Structure, luminosity, and dynamics of the Venus thermosphere
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The difference from modern Venus and Mars is due to XUV heating scaling with the Sun's activity whereas infrared heating remains approximately constant in time.
“This is different to the cases of modern Venus and Mars in which infrared heating is very important (Fox and Bougher 1991), and this difference is due simply to the fact that the XUV heating scales with the Sun's activity whereas the infrared heating (which depends on the Sun's photospheric emission) remains approximately constant in time.”
From The young Sun's XUV-activity as a constraint for lower CO2-limits in the Earth's Archean atmosphere (2021) · cites this paper as Fox and Bougher 1991
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- Authors
- Fox, J. L., & Bougher, S. W.
- Affiliations
- State University of New York (US)
- University of Arizona (US)
- Venue
- Space Science Reviews
- Published
- 1991
- Volume
- 55
- Issue
- 1-4
- ISSN
- 0038-6308 (ISSN-L)
- 1572-9672
- OpenAlex
- W2003199218
- Cited by
- 98
- References
- 406
- Citations by year
- 2026: 1 · 2025: 1 · 2024: 4 · 2021: 2 · 2019: 2 · 2018: 3 · 2017: 2 · 2016: 2 · 2015: 2 · 2014: 1 · 2013: 2 · 2012: 3
- FWCI
- 17.87
- Type
- journal article
- Language
- en
- Open access
- closed
- Licence
- www.springer.com/tdm (tdm)
- Locations
- Space Science Reviews (publishedVersion)
- Journal of Bioresource Management (submittedVersion)
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Ionosphere and magnetosphere dynamics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Planetary Science and Exploration
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astro and Planetary Science
- Keywords
- Venus thermosphere, thermospheric temperature, thermospheric dynamics, airglow, auroral emission, Pioneer Venus, atmospheric escape, superrotation
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