Ionospheric research and space weather services |
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| Institution: | 1. University of Rennes 1, Rennes, France;2. Institute of Atmospheric Physics of ASCR, Prague, Czech Republic;3. Instituto Nazionale di Geofisica e Vulcanologia, Rome, Italy;4. National Central University, Jungli City, Taiwan;1. Key Laboratory of Earthquake Prediction (Institute of Earthquake Science, China Earthquake Administration), Beijing, PR China;2. Institute of Meteorology and Oceanography, PLA University of Science and Technology, Nanjing, PR China;3. Oujiang College, Wenzhou University, Zhejiang, PR China;4. University Corporation for Atmospheric Research, Boulder, CO, USA;5. Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai, PR China;6. National Earthquake Infrastructure Service, China Earthquake Administration, Beijing, PR China;7. National Astronomical Observatory, Chinese Academy of Sciences, Beijing, PR China;1. IZMIRAN, Troitsk, Moscow 142190, Russia;2. Skobeltsyn Institute of Nuclear Physics, Moscow State University, Moscow 119992, Russia;3. Space Research Institute, RAS, Moscow 117997, Russia;1. Instituto de Informática, Universidade Federal de Goiás, Goiânia, Brazil;2. Institut für Optimierung und Operations Research, Universität Ulm, Ulm, Germany;1. Computer Science, Pacific Luthran University, Tacoma, WA, USA;2. Electrical and Computer Engineering, Western Michigan University, Kalamazoo, MI, USA;3. Chemical and Paper Engineering, Western Michigan University, Kalamazoo, MI, USA;1. Department of Geoinformatic Engineering, Inha University, Incheon, South Korea;2. Division of Mathematics, School of Advanced Sciences, Vellore Institute of Technology, Chennai, Tamil Nadu, India;3. Department of Public Works and Town & Country Planning, Division of Survey, Bangkok, Thailand;4. King Mongkut’s Institute of Technology Ladkrabang, Prince of Chumphon Campus, Chumphon, Thailand |
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| Abstract: | This paper concentrates on those major areas where our current physical understanding and recent advances can lead to positive predictions of the expected effects of ionospheric activity on the near-Earth space environment and on technological systems which operate within this environment. It briefly describes some of the key links between solar activity and the various physical processes, which govern ionospheric plasma structure that has been under scientific examination over past several decades but has lately received significant importance in relation to the space weather services. Specific examples during extremely intense solar event show how ionospheric monitoring techniques that have contributed immense data sets and related empirical and theoretical formulations have been incorporated in different ionospheric specification and prediction models for real-time operational applications. Finally, the general question of what might be expected as a result of current activities within different European cooperative projects is addressed. |
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