| 1. Identity statement | ||||
| Reference Type | Journal Article | |||
| Site | mtc-m16d.sid.inpe.br | |||
| Holder Code | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S | |||
| Identifier | 8JMKD3MGP7W/38TLRSH | |||
| Repository | sid.inpe.br/mtc-m19/2011/01.07.13.28 (restricted access) | |||
| Last Update | 2011:01.07.13.31.46 (UTC) administrator | |||
| Metadata Repository | sid.inpe.br/mtc-m19/2011/01.07.13.28.49 | |||
| Metadata Last Update | 2018:06.05.04.35.07 (UTC) administrator | |||
| Secondary Key | INPE--PRE/ | |||
| DOI | 10.1016/j.pss.2010.07.026 | |||
| ISSN | 0032-0633 | |||
| Citation Key | Kane:2010:ScPlDs | |||
| Title | Scatter in the plots of Dst(min) versus Bz(min)  | |||
| Year | 2010 | |||
| Month | Dec. | |||
| Access Date | 2024, Apr. 27 | |||
| Secondary Type | PRE PI | |||
| Number of Files | 1 | |||
| Size | 930 KiB | |||
| 2. Context | ||||
| Author | Kane, R. P. | |||
| Group | DGE-CEA-INPE-MCT-BR | |||
| Affiliation | Instituto Nacional de Pesquisas Espaciais (INPE) | |||
| Journal | Planetary and Space Science | |||
| Volume | 58 | |||
| Number | 14-15 | |||
| Pages | 1792-1801 | |||
| Secondary Mark | B1_ASTRONOMIA_/_FÍSICA A2_GEOCIÊNCIAS B1_INTERDISCIPLINAR | |||
| History (UTC) | 2011-05-24 04:06:38 :: marciana -> administrator :: 2010 2018-06-05 04:35:07 :: 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 | Scatter Dst | |||
| Abstract | In the plots of −Dst(min) versus −Bz(min) in cycle 23, in restricted ranges of −Dst(min), there was lot of scatter and the correlations were low. A bivariate analysis using geomagnetic Dst(min) and auroral AE index did not improve the situation. Substitution of −Dst(min) by the ram-pressure-corrected true ring current Dst*(min) improved the correlations only slightly. Using the product V Bz instead of Bz(min) as a proxy for magnetospheric energy input did not improve the correlations, even for the 12 severe storm events in cycle 23. A multivariate analysis using −Bz(min) versus −Dst(min), with AU, AL and auroral particle precipitation index POES as additional indices improved the correlations and reduced the scatter. It was noticed, however, that for these severe storms, a major part of the solar wind input energy (not, vert, similar85%) was still going to the Dst ring current, but this had an uncertainty of not, vert, similar15%. So in any severe storm event, the ring current could receive anything from 70% to 100% of the solar wind input energy. | |||
| Area | CEA | |||
| Arrangement | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > Scatter in the... | |||
| doc Directory Content | access | |||
| source Directory Content | there are no files | |||
| agreement Directory Content |
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| 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; COMPENDEX. | |||
| Host Collection | sid.inpe.br/mtc-m19@80/2009/08.21.17.02 | |||
| 6. Notes | ||||
| Empty Fields | alternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel documentstage e-mailaddress electronicmailaddress format isbn label lineage mark nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress project readergroup resumeid rightsholder schedulinginformation secondarydate session shorttitle sponsor subject tertiarymark tertiarytype typeofwork url versiontype | |||
| 7. Description control | ||||
| e-Mail (login) | marciana | |||
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