Simulation of one-day cosmic ray solar shadow observations

Guanda He; Haoshen Fan

doi:10.1117/12.2644404

9 September 2022 Simulation of one-day cosmic ray solar shadow observations

Guanda He, Haoshen Fan

Proceedings Volume 12328, Second International Conference on Optics and Image Processing (ICOIP 2022); 1232816 (2022) https://doi.org/10.1117/12.2644404
Event: Second International Conference on Optics and Image Processing (ICOIP 2022), 2022, Taian, China

Abstract

The sun acts as an obstacle to prevent the galactic cosmic rays from propagating from the direction of the sun to the earth. The detectors on the ground are used to observe the direction of the sun, and the absence of the number of cosmic ray particles is found at the center of the sun. This missing phenomenon is called solar shadowing. The magnetic fields of some planetary systems between the Sun and the Sun can be observed by near-Earth satellites. In this article, we utilize a simulation package developed to predict the single-day observational impact of the sun's solar shadow on galactic cosmic rays. And we compared with the magnetic field of the planetary system observed by the near-Earth satellite, and then established the theoretical prediction of cosmic ray solar physics.

Citation Download Citation

Guanda He and Haoshen Fan "Simulation of one-day cosmic ray solar shadow observations", Proc. SPIE 12328, Second International Conference on Optics and Image Processing (ICOIP 2022), 1232816 (9 September 2022); https://doi.org/10.1117/12.2644404

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