Comparison of the results of the solar protons release times in solar proton events obtained by various methods
- Autores: Ochelkov Y.P1
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Afiliações:
- Institute of Applied Geophysics
- Edição: Volume 89, Nº 6 (2025)
- Páginas: 891-896
- Seção: Physics of Cosmic Rays
- URL: https://transsyst.ru/0367-6765/article/view/692818
- DOI: https://doi.org/10.31857/S0367676525060112
- ID: 692818
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Resumo
The comparison was made between the values of the solar release times of unrelativistic protons determined on scailing similarity time profiles of solar proton events and results of papers in which the solar release times of relativistic protons in GLE is determined on first observations with utilizing the method of velocity dispersion and on the first observations on neutron monitors with account of the dependence of the length of Sun–Earth magnetic line on solar wind velocity.
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Bibliografia
- Cane H.V., and Lario D. // Space Sci. Rev. 2006. V. 123. P. 45.
- Trottet G., Samwel S., Klein K.-L. et al. // Solar Physics. 2015. V. 290. No. 3. P. 819.
- Reames D.V. // Astrophys. J. 2009. V. 693. No. 1. P. 812.
- Bazilevskaya G.A. // Adv. Space Res. 2009. V. 43. P. 530.
- Очелков Ю.П. // Гелиогеофиз. иссл. 2018. Т. 19. С. 47.
- Очелков Ю.П. // Изв. РАН. Сер. физ. 2021. Т. 85. №8. С. 1189
- Очелков Ю.П. // Гелиогеофиз. иссл. 2023. Т. 37. С. 16.
- Ochelkov Yu.P. // Bull. Russ. Acad. Sci. Phys. 2023. V. 87. No. 7. P. 1066.
- https://ngdc.noaa.gov/stp/satellite/goes/dataaccess.html.
- Струминский А.Б., Григорьева И.Ю., Логачев Ю.И., Садовский А.М. // Изв. РАН. Сер. физ. 2021. Т. 85. №8. С. 1180
- Aschwanden M.J. // arXiv:1005.0029v5. 2011.
- https://cdaw.gsfc.nasa.gov/CME_list.
- Дорман Л.И., Мирошниченко Л.И. Солнечные космические лучи. М.: Наука, 1968. 468 c.
- Ochelkov Yu.P. // J. Phys. Conf. Ser. 2013. V. 409. Art. No. 012183.
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