Solar corona-induced fluctuations on spacecraft signal amplitude observed during solar superior conjunctions of the Cassini spacecraft-Reference-Cited by-同舟云学术

Solar corona-induced fluctuations on spacecraft signal amplitude observed during solar superior conjunctions of the Cassini spacecraft

Published:2007-05-09 Issue:3 Volume:42 Page:n/a-n/a
ISSN:0048-6604
Container-title:Radio Science
language:en
Short-container-title:Radio Sci.

Author:

Morabito David D.¹

Affiliation:

1. Jet Propulsion Laboratory; California Institute of Technology; Pasadena; California; USA

Publisher

American Geophysical Union (AGU)

Subject

Electrical and Electronic Engineering,General Earth and Planetary Sciences,Condensed Matter Physics

Reference30 articles.

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2. Solar wind motion within 30 Ro: Spacecraft radio scintillation observations;Armstrong;Astron. Astrophys.,1981

3. Armstrong , J. R. Woo 1981 Temporal autocorrelation functions and fluctuation power spectra of amplitude scintillations: Starprobe-Earth communications geometry JPL Internal Publ. IOM 3333 81 048 Jet Propul. Lab. Pasadena, Calif.

4. Propagation observations of the solar wind near the Sun;Coles;Astrophys. J.,1989

5. The solar wind density spectrum near the Sun: Results from Voyager radio measurements;Coles;J. Geophys. Res.,1991

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