Correlation of the Flux of Energetic Rays and Particles with the Solar Cycle
A solar flare is a sudden flash that occurs near the solar surface. Thisresults in the emission of an extensive range of energy from the surface of the Sun.These giant explosions generally contain X-rays and energy that tend to travel in alldirections at the speed of light. Coronal mass ejections (C...
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| Main Authors: | , , |
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| Format: | Article |
| Language: | English |
| Published: |
Damghan university
2022-10-01
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| Series: | Iranian Journal of Astronomy and Astrophysics |
| Subjects: | |
| Online Access: | https://ijaa.du.ac.ir/article_346_0cd89ca4667defbbe5ab5bf7be137293.pdf |
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| Summary: | A solar flare is a sudden flash that occurs near the solar surface. Thisresults in the emission of an extensive range of energy from the surface of the Sun.These giant explosions generally contain X-rays and energy that tend to travel in alldirections at the speed of light. Coronal mass ejections (CMEs) are types of explosionsthat occur on the solar surface. A CMEs releases a large amount of plasma and magneticfield. Our main goal in this research is to prove that the reason for the release of chargedparticles, protons, electrons and X-ray radiation, followed by the release of solar winds,is the occurrence of flares and CMEs. The occurrence of this phenomenon is relatedto other phenomena, such as the magnetic field of the Sun’s surface, the cycle of theSun’s activity, sunspots, the emission of charged particles of electrons and protonsfrom the solar corona, the rate of occurrence of CMEs from the corona, the averageand maximum speed of CME and X-ray radiation in the category Class X, which is thehighest energy category for X-ray radiation, is directly and closely related. |
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| ISSN: | 2322-4924 2383-403X |