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1. Identity statement
Reference TypeConference Paper (Conference Proceedings)
Sitemtc-m21c.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34R/3TKKPM8
Repositorysid.inpe.br/mtc-m21c/2019/07.10.12.55
Metadata Repositorysid.inpe.br/mtc-m21c/2019/07.10.12.55.47
Metadata Last Update2020:01.06.11.42.16 (UTC) administrator
Secondary KeyINPE--PRE/
Citation KeyArrasMosResWicKep:2019:InSoCy
TitleThe Influence of the Solar Cycle on Global Sporadic E Parameters
Year2019
Access Date2024, May 16
Secondary TypePRE CI
2. Context
Author1 Arras, C.
2 Mosna, Z.
3 Resende, Laysa Cristina Araújo
4 Wickert, J.
5 Kepkar, A.
Group1
2
3 DIDAE-CGCEA-INPE-MCTIC-GOV-BR
Affiliation1 GFZ Potsdam
2 Institute of Atmospheric Physics, Aeronomy, Prague, Czech Republic
3 Instituto Nacional de Pesquisas Espaciais (INPE)
4 GFZ Potsdam
5 GFZ Potsdam
Conference NameIUGG General Assembly, 27
Conference LocationMontréal, Canada
Date08-18 July
History (UTC)2019-07-10 12:55:47 :: simone -> administrator ::
2020-01-06 11:42:16 :: administrator -> simone :: 2019
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
AbstractGPS radio occultation measurements are used to observe the occurrence and the intensity of sporadic E layers on a global scale. We analysed data acquired by the FORMOSAT-3/COSMIC satellites. Since their launch in April 2006, the satellites collected about 6 million of globally distributed radio occultation profiles. For our study, we use ionosonde data at midlatitude and low latitude stations as well as Signal-to-Noise Ratio (SNR) GPS L1 radio occultation profiles. The SNR is sensitive to vertical changes in the electron density which is reflected in large fluctuations in the according altitude range of the profile. Therefore, vertically thin ionospheric phenomena like sporadic E layers can easily be identified using numerical filtering techniques. Currently, the radio occultation time series comprises 12 years covering approximately one solar cycle. In this study, we will focus on variations in sporadic E occurrence and intensity in line with the solar cycle. We will show global results, which indicate significant differences between different latitudes. Generally, we observe an indirect correlation between sporadic E and the solar cycle which is most clearly visible in the magnetic equator region.
AreaCEA
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Visibilityshown
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/3ETL868
Host Collectionurlib.net/www/2017/11.22.19.04
6. Notes
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