| 1. Identity statement | ||||
| Reference Type | Journal Article | |||
| Site | mtc-m21d.sid.inpe.br | |||
| Holder Code | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S | |||
| Identifier | 8JMKD3MGP3W34T/48APSC5 | |||
| Repository | sid.inpe.br/mtc-m21d/2023/01.04.17.11 (restricted access) | |||
| Last Update | 2023:01.04.17.11.13 (UTC) simone | |||
| Metadata Repository | sid.inpe.br/mtc-m21d/2023/01.04.17.11.13 | |||
| Metadata Last Update | 2023:01.10.17.38.29 (UTC) administrator | |||
| DOI | 10.1029/2022SW003243 | |||
| ISSN | 1542-7390 | |||
| Citation Key | SousasantosAfMoRoAbSaVa:2022:AmScSe | |||
| Title | Amplitude Scintillation Severity and Fading Profiles Under Alignment Between GPS Propagation Paths and Equatorial Plasma Bubbles  | |||
| Year | 2022 | |||
| Month | Nov. | |||
| Access Date | 2024, May 14 | |||
| Type of Work | journal article | |||
| Secondary Type | PRE PI | |||
| Number of Files | 1 | |||
| Size | 4536 KiB | |||
| 2. Context | ||||
| Author | 1 Sousasantos, J. 2 Affonso, B. J. 3 Moraes, A. 4 Rodrigues, F. S. 5 Abdu, Mangalathayil Ali 6 Salles, L. A. 7 Vani, B. C. | |||
| Resume Identifier | 1 2 3 4 5 8JMKD3MGP5W/3C9JHNK | |||
| ORCID | 1 0000-0001-6572-8009 2 0000-0002-7560-9625 3 0000-0002-6493-1694 4 0000-0002-3555-8165 5 0000-0001-5857-5761 6 7 0000-0002-4022-9227 | |||
| Group | 1 2 3 4 5 DIHPA-CGCE-INPE-MCTI-GOV-BR | |||
| Affiliation | 1 University of Texas at Dallas 2 Instituto Tecnológico de Aeronáutica (ITA) 3 Instituto de Aeronáutica e Espaço (IAE) 4 University of Texas at Dallas 5 Instituto Nacional de Pesquisas Espaciais (INPE) 6 Instituto Tecnológico de Aeronáutica (ITA) 7 Instituto Federal de Educação, Ciência e Tecnologia de São Paulo (IFSP) | |||
| Author e-Mail Address | 1 jonas.ssts@utdallas.edu | |||
| Journal | Space Weather | |||
| Volume | 20 | |||
| Number | 11 | |||
| Pages | e2022SW003243 | |||
| Secondary Mark | B1_INTERDISCIPLINAR B1_GEOCIÊNCIAS B2_ASTRONOMIA_/_FÍSICA | |||
| History (UTC) | 2023-01-04 17:12:12 :: simone -> administrator :: 2022 2023-01-10 17:38:29 :: administrator -> simone :: 2022 | |||
| 3. Content and structure | ||||
| Is the master or a copy? | is the master | |||
| Content Stage | completed | |||
| Transferable | 1 | |||
| Content Type | External Contribution | |||
| Version Type | publisher | |||
| Abstract | Ionospheric scintillation and fading events over low-latitude regions are often caused by severely depleted geomagnetic field-aligned structures known as Equatorial Plasma Bubbles. These events are subject of interest to scientific investigations and concern to technological applications. Over the past several years, most of scintillation studies have focused on the dependence of these events on density gradients, location, local time, geomagnetic conditions, and so forth. This work presents a discussion about the role of the alignment between the signal propagation path and the depleted structures or, equivalently, the geomagnetic field lines, on the observed scintillation and deep fading characteristics. Data from three stations (dip latitudes: 16.13°S, 19.87°S, and 22.05°S) located around the Equatorial Ionization Anomaly (EIA) region were used to assess the amplitude scintillation severity and the deep fading events features under aligned and nonaligned conditions. The results show that the alignment condition plays a crucial role in the occurrence of strong scintillation. The study also revealed that, as stations far from the crests of the EIA are considered, the alignment influence seems to increase, and that a combination of strong plasma density fluctuation and increased aligned path is, presumably, the configuration under which the most severe scintillation and drastic deep fading events are observed. The results indicate that this conjunction is typically met in regions somewhat distinct from that with largest plasma density background over the Brazilian region, therefore, strongest scintillation and largest deep fading rates were observed by a station slightly off-the EIA peak. | |||
| Area | CEA | |||
| Arrangement | urlib.net > Fonds > Produção a partir de 2021 > CGCE > Amplitude Scintillation Severity... | |||
| doc Directory Content | access | |||
| source Directory Content | there are no files | |||
| agreement Directory Content |
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| 4. Conditions of access and use | ||||
| Language | en | |||
| Target File | Space Weather - 2022 - Sousasantos - Amplitude Scintillation Severity and Fading Profiles Under Alignment Between GPS.pdf | |||
| User Group | simone | |||
| Reader Group | administrator simone | |||
| Visibility | shown | |||
| Read Permission | deny from all and allow from 150.163 | |||
| Update Permission | not transferred | |||
| 5. Allied materials | ||||
| Mirror Repository | urlib.net/www/2021/06.04.03.40.25 | |||
| Next Higher Units | 8JMKD3MGPCW/46KTFK8 | |||
| Dissemination | WEBSCI; SCOPUS. | |||
| Host Collection | urlib.net/www/2021/06.04.03.40 | |||
| 6. Notes | ||||
| Empty Fields | alternatejournal archivingpolicy archivist callnumber copyholder copyright creatorhistory descriptionlevel e-mailaddress format isbn keywords label lineage mark nextedition notes parameterlist parentrepositories previousedition previouslowerunit progress project rightsholder schedulinginformation secondarydate secondarykey session shorttitle sponsor subject tertiarymark tertiarytype url | |||
| 7. Description control | ||||
| e-Mail (login) | simone | |||
| update | ||||