Angle distribution and time variation of gamma ray flux from solar and stellar winds, 2. Generation by galactic cosmic rays

In our investigations of galactic cosmic rays (CR)-solar activity hysteresis phenomenon were obtained data on CR modulation parameters changing during solar cycle. Here we use these data to calculate the change of CR density distribution in the Heliosphere during solar cycle in dependence of particle rigidity. Then we calculate the expected gamma ray (GR) emissivity distribution and GR fluxes generated by interaction of modulated galactic CR with solar wind matter. It is shown that GR observations can give important additional information on solar wind distribution and CR modulation during solar cycle as well as on galactic CR modulation by stellar winds, stellar wind matter distribution and on stellar activity cycles