File:Comet Hale-Bopp (eso9521c).jpg

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This image was produced through successive use of photographic enhancement and subtraction, followed by smoothing by computer processing .

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Description
English: This image was produced through successive use of photographic enhancement and subtraction, followed by smoothing by computer processing . When a matching, earlier exposure of the same sky field with the same telescope (on which the comet is not present) is photographically subtracted from the enhanced photo of the same field in which the comet is present, then the images of the stars should in principle cancel out, leaving only that of the comet in the field. A full cancellation is virtually impossible to achieve in practice, but if the resulting image is heavily smoothed (i.e. substituting each image element with the mean intensity of its surroundings), then the smaller images of the stars disappear and the full extent of the comet's large coma becomes visible. This false-colour photo was produced in this way by means of computer processing within the MIDAS image processing system. The images of the brightest stars could not be completely removed by this process and faint remnants are still present. (In technical terms, a 2-D low-pass Fourier filter was used to achieve heavy smoothing over approx. 16 x 16 arcsec cells).
Date 30 August 1995 (upload date)
Source
This media was produced by the European Southern Observatory (ESO), under the identifier eso9521c

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Author ESO
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current22:51, 14 June 2024Thumbnail for version as of 22:51, 14 June 2024908 × 774 (176 KB)OptimusPrimeBot (talk | contribs)#Spacemedia - Upload of https://www.eso.org/public/archives/images/large/eso9521c.jpg via Commons:Spacemedia

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