Development of a new cloud model for Venus (MAD-VenLA) using the Modal Aerosol Dynamics approach

Autor: Anni Määttänen, Sabrina Guilbon, Jérémie Burgalat, Franck Montmessin

Publikováno v: Advances in Space Research. 71:1116-1136

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::d3704ec1a9d347e39d97b0af38cacd63
https://doi.org/10.1016/j.asr.2022.09.063

Investigations of the Mars Upper Atmosphere with ExoMars Trace Gas Orbiter

Autor: Oleg Korablev, Alejandro Cardesin, David M. Kass, Colin Wilson, Nikolai Ignatiev, Ann Carine Vandaele, Daniel J. McCleese, Nicholas M. Schneider, Manish R. Patel, Armin Kleinböhl, J. E. Rodriguez, Jean-Claude Gérard, Maya García-Comas, Jose-Juan Lopez-Moreno, Sabrina Guilbon, Sergio Jiménez-Monferrer, Anna Fedorova, R. T. Clancy, Ian Thomas, Francisco Gonzalez-Galindo, Miguel Lopez-Valverde, Franck Montmessin, Michael Chaffin, Franck Lefèvre, Anni Määttänen

Publikováno v: Space Science Reviews
Space Science Reviews, Springer Verlag, 2018, 214 (1), pp.artcle 29. ⟨10.1007/s11214-017-0463-4⟩
Digital.CSIC. Repositorio Institucional del CSIC
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Space Science Reviews, 2018, 214 (1), pp.artcle 29. ⟨10.1007/s11214-017-0463-4⟩

López-Valverde, M. A. et al.
The Martian mesosphere and thermosphere, the region above about 60 km, is not the primary target of the ExoMars 2016 mission but its Trace Gas Orbiter (TGO) can explore it and address many interesting issues, either

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c99ec0e62f3c950b06601e7d6028a505

A cloud modal representation for the IPSL Venus GCM: validation and first results

Autor: Sabrina Guilbon, Anni Määttänen, Franck Montmessin, Jérémie Burgalat, Sébastien Lebonnois, Aurélien Stolzenbach, Pascal Rannou, Arnaud Beth, Anton Laakso, Harri Kokkola, Kevin Mcgouldrick, Maxence Lefèvre, Franck Lefèvre

Publikováno v: EGU General Assembly 2017
EGU General Assembly 2017, Apr 2017, Vienna, Austria. pp.EGU2017-8180
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International audience; Venus is a terrestrial planet enshrouded by 20 km-thick clouds, which are composed of sulphuric acid-water solution droplets. To understand the Venus atmosphere, LMD and LATMOS laboratories have developed a 3D IPSL Venus Globa

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::59ec1760bdd8f0b058df96502238f059
https://hal-insu.archives-ouvertes.fr/insu-01519247

WITHDRAWN: Climatology of the ozone vertical distribution on Mars from SPICAM/MEX UV occultations

Autor: Oleg Korablev, Anna Fedorova, Sabrina Guilbon, Constantino Listowski, Franck Montmessin, Franck Lefèvre, Anni Määttänen

Publikováno v: Icarus. :113428

The SPICAM/MEX ultraviolet spectrometer probed the Martian atmosphere with the occultation method from 2004 until 2014. SPICAM/MEX performed both stellar and solar occultations during in total four Martian Years with a good spatial and seasonal cover

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::ef21c6aff94b7489d58f82bd80c232fb
https://doi.org/10.1016/j.icarus.2019.113428

VenLA: The LATMOS Venus cloud model

Autor: Anni Määttänen, Sabrina Guilbon, Aurélien Stolzenbach, Slimane Bekki, Franck Montmessin

Publikováno v: European Planetary Science Congress 2015
European Planetary Science Congress 2015, Sep 2015, Nantes, France. pp.EPSC2015-634
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International audience; The LATMOS Venus cloud model VenLA (Venus Liquid Aerosols) is based on a terrestrial Polar Strato-spheric Cloud (PSC) model [7]. VenLA models the formation, growth and decay of sulfuric acid-water droplets. The model has under

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::89aea604101973ce6f5ffa930adea2ef
https://insu.hal.science/insu-01211232/file/EPSC2015-634-1.pdf