1. Identity statement | |
Reference Type | Journal Article |
Site | marte3.sid.inpe.br |
Holder Code | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
Identifier | 6qtX3pFwXQZ3r59YCT/GUhvq |
Repository | sid.inpe.br/iris@1905/2005/07.29.01.25.28 (restricted access) |
Last Update | 2013:04.03.12.49.57 (UTC) jefferson |
Metadata Repository | sid.inpe.br/iris@1905/2005/07.29.01.25.42 |
Metadata Last Update | 2018:06.06.04.02.55 (UTC) administrator |
Secondary Key | INPE-5762-PRE/1923 |
ISSN | 0273-1177 |
Label | 7156 |
Citation Key | BalanBaiSubAbdRao:1996:MoCoEq |
Title | Model comparisons of equatorial plasma fountain and equatorial anomaly at three locations |
Year | 1996 |
Secondary Date | 19960320 |
Access Date | 2024, May 05 |
Secondary Type | PRE PI |
Number of Files | 1 |
Size | 740 KiB |
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2. Context | |
Author | 1 Balan, N. 2 Bailey, G. J. 3 Subbarao, K. S. V. 4 Abdu, Mangalathayil Ali 5 Rao, P. B |
Group | 1 DAE-INPE-MCT-BR 2 3 4 DAE-INPE-MCT-BR |
Journal | Advances in Space Research |
Volume | 18 |
Number | 6 |
Pages | 69-78 |
History (UTC) | 2013-03-17 03:46:37 :: administrator -> jefferson :: 1996 2013-04-03 12:49:57 :: jefferson -> administrator :: 1996 2018-06-06 04:02:55 :: administrator -> marciana :: 1996 |
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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 |
Version Type | publisher |
Keywords | AERONOMIA FORTALEZA (ESTADO)JICAMARCA IONOSPHERIC PLASMA FOUNTAIN IONOSPHERIC EQUATORIAL ANOMALY |
Abstract | The equatorial plasma fountain and equatorial anomaly in the ionospheres over Jicamarca (77 degrees W), Trivandrum (77 degrees E), and Fortaleza (38 degree W) are compared under magnetically quiet (Ap=4) equinoctial conditions (day 264) at high solar activity (F10.7 = 178). The comparison, carried out using the Sheffield University Plasmaphere-Ionosphere Model with the same perpendicular ExB drift velocity at all locations, is aimed to investigate the modulating effect of neutral wind. The neutral wind is found to produce north-south asymmetries in the plasma fountain and anomaly, with larger plasma flow and stronger anomaly crests occurring in opposite hemispheres at all locations. The north-south asymmetry in the plasma fountain is stronger at locations of larger displacement between the geomagnetic and geographic equators than at locations of larger magnetic declination angle. The vertical ExB drift velocities at the magnetic equators of Trivandrum and Fortaleza are also derived by matching the measured and model values of the peak height hmax. The derived velocities (which correspond to the ionospheric peak) are compared with that measured at Jicamarca using the incoherent scatter radar. |
Area | CEA |
Arrangement | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAE > Model comparisons of... |
doc Directory Content | access |
source Directory Content | there are no files |
agreement Directory Content | there are no files |
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4. Conditions of access and use | |
Language | en |
Target File | 1-s2.0-0273117795009027-main.pdf |
User Group | administrator jefferson |
Visibility | shown |
Archiving Policy | denypublisher denyfinaldraft24 |
Read Permission | deny from all and allow from 150.163 |
Update Permission | not transferred |
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5. Allied materials | |
Next Higher Units | 8JMKD3MGPCW/3ETL868 |
Dissemination | WEBSCI; PORTALCAPES; MGA; COMPENDEX. |
Host Collection | sid.inpe.br/banon/2001/04.03.15.36 |
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6. Notes | |
Empty Fields | affiliation alternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel doi e-mailaddress electronicmailaddress format isbn lineage mark mirrorrepository month nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress project readergroup resumeid rightsholder schedulinginformation secondarymark session shorttitle sponsor subject tertiarymark tertiarytype typeofwork url |
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7. Description control | |
e-Mail (login) | marciana |
update | |
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