1. Identity statement | |
Reference Type | Journal Article |
Site | mtc-m21b.sid.inpe.br |
Holder Code | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
Identifier | 8JMKD3MGP3W34P/3MRK48S |
Repository | sid.inpe.br/mtc-m21b/2016/11.22.19.52 (restricted access) |
Last Update | 2016:11.22.19.52.03 (UTC) simone |
Metadata Repository | sid.inpe.br/mtc-m21b/2016/11.22.19.52.04 |
Metadata Last Update | 2022:03.17.16.24.13 (UTC) administrator |
DOI | 10.1016/j.jastp.2016.10.005 |
ISSN | 1364-6826 |
Citation Key | EgitoAndrBati:2016:VeWiMo |
Title | Vertical winds and momentum fluxes due to equatorial planetary scale waves using all-sky meteor radar over Brazilian region |
Year | 2016 |
Month | Nov. |
Access Date | 2024, May 18 |
Type of Work | journal article |
Secondary Type | PRE PI |
Number of Files | 1 |
Size | 2134 KiB |
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2. Context | |
Author | 1 Egito, Fábio 2 Andrioli, Vânia de Fátima 3 Batista, Paulo Prado |
Resume Identifier | 1 2 3 8JMKD3MGP5W/3C9JJ3H |
Group | 1 2 CEA-CEA-INPE-MCTI-GOV-BR 3 DAE-CEA-INPE-MCTI-GOV-BR |
Affiliation | 1 Universidade Federal do Oeste da Bahia (UFOB) 2 Instituto Nacional de Pesquisas Espaciais (INPE) 3 Instituto Nacional de Pesquisas Espaciais (INPE) |
Author e-Mail Address | 1 fabio.egito@ufob.edu.br 2 vania.andrioli@inpe.br 3 paulo.batista@inpe.br |
Journal | Journal of Atmospheric and Solar-Terrestrial Physics |
Volume | 149 |
Pages | 108-119 |
Secondary Mark | A1_ENGENHARIAS_I A2_GEOCIÊNCIAS A2_ENGENHARIAS_III B1_INTERDISCIPLINAR B1_ENGENHARIAS_IV B1_BIODIVERSIDADE B2_ASTRONOMIA_/_FÍSICA C_CIÊNCIAS_BIOLÓGICAS_I |
History (UTC) | 2016-11-22 19:52:04 :: simone -> administrator :: 2016-11-22 19:52:04 :: administrator -> simone :: 2016 2016-11-22 19:52:32 :: simone -> administrator :: 2016 2016-12-06 19:38:02 :: administrator -> simone :: 2016 2016-12-23 14:04:53 :: simone -> administrator :: 2016 2017-01-09 13:59:35 :: administrator -> simone :: 2016 2017-01-09 15:29:08 :: simone -> administrator :: 2016 2022-03-17 16:24:13 :: administrator -> simone :: 2016 |
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3. Content and structure | |
Is the master or a copy? | is the master |
Content Stage | completed |
Transferable | 1 |
Content Type | External Contribution |
Version Type | publisher |
Keywords | Meteor radar Planetary scale waves Vertical wind |
Abstract | In the equatorial region planetary scale waves play an important role transporting significant amount of energy and momentum through atmosphere. Quantifying the momentum transported by these waves and its effects on the mean flow is rather important. Direct estimates of the momentum flux transported by waves require horizontal and vertical wind measurements. Ground-based meteor radars have provided continuous and reliable measurements of the horizontal wind components in the Mesosphere and Lower Thermosphere (MLT) region and have contributed to improve our knowledge of the dynamics of this region. However, instrumental limitations hinder its use for measuring vertical winds and momentum fluxes. On the other hand, according to Babu et al (2012), all- sky meteor radars are able to infer tridimensional winds when using a large number of meteor echoes centered at the meteor ablation peak. Following this approach, we have used measurements performed by a Meteor Radar installed at São João do Cariri, Brazil (7.4°S; 36.5°W) in order to measure vertical winds and calculate the momentum flux transported by equatorial planetary scale waves. In order to evaluate the accuracy of vertical wind values we have performed several tests based on a simple model considering real meteor distributions and theoretical equations for the MLT winds motion. From our tests, we inferred that Brazilian meteor radar data can be used for this purpose with an accuracy of ~ 1.8 m/s. The results show that the vertical wind presents magnitudes of a few meters per second and occasionally reaches magnitudes around 10 m/s. Below 92 km the vertical wind is predominantly upward during the whole year and above exhibits a semi-annual oscillation with downward phase during the equinoxes. Variations associated to planetary scale waves in the vertical wind are also observed and some of them appear simultaneously in the zonal and meridional wind as well. Largest wave induced amplitudes in the vertical wind are found in the 34 d band, reaching up to 4 m/s. From the vertical and zonal wind measurements, we calculated the vertical transport of zonal momentum in the 34 d band and found it to be maximum near autumn equinox, when its value reaches almost 20 m2/s2, while minimum momentum flux is observed after the winter solstice. |
Area | CEA |
Arrangement 1 | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAE > Vertical winds and... |
Arrangement 2 | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > CGCEA > Vertical winds and... |
doc Directory Content | access |
source Directory Content | there are no files |
agreement Directory Content | |
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4. Conditions of access and use | |
Language | en |
Target File | egito_vertical.pdf |
User Group | simone |
Reader Group | administrator simone |
Visibility | shown |
Archiving Policy | denypublisher denyfinaldraft24 |
Read Permission | deny from all and allow from 150.163 |
Update Permission | not transferred |
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5. Allied materials | |
Mirror Repository | urlib.net/www/2011/03.29.20.55 |
Next Higher Units | 8JMKD3MGPCW/3ETL868 8JMKD3MGPCW/3EU2FR5 |
Citing Item List | sid.inpe.br/bibdigital/2013/10.01.23.29 2 sid.inpe.br/bibdigital/2013/09.29.20.43 1 |
Dissemination | WEBSCI; PORTALCAPES; AGU; COMPENDEX; SCOPUS. |
Host Collection | sid.inpe.br/mtc-m21b/2013/09.26.14.25.20 |
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6. Notes | |
Empty Fields | alternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel e-mailaddress format isbn label lineage mark nextedition notes number orcid parameterlist parentrepositories previousedition previouslowerunit progress project rightsholder schedulinginformation secondarydate secondarykey session shorttitle sponsor subject tertiarymark tertiarytype url |
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7. Description control | |
e-Mail (login) | simone |
update | |
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