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Atmospheric Brown Clouds in the Himalayas: first two years of continuous observations at the Nepal Climate Observatory-Pyramid (5079 m).

Authors :
Bonasoni, P.
Laj, P.
Marinoni, A.
Sprenger, M.
Angelini, F.
Arduini, J.
Bonafè, U.
Calzolari, F.
Colombo, T.
Decesari, S.
Di Biagio, C.
di Sarra, A. G.
Evangelisti, F.
Duchi, R.
Facchini, M. C.
Fuzzi, S.
Gobbi, G. P.
Maione, M.
Panday, A.
Roccato, F.
Source :
Atmospheric Chemistry & Physics; 2010, Vol. 10 Issue 15, p7515-7531, 17p, 2 Color Photographs, 2 Charts, 9 Graphs
Publication Year :
2010

Abstract

This paper provides a detailed description of the atmospheric conditions characterizing the high Himalayas, thanks to continuous observations begun in March 2006 at the Nepal Climate Observatory-Pyramid (NCO-P) located at 5079ma.s.l. on the southern foothills of Mt. Everest, in the framework of ABC-UNEP and SHARE-Ev-K2-CNR projects. The work presents a characterization of meteorological conditions and air-mass circulation at NCO-P during the first two years of activity. The mean values of atmospheric pressure, temperature and wind speed recorded at the site were: 551 hPa, -3.0 °C, 4.7ms<superscript>-1</superscript>, respectively. The highest seasonal values of temperature (1.7 °C) and relative humidity (94%) were registered during the monsoon season, which was also characterized by thick clouds, present in about 80% of the afternoon hours, and by a frequency of cloud-free sky of less than 10%. The lowest temperature and relative humidity seasonal values were registered during winter, -6.3 °C and 22%, respectively, the season being characterised by mainly cloud-free sky conditions and rare thick clouds. The summer monsoon influenced rain precipitation (seasonal mean: 237 mm), while wind was dominated by flows from the bottom of the valley (S-SW) and upper mountain (N-NE). The atmospheric composition at NCO-P has been studied thanks to measurements of black carbon (BC), aerosol scattering coefficient, PM<subscript>1</subscript>, coarse particles and ozone. The annual behaviour of the measured parameters shows the highest seasonal values during the premonsoon (BC: 316.9 ngm<superscript>-3</superscript>, PM<subscript>1</subscript>: 3.9 μgm<superscript>-3</superscript>, scattering coefficient: 11.9Mm<superscript>-1</superscript>, coarse particles: 0.37 cm<superscript>-3</superscript> and O<subscript>3</subscript>: 60.9 ppbv), while the lowest concentrations occurred during the monsoon (BC: 49.6 ngm<superscript>-3</superscript>, PM<subscript>1</subscript>: 0.6 μgm<superscript>-3</superscript>, scattering coefficient: 2.2Mm<superscript>-1</superscript>, and O<subscript>3</subscript>: 38.9 ppbv) and, for coarse particles, during the post-monsoon (0.07 cm<superscript>-3</superscript>). At NCO-P, the synoptic-scale circulation regimes present three principal contributions: Westerly, South-Westerly and Regional, as shown by the analysis of in-situ meteorological parameters and 5-day LAGRANTO back-trajectories. The influence of the brown cloud (AOD>0.4) extending over Indo-Gangetic Plains up to the Himalayan foothills has been evaluated by analysing the in-situ concentrations of the ABC constituents. This analysis revealed that brown cloud hot spots mainly influence the South Himalayas during the pre-monsoon, in the presence of very high levels of atmospheric compounds (BC: 1974.1 ngm<superscript>-3</superscript>, PM<subscript>1</subscript>: 23.5 μgm<superscript>-3</superscript>, scattering coefficient: 57.7Mm<superscript>-1</superscript>, coarse particles: 0.64 cm<superscript>-3</superscript>, O<subscript>3</subscript>: 69.2 ppbv, respectively). During this season 20% of the days were characterised by a strong brown cloud influence during the afternoon, leading to a 5-fold increased in the BC and PM<subscript>1</subscript> values, in comparison with seasonal means. Our investigations provide clear evidence that, especially during the pre-monsoon, the southern side of the high Himalayan valleys represent a "direct channel" able to transport brown cloud pollutants up to 5000ma.s.l., where the pristine atmospheric composition can be strongly influenced. [ABSTRACT FROM AUTHOR]

Details

Language :
English
ISSN :
16807316
Volume :
10
Issue :
15
Database :
Complementary Index
Journal :
Atmospheric Chemistry & Physics
Publication Type :
Academic Journal
Accession number :
53171618
Full Text :
https://doi.org/10.5194/acp-10-7515-2010