The DOI matches its Crossref record; 9 of the 9 references it cites were found in a registry or an index.
THE EVOLUTION OF SOLAR FLUX FROM 0.1 nm TO 160 μm: QUANTITATIVE ESTIMATES FOR PLANETARY STUDIES
Open accessAbstract
Understanding changes in the solar flux over geologic time is vital for understanding the evolution of planetary atmospheres because it affects atmospheric escape and chemistry, as well as climate. We describe a numerical parameterization for wavelength-dependent changes to the non-attenuated solar flux appropriate for most times and places in the solar system. We combine data from the Sun and solar analogs to estimate enhanced UV and X-ray fluxes for the young Sun and use standard solar models to estimate changing visible and infrared fluxes. The parameterization, a series of multipliers relative to the modern top of the atmosphere flux at Earth, is valid from 0.1 nm through the infrared, and from 0.6 Gyr through 6.7 Gyr, and is extended from the solar zero-age main sequence to 8.0 Gyr subject to additional uncertainties. The parameterization is applied to a representative modern day flux, providing quantitative estimates of the wavelength dependence of solar flux for paleodates relevant to the evolution of atmospheres in the solar system (or around other G-type stars). We validate the code by Monte Carlo analysis of uncertainties in stellar age and flux, and with comparisons to the solar proxies κ 1 Cet and EK Dra. The model is applied to the computation of photolysis rates on the Archean Earth.
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Citations
Cites
Habitable Zones around Main Sequence Stars
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Atmospheric Influence of Earth's Earliest Sulfur Cycle
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Earth and Mars: evolution of atmospheres and surface temperatures
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Solar interior structure and luminosity variations
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Self-citationA bistable organic-rich atmosphere on the Neoarchaean Earth
Zerkle, A. L., Claire, M. W., Domagal-Goldman, S. D., Farquhar, J., & Poulton, S. W. (2012) · Nature Geoscience · doi:10.1038/ngeo1425 · Cited by 239
Self-citationOrganic haze, glaciations and multiple sulfur isotopes in the Mid-Archean Era
Domagal-Goldman, S. D., Kasting, J. F., Johnston, D. T., & Farquhar, J. (2008) · Earth and Planetary Science Letters · doi:10.1016/j.epsl.2008.01.040 · Cited by 204
The evolution of atmospheric ozone
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Kulikov, Y. N., Lammer, H., Lichtenegger, H. I. M., Penz, T., Breuer, D., Spohn, T., Lundin, R., & Biernat, H. K. (2007) · Space Science Reviews · doi:10.1007/s11214-007-9192-4 · Cited by 139
Cited by
The Pale Orange Dot: The Spectrum and Habitability of Hazy Archean Earth
Arney, G., Domagal-Goldman, S. D., Meadows, V. S., Wolf, E. T., Schwieterman, E., Charnay, B., Claire, M., Hébrard, E., & Trainer, M. G. (2016) · Astrobiology · doi:10.1089/ast.2015.1422 · Cited by 327
“…particle microphysics) is run first to generate an initial atmospheric state based on user-specified boundary conditions [gas mixing ratios or fluxes, the solar constant at 2.7 Ga (Claire et al. , 2012), the stellar spectral type, total atmospheric pressure, the initial temperature-pressure profile].”
InfluentialSelf-citationOrigin and evolution of the atmospheres of early Venus, Earth and Mars
Lammer, H., Zerkle, A. L., Gebauer, S., Tosi, N., Noack, L., Scherf, M., Pilat-Lohinger, E., Güdel, M., Grenfell, J. L., Godolt, M., et al. (2018) · The Astronomy and Astrophysics Review · doi:10.1007/s00159-018-0108-y · Cited by 202
Outgassing History and Escape of the Martian Atmosphere and Water Inventory
Lammer, H., Chassefière, E., Karatekin, Ö., Morschhauser, A., Niles, P. B., Mousis, O., Odert, P., Möstl, U. V., Breuer, D., Dehant, V., et al. (2013) · Space Science Reviews · doi:10.1007/s11214-012-9943-8 · Cited by 180
Strange messenger: a new history of hydrogen on Earth, as told by xenon
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Influence of the UV Environment on the Synthesis of Prebiotic Molecules
Ranjan, S., & Sasselov, D. D. (2016) · Astrobiology · doi:10.1089/ast.2015.1359 · Cited by 159
Habitable Zone Lifetimes of Exoplanets around Main Sequence Stars
Rushby, A. J., Claire, M. W., Osborn, H., & Watson, A. J. (2013) · Astrobiology · doi:10.1089/ast.2012.0938 · Cited by 138
Self-citationEvolution of atmospheric xenon and other noble gases inferred from Archean to Paleoproterozoic rocks
Avice, G., Marty, B., Burgess, R., Hofmann, A., Philippot, P., Zahnle, K., & Zakharov, D. (2018) · Geochimica et Cosmochimica Acta · doi:10.1016/j.gca.2018.04.018 · Cited by 136
Deal, A. M., Rapf, R. J., & Vaida, V. (2021) · The Journal of Physical Chemistry A · doi:10.1021/acs.jpca.1c02864 · Cited by 105
Johnstone, C. P., Güdel, M., Lammer, H., & Kislyakova, K. G. (2018) · Astronomy & Astrophysics · doi:10.1051/0004-6361/201832776 · Cited by 97
“Since Claire et al. (2012) used a more realistic method for estimating the spectra of the Sun at higher activity levels, we should not expect any exact agreement between our models and those of Tian et al. (2008a) even for the same total input XUV flux.”
