Paper
13 February 2003 Keck AO observations of Io in and out of eclipse
Author Affiliations +
Abstract
We present AO observations of Io before the satellite went into eclipse, and while it was in Jupiter's shadow. For the sunlit images Io itself was used as the wavefront reference source, while nearby Ganymede was used as reference 'star' when Io was in eclipse. Observations were obtained in Kp, Lp, and Ms bands. We show results before and after deconvolution of the data. We determined the flux densities for the hot spots from the original Io-in-eclipse data via a FFT method, and from the sunlit images after deconvolution of the images with MISTRAL. We present preliminary temperatures and areal coverages for the 6 brightest volcanoes.
© (2003) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Imke de Pater, Franck Marchis, Bruce A. Macintosh, Henry G Roe, David Le Mignant, and James R. Graham "Keck AO observations of Io in and out of eclipse", Proc. SPIE 4834, Discoveries and Research Prospects from 6- to 10-Meter-Class Telescopes II, (13 February 2003); https://doi.org/10.1117/12.457096
Lens.org Logo
CITATIONS
Cited by 1 scholarly publication.
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Information operations

Point spread functions

Adaptive optics

Stars

Image processing

Satellites

Deconvolution

RELATED CONTENT

Image restoration with spatially variable PSF
Proceedings of SPIE (August 07 2014)
Image processing in the BRITE nano-satellite mission
Proceedings of SPIE (July 29 2016)
Post-processing for anisoplanatic AO corrected images
Proceedings of SPIE (November 17 2000)
Deconvolution of ADONIS images
Proceedings of SPIE (September 11 1998)

Back to Top