1. Identity statement | |
Reference Type | Conference Paper (Conference Proceedings) |
Site | mtc-m21c.sid.inpe.br |
Holder Code | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
Identifier | 8JMKD3MGP3W34R/3TKKPM8 |
Repository | sid.inpe.br/mtc-m21c/2019/07.10.12.55 |
Metadata Repository | sid.inpe.br/mtc-m21c/2019/07.10.12.55.47 |
Metadata Last Update | 2020:01.06.11.42.16 (UTC) administrator |
Secondary Key | INPE--PRE/ |
Citation Key | ArrasMosResWicKep:2019:InSoCy |
Title | The Influence of the Solar Cycle on Global Sporadic E Parameters |
Year | 2019 |
Access Date | 2024, May 16 |
Secondary Type | PRE CI |
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2. Context | |
Author | 1 Arras, C. 2 Mosna, Z. 3 Resende, Laysa Cristina Araújo 4 Wickert, J. 5 Kepkar, A. |
Group | 1 2 3 DIDAE-CGCEA-INPE-MCTIC-GOV-BR |
Affiliation | 1 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 Name | IUGG General Assembly, 27 |
Conference Location | Montréal, Canada |
Date | 08-18 July |
History (UTC) | 2019-07-10 12:55:47 :: simone -> administrator :: 2020-01-06 11:42:16 :: administrator -> simone :: 2019 |
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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 |
Abstract | GPS 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. |
Area | CEA |
Arrangement | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAE > The Influence of... |
doc Directory Content | there are no files |
source Directory Content | there are no files |
agreement Directory Content | |
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4. Conditions of access and use | |
User Group | simone |
Visibility | shown |
Update Permission | not transferred |
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5. Allied materials | |
Next Higher Units | 8JMKD3MGPCW/3ETL868 |
Host Collection | urlib.net/www/2017/11.22.19.04 |
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6. Notes | |
Empty Fields | archivingpolicy archivist booktitle callnumber copyholder copyright creatorhistory descriptionlevel dissemination doi e-mailaddress edition editor electronicmailaddress format isbn issn keywords label language lineage mark mirrorrepository nextedition notes numberoffiles numberofvolumes orcid organization pages parameterlist parentrepositories previousedition previouslowerunit progress project publisher publisheraddress readergroup readpermission resumeid rightsholder schedulinginformation secondarydate secondarymark serieseditor session shorttitle size sponsor subject targetfile tertiarymark tertiarytype type url versiontype volume |
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7. Description control | |
e-Mail (login) | simone |
update | |
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