作者: S. Chakrabarti , J.C. Green , Y.T. Chiu , R.M. Robinson , G.R. Swenson
DOI: 10.1016/0273-1177(86)90335-2
关键词: Magnetosphere 、 Physics 、 Line (formation) 、 Plasma 、 Doppler effect 、 Telescope 、 Extreme ultraviolet 、 Ion 、 Atomic physics 、 Ionosphere
摘要: The distribution of He+, O+, and charge-exchanged auroral protons can be obtained by tomographic deconvolution resonantly scattered solar 304, 834 1216 A signals, respectively, these ions in the sunlit magnetosphere. Doppler shifts emission features, if any, used to infer energies ions. This concept have been verified for case plasmaspheric He+ Extreme Ultraviolet telescope on board Apollo-Soyuz mission. Our calculations OII834A line are agreement with observations STP78-1 satellite experiment. One Spacelab I experiment has observed “hot emissions” near 1216A which predicted charge exchange geocoronal neutral hydrogen atoms. We discuss results a simulation expected intensities from various observing conditions describe design an instrument capable verifying hypothesis.