| 1. Identity statement | |||||||
| Reference Type | Report | ||||||
| Site | marte3.sid.inpe.br | ||||||
| Holder Code | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S | ||||||
| Identifier | 6qtX3pFwXQZ3r59YCT/GSqLj | ||||||
| Repository | sid.inpe.br/iris@1905/2005/07.25.21.10.35 | ||||||
| Last Update | 2016:05.20.12.45.22 (UTC) administrator | ||||||
| Metadata Repository | sid.inpe.br/iris@1905/2005/07.25.21.10.38 | ||||||
| Metadata Last Update | 2021:02.06.22.00.56 (UTC) administrator | ||||||
| Report Number | INPE-933-PE/036 | ||||||
| Label | 1740 | ||||||
| Citation Key | Gonzalez-AlarconGonz:1976:XRaSo | ||||||
| Title | X ray sources and magnetic field merging  | ||||||
| Year | 1976 | ||||||
| Access Date | 2024, May 01 | ||||||
| Type | RPQ | ||||||
| Number of Pages | 10 | ||||||
| Number of Files | 1 | ||||||
| Size | 3977 KiB | ||||||
| 2. Context | |||||||
| Author | 1 Gonzalez-Alarcon, Walter Demétrio 2 Gonzalez, Alícia Luisa Clua de | ||||||
| Group | 1 DGE-INPE-BR 2 DGE-INPE-BR | ||||||
| Affiliation | 1 Instituto Nacional de Pesquisas Espaciais (INPE) 2 Instituto Nacional de Pesquisas Espaciais (INPE) | ||||||
| Author e-Mail Address | 1 walter.alarcon@inpe.br | ||||||
| e-Mail Address | marcelo.pazos@inpe.br | ||||||
| Institution | Instituto Nacional de Pesquisas Espaciais | ||||||
| City | São José dos Campos | ||||||
| History (UTC) | 2005-07-25 21:10:39 :: administrator -> jefferson :: 2007-10-03 13:45:27 :: jefferson -> administrator :: 2016-01-29 13:26:04 :: administrator -> marcelo.pazos@sid.inpe.br :: 1977 2016-05-19 16:17:26 :: marcelo.pazos@sid.inpe.br :: 1977 -> 1976 2016-05-20 12:48:26 :: marcelo.pazos@sid.inpe.br -> administrator :: 1976 2021-02-06 22:00:56 :: administrator -> :: 1976 | ||||||
| 3. Content and structure | |||||||
| Is the master or a copy? | is the master | ||||||
| Content Stage | completed | ||||||
| Transferable | 1 | ||||||
| Keywords | X ray sources magnetic field merging astrophysical binaries | ||||||
| Abstract | Due to the accumulation of data and theoretical work during the last decade, it has become conclusive the importance that magnetic field merging (MFM) between the interplanetary and terrestrial magnetic fields plays for the earth's magnetosphere. What MFM does for the magnetosphere can be summarized as follows. The topology of the closed geomagnetic field at the merging regions (dayside magnetopause and tail) changes to an OPEN configuration facilitating the entry of plasma and establishing of convection in the magnetosphere. The plasma enters the magnetosphere at the dayside through the northern and southern clefts and at the nightside from the tail, populating the plasma sheet. The less energetic components of the plasma contribute to convection and the more energetic ones populate the ring current, precipitate into the auroral regions via the cusps and may even contribute to populate the Van Allen belts. The power gained by the plasma due to the merging process and the stretching of the open field lines by the solar wind is enough to energize the magnetosphere. | ||||||
| Area | CEA | ||||||
| Arrangement | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > X ray sources... | ||||||
| doc Directory Content | access | ||||||
| source Directory Content |
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| agreement Directory Content |
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| 4. Conditions of access and use | |||||||
| data URL | http://urlib.net/ibi/6qtX3pFwXQZ3r59YCT/GSqLj | ||||||
| zipped data URL | http://urlib.net/zip/6qtX3pFwXQZ3r59YCT/GSqLj | ||||||
| Language | en | ||||||
| Target File | publicacao.pdf | ||||||
| User Group | administrator marcelo.pazos@inpe.br | ||||||
| Reader Group | administrator marcelo.pazos@inpe.br | ||||||
| Visibility | shown | ||||||
| Copyright License | urlib.net/www/2012/11.12.15.10 | ||||||
| Copy Holder | SID/SCD | ||||||
| Read Permission | allow from all | ||||||
| Update Permission | not transferred | ||||||
| 5. Allied materials | |||||||
| Next Higher Units | 8JMKD3MGPCW/3EU29DP | ||||||
| Dissemination | NTRSNASA; BNDEPOSITOLEGAL. | ||||||
| Host Collection | sid.inpe.br/banon/2001/04.03.15.36 | ||||||
| 6. Notes | |||||||
| Notes | This work is to be submitted as a Letter to Nature Physical Science. | ||||||
| Empty Fields | archivingpolicy archivist callnumber contenttype creatorhistory date descriptionlevel doi edition format isbn issn lineage mark mirrorrepository nextedition orcid parameterlist parentrepositories previousedition previouslowerunit progress project recipient resumeid rightsholder schedulinginformation secondarydate secondarykey secondarymark secondarytype session shorttitle sponsor subject tertiarymark tertiarytype translator url versiontype | ||||||