1. Identity statement | |
Reference Type | Journal Article |
Site | mtc-m16.sid.inpe.br |
Holder Code | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
Repository | sid.inpe.br/iris@1916/2005/12.19.13.09 (restricted access) |
Last Update | 2005:12.19.13.09.00 (UTC) administrator |
Metadata Repository | sid.inpe.br/iris@1916/2005/12.19.13.09.41 |
Metadata Last Update | 2018:06.05.01.16.35 (UTC) administrator |
Secondary Key | INPE--13222-PRE/8478 |
ISSN | 0273-1177 |
Citation Key | TakahashiNaShTsLiGo:2005:AiOHEm |
Title | Airglow OH emission height inferred from the OH temperature and meteor trail diffusion coefficient |
Year | 2005 |
Access Date | 2024, May 08 |
Secondary Type | PRE PI |
Number of Files | 1 |
Size | 160 KiB |
|
2. Context | |
Author | 1 Takahashi, Hisao 2 Nakamura, T. 3 Shiokawa, K. 4 Tsuda, T. 5 Lima, L. M. 6 Gobbi, Delano |
Resume Identifier | 1 8JMKD3MGP5W/3C9JHCM 2 3 4 5 6 8JMKD3MGP5W/3C9JGTE |
Group | 1 DAE-INPE-MCT-BR |
Affiliation | 1 Instituto Nacional de Pesquisas Espaciais, Divisão de Aeronomia (INPE, DAE) |
Journal | Advances in Space Research |
Volume | 35 |
Number | 11 |
Pages | 1940-1944 |
History (UTC) | 2006-01-18 17:59:31 :: simone -> administrator :: 2012-07-17 12:41:15 :: administrator -> simone :: 2012-10-03 14:53:09 :: simone -> administrator :: 2005 2018-06-05 01:16:35 :: 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 |
Version Type | publisher |
Keywords | Airglow OH emission height Meteor diffusion OH temperature |
Abstract | Simultaneous observations of the airglow OH(6,2) band rotational temperature, TOH, and meteor trail ambipolar diffusion coefficient, D, were carried out at Shigaraki (35°N, 136°E), during PSMOS 2003 Campaign, January 28 to February 8, 2003. The OH emission height was estimated by cross correlation analysis of the TOH and D nocturnal variations. A good correlation between TOH and D was obtained at 85 km of altitude. From the nocturnal variations of TOH and D, it is found that the OH emission peak height varied from 88 km before the midnight to 84 km in the early morning. The height variation could be caused by an atmospheric tidal effect in the emission height. |
Area | CEA |
Arrangement | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAE > Airglow OH emission... |
doc Directory Content | access |
source Directory Content | there are no files |
agreement Directory Content | there are no files |
|
4. Conditions of access and use | |
Target File | takahashi.pdf |
User Group | administrator simone |
Reader 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 | not transferred |
|
5. Allied materials | |
Next Higher Units | 8JMKD3MGPCW/3ETL868 |
Citing Item List | sid.inpe.br/mtc-m21/2012/07.13.14.44.27 1 |
Dissemination | WEBSCI; PORTALCAPES; 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 identifier isbn label language lineage mark mirrorrepository month nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress project rightsholder schedulinginformation secondarydate secondarymark session shorttitle sponsor subject tertiarymark tertiarytype typeofwork url |
|
7. Description control | |
e-Mail (login) | marciana |
update | |
|