Propagation of solar protons and the interplanetary magnetic field |
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| Affiliation: | 1. Embrapa Agroindústria de Alimentos – Avenida das Américas, 29501, Guaratiba, Rio de Janeiro, RJ, 23020470, Brazil;2. Universidade Federal Rural do Rio de Janeiro – BR 465, Km 7, Seropédica 8, RJ, 238908000, Brazil;3. Fundação Centro Universitário Estadual da Zona Oeste – Avenida Manuela Caldeira de Alvarenga, 1203, Campo Grande, Rio de Janeiro, RJ, 23070-200, Brazil;4. Universidade Federal do Rio de Janeiro – Avenida Athos da Silveira Ramos, 149, Bloco E, Ilha do Fundão, Rio de Janeiro, RJ, 21941909, Brazil;1. College of Chemistry & Chemical Engineering, Lanzhou City University, Lanzhou 730070, China;2. Key Laboratory of Bioelectrochemistry & Environmental Analysis of Gansu Province, College of Chemistry & Chemical Engineering, Northwest Normal University, Lanzhou 730070, China;1. Beijing Key Laboratory of Resource-oriented Treatment of Industrial Pollutants, School of Energy and Environmental Engineering, University of Science and Technology Beijing, Beijing 100083, China;2. Baiyi Environment Investment Jiangsu Co, Ltd., Jiangyin, 214000, China;1. Department of Engineering, Federal University of Santa Catarina (UFSC), Campus Blumenau, 89036-002, Blumenau, SC, Brazil;2. Ceramic and Composite Materials Research Group (CERMAT), Mechanical Engineering Department (EMC), Federal University of Santa Catarina, Campus Trindade, 88040-900, Florianópolis, SC, Brazil;3. Department of Chemical and Food Engineering (EQA), Federal University of Santa Catarina (UFSC), Campus Trindade, 88040-900, Florianópolis, SC, Brazil;4. School of Dentistry (DODT), Postgraduate Program in Dentistry (PPGO), Federal University of Santa Catarina, Campus Trindade, 88040-900, Florianópolis, SC, Brazil;5. CMEMS-UMinho, University of Minho, Campus de Azurém, 4800-058, Guimarães, Portugal;1. Department of Metallurgical and Materials Engineering, University of Texas at El Paso, El Paso, TX 79968, USA;2. Materials and Manufacturing Directorate (RX), 3005 Hobson Way, Wright-Patterson Air Force Base (WPAFB), Dayton, OH 45433, USA;3. Department of Mechanical Engineering, University of Texas at El Paso, El Paso, TX 79968, USA |
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| Abstract: | Solar proton events are classified into three types, F,F1 and S, based on the intensity time variation and related solar phenomena. The propagation mechanism for each is considered. The structure of the magnetic fields near the Sun and in interplanetary space are deduced, and the structure of the flare nimbus is discussed. The influence of the interplanetary magnetic fields on the propagation of solar protons is examined in detail. |
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