Please use this identifier to cite or link to this item: http://nopr.niscpr.res.in/handle/123456789/36775
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dc.contributor.authorSingh, Darshan-
dc.contributor.authorSomal, H S-
dc.contributor.authorDhillon, G S-
dc.contributor.authorGurm, H S-
dc.contributor.authorDuita, H N-
dc.contributor.authorSarkar, S K-
dc.contributor.authorReddy, B M-
dc.date.accessioned2016-11-04T07:14:30Z-
dc.date.available2016-11-04T07:14:30Z-
dc.date.issued1982-02-
dc.identifier.issn0975-105X (Online); 0367-8393 (Print)-
dc.identifier.urihttp://nopr.niscair.res.in/handle/123456789/36775-
dc.description23-28en_US
dc.description.abstractTemperature inversions of several types have been observed over Patiala during initial phases of setting up of an acoustic echosonde in Aug 1980. Surface-based inversions and elevated layers have been observed to be predominantly nighttime phenomena. The thickness of the surface-based inversion is found to be around 100 m while the elevated layers have thickness varying from 20 to 180 m with a peak of occurrence between 30 and 60 m. The surface-based layer rises after sunrise. The total structure in the morning is found to be correlated with radiosonde observations. The water vapour in the atmosphere seems to play a role in controlling the thickness and intensity of the surface-based inversions.en_US
dc.language.isoen_USen_US
dc.publisherNISCAIR-CSIR, Indiaen_US
dc.rights CC Attribution-Noncommercial-No Derivative Works 2.5 Indiaen_US
dc.sourceIJRSP Vol.11(1) [February 1982]en_US
dc.titleTemperature Inversions in the Planetary Boundary Layeren_US
dc.typeArticleen_US
Appears in Collections:IJRSP Vol.11(1) [February 1982]

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