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  Understanding nighttime methane signals at the Amazon Tall Tower Observatory (ATTO)

Botia, S., Gerbig, C., Marshall, J., Lavric V, J., Walter, D., Pöhlker, C., et al. (2020). Understanding nighttime methane signals at the Amazon Tall Tower Observatory (ATTO). Atmospheric Chemistry and Physics, 20(11), 6583-6606. doi:10.5194/acp-20-6583-2020.

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Botia, Santiago1, Author
Gerbig, Christoph1, Author
Marshall, Julia1, Author
Lavric V, Jost1, Author
Walter, David1, Author
Pöhlker, Christopher2, Author           
Holanda, Bruna2, Author           
Fisch, Gilberto1, Author
de Araujo, Alessandro Carioca1, Author
Sa, Marta O.1, Author
Teixeira, Paulo R.1, Author
Resende, Angelica F.1, Author
Dias-Junior, Cleo Q.1, Author
van Asperen, Hella1, Author
Oliveira, Pablo S.1, Author
Stefanello, Michel1, Author
Acevedo, Otavio C.1, Author
Affiliations:
1external, ou_persistent22              
2Multiphase Chemistry, Max Planck Institute for Chemistry, Max Planck Society, ou_1826290              

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 Abstract: Methane (CH4) atmospheric mixing ratio measurements are analyzed for the period between June 2013 and November 2018 at the Amazon Tall Tower Observatory (ATTO). We describe the seasonal and diurnal patterns of nighttime events in which CH4 mixing ratios at the uppermost (79 m a.g.l.) inlet are significantly higher than the lowermost inlet (4 m a.g.l.) by 8 ppb or more. These nighttime events were found to be associated with a wind direction originating from the southeast and wind speeds between 2 and 5 m s−1. We found that these events happen under specific nighttime atmospheric conditions when compared to other nights, exhibiting less variable sensible heat flux, low net radiation and a strong thermal stratification above the canopy. Our analysis indicates that even at wind speeds of 5.8 m s−1 the turbulence intensity, given by the standard deviation of the vertical velocity, is suppressed to values lower than 0.3 m s−1. Given these findings, we suggest that these nighttime CH4 enhancements are advected from their source location by horizontal nonturbulent motions. The most likely source location is the Uatumã River, possibly influenced by dead stands of flooded forest trees that may be enhancing CH4 emissions from those areas. Finally, biomass burning and the Amazon River were discarded as potential CH4 sources.

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Language(s): eng - English
 Dates: 2020-06-05
 Publication Status: Issued
 Pages: -
 Publishing info: -
 Table of Contents: -
 Rev. Type: -
 Identifiers: ISI: 000538583100006
DOI: 10.5194/acp-20-6583-2020
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Title: Atmospheric Chemistry and Physics
  Abbreviation : ACP
Source Genre: Journal
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Publ. Info: Göttingen : Copernicus Publications
Pages: - Volume / Issue: 20 (11) Sequence Number: - Start / End Page: 6583 - 6606 Identifier: ISSN: 1680-7316
CoNE: https://pure.mpg.de/cone/journals/resource/111030403014016