2013
DOI: 10.1051/e3sconf/20130127004
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First Measurements of Ambient Total Gaseous Mercury (TGM) at the EvK2CNR Pyramid Observatory in Nepal

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Cited by 6 publications
(2 citation statements)
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“…The mean concentration of TGM is slightly lower than the annual mean concentration at background sites in the Northern Hemisphere (1.55 ng m −3 in 2013 and 1.51 ng m −3 in 2014), and higher than those in the Southern Hemisphere (0.93 ng m −3 in 2013 and 0.97 ng m −3 in 2014) (Sprovieri et al, 2016). Comparable results were reported from EvK2CNR on the south slope of the Himalayas (1.2 ng m −3 , Gratz et al, 2013) and from tropical sites in the Global Mercury Observation System in the Northern Hemisphere (1.23 ng m −3 in 2013 and 1.22 ng m −3 in 2014) (Sprovieri et al, 2016). Compared to the three sites at the edge of the Tibetan Plateau (Mt.…”
Section: Tgm Concentrationsmentioning
confidence: 46%
“…The mean concentration of TGM is slightly lower than the annual mean concentration at background sites in the Northern Hemisphere (1.55 ng m −3 in 2013 and 1.51 ng m −3 in 2014), and higher than those in the Southern Hemisphere (0.93 ng m −3 in 2013 and 0.97 ng m −3 in 2014) (Sprovieri et al, 2016). Comparable results were reported from EvK2CNR on the south slope of the Himalayas (1.2 ng m −3 , Gratz et al, 2013) and from tropical sites in the Global Mercury Observation System in the Northern Hemisphere (1.23 ng m −3 in 2013 and 1.22 ng m −3 in 2014) (Sprovieri et al, 2016). Compared to the three sites at the edge of the Tibetan Plateau (Mt.…”
Section: Tgm Concentrationsmentioning
confidence: 46%
“…Generally, the GEM concentration in the QNNP was similar to the reported values in the Northern Hemisphere (∼ 1.5 to 1.7 ng m −3 ) and was higher than those found in the Southern Hemisphere (∼ 1.1 to 1.3 ng m −3 ) (Lindberg et al, 2007;Slemr et al, 2015;Venter et al, 2015;Sprovieri et al, 2016). Among the global Hg monitoring sites, the Ev-K2-CNR monitoring site on the southern slope of the Tibetan Plateau, Nepal, is the nearest station (at a straight-line distance of approximately 50 km) from the monitoring site used in this study (Gratz et al, 2013). The average GEM concentration at Ev-K2-CNR (1.2 ± 0.2 ng m −3 , from November 2011 to April 2012) was slightly lower than that in the QNNP (1.31 ± 0.42 ng m −3 during the PISM period and 1.44 ± 0.36 ng m −3 during the ISM period).…”
Section: Backward Trajectory Simulationmentioning
confidence: 99%