On the dependence of maximum GCR intensity on heliospheric factors for the last five sunspot minima

Author:

Krainev Mikhail,Kalinin Mikhail,Aslam O.P.M.,Ngobeni Donald,Potgieter Marius S

Funder

RFBR

Publisher

Elsevier BV

Subject

Space and Planetary Science,Aerospace Engineering,General Earth and Planetary Sciences,Atmospheric Science,Geophysics,Astronomy and Astrophysics

Reference40 articles.

1. Time dependence of the proton flux measured by PAMELA during the 2006 July to 2009 December solar minimum;Adriani;Astrophys. J.,2013

2. Modeling of heliospheric modulation of cosmic-ray positrons in a very quiet heliosphere;Aslam;Astrophys. J.,2019

3. Time and charge-sign dependence of the heliospheric modulation of cosmic rays;Aslam;Astrophys. J.,2021

4. Galactic cosmic-ray hydrogen spectra in the 40–250 MeV Range measured by the High-energy Particle Detector (HEPD) on board the CSES-01 Satellite between 2018 and 2020;Bartocci;Astrophys. J.,2020

5. On the stratospheric measurements of cosmic rays;Bazilevskaya;Space Sci. Rev.,1998

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