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dc.contributor.authorNaja, Manish-
dc.contributor.authorLal, Shyam-
dc.date.accessioned2016-10-04T09:49:53Z-
dc.date.available2016-10-04T09:49:53Z-
dc.date.issued1997-12-
dc.identifier.issn0975-105X (Online); 0367-8393 (Print)-
dc.identifier.urihttp://nopr.niscair.res.in/handle/123456789/35536-
dc.description312-318en_US
dc.description.abstractMeasurements 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.isoen_USen_US
dc.publisherNISCAIR-CSIR, Indiaen_US
dc.rights CC Attribution-Noncommercial-No Derivative Works 2.5 Indiaen_US
dc.sourceIJRSP Vol.26(6) [December 1997]en_US
dc.titleSolar eclipse induced changes in surface ozone at Ahmedabaden_US
dc.typeArticleen_US
Appears in Collections:IJRSP Vol.26(6) [December 1997]

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