Solar Cosmic Rays and Hard X-Ray Emission from Solar Flares in the First Half of 2024 according to the Data of Experiments on Moscow State University CubeSat Satellites
摘要
Abstract
A discussion is made of the results of observations of electrons of solar cosmic rays and hard X-ray emission from solar flares in the first half of 2024 in experiments on CubeSat satellites on a low polar orbit (LEO, altitude ∼550 km and inclination ∼98°) using scientific instruments created at the Skobeltsyn Institute of Nuclear Physics (SINP), Moscow State University.