Citation
Abstract
This report considers two-way coherent Doppler error resulting from phase scintillations induced on the uplink by the solar corona. It is shown that this error can be estimated by taking Statistics on the differential Doppler measurements. Typical estimates for the error are given for four Sun-Earth-probe angles and for integration times ranging from I second to I minute. These results are based on data collected during the 1985 Voyager 2 solar conjunction.
Details
- Volume
- 42-95
- Published
- November 15, 1988
- Pages
- 28–31
- File Size
- 135.9 KB