| 1. Identity statement | |
| Reference Type | Journal Article |
| Site | mtc-m16.sid.inpe.br |
| Holder Code | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
| Identifier | 6qtX3pFwXQZGivnJVY/LtwQL |
| Repository | sid.inpe.br/mtc-m16@80/2006/06.16.17.58 (restricted access) |
| Last Update | 2006:06.16.17.58.35 (UTC) administrator |
| Metadata Repository | sid.inpe.br/mtc-m16@80/2006/06.16.17.58.36 |
| Metadata Last Update | 2021:07.18.04.01.22 (UTC) administrator |
| Secondary Key | INPE-13789--PRE/8975 |
| ISSN | 1364-6826 |
| Citation Key | Kane:2006:ArDoSo |
| Title | Are the double-peaks in solar indices during solar maxima of cycle 23 reflected in ionospheric foF2?  |
| Year | 2006 |
| Month | May |
| Access Date | 2024, Apr. 28 |
| Secondary Type | PRE PI |
| Number of Files | 1 |
| Size | 138 KiB |
| 2. Context | |
| Author | Kane, Rajaram Purushottam |
| Resume Identifier | 8JMKD3MGP5W/3C9JJ4U |
| Group | DGE-INPE-MCT-BR |
| Affiliation | Instituto Nacional de Pesquisas Espaciais, Divisão de Geofísica Espacial (INPE.DGE) |
| Journal | Journal of Atmospheric and Solar-Terrestrial Physics |
| Volume | 68 |
| Number | 8 |
| Pages | 877-880 |
| History (UTC) | 2006-06-16 17:58:36 :: simone -> administrator :: 2008-06-10 22:42:34 :: administrator -> simone :: 2011-05-29 00:45:37 :: simone -> administrator :: 2021-07-18 04:01:22 :: administrator -> marciana :: 2006 |
| 3. Content and structure | |
| Is the master or a copy? | is the master |
| Content Stage | completed |
| Transferable | 1 |
| Content Type | External Contribution |
| Keywords | solar indices Euv ionospheric foF2 EUV DENSITY MODEL |
| Abstract | The 12-month running means of solar indices indicated that during 2000-2002, all solar indices (including EUV) had two maxima. one near July 2000 and another near end of 2001. but the magnitudes of the second maximum relative to the first maximum were different for different solar indices. For EUV 26-34 nm relevant for ionospheric (foF2)(2), the second maximum was similar to 3% higher than the first maximum. The 12-month running means of (foF2)(2) at some mid-latitude locations in both hemispheres showed similar two maxima, but the magnitudes of the second maximum relative to the first maximum were not similar to those of observed solar EUV (similar to 3%) and were very different at different locations (-3% to + 18%). Even on the solar cycle time scale (solar minimum to solar maximum), changes of (foF2)(2) at different locations were not alike (factors of 3.1-4.5). |
| Area | CEA |
| Arrangement | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > Are the double-peaks... |
| 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 | Are the double peaks in solar indices.pdf |
| User Group | administrator simone |
| Visibility | shown |
| Copy Holder | SID/SCD |
| Archiving Policy | denypublisher denyfinaldraft24 |
| Read Permission | deny from all and allow from 150.163 |
| Update Permission | transferred to simone |
| 5. Allied materials | |
| Next Higher Units | 8JMKD3MGPCW/3EU29DP |
| Dissemination | WEBSCI; PORTALCAPES; AGU; MGA; COMPENDEX. |
| Host Collection | sid.inpe.br/banon/2003/08.15.17.40 |
| 6. Notes | |
| Empty Fields | alternatejournal archivist callnumber copyright creatorhistory descriptionlevel 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 |
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