The Solar Cycle Temporal Variation of the Solar Wind Charge Exchange X-Ray Lines
Solar wind charge exchange (SWCX) is the primary contamination of soft X-ray emission lines from the Milky Way (MW) hot gas. We report a solar cycle (≈10 yr) temporal variation of observed O vii and O viii emission line measurements in the XMM-Newton archive, which is tightly correlated with the sol...
| Main Authors: | , , , , |
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| Format: | Article |
| Language: | English |
| Published: |
Institute of Physics
2022
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| Online Access: | View Fulltext in Publisher |