.D.; Bomans, D.J.; Fichtner, H. (IOP Publishing, 2016)
      Simulations of astrospheres around hot and cool stars have recently move into the focus of scientific research. We describe here the differences between the astrospheres around hot and cool stars. While those around the ...
    • Cosmic ray flux at the earth in a variable heliosphere 

      Scherer, K.; Ferreira, S.E.S.; Potgieter, M.S.; Fichtner, H.; Heber, B. (Elsevier, 2008)
      In recent years the variability of the cosmic ray flux has become one of the main issues not only for the interpretation of the abundances of cosmogenic isotopes in cosmochronic archives like, e.g., ice cores, but also for ...
    • Heliosheath processes and the structure of the heliopause: modeling energetic particles, cosmic rays, and magnetic fields 

      Pogorelov, N.V.; Potgieter, M.S.; Strauss, R.D.; Fichtner, H.; Czechowski, A. (Springer, 2017)
      This paper summarizes the results obtained by the team “Heliosheath Processes and the Structure of the Heliopause: Modeling Energetic Particles, Cosmic Rays, and Magnetic Fields” supported by the International Space Science ...
    • On aspects pertaining to the perpendicular diffusion of solar energetic particles 

      Strauss, R.D.; Fichtner, H. (IOP Publishing, 2015)
      The multitude of recent multi-point spacecraft observations of solar energetic particle (SEP) events has made it possible to study the longitudinal distribution of SEPs in great detail. SEPs, even those accelerated during ...