| 1. Identity statement | |
| Reference Type | Journal Article |
| Site | mtc-m16c.sid.inpe.br |
| Holder Code | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
| Identifier | 8JMKD3MGP8W/35MGNL5 |
| Repository | sid.inpe.br/mtc-m18@80/2009/07.20.11.47 (restricted access) |
| Last Update | 2009:07.20.11.52.32 (UTC) administrator |
| Metadata Repository | sid.inpe.br/mtc-m18@80/2009/07.20.11.47.03 |
| Metadata Last Update | 2020:04.28.17.48.47 (UTC) administrator |
| Secondary Key | INPE--PRE/ |
| DOI | 10.1007/s11207-008-9303-8 |
| ISSN | 0038-0938 1573-093X |
| Citation Key | Kane:2009:FlSoAc |
| Title | Fluctuations of Solar Activity during the Declining Phase of the 11-Year Sunspot Cycle  |
| Year | 2009 |
| Access Date | 2024, Apr. 28 |
| Secondary Type | PRE PI |
| Number of Files | 1 |
| Size | 308 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 | Solar Physics |
| Volume | 255 |
| Number | 1 |
| Pages | 163-168 |
| History (UTC) | 2009-07-20 11:52:32 :: marciana -> administrator :: 2020-04-28 17:48:47 :: administrator -> simone :: 2009 |
| 3. Content and structure | |
| Is the master or a copy? | is the master |
| Content Stage | completed |
| Transferable | 1 |
| Content Type | External Contribution |
| Abstract | The number of coronal mass ejections (CMEs) erupting from the Sun follows a trend similar to that of sunspot numbers during the rising and maximum phase of the solar cycle. In the declining phase, the CME number has large fluctuations, dissimilar to those of sunspot numbers. In several studies of solar -aEuro parts per thousand interplanetary and solar -aEuro parts per thousand terrestrial relationships, the sunspot numbers and the 2800-MHz flux (F10) are used as representative of solar activity. In the rising phase, this may be adequate, but in the declining phase, solar parameters such as CMEs may have a different behaviour. Cosmic-ray Forbush decreases may occur even when sunspot activity is low. Therefore, when studying the solar influence on the Earth, one has to consider that although geomagnetic conditions at solar maximum will be disturbed, conditions at solar minimum may not be necessarily quiet. |
| Area | CEA |
| Arrangement | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > Fluctuations of Solar... |
| 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 fluctuation.pdf |
| User Group | administrator marciana |
| Visibility | shown |
| Archiving Policy | denypublisher denyfinaldraft12 |
| Read Permission | deny from all and allow from 150.163 |
| 5. Allied materials | |
| Mirror Repository | sid.inpe.br/mtc-m18@80/2008/03.17.15.17.24 |
| Next Higher Units | 8JMKD3MGPCW/3EU29DP |
| Dissemination | WEBSCI; PORTALCAPES. |
| Host Collection | sid.inpe.br/mtc-m18@80/2008/03.17.15.17 |
| 6. Notes | |
| Notes | 0038-0938 |
| Empty Fields | alternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel documentstage e-mailaddress electronicmailaddress format isbn keywords label lineage mark month nextedition 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) | simone |
| update | |