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Energetic Particle Observations |
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| Authors: | B Klecker H Kunow H V Cane S Dalla B Heber K Kecskemety K-L Klein J Kota H Kucharek D Lario M A Lee M A Popecki A Posner J Rodriguez-Pacheco T Sanderson G M Simnett E C Roelof |
| Institution: | 1. Max-Planck-Institut fürextraterrestrische Physik, 85740, Garching, Germany 2. Institut für Experimentelle und Angewandte Physik, University of Kiel, 24118, Kiel, Germany 3. School of Mathematics and Physics, University of Tasmania, Tasmania, Australia 4. School of Physics and Astronomy, University of Manchester, Manchester, M60 1QD, UK 5. Hungarian Academy of Sciences, Central Research Institute for Physics, Budapest, Hungary 6. Observatoire de Paris, LESIA-CNRS UMR 8109, Bat. 14, F-92195, Meudon, France 7. Department of Physics, University of Arizona, Tucson, AZ, 85721, USA 8. University of New Hampshire, Durham, NH, 03824, USA 9. Applied Physics Laboratory, Johns Hopkins University, Laurel, MD, USA 10. Southwest Research Institute, Space Science and Engineering Division, 6220 Culebra Rd., San Antonio, TX, 78228, USA 11. Space Research Group, Departamento de Fisica, Universidad de Alcalá, Ctra. Madrid-Barcelona, 28871, Alcalá de Henares, Espana 12. Space Science Dept. of ESA, Postbus 299, 2200, AG, Noordwijk, The Netherlands 13. School of Physics and Space Research, University of Birmingham, B15 2TT, Birmingham, UK |
| Abstract: | The characteristics of solar energetic particles (SEP) as observed in interplanetary space provide fundamental information about the origin of these particles, and the acceleration and propagation processes at the Sun and in interplanetary space. Furthermore, energetic particles provide information on the development and structure of coronal mass ejections as they propagate from the solar corona into the interplanetary medium. In this paper we review the measurements of energetic particles in interplanetary space and discuss their implication for our understanding of the sources, and of acceleration and propagation processes. |
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