Comparative analysis of radio occultation processing approaches based on Fourier integral operators

We analyze and compare two approaches to processing radio occultation data: (1) canonical transform method and (2) full spectrum inversion method. We show that these methods are closely related and can be explained from two view points: (1) both methods apply a Fourier transform like operator to the...

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Bibliographic Details
Published in:Radio science Vol. 39; no. 6; pp. RS6004 - n/a
Main Authors: Gorbunov, M. E., Benzon, H.-H., Jensen, A. S., Lohmann, M. S., Nielsen, A. S.
Format: Journal Article
Language:English
Published: American Geophysical Union 01-12-2004
Blackwell Publishing Ltd
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Summary:We analyze and compare two approaches to processing radio occultation data: (1) canonical transform method and (2) full spectrum inversion method. We show that these methods are closely related and can be explained from two view points: (1) both methods apply a Fourier transform like operator to the entire radio occultation signal, and the derivative of the phase of the transformed signal is used for the computation of bending angles, and (2) they can be explained from a signal processing view point as the location of multiple tones constituting the complete signal. The full spectrum inversion method is a composition of phase correction and Fourier transform, which makes the numerical algorithm computationally more efficient as compared to the canonical transform method. We investigate the relative performance of the two methods in simulations using a wave optics propagator. We use simple analytical models of the atmospheric refractivity as well as radiosonde data in order to reproduce complex multipath situations. The numerical simulations as well as the analytical estimations indicate that a resolution of 60 m (or even higher) can be achieved.
Bibliography:ark:/67375/WNG-X5NL1VDZ-5
istex:17034E25374F4DEAC0C856E588B744F3D0E05A8E
ArticleID:2003RS002916
ObjectType-Article-2
SourceType-Scholarly Journals-1
ObjectType-Feature-1
content type line 23
ISSN:0048-6604
1944-799X
DOI:10.1029/2003RS002916