BackgroundMethodInfluentialNitrogen Oxide Concentrations in Natural Waters on Early Earth
Ranjan, S., Todd, Z. R., Rimmer, P. B., Sasselov, D. D., & Babbin, A. R. (2019) · Geochemistry, Geophysics, Geosystems · doi:10.1029/2018gc008082 · Cited by 94
Atmospheric sulfur rearrangement 2.7 billion years ago: Evidence for oxygenic photosynthesis
Kurzweil, F., Claire, M., Thomazo, C., Peters, M., Hannington, M., & Strauss, H. (2013) · Earth and Planetary Science Letters · doi:10.1016/j.epsl.2013.01.028 · Cited by 91
Self-citationBiological regulation of atmospheric chemistry en route to planetary oxygenation
Izon, G., Zerkle, A. L., Williford, K. H., Farquhar, J., Poulton, S. W., & Claire, M. W. (2017) · Proceedings of the National Academy of Sciences · doi:10.1073/pnas.1618798114 · Cited by 86
Self-citationExtreme hydrodynamic losses of Earth-like atmospheres in the habitable zones of very active stars
Johnstone, C. P., Khodachenko, M. L., Lüftinger, T., Kislyakova, K. G., Lammer, H., & Güdel, M. (2019) · Astronomy & Astrophysics · doi:10.1051/0004-6361/201935279 · Cited by 79
Hydrodynamic escape of water vapor atmospheres near very active stars
Johnstone, C. P. (2020) · The Astrophysical Journal · doi:10.3847/1538-4357/ab6224 · Cited by 63
Coupled noble gas–hydrocarbon evolution of the early Earth atmosphere upon solar UV irradiation
Hébrard, E., & Marty, B. (2014) · Earth and Planetary Science Letters · doi:10.1016/j.epsl.2013.10.022 · Cited by 54
Atmospheric hydrogen peroxide and Eoarchean iron formations
Pecoits, E., Smith, M. L., Catling, D. C., Philippot, P., Kappler, A., & Konhauser, K. O. (2015) · Geobiology · doi:10.1111/gbi.12116 · Cited by 52
Self-citationThe young Sun's XUV-activity as a constraint for lower CO2-limits in the Earth's Archean atmosphere
Johnstone, C. P., Lammer, H., Kislyakova, K. G., Scherf, M., & Güdel, M. (2021) · Earth and Planetary Science Letters · doi:10.1016/j.epsl.2021.117197 · Cited by 47
Evolution of the Earth's polar outflow from mid-Archean to present
Kislyakova, K. G., Johnstone, C. P., Scherf, M., Holmström, M., Alexeev, I. I., Lammer, H., Khodachenko, M. L., & Güdel, M. (2020) · Journal of Geophysical Research Space Physics · doi:10.1029/2020ja027837 · Cited by 20
Metadata
- Authors
- Claire, M. W., Sheets, J., Cohen, M., Ribas, I., Meadows, V. S., & Catling, D. C.
- Venue
- The Astrophysical Journal
- Publisher
- American Astronomical Society
- Published
- 2012-09-06
- Volume
- 757
- Issue
- 1
- Pages
- 95
- ISSN
- 0004-637X (ISSN-L)
- 1538-4357
- OpenAlex
- W2033808067
- Cited by
- 271
- References
- 9
- FWCI
- 6.20
- Type
- journal article
- Language
- en
- Open access
- bronze
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