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| = Workshop: "Instabilities and Structures in Proto-Planetary disks" = | # {{attachment:Logo-ISPP-3.png}} = Instabilities and Structures in Proto-Planetary disks = ---- {{attachment:Vieux-Port-Night.jpg|| width=200, align="left"}} ---- {{attachment:Marseille-4.jpg|| width=200, align="right"}} ==== Meeting ==== * ''' Dates: 17th - 20th september 2012 ''' ## * ''' Location: Salle de l'Académie - [[http://marseille.cityseekr.com/des-accoules-church/tourist-attractions-sightseeing/venue/73217#|Les Accoules]] - [[http://en.wikipedia.org/wiki/Marseille|Marseille]] - France ''' ## * '''Rationale:''' . The meeting will address the evolution of the protoplanetary disks at the decoupling stage. The goal is to focus on: * the possible formation of gaseous structures in the protoplanetary disks, particularly in the dead-zone, under various instabilities (baroclinic, or via Rossby or edge modes) * their lifetime and evolution (stability, migration, collisions ....), * their ability to capture the solid material and to survive once loaded. . Emphasis will be placed on the hydrodynamical aspects of the problem, without and with self-gravity, but MHD processes will not be forgotten. We will look also at the links with the experimental and numerical works performed in the physics of rotating flows and granular media. . The burning center of the discussions will be the possible (or impossible) routes toward planetesimals and planetary cores. ==== Registration ==== Due to the capacity of the lecture room the number of participants is limited to ~ 50. * To register please send an email to pierre.barge@oamp.fr * Deadline: Application for registration is limited to ---- [[http://lam.oamp.fr/index.php|{{attachment:Logo-LAM.jpg||width=140}}|target="LAM/OAMP"]] [[http://www.univ-provence.fr/public_html/univ-provence/index.php?pages=article&id=2144&idnum=2405&m=872|{{attachment:Univ_Provence_logo.jpg||width=45}}|target="Provence University"]] [[http://www.cnrs.fr/index.php|{{attachment:Logo-CNRS.gif||width=80}}|target="CNRS"]] [[http://www.regionpaca.fr/en.html|{{attachment:logo-paca.jpg||width=200}}|target="Region PACA"]] ---- |
Instabilities and Structures in Proto-Planetary disks
![[ATTACH]](/ispp/IsppWorkShop?action=AttachFile&do=upload_form&ticket=006648764b.acfc7c731a16483915955d7381e06e070a5bb1ee&target=Vieux-Port-Night.jpg "[ATTACH]"){kind=small}
![[ATTACH]](/ispp/IsppWorkShop?action=AttachFile&do=upload_form&ticket=006648764b.acfc7c731a16483915955d7381e06e070a5bb1ee&target=Marseille-4.jpg "[ATTACH]"){kind=small}
Meeting
Dates: 17th - 20th september 2012
Location: Salle de l'Académie - Les Accoules - Marseille - France
Rationale:
- The meeting will address the evolution of the protoplanetary disks at the decoupling stage. The goal is to focus on:
- the possible formation of gaseous structures in the protoplanetary disks, particularly in the dead-zone, under various instabilities (baroclinic, or via Rossby or edge modes)
- their lifetime and evolution (stability, migration, collisions ....),
- their ability to capture the solid material and to survive once loaded.
- Emphasis will be placed on the hydrodynamical aspects of the problem, without and with self-gravity, but MHD processes will not be forgotten. We will look also at the links with the experimental and numerical works performed in the physics of rotating flows and granular media.
- The burning center of the discussions will be the possible (or impossible) routes toward planetesimals and planetary cores.
Registration
- Due to the capacity of the lecture room the number of participants is limited to ~ 50.
To register please send an email to pierre.barge@oamp.fr
- Deadline: Application for registration is limited to
