Using stars for remote sensing of the Earth's stratosphere

Details Using stars for remote sensing of the Earth's stratosphere Using stars for remote sensing of the Earth's stratosphere

Oct 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994apopt..33.7126r&link_type=abstract

Applied Optics (ISSN 0003-6935), vol. 33, no. 30, p. 7126-7131

Physics

Optics

9

Atmospheric Optics, Earth (Planet), Earth Observations (From Space), Electromagnetic Absorption, Light (Visible Radiation), Planetary Radiation, Remote Sensing, Stellar Radiation, Stratosphere, Ultraviolet Astronomy, Ultraviolet Radiation, Atmospheric Composition, Ozone, Ozone Depletion, Polar Regions, Radiation Detectors, Telescopes, Ultraviolet Spectrometers

Scientific paper

A UV-visible spectrometer system is reported to measure light absorption from planets and stars by Earth's atmospheric constituents. Wavelength coverage of the system is suitable for stratospheric measurements concerning polar ozone loss and measurements of ozone itself. The system involves a small telescope, a UV-visible spectrometer, and an array detector.

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