Angular distributions of energetic charged particles observed with HELIOS-1 and -2 between 0.3 amd 1 AU and their relevance to manned interplanetary space missions.
The University of Kiel Cosmic Ray Instrument on board the solar probes HELIOS-1 and -2 measured angular distributions of electrons, protons, and heavier nuclei between 0.3 and 1 AU over one complete solar cycle between 1974 and 1986. Anisotropies are observed mainly during the rising phase of solar particle events or close to the passage of certain interplanetary shocks. The anisotropies are presented as proton data of energies between 27 and 37 MeV. The dependence of the anisotropies on particle energy and distance from the sun is provided based on diffusive propagation in interplanetary space. Strong anisotropies could provide a chance of efficient shielding of the passenger compartment by moving heavier parts of the spacecraft structure into the direction of the highest flux. A reduction of the total radiation dose by less than a factor of 2 might be achievable, however, selection of quiet times for the mission reduces the radiation hazard much more.
Kunow
H
H
Institut fur Reine und Angewandte Kernphysik, Universitat Kiel, Germany.
D016880:Anisotropy; D003359:Cosmic Radiation; D008280:Magnetics; D008433:Mathematics; D011522:Protons; D011834:Radiation Monitoring / Q000295:instrumentation*; D011835:Radiation Protection; D012542:Scattering, Radiation; D019445:Solar Activity; D016082:Solar System; D013026:Space Flight; D018531:Spacecraft / Q000295:instrumentation*
D011522:Protons