| 1. Identity statement | |
| Reference Type | Journal Article |
| Site | mtc-m16d.sid.inpe.br |
| Holder Code | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
| Identifier | 8JMKD3MGP7W/37TS23E |
| Repository | sid.inpe.br/mtc-m19@80/2010/07.26.15.38 (restricted access) |
| Last Update | 2010:08.12.14.13.48 (UTC) administrator |
| Metadata Repository | sid.inpe.br/mtc-m19@80/2010/07.26.15.38.28 |
| Metadata Last Update | 2018:06.05.04.36.48 (UTC) administrator |
| Secondary Key | INPE--PRE/ |
| DOI | 10.1016/j.pss.2009.12.001 |
| ISSN | 0032-0633 |
| Citation Key | Kane:2010:GnPeGe |
| Title | Gnevyshev peaks in geomagnetic indices  |
| Project | FINEP-537/CT. |
| Year | 2010 |
| Access Date | 2024, Apr. 28 |
| Secondary Type | PRE PI |
| Number of Files | 1 |
| Size | 185 KiB |
| 2. Context | |
| Author | Kane, Rajaram Purushottam |
| Resume Identifier | 8JMKD3MGP5W/3C9JJ4U |
| Group | DGE-CEA-INPE-MCT-BR |
| Affiliation | Instituto Nacional de Pesquisas Espaciais (INPE) |
| Journal | Planetary and Space Science |
| Volume | 58 |
| Number | 5 |
| Pages | 749 - 751 |
| History (UTC) | 2010-08-12 14:13:48 :: marciana -> administrator :: 2010 2018-06-05 04:36:48 :: administrator -> marciana :: 2010 |
| 3. Content and structure | |
| Is the master or a copy? | is the master |
| Content Stage | completed |
| Transferable | 1 |
| Content Type | External Contribution |
| Keywords | coronal mass ejections latitude dependence solar solar-cycle-23 parameters gaps cmes |
| Abstract | Sunspots have a major 11-year cycle, but the years near the maximum show two or more peaks called Gnevyshev peaks. It was noticed that in cycle 23, the double peaks in sunspot numbers are reflected in the electromagnetic radiations and coronal mass ejections (CMEs) in the solar atmosphere. But, in the interplanetary space, the ICMEs (interplanetary CMEs) show peaks not all coinciding with the peaks of sunspot numbers. Also, there are stream interaction regions (SIR), including co-rotating interaction regions (CIR), which evolve quite differently from sunspot numbers. In the geomagnetic indices, the peaks are related mainly to the peaks in SIRs, indicating that geomagnetic indices have no direct relationship with most of the phenomena at the Sun but are responding only to the interplanetary blobs due to SIRs, which are more predominant in the declining phase of sunspot activity. |
| Area | CEA |
| Arrangement | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > Gnevyshev peaks in... |
| 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 | kane.pdf |
| User Group | administrator marciana |
| Visibility | shown |
| Archiving Policy | denypublisher denyfinaldraft24 |
| Read Permission | deny from all and allow from 150.163 |
| 5. Allied materials | |
| Mirror Repository | sid.inpe.br/mtc-m19@80/2009/08.21.17.02.53 |
| Next Higher Units | 8JMKD3MGPCW/3EU29DP |
| Dissemination | WEBSCI; PORTALCAPES. |
| Host Collection | sid.inpe.br/mtc-m19@80/2009/08.21.17.02 |
| 6. Notes | |
| Notes | This work was partially supported by FNDCT, Brazil, under contract FINEP-537/CT. |
| Empty Fields | alternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel documentstage e-mailaddress electronicmailaddress format isbn label lineage mark month nextedition orcid parameterlist parentrepositories previousedition previouslowerunit progress readergroup rightsholder schedulinginformation secondarydate secondarymark session shorttitle sponsor subject tertiarymark tertiarytype typeofwork url versiontype |
| 7. Description control | |
| e-Mail (login) | marciana |
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