Xref: utzoo sci.astro:3986 sci.space.shuttle:2999 Path: utzoo!utgpu!jarvis.csri.toronto.edu!mailrus!tut.cis.ohio-state.edu!ucbvax!pasteur!ames!oliveb!apple!bloom-beacon!athena.mit.edu!pgf From: pgf@athena.mit.edu (Peter G. Ford) Newsgroups: sci.astro,sci.space.shuttle Subject: Re: Data Volume Message-ID: <11140@bloom-beacon.MIT.EDU> Date: 5 May 89 03:20:02 GMT References: <3801@aplcomm.jhuapl.edu> Sender: daemon@bloom-beacon.MIT.EDU Reply-To: pgf@space.mit.edu (Peter G. Ford) Organization: MIT Center for Space Research Lines: 21 In article <3801@aplcomm.jhuapl.edu> jwm@aplvax.jhuapl.edu (Jim Meritt) writes: > >Given that the Magellan is suppose to have "resolution down to football >sizes" and all of Venus is dry, how many pixels would we be talking >about here (assume pixel tone is function of height, so only one >pixel per resolution cell). How much data are we talking about here, >beside "a bunch"? The downlink telemetry rate will be 268 Kbaud. During the "nominal" 243-day mapping mission, Magellan will return about 5 terabits (5.0e+12) of data. This will be further processed back on earth, and the primary data product will consist of over 400 images, each of 8192x7168 pixels (bytes), i.e. about 250 gigabytes total. In one series of images, each pixel represents a 75x75 meter area of Venus surface. In a series of lower resolution images, each pixel represents 225x225 meters. Pixel intensity will be a function of radar "brightness", not height. A separate altimeter experiment will return topography information, but at a much lower horizontal resolution, i.e. 10x10 km. Peter Ford MIT and Magellan Project