2000
DOI: 10.1029/1999gl011218
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Seasonal variations of HCN over northern Japan measured by ground‐based infrared solar spectroscopy

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Cited by 33 publications
(44 citation statements)
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“…Atmospheric mixing ratios of HCN in the range of 100-300 ppt were reported for springtime over the Pacific during TRACE-P (Singh et al, 2003), with somewhat higher concentrations found in biomass burning plumes. The in-situ measurements were in good agreement with the tropospheric column of HCN (4·10 15 cm −2 ) measured over Japan (Zhao et al, 2000). HCN-columns of 2-3·10 15 cm −2 obtained over Jungfraujoch and Mauna Loa (Rinsland et al, 1999(Rinsland et al, , 2000 would lead to similar tropospheric mixing ratios because of the higher altitude of the observatories.…”
Section: Convertersupporting
confidence: 73%
“…Atmospheric mixing ratios of HCN in the range of 100-300 ppt were reported for springtime over the Pacific during TRACE-P (Singh et al, 2003), with somewhat higher concentrations found in biomass burning plumes. The in-situ measurements were in good agreement with the tropospheric column of HCN (4·10 15 cm −2 ) measured over Japan (Zhao et al, 2000). HCN-columns of 2-3·10 15 cm −2 obtained over Jungfraujoch and Mauna Loa (Rinsland et al, 1999(Rinsland et al, , 2000 would lead to similar tropospheric mixing ratios because of the higher altitude of the observatories.…”
Section: Convertersupporting
confidence: 73%
“…The total column of CO is also measured at several locations around the world, with data collected at a few sites since the 1970s (Zander et al, 1989;Yurganov et al, 1997;Mahieu et al, 1997;Zhao et al, 2000;Rinsland et al, , 1999Rinsland et al, , 2000. This database provides the means with which to derive trends in observed CO and to evaluate model performance.…”
Section: Introductionmentioning
confidence: 99%
“…In 1994 the first measurements using the moon as a light source were reported from Spitzbergen, enabling measurements of the Arctic atmosphere during polar night (Notholt, 1994). In 1995 three additional sites were added to the network at Zugspitze, Germany (47°N, 11°E) (Sussmann and Schafer, 1997), Rikubetsu, Japan (44°N, 144°E) (Zhao et al, 2000) and Wollongong, Australia (34°S, 151°E) (Rinsland et al, 2001). The following year saw a further three sites established at Kiruna, Sweden, (68°N, 20°E) (Blumenstock et al, 1997), Eureka, Nunavit (80°N, 86°W) (Batchelor et al, 2009;Donovan et al, 1997) and Moshiri, Japan (44°N, 142°E) (Zhao et al, 2000).…”
Section: A Summary Of Past Successes For Ground-based Solar Fourier Tmentioning
confidence: 99%
“…In 1995 three additional sites were added to the network at Zugspitze, Germany (47°N, 11°E) (Sussmann and Schafer, 1997), Rikubetsu, Japan (44°N, 144°E) (Zhao et al, 2000) and Wollongong, Australia (34°S, 151°E) (Rinsland et al, 2001). The following year saw a further three sites established at Kiruna, Sweden, (68°N, 20°E) (Blumenstock et al, 1997), Eureka, Nunavit (80°N, 86°W) (Batchelor et al, 2009;Donovan et al, 1997) and Moshiri, Japan (44°N, 142°E) (Zhao et al, 2000). Measurements at Tsukuba, Japan (36°N, 140°E) started in 1998, followed by Thule, Greenland (77°N, 69°W), Poker Flat, Alaska (65°N, 147°W) and Izana, Tenerife Island (28°N, 16°W) all in 1999.…”
Section: A Summary Of Past Successes For Ground-based Solar Fourier Tmentioning
confidence: 99%
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