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    Recent Results from MPE-3D

    Venus at 2.2 microns. 

    This is a preliminary mosaic of the night side of Venus. We obtained the data using MPE-3D at the Anglo-Australian Telescope in December, 1997.  Assembling this mosaic required 112 individual 3D fields, each 6.4 arcseconds square. The day side is the saturated crescent on the right side of the mosaic; it appears dark on the right side of the terminator as an artifact of over-exposure. Courtesy David Crisp and Vikki Meadows; preliminary data reduction and mosaicking by Jack Gallimore and Lowell Tacconi-Garman.


 


 
 
 
 
 
 
 
 

 This page was last modified on 10 November 1998.


MPE-3D Homepage The Instrument References and Links Data Reduction
SPECIAL NOTES FOR SPECIFIC
 RUNS
Public FTP-Site