Citation
Abstract
The 1976 Pioneer 11 Solar Conjunction provided the opportunity to accumulate a substantial quantity of doppler noise data over a dynamic range of signal closest approach point heliographic latitudes. The observed doppler noise data were fit to the (previously developed) doppler noise model “ISED,” and the deviations of the observed doppler noise data from the model were used to construct a (multiplicative) function to describe the effect of heliographic latitude (45): fl ) = 10 -0.9(P ./90 deg) This expression was then incorporated (back) into the ISED model to produce a new doppler noise model — “ISEDB.”
Details
- Volume
- 42-35
- Published
- October 15, 1976
- Pages
- 136–147
- File Size
- 674.8 KB