| 1. Identity statement | |
| Reference Type | Journal Article |
| Site | mtc-m16.sid.inpe.br |
| Holder Code | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
| Identifier | 6qtX3pFwXQZ3r59YDa/JtKru |
| Repository | sid.inpe.br/iris@1916/2005/12.16.12.10 (restricted access) |
| Last Update | 2005:12.16.12.10.00 (UTC) administrator |
| Metadata Repository | sid.inpe.br/iris@1916/2005/12.16.12.10.52 |
| Metadata Last Update | 2018:06.05.01.16.32 (UTC) administrator |
| Secondary Key | INPE-13253-PRE/8509 |
| ISSN | 0378-4371 |
| Citation Key | MagalhaesMariAguiFraj:2005:CaLiNo |
| Title | Can lightning be a noise source for a spherical gravitational wave antenna?  |
| Year | 2005 |
| Access Date | 2024, Apr. 28 |
| Secondary Type | PRE PI |
| Number of Files | 1 |
| Size | 967 KiB |
| 2. Context | |
| Author | 1 Magalhaes, N. S. 2 Marinho, R. D. 3 Aguiar, Odylio Denys de 4 Frajuca, C. |
| Resume Identifier | 1 2 3 8JMKD3MGP5W/3C9JJ2A |
| Group | 1 DAS-INPE-MCT-BR |
| Affiliation | 1 Ctr Fed Educ Tecnol Sao Paulo, Sao Paulo 2 Inst Tecnol Aeronaut, Dept Fis 3 Instituto Nacional de Pesquisas Espaciais, Divisão de Astrofísica (INPE, DAS) |
| Journal | Physica A: Statistical Mechanics and its Applications |
| Volume | 72 |
| Number | 10 |
| History (UTC) | 2005-12-16 12:17:48 :: sergio -> administrator :: 2007-03-21 14:16:33 :: administrator -> sergio :: 2008-01-07 12:53:15 :: sergio -> administrator :: 2008-06-10 22:40:58 :: administrator -> banon :: 2010-05-17 18:17:09 :: banon -> administrator :: 2018-06-05 01:16:32 :: administrator -> marciana :: 2005 |
| 3. Content and structure | |
| Is the master or a copy? | is the master |
| Content Stage | completed |
| Transferable | 1 |
| Content Type | External Contribution |
| Abstract | The detection of gravitational waves is a very active research field at the moment. In Brazil the gravitational wave detector is called Mario SCHENBERG. Because of its high sensitivity it is necessary to model mathematically all known noise sources so that digital filters can be developed that maximize the signal-to-noise ratio. One of the noise sources that must be considered are the disturbances caused by electromagnetic pulses due to lightnings close to the experiment. Such disturbances may influence the vibrations of the antenna's normal modes and mask possible gravitational wave signals. In this work we model the interaction between lightnings and SCHENBERG antenna and calculate the intensity of the noise due to a close lightning stroke in the detected signal. We find that the noise generated does not disturb the experiment significantly.. |
| Area | CEA |
| Arrangement | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > Can lightning be... |
| 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 | can lightning be noise.pdf |
| User Group | administrator banon sergio |
| Visibility | shown |
| Copy Holder | SID/SCD |
| Archiving Policy | denypublisher denyfinaldraft24 |
| Read Permission | deny from all and allow from 150.163 |
| 5. Allied materials | |
| Next Higher Units | 8JMKD3MGPCW/3ETR8EH |
| Dissemination | WEBSCI; PORTALCAPES; COMPENDEX. |
| Host Collection | sid.inpe.br/banon/2003/08.15.17.40 |
| 6. Notes | |
| Empty Fields | alternatejournal archivist callnumber copyright creatorhistory descriptionlevel documentstage doi e-mailaddress electronicmailaddress format isbn keywords label lineage mark mirrorrepository month nextedition notes orcid pages 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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