| 1. Identity statement | |
| Reference Type | Journal Article |
| Site | mtc-m16.sid.inpe.br |
| Holder Code | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
| Identifier | 6qtX3pFwXQZsFDuKxG/EEjRE |
| Repository | sid.inpe.br/marciana/2005/01.03.08.43 (restricted access) |
| Last Update | 2005:01.03.02.00.00 (UTC) administrator |
| Metadata Repository | sid.inpe.br/marciana/2005/01.03.08.43.39 |
| Metadata Last Update | 2018:06.05.01.21.19 (UTC) administrator |
| Secondary Key | INPE-13411-PRE/8624 |
| ISSN | 0038-0938 1573-093X |
| Citation Key | VieiraAlarEcheEsur:2004:StInCr |
| Title | Storm intensity criteria for several classes of the driving interplanetary structures  |
| Year | 2004 |
| Month | June |
| Access Date | 2024, Apr. 28 |
| Secondary Type | PRE PI |
| Number of Files | 1 |
| Size | 145 KiB |
| 2. Context | |
| Author | 1 Vieira, Luiz Eduardo Antunes 2 Alarcon, Walter Demétrio Gonzalez 3 Echer, Ezequiel 4 Esurutani, Bruce T. |
| Resume Identifier | 1 2 8JMKD3MGP5W/3C9JJC4 3 8JMKD3MGP5W/3C9JH3D |
| Group | 1 DGE-INPE-MCT-BR |
| Affiliation | 1 Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, U.S.A. |
| Journal | Solar Physics |
| Volume | Aceito |
| Number | ?? |
| Pages | 1-14 |
| History (UTC) | 2006-02-02 16:39:18 :: jefferson -> administrator :: 2018-06-05 01:21:19 :: administrator -> marciana :: 2004 |
| 3. Content and structure | |
| Is the master or a copy? | is the master |
| Content Stage | completed |
| Transferable | 1 |
| Content Type | External Contribution |
| Keywords | Estruturas interplanetárias |
| Abstract | In this paper we discuss the main phase evolution of intense magnetic storms, associated with the passage of different interplanetary magnetic structures. It is shown that their evolution, driven by intense magnetic fields in the sheath region just behind interplanetary shocks, evolves faster (implying physically different magnetospheric configurations) than that associated with intense magnetic fields in the ejecta itself and in corotating streams. The estimated ring current injection rate for the main phase of intense magnetic storms caused by sheath fields is 10 times greater than the estimated injection rate for NS magnetic clouds. Based on these results, we propose storm-intensity criteria for several classes of the driving interplanetary structures. The time necessary to reach a Dst/SYM index threshold level is an important parameter for the space weather forecast. |
| Area | CEA |
| Arrangement | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > Storm intensity criteria... |
| doc Directory Content | access |
| source Directory Content | there are no files |
| agreement Directory Content | there are no files |
| 4. Conditions of access and use | |
| Language | en |
| Target File | fulltext.pdf |
| User Group | administrator jefferson |
| Visibility | shown |
| Copy Holder | SID/SCD |
| Archiving Policy | denypublisher denyfinaldraft12 |
| Read Permission | deny from all and allow from 150.163 |
| 5. Allied materials | |
| Next Higher Units | 8JMKD3MGPCW/3EU29DP |
| Dissemination | WEBSCI; PORTALCAPES. |
| Host Collection | sid.inpe.br/banon/2003/08.15.17.40 |
| 6. Notes | |
| Empty Fields | alternatejournal archivist callnumber copyright creatorhistory descriptionlevel documentstage doi e-mailaddress electronicmailaddress format isbn label lineage mark mirrorrepository nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress project readergroup rightsholder schedulinginformation secondarydate secondarymark session shorttitle sponsor subject tertiarymark tertiarytype typeofwork url versiontype |
| 7. Description control | |
| e-Mail (login) | marciana |
| update | |