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Characteristics of black carbon over Delhi and Manora Peak – a comparative study

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dc.contributor.author Srivastava, A. K.
dc.contributor.author Singh, S.
dc.contributor.author Pant, P.
dc.contributor.author Dumka, U. C.
dc.date.accessioned 2015-05-01T07:24:17Z
dc.date.available 2015-05-01T07:24:17Z
dc.date.issued 2012
dc.identifier.uri http://hdl.handle.net/123456789/1048
dc.description.abstract The characteristics of aerosol black carbon (BC) were studied at two different climatic regimes, i.e. Delhi and Manora Peak during winter and spring of 2007. Spring BC was found to be ∼59% lower at Delhi and ∼23% higher at Manora Peak than their corresponding winter BC. Diurnal BC variation showed two enhanced peaks at Delhi (morning and night) whereas a single late afternoon peak at Manora Peak. Delhi BC showed a clear correlation with prevailing winds whereas no correlation was observed at Manora Peak. The major contribution of BC at Manora Peak can be expected from biomass burning while at Delhi fossil fuel dominates. Copyright ©2012 Royal Meteorological Society. en_US
dc.language.iso en_US en_US
dc.relation.ispartofseries asl13-223
dc.subject Black carbon; emission sources; boundary layer; wind speed; urban; Himalayan foothills en_US
dc.title Characteristics of black carbon over Delhi and Manora Peak – a comparative study en_US
dc.type Article en_US


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