Close

1. Identity statement
Reference TypeJournal Article
Sitemtc-m16.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier6qtX3pFwXQZGivnJVY/LsoHL
Repositorysid.inpe.br/mtc-m16@80/2006/06.14.18.16   (restricted access)
Last Update2006:06.14.18.16.19 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m16@80/2006/06.14.18.16.20
Metadata Last Update2021:07.18.04.01.22 (UTC) administrator
Secondary KeyINPE--13780-PRE/8966
ISSN1364-6826
Citation KeyWrasseSAANTTMTGS:2006:ReRaTr
TitleReverse ray tracing of the mesospheric gravity waves observed at 23°S (Brazil) and 7°S (Indonesia) in airglow imagers
Year2006
MonthJan.
Access Date2024, Apr. 27
Secondary TypePRE PI
Number of Files1
Size1140 KiB
2. Context
Author 1 Wrasse, Cristiano Max
 2 Suratno, E.
 3 Admiranto, A. G.
 4 Achmad, E.
 5 Nakamura, T.
 6 Tsuda, T.
 7 Takahashi, Hisao
 8 Medeiros, A. F.
 9 Taylor, M. J.
10 Gobbi, Delano
11 Salatum, A.
Resume Identifier 1
 2
 3
 4
 5
 6
 7 8JMKD3MGP5W/3C9JHCM
 8
 9
10 8JMKD3MGP5W/3C9JGTE
Group 1 DAE-INPE-MCT-BR
 2 DAE-INPE-MCT-BR
 3 DAE-INPE-MCT-BR
Affiliation 1 Instituto Nacional de Pesquisas Espaciais, Divisão de Aeronomia (INPE/DAE)
 2 Space Science Center, National Institute of Aeronautics and Space
 3 Space Science Center, National Institute of Aeronautics and Space
 4 Space Science Center, National Institute of Aeronautics and Space
 5 Research Institute for Sustainable Humanosphere (RISH)
 6 Research Institute for Sustainable Humanosphere (RISH)
 7 Instituto Nacional de Pesquisas Espaciais, Divisão de Aeronomia (INPE/DAE)
 8 Universidade Federal de Campina Grande (UFCG)
 9 Space Dynamics Laboratory and Physics Department, Utah State University
10 Instituto Nacional de Pesquisas Espaciais, Divisão de Aeronomia (INPE/DAE)
11 Space Science Center, National Institute of Aeronautics and Space
JournalJournal of Atmospheric and Solar-Terrestrial Physics
Volume68
Number2
Pages163-181
History (UTC)2006-06-14 18:16:20 :: simone -> administrator ::
2021-07-18 04:01:22 :: administrator -> marciana :: 2006
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
KeywordsGravity waves
Ray tracing
Mesosphere
Sources
Troposphere
Airglow
MIDDLE ATMOSPHERE
RADAR OBSERVATIONS
MESOSCALE VARIABILITY
NIGHTGLOW EMISSIONS
CACHOEIRA-PAULISTA
JET-STREAM
OH AIRGLOW
WIND
PROPAGATION
TIDES
AbstractGravity wave observations using all-sky CCD imager to measure the airglow OH, 02, and 01 emissions were made at Cachoeira Paulista (22.7 degrees S, 45 degrees W) (CP), at the low-middle latitude in Brazil, from October 1998 to September 1999. Near the equator, at Tanjungsari observatory (6.9 degrees S, 107.9 degrees E) (TJS), Indonesia, another wide angle CCD imager measuring the OH airglow emission layer has been operated from September 2000 to September 2001. With these data sets, a reverse ray tracing method was used to study propagation of gravity waves through the middle atmosphere and to estimate the source region. The CIRA-86 reference zonal wind and temperature models and the GSWM-02 tidal wind model were used in the present analysis. Both observation sites showed apparently similar wave characteristics, except for the horizontal phase speed.. which was much faster in the equatorial region. From the inverse ray tracing calculations, it was found that at CP, only about 15% of the wave events originated in the troposphere. Most of the events were located over the continent within an area of less than 400 km from the observation site. The identified source region in the troposphere showed a seasonal anisotropy, being mainly to the northwest of CP during summer and to the southeast and northwest in winter. This corresponds to the region of high tropospheric convection activity in the South American continent during summer and high meteorological front activity on the southwestern side during winter. At CP more than 70% of the waves showed that the ray tracing paths stopped in the mesosphere. At TJS the ray tracing indicates that 60% of the gravity wave sources might be located in the troposphere with an area of less than 200 km from the observation site, much closer than the case of CP. This corresponds to convective cloud activities on the north and northwest side of TJS. However, during southern hemisphere summer at both observation sites, most of the ray tracing paths stopped at the mesosphere owing to a condition of m(2) < 0 or critical level interactions. (c) 2005 Elsevier Ltd. All rights reserved.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAE > Reverse ray tracing...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Contentthere are no files
4. Conditions of access and use
Languageen
Target FileReverse ray tracing of the mesospheric gravity waves.pdf
User Groupadministrator
simone
Visibilityshown
Copy HolderSID/SCD
Archiving Policydenypublisher denyfinaldraft24
Read Permissiondeny from all and allow from 150.163
Update Permissiontransferred to simone
5. Allied materials
Next Higher Units8JMKD3MGPCW/3ETL868
DisseminationWEBSCI; PORTALCAPES; AGU; MGA; COMPENDEX.
Host Collectionsid.inpe.br/banon/2003/08.15.17.40
6. Notes
Empty Fieldsalternatejournal archivist callnumber copyright creatorhistory descriptionlevel doi e-mailaddress electronicmailaddress format isbn label lineage mark mirrorrepository nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress project readergroup rightsholder schedulinginformation secondarydate secondarymark session shorttitle sponsor subject tertiarymark tertiarytype typeofwork url versiontype
7. Description control
e-Mail (login)marciana
update 


Close