Published December 18, 2025
| Version 1.0
Dataset
Open
stellar_spectra/solar
Description
Solar spectra for planetary modelling.
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sun.txt: Modern solar spectrum from the National Renewable Energy Laboratory (NREL) by Christian Gueymard.-
Sun0.6Ga.txt - Sun4.4Ga.txt: Past solar spectra (Ga = Gyr ago) from the Virtual Planetary Laboratory (VPL). By Claire et al, 2012.-
SunModern.txt: Modern solar spectrum from the Virtual Planetary Laboratory (VPL). By Claire et al, 2012.-
Sun5.6Gyr.txt: Future solar spectrum from the Virtual Planetary Laboratory (VPL). By Claire et al, 2012.See:
Gueymard, C. A. (2004). The sun’s total and spectral irradiance for solar energy applications and solar radiation models. Solar energy, 76(4), 423-453. https://doi.org/10.1016/j.solener.2003.08.039
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, 757(1), 95. https://doi.org/10.1088/0004-637X/757/1/95
Files
Sun0.6Ga.txt
Files
(7.2 MB)
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md5:4d436397be6385b00f6b5e223f133123
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md5:f694106a6b6e0f2ac4f7a20ddf307392
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md5:410507a37b2375ece9e2e2235cabb093
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Additional details
Related works
- Is derived from
- Journal article: 10.1088/0004-637X/757/1/95 (DOI)
- Journal article: 10.1016/j.solener.2003.08.039 (DOI)
References
- 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, 757(1), 95. https://doi.org/10.1088/0004-637X/757/1/95
- Gueymard, C. A. (2004). The sun's total and spectral irradiance for solar energy applications and solar radiation models. Solar energy, 76(4), 423-453. https://doi.org/10.1016/j.solener.2003.08.039