Using phase scintillation spectral measurements to determine angle-of-arrival fluctuations during solar superior conjunction-Reference-Cited by-同舟云学术

Using phase scintillation spectral measurements to determine angle-of-arrival fluctuations during solar superior conjunction

Published:2010-05-25 Issue:3 Volume:45 Page:n/a-n/a
ISSN:0048-6604
Container-title:Radio Science
language:en
Short-container-title:Radio Sci.

Author:

Ho Christian M.¹,Morabito David D.¹,Woo Richard¹

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

Link

http://www.agu.org/journals/rs/rs1003/2009RS004176/2009RS004176.pdf

Reference14 articles.

1. Berman , A. L. 1977 Phase fluctuation spectra: New radio science information to become available in the DSN tracking system Mark III-77 JPL DSN Prog. Rep. 42-40 134 140 Jet Propul. Lab. Pasadena, Calif.

2. A theoretical model for equatorial ionospheric spread-F echoes in the HF and VHF bands;Booker;J. Atmos. Terr. Phys.,1978

3. Variance and spectra of angle-of-arrival and Doppler fluctuations caused by ionospheric scintillation;Crane;J. Geophys. Res.,1978

4. Solar corona effects on angle of arrival fluctuations for microwave telecommunication links during superior solar conjunction;Ho;Radio Sci.,2008

5. Effects of ionospheric scintillation on transit satellite measurement of total electron content;Knepp;Radio Sci.,2004

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3. Phase fluctuations model for EM wave propagation through solar scintillation at superior solar conjunction;Waves in Random and Complex Media;2016-08-31