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1. Identity statement
Reference TypeJournal Article
Sitemtc-m16.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier6qtX3pFwXQZGivnJVY/LErBc
Repositorysid.inpe.br/mtc-m16@80/2006/07.05.12.46   (restricted access)
Last Update2006:07.05.12.46.46 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m16@80/2006/07.05.12.46.47
Metadata Last Update2021:07.18.04.01.22 (UTC) administrator
Secondary KeyINPE--PRE/
ISSN1364-6826
Citation KeyClemeshaBati:2006:QuLoAt
TitleThe quantification of long-term atmospheric change via meteor ablation height measurements
Year2006
Access Date2024, Apr. 28
Secondary TypePRE PI
Number of Files1
Size644 KiB
2. Context
Author1 Clemesha, Barclay Robert
2 Batista, Paulo Prado
Resume Identifier1 8JMKD3MGP5W/3C9JGKH
2 8JMKD3MGP5W/3C9JJ3H
Group1 DAE-INPE-MCT-BR
2 DAE-INPE-MCT-BR
Affiliation1 Instituto Nacional de Pesquisas Especiais, Divisão de Aeronomia (INPE.DAE)
2 Instituto Nacional de Pesquisas Especiais, Divisão de Aeronomia (INPE.DAE)
JournalJournal of Atmospheric and Solar-Terrestrial Physics
VolumeIn Press
History (UTC)2006-07-05 12:46:47 :: simone -> administrator ::
2010-05-11 20:07:35 :: administrator -> simone ::
2011-05-25 10:50:55 :: 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
KeywordsGlobal trend
Meteor ablation height
Meteor radar
AbstractModern meteor radars, with peak pulse powers typically of the order of 10 kW, detect around 5000 meteors per day and determine the spatial coordinates and radial velocity of each meteor trail detected. This information is mainly used to determine horizontal winds at heights between about 80 and 100 km with a time resolution of about 1 h, adequate for the study of tides, planetary waves and prevailing winds. Since the detected meteor trails are accurately located in space, it is also possible to determine their mean height distribution. This height distribution depends on the meteor characteristics, in terms of distributions of size, velocity and entrance angle, and the vertical profile of atmospheric density in the height range in question. For sporadic meteors the meteor characteristics appear to depend only on local time, so the measured height distribution can, in principle, be used to obtain information on atmospheric density and its time variations on scales greater than one day. An analysis of more than 5 years of data acquired with a Skiymet meteor radar, installed at Cachoeira Paulista, Brazil (23°S, 45°W), shows the presence of planetary waves, seasonal and long-term variations in atmospheric density. Of particular interest is the potential of this technique for quantifying long-term changes in the atmosphere via ground-based measurements which should not be difficult to maintain over the long time periods required for global change studies.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAE > The quantification of...
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4. Conditions of access and use
Languageen
Target Filethe quantification a long term atmospheric.pdf
User Groupadministrator
simone
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5. Allied materials
Next Higher Units8JMKD3MGPCW/3ETL868
DisseminationWEBSCI; PORTALCAPES; AGU; MGA; COMPENDEX.
Host Collectionsid.inpe.br/banon/2003/08.15.17.40
6. Notes
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7. Description control
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