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http://nopr.niscpr.res.in/handle/123456789/35536Full metadata record
| DC Field | Value | Language |
|---|---|---|
| dc.contributor.author | Naja, Manish | - |
| dc.contributor.author | Lal, Shyam | - |
| dc.date.accessioned | 2016-10-04T09:49:53Z | - |
| dc.date.available | 2016-10-04T09:49:53Z | - |
| dc.date.issued | 1997-12 | - |
| dc.identifier.issn | 0975-105X (Online); 0367-8393 (Print) | - |
| dc.identifier.uri | http://nopr.niscair.res.in/handle/123456789/35536 | - |
| dc.description | 312-318 | en_US |
| dc.description.abstract | Measurements of surface ozone and related gases were made at Ahmedabad was 79.2%. The diurnal increase in ozone concentration due to photo-oxidation of pollutants like CO, CH4 and non-methane hydrocarbons (NMHCs) observed on normal days after the sunrise was not observed until the time of maximum obscuration. In fact, there was a decrease in ozone concentration in the range of 18-21% at the maximum phase. Ozone levels were found to be lower even after the eclipse due to loss and delay in ozone production. The eclipse conditions were simulated in a photochemical box model which was used to calculate ozone changes. The model shows a decrease of ozone by about 16% as compared to a control day at the time of maximum obscuration. The model also shows significant role of boundary layer variations in the morning hours. | 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.26(6) [December 1997] | en_US |
| dc.title | Solar eclipse induced changes in surface ozone at Ahmedabad | en_US |
| dc.type | Article | en_US |
| Appears in Collections: | IJRSP Vol.26(6) [December 1997] | |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| IJRSP 26(6) 312-318.pdf | 544.79 kB | Adobe PDF | View/Open |
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