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Microwave Propagation and Troposphere: Eclipse Time Observation

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dc.contributor.author Mishra, U
dc.contributor.author Sen, S
dc.contributor.author Sharma, S
dc.contributor.author Barbara, A. K
dc.contributor.author Devi, M
dc.date.accessioned 2005-01-28T11:14:16Z
dc.date.available 2005-01-28T11:14:16Z
dc.date.issued 1997
dc.identifier.citation Kodaikanal Observatory Bulletins Series A, Vol. 13, pp. 217-220 en
dc.identifier.issn 0374-3632
dc.identifier.uri http://hdl.handle.net/2248/266
dc.description.abstract The effect of 24th October 1995 solar eclipse were studied on the reception of Latikor-Shillong and Nongpiur-Shillong links both operating at a frequency of 11GHz. The surface temperature, pressure and humidity were continuously recorded and the radio donde and SODAR observations are available during that period. These links (generally stable) showed an attenuation of 8dB during the maximum solar obscuration period (82%). The ratio refractive index gradient maintained a normal lapse rate during the initial phase of the eclipse, but with the progress of eclipse and during the maximum obscuration period, the gradient reflected development of sub-refractive conditions. The paper discusses the effects of refractive fading on microwave signal by eclipse included sub-refractive situation through a simple ray tracing model over the link path. en
dc.format.extent 80384 bytes
dc.format.mimetype application/pdf
dc.language.iso en
dc.publisher Indian Institute of Astrophysics, Bangalore en
dc.subject Solar eclipse en
dc.subject Microwave propagation en
dc.subject Radio refractive index en
dc.title Microwave Propagation and Troposphere: Eclipse Time Observation en
dc.type Article en


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