1. Identity statement | |
Reference Type | Journal Article |
Site | marte3.sid.inpe.br |
Holder Code | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
Identifier | 6qtX3pFwXQZ3r59YCT/GUKJ5 |
Repository | sid.inpe.br/iris@1905/2005/07.29.22.40.40 (restricted access) |
Last Update | 2013:04.02.11.34.01 (UTC) jefferson |
Metadata Repository | sid.inpe.br/iris@1905/2005/07.29.22.40.48 |
Metadata Last Update | 2018:06.06.04.03.54 (UTC) administrator |
Secondary Key | INPE-8328-PRE/4111 |
ISSN | 0273-1177 |
Label | 9299 |
Citation Key | TakahashiGoBaMeTeBu:1998:DyInEq |
Title | Dynamical influence on the equatorial airglow observed from the South American Sector |
Year | 1998 |
Secondary Date | 20010724 |
Access Date | 2024, May 02 |
Secondary Type | PRE PI |
Number of Files | 1 |
Size | 3981 KiB |
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2. Context | |
Author | 1 Takahashi, Hisao 2 Gobbi, Delano 3 Batista, Paulo Prado 4 Melo, S. M. L. 5 Teixeira, Nelson Rodrigues 6 Buriti, R. A. |
Group | 1 DAE-INPE-MCT-BR 2 DAE-INPE-MCT-BR 3 DAE-INPE-MCT-BR 4 5 DAE-INPE-MCT-BR |
Journal | Advances in Space Research |
Volume | 21 |
Number | 6 |
Pages | 817-825 |
History (UTC) | 2013-04-02 11:33:07 :: administrator -> jefferson :: 1998 2013-04-02 11:34:01 :: jefferson -> administrator :: 1998 2018-06-06 04:03:54 :: administrator -> marciana :: 1998 |
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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 | AERONOMIA America do Sul emissao atmosférica ondas mares luminescência atmosférica equatorial atmospheric emission tides (tidal oscillation) equatorial atmosphere airglow (atmosphere emission) |
Abstract | The upper atmospheric airglow emissions, OI 557.7 nm, NaD 589.3 nm, OH (9,4) and O2 atmospheric (0,1) bands and their rotational temperatures have been measured using ground-based multichannel airglow photometers, one located near the equator at Fortaleza (3.9 S, 38.4 W) and the other at low-middle latitude Cachoeira. Paulista (22.7 S, 45.0 W). Monthly averaged nocturnal variations calculated from the data from 1987 to 1993 were used to study the influence of atmospheric dynamical processes on these emissions. Harmonic analysis revealed that the Cachoeira Paulista data are mainly represented 12 hour period oscillation. Phase differences between the different emissions reveal that the vertical phase velocity is about 4 km/h and the vertical wavelength about 50 km. Fortaleza data on the other f. showed longer period, 24 hours, slow vertical propagation velocity, 1.1 km/h, and short veil wavelength, about 30 km. These facts lead us to conclude that the Cachoeira Paulista data are mainly controlled by the semidiurnal tidal oscillation and the Fortaleza data are controlled by the diurnal tide. |
Area | CEA |
Arrangement | Dynamical influence on... |
doc Directory Content | access |
source Directory Content | there are no files |
agreement Directory Content | there are no files |
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4. Conditions of access and use | |
Language | en |
Target File | 1-s2.0-S0273117798001112-main.pdf |
User Group | administrator jefferson |
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 | |
Next Higher Units | 8JMKD3MGPCW/3ETL868 |
Dissemination | WEBSCI; PORTALCAPES; MGA; COMPENDEX. |
Host Collection | sid.inpe.br/banon/2001/04.03.15.36 |
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6. Notes | |
Empty Fields | affiliation alternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel doi e-mailaddress electronicmailaddress format isbn lineage mark mirrorrepository month nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress project readergroup resumeid rightsholder schedulinginformation secondarymark session shorttitle sponsor subject tertiarymark tertiarytype typeofwork url |
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7. Description control | |
e-Mail (login) | marciana |
update | |
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