dc.contributor.author | Robertson, I. P. | |
dc.contributor.author | Cravens, Thomas Edward | |
dc.date.accessioned | 2005-04-15T13:52:34Z | |
dc.date.available | 2005-04-15T13:52:34Z | |
dc.date.issued | 2003-04-29 | |
dc.identifier.citation | Robertson, IP; Cravens, TE. X-ray emission from the terrestrial magnetosheath. GEOPHYSICAL RESEARCH LETTERS. April 29 2003. 30(8): | |
dc.identifier.other | ISI:000182857600001 | |
dc.identifier.uri | http://hdl.handle.net/1808/285 | |
dc.description.abstract | [1] X-rays are generated throughout the terrestrial magnetosheath as a consequence of charge transfer collisions between heavy solar wind ions and geocoronal neutrals. The solar wind ions resulting from these collisions are left in highly excited states and emit extreme ultraviolet or soft X-ray photons. A model has been created to simulate this X-ray radiation. Published terrestrial exospheric hydrogen distributions and solar wind speed, density and temperature distributions were used in this model. Simulated images were created as seen from an observation point outside the geocorona. The locations of the bow shock and magnetopause are evident in these images. Perhaps this Xray emission can be used to remotely sense the solar wind flow around the magnetosphere. Since similar X-rays are produced in the heliosphere, the challenge will be, however, to eliminate this background emission. | |
dc.format.extent | 1553198 bytes | |
dc.format.extent | 1553198 bytes | |
dc.format.extent | 8567364 bytes | |
dc.format.extent | 3445772 bytes | |
dc.format.extent | 169534 bytes | |
dc.format.mimetype | image/tiff | |
dc.format.mimetype | image/tiff | |
dc.format.mimetype | image/tiff | |
dc.format.mimetype | image/tiff | |
dc.format.mimetype | application/pdf | |
dc.language.iso | en_US | |
dc.publisher | AMER GEOPHYSICAL UNION | |
dc.subject | multidisciplinary geosciences | |
dc.title | X-ray emission from the terrestrial magnetosheath | |
dc.type | Article | |
kusw.kuauthor | Cravens, Thomas Edward | |
dc.identifier.doi | 10.1029/2002GL016770 | |
dc.rights.accessrights | openAccess | |