| 1. Identity statement | ||||
| Reference Type | Journal Article | |||
| Site | mtc-m21b.sid.inpe.br | |||
| Holder Code | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S | |||
| Identifier | 8JMKD3MGP3W34P/3PP6EQB | |||
| Repository | sid.inpe.br/mtc-m21b/2017/10.05.19.18 (restricted access) | |||
| Last Update | 2017:10.05.19.18.56 (UTC) administrator | |||
| Metadata Repository | sid.inpe.br/mtc-m21b/2017/10.05.19.18.56 | |||
| Metadata Last Update | 2018:06.04.02.27.55 (UTC) administrator | |||
| DOI | 10.1016/j.pss.2017.08.011 | |||
| ISSN | 0032-0633 | |||
| Citation Key | FranzEchSouDubZha:2017:ObVeEx | |||
| Title | Ultra low frequency waves at Venus: observations by the venus express spacecraft  | |||
| Year | 2017 | |||
| Month | Oct. | |||
| Access Date | 2024, Apr. 26 | |||
| Type of Work | journal article | |||
| Secondary Type | PRE PI | |||
| Number of Files | 1 | |||
| Size | 7405 KiB | |||
| 2. Context | ||||
| Author | 1 Franz, M. 2 Echer, Ezequiel 3 Souza, Adriane Marques de 4 Dubinin, E. 5 Zhang, T. L. | |||
| Resume Identifier | 1 2 8JMKD3MGP5W/3C9JH3D | |||
| Group | 1 2 DIDGE-CGCEA-INPE-MCTIC-GOV-BR 3 GES-CEA-SESPG-INPE-MCTIC-GOV-BR | |||
| Affiliation | 1 Max-Planck-Institut für Sonnensystemforschung 2 Instituto Nacional de Pesquisas Espaciais (INPE) 3 Instituto Nacional de Pesquisas Espaciais (INPE) 4 Max-Planck-Institut für Sonnensystemforschung 5 Space Research Institute of the Austrian Academy of Sciences | |||
| Author e-Mail Address | 1 fraenz@mps.mpg.de 2 ezequiel.echer@inpe.br 3 adriane.souza@inpe.br | |||
| Journal | Planetary and Space Science | |||
| Volume | 146 | |||
| Pages | 55-65 | |||
| Secondary Mark | A2_INTERDISCIPLINAR A2_GEOCIÊNCIAS B1_MATEMÁTICA_/_PROBABILIDADE_E_ESTATÍSTICA B1_CIÊNCIAS_BIOLÓGICAS_I B1_BIOTECNOLOGIA B1_BIODIVERSIDADE B1_ASTRONOMIA_/_FÍSICA B2_ENSINO B2_CIÊNCIAS_BIOLÓGICAS_II | |||
| History (UTC) | 2017-10-05 19:18:57 :: simone -> administrator :: 2017-10-05 19:18:57 :: administrator -> simone :: 2017 2017-10-05 19:19:55 :: simone -> administrator :: 2017 2018-06-04 02:27:55 :: administrator -> simone :: 2017 | |||
| 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 | Solar wind-Venus interactionPlanetary magnetosheathsPlasma wavesInduced magnetospheres | |||
| Abstract | The generation of waves with low frequencies (below 100 mHz) has been observed in the environment of most bodies in the solar system and well studied at Earth. These waves can be generated either upstream of the body in the solar wind by ionization of planetary exospheres or ions reflected from a bow shock or in the magnetosheath closer to the magnetic barrier. For Mars and Venus the waves may have special importance since they can contribute to the erosion of the ionopause and by that enhance atmospheric escape. While over the past years many case studies on wave phenomena observed at Venus have been published most statistical studies have been based on magnetic observations only. On the other hand the generation mechanisms and transport of these waves through the magnetosphere can only be quantified using both magnetic and particle observations. We use the long time observations of Venus Express (20062014) to determine the predominant processes and transport parameters. First we demonstrate the analysis methods in four case studies, then we present a statistical analysis by determining transport ratios from the complete Venus Express dataset. We find that Alfvenic waves are very dominant (>80%) in the solar wind and in the core magnetosheath. Fast waves are observed mainly at the bow shock (around 40%) but also at the magnetic barrier where they may be most important for the energy transfer into the ionosphere. Their occurrence in the magnetotail may be an artifact of the detection of individual plasma jets in this region. Slow mode waves are rarely dominating but occur with probability of about 10% at the bow shock and in the pile-up-region. Mirror mode waves have probability <20% in the magnetosheath slightly increasing towards the pile-up-boundary. | |||
| Area | CEA | |||
| Arrangement 1 | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > Ultra low frequency... | |||
| Arrangement 2 | urlib.net > BDMCI > Fonds > Produção pgr ATUAIS > GES > Ultra low frequency... | |||
| doc Directory Content | access | |||
| source Directory Content | there are no files | |||
| agreement Directory Content |
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| 4. Conditions of access and use | ||||
| Language | en | |||
| Target File | franz_ultra.pdf | |||
| User Group | simone | |||
| Reader Group | administrator simone | |||
| 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/3EU29DP 8JMKD3MGPCW/3F2PBEE | |||
| Citing Item List | sid.inpe.br/bibdigital/2013/10.01.22.11 6 sid.inpe.br/mtc-m21/2012/07.13.14.45.47 3 | |||
| Dissemination | WEBSCI; PORTALCAPES; MGA; COMPENDEX; SCOPUS. | |||
| Host Collection | sid.inpe.br/mtc-m21b/2013/09.26.14.25.20 | |||
| 6. Notes | ||||
| Empty Fields | alternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel e-mailaddress format isbn label lineage mark mirrorrepository nextedition notes number orcid parameterlist parentrepositories previousedition previouslowerunit progress project rightsholder schedulinginformation secondarydate secondarykey session shorttitle sponsor subject tertiarymark tertiarytype url | |||
| 7. Description control | ||||
| e-Mail (login) | simone | |||
| update | ||||