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- W2009908708 abstract "X-rays should be generated throughout the heliosphere as a consequence of charge transfer collisions between heavy (Z>2) solar wind ions and interstellar neutrals. The high charge state solar wind ions resulting from these collisions are left in highly excited states and emit extreme ultraviolet or soft X-ray photons. This solar wind charge exchange mechanism applied to cometary neutrals has been used to explain the soft X-ray emission observed from comets. A simple model demonstrates that heliospheric X-ray emission can account for about 25%-50% of the observed soft X-ray background intensities. The spatial and temporal variations of heliospheric X-ray emission should reflect variations in the solar wind flux and composition as well as variations in the distribution of interstellar neutrals within the heliosphere. The heliospheric X-ray background can perhaps be identified with the long-term enhancements in the soft X-ray background measured by ROSAT." @default.
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- W2009908708 date "2000-04-01" @default.
- W2009908708 modified "2023-09-30" @default.
- W2009908708 title "Heliospheric X-ray Emission Associated with Charge Transfer of the Solar Wind with Interstellar Neutrals" @default.
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- W2009908708 doi "https://doi.org/10.1086/312574" @default.
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