Experimental Study of Galactic Cosmic Ray Fluxes in the Solar Modulation Energy Range
摘要
Abstract
A new approach was proposed to the development of scientific equipment for the study of galactic and solar cosmic ray fluxes in the solar modulation energy range (30–1000 MeV/nucleon) with element-by-element charge and mass resolution. The equipment was proposed to be placed on the ROS Russian space station (Modulation project) and on the MNLS international scientific lunar station (Moon–Modulation project), if it is created. The projects involve the creation of a database of galactic and solar cosmic rays (SCR) for the entire solar activity cycle. Such a database is necessary to improve numerical models of fluxes of energetic heliospheric particles in interplanetary and near-Earth space.