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1. Identity statement
Reference TypeJournal Article
Sitemtc-m16c.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier6qtX3pFwXQZ3P8SECKy/CUaAj
Repositorysid.inpe.br/jeferson/2004/07.28.12.50   (restricted access)
Last Update2006:06.14.04.09.58 (UTC) administrator
Metadata Repositorysid.inpe.br/jeferson/2004/07.28.12.50.08
Metadata Last Update2018:06.04.04.12.54 (UTC) administrator
Secondary KeyINPE-11203-PRE/6652
ISSN0016-7169
Citation KeyEcherSchuMakiOkan:2004:ObBrSo
TitleObservations of broadband solar UV-A irradiance at Santa Maria, Brazil (29°S, 53° W)
Year2004
MonthJan.-Mar.
Access Date2024, Apr. 28
Secondary TypePRE PN
Number of Files1
Size684 KiB
2. Context
Author1 Echer, Ezequiel
2 Schuch, Nelson Jorge
3 Makita, K.
4 Okano, S.
Resume Identifier1 8JMKD3MGP5W/3C9JH3D
2 8JMKD3MGP5W/3C9JHUD
Group1 DGE-INPE-MCT-BR
2 RSU-INPE-MCT-BR
Affiliation1 Instituto Nacional de Pesquisas Espaciais
2 Centro Regional Sul de Pesquisas Espaciais, CRSPE/INPE
3 Takushoku University - Tokyo
4 National Institute of Polar Research, Tokyo
JournalGeofísica Internacional
Volume43
Number1
Pages53-59
History (UTC)2006-03-17 17:05:58 :: marciana -> administrator ::
2006-09-27 21:33:22 :: administrator -> marciana ::
2008-05-02 16:20:26 :: marciana -> administrator ::
2018-06-04 04:12:54 :: administrator -> marciana :: 2004
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
KeywordsSolar radiation
solar UV
atmosphere
atmospheric radiative transfer
AbstractObservations of broadband solar UV-A irradiance (320-400 nm) were made at Santa Maria, Brazil (29° S, 53° W) between September 1993 and December 1996. Two different measurement techniques were used, the direct sun (DS) with the sensor pointed directly to the sun, and the zenith sky (ZS), with the sensor pointed to the zenith. The seasonal variation of UV-A DS and ZS irradiances measured at local noon is analysed. Both UV-A DS and ZS irradiances have a strong seasonal variability, anticorrelated to the solar zenith angle variation. It is shown that UV-A ZS irradiance has a larger seasonal variation than UV-A DS irradiance, with summer/winter ratios of 3.4 for UV-A ZS and 1.4 for UV-A DS. This difference is explained because of the geometrical arrangement of the observations; UV-A DS irradiance is easured tracking the sun and its variability is due to the atmospheric optical path variation during the year. UV-A ZS irradiance is diffuse irradiance measured pointing at a fixed direction, the zenith, and besides the atmospheric optical path variability, the component of direct irradiance incident on the horizontal surface has also a variation with solar zenith angle. Analysing UV-A DS and ZS irradiances versus solar zenith angle, it was observed that UV-A ZS decreases faster with higher solar zenith angles than UV-A DS. Calculations using Beers law at 370 nm were made and show similar behaviour for irradiances at a horizontal surface, compared to UV-A ZS, and at a surface perpendicular to the solar beam, compared to UV-A DS irradiance.
AreaCEA
Arrangement 1urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > Observations of broadband...
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4. Conditions of access and use
Languageen
Target FileEcher1.pdf
User Groupadministrator
alexandra
marciana
Visibilityshown
Copy HolderSID/SCD
Archiving Policydenypublisher denyfinaldraft
Read Permissiondeny from all and allow from 150.163
5. Allied materials
Next Higher Units8JMKD3MGPCW/3EU29DP
8JMKD3MGPCW/3EUFCFP
DisseminationWEBSCI; PORTALCAPES; AGU.
Host Collectionsid.inpe.br/mtc-m18@80/2008/03.17.15.17
6. Notes
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