r1 - 07 May 2004 - 11:56:18 - AnitaRichardsYou are here: TWiki >  Astrogrid Web  >  DocStore > InterOperability > InteropDataModel > ObservationDataModelRevision > FoV
FoV = Field of View. This may be limited by the size of a CCD or a collection of overlapping frames. In radio interferometry it is ultimately limited by the primary beam of the individual antennae but this is a continuous funtion usually described as FWHM (full width hald maximum). In addition the edges of the field may suffer worse degredation due to time- or spectral-smearing, so the effective field of view is expressed as a sum of functions or as the point at which the worst effect leads to a 10% or 50% etc. degredation.

-- AnitaRichards - 07 May 2004

Edit | Attach | Printable | Raw View | Backlinks: Web, All Webs | History: r1 | More topic actions
 
AstroGrid Service Click here for the
AstroGrid Service Web
This is the AstroGrid
Development Wiki
This site is powered by the TWiki collaboration platformCopyright © by the contributing authors. All material on this collaboration platform is the property of the contributing authors.
Ideas, requests, problems regarding TWiki? Send feedback