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1. Identity statement
Reference TypeConference Paper (Conference Proceedings)
Sitemtc-m21c.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34R/44D566S
Repositorysid.inpe.br/mtc-m21c/2021/03.25.14.19
Metadata Repositorysid.inpe.br/mtc-m21c/2021/03.25.14.19.04
Metadata Last Update2022:04.03.22.39.46 (UTC) administrator
Secondary KeyINPE--PRE/
Citation KeyBagestonGiKlPeWrGoTa:2021:MeTeOv
TitleMesospheric temperature over Comandante Ferraz Antarctic Station from 2005 to 2007
Year2021
Access Date2024, May 09
Secondary TypePRE CN
2. Context
Author1 Bageston, José Valentin
2 Giongo, G. A.
3 Klipp, Telmo dos Santos
4 Petry, Adriano
5 Wrasse, Cristiano Max
6 Gobbi, Delano
7 Takahashi, Hisao
Resume Identifier1
2
3
4
5
6 8JMKD3MGP5W/3C9JGTE
7 8JMKD3MGP5W/3C9JHCM
Group1 COESU-CGGO-INPE-MCTI-GOV-BR
2
3 COESU-CGGO-INPE-MCTI-GOV-BR
4 COESU-CGGO-INPE-MCTI-GOV-BR
5 DICEP-CGCE-INPE-MCTI-GOV-BR
6 DICEP-CGCE-INPE-MCTI-GOV-BR
7 DIHPA-CGCE-INPE-MCTI-GOV-BR
Affiliation1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 Universidade Federal de Santa Maria (UFSM)
3 Instituto Nacional de Pesquisas Espaciais (INPE)
4 Instituto Nacional de Pesquisas Espaciais (INPE)
5 Instituto Nacional de Pesquisas Espaciais (INPE)
6 Instituto Nacional de Pesquisas Espaciais (INPE)
7 Instituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Address1 jose.bageston@inpe.br
2
3
4 adriano.petry@inpe.br
5 cristiano.wrasse@inpe.br
6 delano.gobbi@uol.com.br
Conference NameSimpósio Brasileiro de Geofísica Espacial e Aeronomia, 8 (SBGEA)
Conference LocationOnline
Date22-26 mar.
History (UTC)2021-03-25 14:19:04 :: simone -> administrator ::
2021-06-22 19:11:15 :: administrator -> simone :: 2021
2021-06-22 21:05:33 :: simone -> administrator :: 2021
2022-04-03 22:39:46 :: administrator -> simone :: 2021
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
AbstractThe mesospheric temperature around the peak of the OH emission layer (∼87 km height) is very changeable and, as it is located at altitudes where the atmospheric density is very low, this temperature is more sensitive to the global changes then the temperatures in the lower atmosphere (troposphere). An airglow spectral imager with a filter for the OH (6-2) emission band (8362 to 8470 ˚A) was installed at Comandante Ferraz Station (62.1oS, 58.4oW) on May of 2005, and operated successfully until late winter 2007. Until now these data have not been analyzed yet and neither compared to other temperature methods for the upper mesosphere. The present work investigates these observations, including some examples of nocturnal time series of OH rotational temperature, and comparisons of coincident measurements of the ground-based technique (analyses of relative intensities of airglow lines) with satellite data around Ferraz station (radius<600 km). Two satellite instruments have been used, which are the SABER and MLS. The temperature averaged between 3 km below and 3 km above the OH peak. The standard deviation of the mean temperature profiles, considering the radius around the station and the time of each pass during the night, will be considered, and the ground-based instrument error and an hourly mean standard deviation will be used to check how close are the temperatures, and also verify whether the time series of consecutive days are consistent in terms of temperature trends (day-to-day variability). Preliminary results have shown that the temperatures are quite distinct in terms of absolute values, probably due to the distances of the satellite measurement points from the observatory and other factors (such as methodologies). The error bars of both measurements cross one another several times, and the day-to-day variability is consistent between the ground-based instrument and the satellite instruments.
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Arrangement 1urlib.net > BDMCI > Fonds > Produção a partir de 2021 > CGCE > Mesospheric temperature over...
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Languageen
User Groupsimone
Reader Groupadministrator
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Visibilityshown
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/46KTFK8
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Host Collectionurlib.net/www/2017/11.22.19.04
6. Notes
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