Citation

Abstract

In support of the Mariner Venus/Mercury 1973 (MVM’73) X-band experiment and planned future Mariner missions, the 64-m antenna network is being supplied with S- and X-band reflex feed systems. The initial installation, for MVM’73, was implemented at DSS 14 and provides satisfactory performance for that mission. The X-band performance of the dichroic reflector is, however, not acceptable for planned future missions which have more stringent X-band performance requirements. A new dichroic reflector which grossly reduces the X-band ellipticity and noise temperature degradation has been designed. In this reporting, the theory and experimental performance of this new design is reported.

Details

Volume
XIX
Published
February 15, 1974
Pages
55–62
File Size
900.8 KB