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Solar Temperature Variations Computed from SORCE SIM Irradiances Observed During 2003-2020
by
Cahalan, Robert F
, Yatáz, Gaspar
, Ajiquichi, Paulino
in
Approximation
/ Astrophysics and Astroparticles
/ Atmospheric Sciences
/ Brightness temperature
/ Computation
/ Irradiance
/ Physics
/ Physics and Astronomy
/ Root-mean-square errors
/ Solar activity
/ Solar irradiance
/ Solar Physics
/ Solar radiation
/ Solar spectral irradiance
/ Solar temperature
/ Space Exploration and Astronautics
/ Space Sciences (including Extraterrestrial Physics
/ Spectra
/ Statistical models
/ Taylor series
/ Temperature variations
/ The Solar Radiation and Climate Experiment (SORCE) Mission: Final Calibrations and Data Products
/ Wavelengths
2022
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Solar Temperature Variations Computed from SORCE SIM Irradiances Observed During 2003-2020
by
Cahalan, Robert F
, Yatáz, Gaspar
, Ajiquichi, Paulino
in
Approximation
/ Astrophysics and Astroparticles
/ Atmospheric Sciences
/ Brightness temperature
/ Computation
/ Irradiance
/ Physics
/ Physics and Astronomy
/ Root-mean-square errors
/ Solar activity
/ Solar irradiance
/ Solar Physics
/ Solar radiation
/ Solar spectral irradiance
/ Solar temperature
/ Space Exploration and Astronautics
/ Space Sciences (including Extraterrestrial Physics
/ Spectra
/ Statistical models
/ Taylor series
/ Temperature variations
/ The Solar Radiation and Climate Experiment (SORCE) Mission: Final Calibrations and Data Products
/ Wavelengths
2022
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Solar Temperature Variations Computed from SORCE SIM Irradiances Observed During 2003-2020
by
Cahalan, Robert F
, Yatáz, Gaspar
, Ajiquichi, Paulino
in
Approximation
/ Astrophysics and Astroparticles
/ Atmospheric Sciences
/ Brightness temperature
/ Computation
/ Irradiance
/ Physics
/ Physics and Astronomy
/ Root-mean-square errors
/ Solar activity
/ Solar irradiance
/ Solar Physics
/ Solar radiation
/ Solar spectral irradiance
/ Solar temperature
/ Space Exploration and Astronautics
/ Space Sciences (including Extraterrestrial Physics
/ Spectra
/ Statistical models
/ Taylor series
/ Temperature variations
/ The Solar Radiation and Climate Experiment (SORCE) Mission: Final Calibrations and Data Products
/ Wavelengths
2022
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Solar Temperature Variations Computed from SORCE SIM Irradiances Observed During 2003-2020
Journal Article
Solar Temperature Variations Computed from SORCE SIM Irradiances Observed During 2003-2020
2022
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Overview
NASA’s Solar Radiation and Climate Experiment (SORCE) Spectral Irradiance Monitor (SIM) instrument produced about 17 years of daily average Spectral Solar Irradiance (SSI) data for wavelengths 240 nm – 2416 nm. We choose a day of minimal solar activity, 2008-08-24, during the 2008 − 2009 minimum between cycles 23 and 24, and compute the brightness temperature (𝑇o) from that day’s solar spectral irradiance (𝑆𝑆𝐼o). We consider small variations of T and SSI about these reference values, and derive linear and quadratic analytic approximations by Taylor expansion about the reference day values. To determine approximation accuracy, we compare to exact brightness temperatures T computed from the Planck spectrum, by solving analytically for T, or equivalent root-finding in Wolfram Mathematica. We find that the linear analytic approximation overestimates, while the quadratic underestimates the exact result. This motivates search for statistical “fit” models “in between” the two analytic models, with minimum root-mean-square-error RMSE. We make this search using open-source statistical R software, determine coefficients for linear and quadratic fit models, and compare statistical with analytic RMSE’s. When only linear analytic and fit models are compared, the fit model is superior at ultraviolet, visible, and near infrared wavelengths. This again holds true when comparing only quadratic models. Quadratic is superior to linear for both analytic and statistical models, and statistical fits give smallest RMSE’s. Lastly, we use linear analytic and fit models to find an interpolating function in wavelength, useful in case the SIM results need adjustment to another choices of wavelengths, to compare or extend to any other instrument.
Publisher
Springer,Springer Netherlands,Springer Nature B.V
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