Low energy galactic cosmic rays in the heliosphere |
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| Institution: | 1. Instituto de Astronomia, Geofísica e Ciências Atmosféricas (IAG), Universidade de São Paulo, Cidade Universitária, São Paulo - SP 05508-900, Brazil;2. Instituto Nacional de Pesquisas Espaciais (INPE) and World Institute for Space Environment Research (WISER), P. O. Box 515, São José dos Campos - SP 12227-010, Brazil;3. Instituto de Geofisica, Universidad Nacional Autónoma de México, 04510 México, D.F., México;4. CSPAR, University of Alabama in Huntsville, Huntsville, AL, 35899, USA;5. Emeritus, AFRL(VSBX), Hanscom AFB, Bedford, MA, 01731, USA |
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| Abstract: | The flux of galactic cosmic rays (GCR) extends over a wide range of energies (from 108 to 1020 eV); it has a strong dependence on particle energy. Given the large span of energies the detection techniques, transport mechanisms and other characteristics vary as energy increases. In the low energy region (<1012 eV) the flux of GCR is modulated by the solar activity. Continuous registers are necessary to study intensity variations that must have their origin in the Sun. Detectors were designed and constructed for the purpose, they operate since the middle of the last century providing valuable information to study recurrent periodicities and their relationship to those of solar phenomena, but also to elucidate whose are the relevant transport mechanisms inside the heliosphere. A brief review of the advancement in the comprehension of these phenomena is presented. |
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