| 1. Identity statement | |
| Reference Type | Journal Article |
| Site | mtc-m16.sid.inpe.br |
| Holder Code | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
| Identifier | 6qtX3pFwXQZsFDuKxG/AR72P |
| Repository | sid.inpe.br/marciana/2004/01.22.14.21 (restricted access) |
| Last Update | 2013:04.02.11.50.08 (UTC) administrator |
| Metadata Repository | sid.inpe.br/marciana/2004/01.22.14.21.20 |
| Metadata Last Update | 2018:06.05.01.28.38 (UTC) administrator |
| Secondary Key | INPE-10291-TDI/910 |
| DOI | {10.1016/S0273-1177(97)01047-8;} |
| ISSN | 0273-1177 |
| Citation Key | SawantSrTrSoFeCeSu:1997:RaObTo |
| Title | Radio observations of total solar eclipse of November 3, 1994 at Chapecó (Brazil)  |
| Year | 1997 |
| Access Date | 2024, May 05 |
| Secondary Type | PRE PI |
| Number of Files | 1 |
| Size | 372 KiB |
| 2. Context | |
| Author | 1 Sawant, Hanumant Shankar 2 Srivastava, N. 3 Trigoso, H. E. 4 Sobral, José Humberto Andrade 5 Fernandes, Francisco Carlos Rocha 6 Cecatto, José Roberto 7 Subramanian, K. R. |
| Group | 1 DAS-INPE-MCT-BR 2 3 4 DAS-INPE-MCT-BR 5 6 DAS-INPE-MCT-BR |
| Journal | Advances in Space Research |
| Volume | 20 |
| Number | 12 |
| Pages | 2359-2363 |
| History (UTC) | 2012-10-15 16:05:16 :: administrator -> marciana :: 2013-02-19 17:49:14 :: marciana -> administrator :: 1997 2013-04-02 11:49:06 :: administrator -> marciana :: 1997 2013-04-02 11:50:09 :: marciana -> administrator :: 1997 2018-06-05 01:28:38 :: administrator -> marciana :: 1997 |
| 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 |
| Abstract | Radio observations of the eclipse on November 3, 1994, were carried out at Chapecó, Brazil by using a decimetric spectrograph having high spectral and time resolution. The light curve shows that: (1) Time variation of the radio flux before the totality was more compared to that after. (2) During the totality radio emission at 1.5 GHz was observed. Advantage of high spatial resolution (~ 3.2 arc sec) possible during solar eclipse enabled us to determine the height of radio emission at 1.5 GHz. (3) Microwave bursts were observed associated with metric Type III-RS bursts. The source size of one of the microwave bursts was ~ 7 arc sec and its physical parameters have been estimated. (4) The time difference between radio and optical contacts suggested for the first time asymmetrical limb brightening at 1.5 GHz. |
| Area | CEA |
| Arrangement | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > Radio observations of... |
| 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-S0273117797010478-main.pdf |
| User Group | administrator marciana |
| Visibility | shown |
| Copy Holder | SID/SCD |
| 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/2003/08.15.17.40 |
| 6. Notes | |
| Empty Fields | affiliation alternatejournal archivist callnumber copyright creatorhistory descriptionlevel e-mailaddress electronicmailaddress format isbn keywords label 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 | |