| 1. Identity statement | |
| Reference Type | Journal Article |
| Site | marte3.sid.inpe.br |
| Holder Code | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
| Identifier | 6qtX3pFwXQZ3r59YCT/GUKMM |
| Repository | sid.inpe.br/iris@1905/2005/07.29.22.44 (restricted access) |
| Last Update | 2013:04.03.12.34.41 (UTC) jefferson |
| Metadata Repository | sid.inpe.br/iris@1905/2005/07.29.22.44.18 |
| Metadata Last Update | 2018:06.06.04.03.54 (UTC) administrator |
| Secondary Key | INPE-8336-PRE/4119 |
| DOI | 10.1016/0273-1177(95)00557-U |
| ISSN | 0273-1177 |
| Label | 9306 |
| Citation Key | FernandesSawaZhel:1996:DeSlDr |
| Title | Decimetric slow drift split pair  |
| Year | 1996 |
| Access Date | 2024, May 02 |
| Secondary Type | PRE PI |
| Number of Files | 1 |
| Size | 420 KiB |
| 2. Context | |
| Author | 1 Fernandes, Francisco Carlos Rocha 2 Sawant, Hanumant Shankar 3 Zheleznyakov, V. V. |
| Group | 1 DAS-INPE-MCT-BR 2 DAS-INPE-MCT-BR |
| Journal | Advances in Space Research |
| Volume | 17 |
| Number | 4-5 |
| Pages | 143-146 |
| History (UTC) | 2012-10-15 02:14:27 :: administrator -> jefferson :: 2013-02-19 14:55:24 :: jefferson -> administrator :: 1996 2013-04-03 12:34:20 :: administrator -> jefferson :: 1996 2013-04-03 12:34:42 :: jefferson -> administrator :: 1996 2018-06-06 04:03:54 :: administrator -> marciana :: 1996 |
| 3. Content and structure | |
| Is the master or a copy? | is the master |
| Content Stage | completed |
| Transferable | 1 |
| Content Type | External Contribution |
| Version Type | publisher |
| Keywords | ASTROFÍSICA espectro solar eclosao tipo 3 ondas de plasma emissoes de radiacao solar solar spectra type 3 bursts plasma waves solar radio emission |
| Abstract | We report examples of the type III bursts and a patch like emission exhibiting split in frequency observed for the first time. This burst was observed over a frequency range of (1630-1580) MHz lasting for about 15 s, on 15th June, 1991. The separation between the two split components is - 30 MHz and lower split frequency component is less intense compared to the higher split frequency component. These observed characteristics favour the hypothesis of conversion of plasma waves by combinational scattering on upgoing ion-sound waves in a magnetic loop. Emission is assumed to be at fundamental and propagation effect explains, the observed characteristics of the decimetric long lasting split frequency burst. Detailed analysis permits to estimate parameters of the exciter and that of the source sizes. |
| Area | CEA |
| Arrangement | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > Decimetric slow drift... |
| 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 | 1-s2.0-027311779500557U-main.pdf |
| User Group | administrator jefferson |
| Visibility | shown |
| Archiving Policy | denypublisher denyfinaldraft24 |
| Read Permission | deny from all and allow from 150.163 |
| Update Permission | not transferred |
| 5. Allied materials | |
| Next Higher Units | 8JMKD3MGPCW/3ETR8EH |
| Dissemination | WEBSCI; PORTALCAPES; MGA; COMPENDEX. |
| Host Collection | sid.inpe.br/banon/2001/04.03.15.36 |
| 6. Notes | |
| Empty Fields | affiliation alternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel e-mailaddress electronicmailaddress format isbn lineage mark mirrorrepository month nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress project readergroup resumeid rightsholder schedulinginformation secondarydate secondarymark session shorttitle sponsor subject tertiarymark tertiarytype typeofwork url |
| 7. Description control | |
| e-Mail (login) | marciana |
| update | |