Celestial radiation below 25 MHz, heretofore inaccessible, yields new insights. Report discusses feasibility of array of small satellites deployed in high orbit around Earth to monitor celestial radio sources at frequencies less than 25 MHz. Objective to make high-angular-resolution map of such sources over entire sky by use of very-long-baseline interferometry (VLBI).
Very-Long-Baseline Interferometry Using Cheap Satellites
NASA Tech Briefs ; 13 , 11
1989-11-01
Sonstige
Keine Angabe
Englisch
Very long baseline interferometry
NTRS | 1973
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