Publikationsdatum:
2016-06-07
Beschreibung:
A 64m radar antenna was used to observe Saturn's rings at 12.6 cm wavelength, with reduced Doppler spread. The results show a positive radar return corresponding to about a 60 percent return from an isotropic scatterer with the projected area of the rings, allowing for the Cassini division. A radar spectrogram of the rings is shown with power density plotted against Doppler frequency shift.
Schlagwort(e):
ASTROPHYSICS
Materialart:
NASA, Washington The Rings of Saturn; p 73-82
Format:
application/pdf
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