The solar spectrum measured by FTS

Geoffrey C. Toon

doi:10.1364/FTS.2013.FTh1C.3

Imaging and Applied Optics Postdeadline
OSA Postdeadline Paper Digest (Optica Publishing Group, 2013),
paper FTh1C.3
•https://doi.org/10.1364/FTS.2013.FTh1C.3

The solar spectrum measured by FTS

Geoffrey C. Toon

Fourier Transform Spectroscopy 2013

Arlington, Virginia United States
23–24 June 2013
ISBN: 978-1-55752-979-4

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Satellite Atmospheric Science IV (FTh1C)

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G. C. Toon, "The solar spectrum measured by FTS," in Imaging and Applied Optics Postdeadline, OSA Postdeadline Paper Digest (Optica Publishing Group, 2013), paper FTh1C.3.

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Abstract

Accurate knowledge of the solar spectrum is important for interpreting remote sensing measurements that utilize sunlight. Fourier Transform Spectrometers have played an essential role in defining the high-resolution structure of the solar spectrum.

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The solar spectrum measured by FTS

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FTS Measurements of Solar Magnetic Fields Using the MgI Zeeman Line at 12.3 Microns

D. E. Jennings
FFD7 Fourier Transform Spectroscopy (FTS) 1995

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