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
Kasting, J. F., Whitmire, D. P., & Reynolds, R. T. (1993) · Icarus · doi:10.1006/icar.1993.1010 · Cited by 2,501 · cited 1×
“This increasing luminosity leads to the “faint young Sun” problem of atmospheric evolution on the terrestrial planets (Sagan & Mullen 1972; Kasting & Catling 2003), as well as the temporal expansion of the circumstellar habitable zone (Kasting et al. 1993; Rushby et al. 2012).”
Atmospheric Influence of Earth's Earliest Sulfur Cycle
Farquhar, J., Bao, H., & Thiemens, M. (2000) · Science · doi:10.1126/science.289.5480.756 · Cited by 1,805
Earth and Mars: evolution of atmospheres and surface temperatures
Sagan, C., & Mullen, G. (1972) · Science · doi:10.1126/science.177.4043.52 · Cited by 942
Solar interior structure and luminosity variations
Gough, D. O. (1981) · Solar Physics · doi:10.1007/bf00151270 · Cited by 798
ZAHNLE, K., CLAIRE, M., & CATLING, D. (2006) · Geobiology · doi:10.1111/j.1472-4669.2006.00085.x · Cited by 315
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
Kasting, J. F., & Donahue, T. M. (1980) · Journal of Geophysical Research: Oceans · doi:10.1029/jc085ic06p03255 · Cited by 165
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
Zahnle, K. J., Gacesa, M., & Catling, D. C. (2019) · Geochimica et Cosmochimica Acta · doi:10.1016/j.gca.2018.09.017 · Cited by 175
Self-citationLammer, H., Stökl, A., Erkaev, N. V., Dorfi, E. A., Odert, P., Güdel, M., Kulikov, Y. N., Kislyakova, K. G., & Leitzinger, M. (2014) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stu085 · Cited by 157
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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- Claire, M. W., Sheets, J., Cohen, M., Ribas, I., Meadows, V. S., & Catling, D. C. (2012). THE EVOLUTION OF SOLAR FLUX FROM 0.1 nm TO 160 μm: QUANTITATIVE ESTIMATES FOR PLANETARY STUDIES. The Astrophysical Journal. https://doi.org/10.1088/0004-637x/757/1/95
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