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Radiation belt electron flux variability during three CIR-driven geomagnetic storms
Authors:MM Lam  RB Horne  NP Meredith  SA Glauert
Institution:1. Centre for Space Engineering, Utah State University, 4120 Old Main Hill, Logan, UT 84322-4120, USA;2. Department of Physics, Centre of Excellence in Research, PO Box 3000, FIN-90014, University of Oulu, Finland;1. Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, United States;2. Center for Space and Aeronomy Research, UAH, Huntsville, AL, United States;3. NASA Langley Research Center, Hampton, VA, United States;4. Sciences Systems and Applications, Inc., Hampton, VA, United States;5. Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States;1. Department of Geosciences, Tel Aviv University, Tel Aviv, Israel;2. Department of Meteorology and Atmospheric Science, Pennsylvania State University, University Park, PA, USA;3. German Remote Sensing Data Center – German Aerospace Center (DLR), Oberpfaffenhofen, Germany;4. Institute of Physics, University of Augsburg, Germany;5. National Institute of Geophysics and Volcanology (I.N.G.V.), Osservatorio Etneo, Section of Catania, Catania, Italy;1. National Atmospheric Research Laboratory, Gadanki 517112, India;2. Government College (Autonomous), Rajahmundry 533105, India;3. Department of Physics, Andhra University, Visakhapatnam 530003, India;1. Department of Physics and Astronomy, Dartmouth College, Hanover, NH, USA;2. Space Sciences Laboratory, University of California, Berkeley, CA, USA
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