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Applied Optics

Applied Optics


  • Editor: James C. Wyant
  • Vol. 47, Iss. 34 — Dec. 1, 2008
  • pp: H149–H156

Simulating irradiance and color during lunar eclipses using satellite data

Stanley David Gedzelman and Michael Vollmer  »View Author Affiliations

Applied Optics, Vol. 47, Issue 34, pp. H149-H156 (2008)

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Irradiance and color during the total lunar eclipses of 2007 and 2008 are simulated using a ray tracing model that includes refraction, scattering by molecules, and observed or climatological distributions of aerosols, ozone, clouds, and topography around the terminator. Central portions of the umbra appear deep red for almost all eclipses due to preferential removal of short wavelengths in the spectrum of sunlight by scattering in the lower troposphere. The fringe of the umbra appears turquoise or blue due to selective removal of wavelengths around 600 nm by the Chappuis absorption bands of ozone in the stratosphere. Asymmetric distributions of clouds and aerosols, particularly for the 2008 eclipse, produce minimum calculated irradiance up to 17   arc min from the umbra center, while high ozone content over the arctic makes the northern edge of the umbra deepest blue.

© 2008 Optical Society of America

OCIS Codes
(010.1110) Atmospheric and oceanic optics : Aerosols
(010.1290) Atmospheric and oceanic optics : Atmospheric optics
(010.4950) Atmospheric and oceanic optics : Ozone
(010.1615) Atmospheric and oceanic optics : Clouds
(010.1690) Atmospheric and oceanic optics : Color
(010.5620) Atmospheric and oceanic optics : Radiative transfer

Original Manuscript: April 29, 2008
Manuscript Accepted: June 16, 2008
Published: September 30, 2008

Stanley David Gedzelman and Michael Vollmer, "Simulating irradiance and color during lunar eclipses using satellite data," Appl. Opt. 47, H149-H156 (2008)

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