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8篇 您的检索式:作者名="Ghude"
    题名 作者 年代 出处 被引量
1Satellite Derived Trends in NOx over the Major Global Hotspot Regions during the Past Decade and Their Int er-cornparison显示文摘Ghude SO Van der A R J Beig G 2009Environmental Pollution2009,157,6:1
2Satellite derived trends in NO 2 over the major global hotspot regions during the past decade and their inter-comparison显示文摘Sachin D. Ghude R.J. Van der A G. Beig S. Fadnavis S.D. Polade 2009Environmental Pollution2009,,6:1
3Application of satellite observations for identifying regions of domi- nant sources of nitrogen oxides over the Indian Subcontinent 显示文摘GHUDE S D KULKARNI S H JENA C et O1 2013J Geophys Res Atmos2013,118,2:1
4Quantifying the effect of air quality control measures during the 2010 CommonwealthGames at Delhi, India 显示文摘Beig G Dilip M C Ghude S D 2013Atmospheric Environment2013,80,:1
5Satellite derived trends in NO2over the major global hotspot regions during the past decade and their inter-comparison显示文摘Ghude S D Van der A R J Beig G 2009Environmental Pollution2009,157,6:1
6Evaluating population exposure to environmental pollutants during deepavali fireworks displays using air quality measure- ments of the SAFAR network显示文摘BEIG G CHATE D M GHUDE S D 2013Chemosphere2013,92,1:1
7Cloud Condensation Nuclei over the Bay of Bengal during the Indian Summer Monsoon显示文摘The first measurements of cloud condensation nuclei(CCN) at five supersaturations were carried out onboard the research vessel 'Sagar Kanya'(cruise SK-296) from the south to the head-bay of the Bay of Bengal as part of the Continental Tropical Convergence Zone(CTCZ) Project during the Indian summer monsoon of 2012. In this paper, we assess the diurnal variation in CCN distributions at supersaturations from 0.2% to 1%(in steps of 0.2%) and the power-law fit at supersaturation of 1%.The diurnal pattern shows peaks in CCN concentration(NCCN) at supersaturations from 0.2% to 1% between 0600 and 0700 LST(local standard time, UTC+0530), with relatively low concentrations between 1200 and 1400 LST, followed by a peak at around 1800 LST. The power-law fit for the CCN distribution at different supersaturation levels relates the empirical exponent(k) of supersaturation(%) and the NCCNat a supersaturation of 1%. The NCCNat a supersaturation of 0.4% is observed to vary from 702 cm^(-3) to 1289 cm^(-3), with a mean of 961 ± 161 cm^(-3)(95% confidence interval), representing the CCN activity of marine air masses. Whereas, the mean NCCNof 1628 ± 193 cm^(-3) at a supersaturation of 1% is higher than anticipated for the marine background. When the number of CCN spectra is 1293, the value of k is 0.57 ± 0.03(99% confidence interval)and its probability distribution shows cumulative counts significant at k ≈ 0.55 ± 0.25. The results are found to be better at representing the features of the marine environment(103 cm^(-3) and k ≈ 0.5) and useful for validating CCN closure studies for Indian sea regions.D. M. CHATE R. T. WAGHMARE C. K. JENA V. GOPALAKRISHNAN P. MURUGAVEL Sachin D. GHUDE Rachana KULKARNI P. C. S. DEVARA 2018Advances in Atmospheric Sciences2018,35,2:1
8Modulation of Cy- clone tracks in the Bay of Bengal by QBO显示文摘Fadnavis S Chakraborty T Ghude S D 2011Journal of Atmos- pheric and Solar-Terrestrial Physics2011,73,13:1
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