The measurement of inhomogeneities in the electron content along the orbital paths of Gemini 8 and Gemini 9 missions was not accomplished because the tracking information was not available. The use of ultrahigh frequency radio transmission was the primary factor in the successful removal of a very high frequency Faraday rotation ambiguity; but, as was expected, this was not very useful for fine-scale polarization studies. Ionosonde data were useful in the computation of the slab thickness at the closest point of approach of the spacecraft.
Experiment Do14: Ultrahigh and very high frequency polarization
01.09.1971
Sonstige
Keine Angabe
Englisch
Ultrahigh-speed polarization modulator
IEEE | 2005
|Engineering Index Backfile | 1946
|Engineering Index Backfile | 1946
|Engineering Index Backfile | 1946
|System design of the ultrahigh velocity GEDI experiment
Tema Archiv | 1986
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