Study of trends of total CO and CH4 contents over Eurasia through analysis of ground-based and satellite spectroscopic measurements
- Authors: Rakitin V.S.1, Elansky N.F.1, Pankratova N.V.1, Skorokhod A.I.1, Dzhola A.V.1, Shtabkin Y.A.1, Wang P.2, Wang G.2, Vasilieva A.V.1, Makarova M.V.3, Grechko E.I.1
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Affiliations:
- Obukhov Institute of Atmospheric Physics
- Institute of Atmospheric Physics
- St. Petersburg State University
- Issue: Vol 30, No 6 (2017)
- Pages: 517-526
- Section: Atmospheric Radiation, Optical Weather, and Climate
- URL: https://journals.rcsi.science/1024-8560/article/view/188204
- DOI: https://doi.org/10.1134/S1024856017060112
- ID: 188204
Cite item
Abstract
Trends of total CO and CH4 contents are estimated from satellite AIRS spectrometer data for the Eurasian domain (0–180° E, 0–85° N) for different time periods and seasons. The results are compared with similar estimates, obtained from ground-based spectroscopic measurements at seven stations of the European Network for the Detection of Atmospheric Composition Change (NDACC) and at measurement sites of the Institute of Atmospheric Physics, Russian Academy of Sciences (Zvenigorod Scientific Station (ZSS), Zotto, and Beijing) and St. Petersburg University (Peterhof), located in the study domain. Overall, the total CO decreased over northern Eurasia during the period of 2003–2015 at a rate of 0.05–1.5%/yr, depending on the region; while the total CH4 increased at a rate of 0.16–0.65%/yr. Since 2007, the total CO has been increased during summer and autumn months in most mid- and high-latitude Eurasian background regions, and the total CH4 growth has been accelerated. Changes in the global photochemical system, proceeding against the background of global climate change and, in particular, changes in the “sources/sinks” ratio for minor atmospheric admixtures are suggested as possible causes of this dynamic of trends of the atmospheric CO and CH4 contents.
About the authors
V. S. Rakitin
Obukhov Institute of Atmospheric Physics
Author for correspondence.
Email: vadim@ifaran.ru
Russian Federation, Moscow, 119017
N. F. Elansky
Obukhov Institute of Atmospheric Physics
Author for correspondence.
Email: n.f.elansky@mail.ru
Russian Federation, Moscow, 119017
N. V. Pankratova
Obukhov Institute of Atmospheric Physics
Email: n.f.elansky@mail.ru
Russian Federation, Moscow, 119017
A. I. Skorokhod
Obukhov Institute of Atmospheric Physics
Email: n.f.elansky@mail.ru
Russian Federation, Moscow, 119017
A. V. Dzhola
Obukhov Institute of Atmospheric Physics
Email: n.f.elansky@mail.ru
Russian Federation, Moscow, 119017
Yu. A. Shtabkin
Obukhov Institute of Atmospheric Physics
Email: n.f.elansky@mail.ru
Russian Federation, Moscow, 119017
P. Wang
Institute of Atmospheric Physics
Email: n.f.elansky@mail.ru
China, Beijing, 100029
G. Wang
Institute of Atmospheric Physics
Email: n.f.elansky@mail.ru
China, Beijing, 100029
A. V. Vasilieva
Obukhov Institute of Atmospheric Physics
Email: n.f.elansky@mail.ru
Russian Federation, Moscow, 119017
M. V. Makarova
St. Petersburg State University
Email: n.f.elansky@mail.ru
Russian Federation, Peterhof, 198504
E. I. Grechko
Obukhov Institute of Atmospheric Physics
Email: n.f.elansky@mail.ru
Russian Federation, Moscow, 119017
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