Association of solar flux (2800 MHz) and cosmic ray intensity for solar cycle 22 and 23

Abstract

The variation of galactic cosmic rays in the heliosphere in correlation with the solar activity presents a high scientific interest for several aspects. The possibility of studying the energy charge (& mass), spatial & temporal distribution of cosmic rays in the interstellar space, in the vicinity of the solar system, can provide a better understanding of astrophysical mechanism like, for instance, the acceleration of charged particles in a shocked plasma. Galactic cosmic rays in turn can be used as a unique tool for deeply understanding the characteristics & the dynamics of the heliosphere. So it is necessary & significant to investigate the role of various solar parameters in the variation of galactic cosmic rays. Solar radio flux is the energy emitted by the sun with a slowly varying intensity. The amount of this energy is high in the corona & it changes gradually day to day in response to the numbers of spot groups on the solar disk.