Citation
Abstract
The effects of deep-space probes on future radio-astronomy observations from the shielded zone of the Moon (SZM) are quantified by means of the radio-frequency power densities produced at the lunar surface in those deep-space exploration frequency bands with primary status in the International Telecommunications Union Table of Frequency Allocations. A worst-case approximation is used to determine the maximum number of deep-space probes that would be needed to produce harmful interference to the radio-astronomy observations in those bands.
Details
- Volume
- 42-129
- Published
- May 15, 1997
- Pages
- 1–9
- File Size
- 303.7 KB