Citation
Abstract
In a previous report, a geometric model to predict doppler noise during solar conjunctions was developed. In this report, deviations between observed doppler noise and the noise model are analyzed. Based on the analysis, it is tentatively concluded that deviations between the observed noise and the model are due to short-term fluctuations in solar activity as seen along the signal path, and not to solar/antenna structure effects or system noise temperature. NOISE» (Hz) = K, (ISI)**, ISI > 223 K, = 2.8 « 10°° IST] = B
Details
- Volume
- 42-30
- Published
- December 15, 1975
- Pages
- 264–272
- File Size
- 503.8 KB