Deterministic retrieval of ionopsheric phase screen from amplitude scintillations

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dc.contributor.author Bhattacharyya, A.
dc.date.accessioned 2015-05-13T10:13:42Z
dc.date.accessioned 2021-02-12T09:47:56Z
dc.date.available 2015-05-13T10:13:42Z
dc.date.available 2021-02-12T09:47:56Z
dc.date.issued 1999
dc.identifier.citation Radio Science, v.34/1,p.229-240, 1999. en_US
dc.identifier.uri http://localhost:8080/xmlui/handle/123456789/69
dc.description.abstract In the phase screen theory of ionospheric scintillations the ionospheric irregularities are considered as pure phase objects, and the diffraction pattern produced on the ground, by radio waves propagating through this phase screen, is obtained from conventional Fresnel diffraction theory. In the present paper the inverse problem of retrieving phase variations in the screen from the diffraction pattern on the ground is treated by using the transport-of-intensity equation (TIE), which is derived from the Fresnel diffraction theory result. An approximate version of the TIE is solved to obtain the phase variation in the screen from the intensity distribution on the ground. It is seen that when the phase variations involve spatial scale lengths ∼400 m, phase fluctuations of ∼5 rad can be recovered from intensity variations on the ground, for a 300-MHz signal. For larger spatial scale lengths and higher frequencies this method can be used to retrieve larger phase variations in the screen. en_US
dc.language.iso en en_US
dc.subject Ionosphere en_US
dc.subject Radio science en_US
dc.subject Scintillations en_US
dc.subject Transport-of-intensity equation en_US
dc.title Deterministic retrieval of ionopsheric phase screen from amplitude scintillations en_US
dc.type Article en_US
dc.identifier.accession 090559


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