Physics
Scientific paper
Dec 1976
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976dsnpr..36..121b&link_type=abstract
In its The Deep Space Network p 121-137 (SEE N77-14044 05-12)
Physics
Doppler Radar, Helios 1, Helios 2, Pioneer 10 Space Probe, Pioneer 11 Space Probe, Signal Transmission, Correlation Detection, Deep Space Network, Ionospheric Noise, Plasma Density, Signal To Noise Ratios
Scientific paper
Observed Doppler noise (rms phase jitter) from the 1976 solar conjunctions of the Helios 1 and 2 and the Pioneer 10 and 11 spacecraft was processed with a recently developed Doppler noise model ISEDB. Good agreement is obtained between the observed data and the model. Correlation is shown between deviations from the ISEDB model and sunspot activity, but it is insufficient to be modeled. Correlation is also shown between ISEDB model deviations for (spacecraft) signal paths on the same side of the sun.
Berman A. L.
Rockwell S. T.
Wackley J. A.
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