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http://nopr.niscpr.res.in/handle/123456789/36775Full metadata record
| DC Field | Value | Language |
|---|---|---|
| dc.contributor.author | Singh, Darshan | - |
| dc.contributor.author | Somal, H S | - |
| dc.contributor.author | Dhillon, G S | - |
| dc.contributor.author | Gurm, H S | - |
| dc.contributor.author | Duita, H N | - |
| dc.contributor.author | Sarkar, S K | - |
| dc.contributor.author | Reddy, B M | - |
| dc.date.accessioned | 2016-11-04T07:14:30Z | - |
| dc.date.available | 2016-11-04T07:14:30Z | - |
| dc.date.issued | 1982-02 | - |
| dc.identifier.issn | 0975-105X (Online); 0367-8393 (Print) | - |
| dc.identifier.uri | http://nopr.niscair.res.in/handle/123456789/36775 | - |
| dc.description | 23-28 | en_US |
| dc.description.abstract | Temperature 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.iso | en_US | en_US |
| dc.publisher | NISCAIR-CSIR, India | en_US |
| dc.rights | CC Attribution-Noncommercial-No Derivative Works 2.5 India | en_US |
| dc.source | IJRSP Vol.11(1) [February 1982] | en_US |
| dc.title | Temperature Inversions in the Planetary Boundary Layer | en_US |
| dc.type | Article | en_US |
| Appears in Collections: | IJRSP Vol.11(1) [February 1982] | |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| IJRSP 11(1) 23-28.pdf | 2.14 MB | Adobe PDF | View/Open |
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