FLUIDOS Archivos

Mecánica de Fluidos

FLUIDOS@LISTSERV.REDIRIS.ES

Opciones: Vista Forum

Use Monospaced Font
Mostrar las partes HTML
Mostrar todas las cabeceras de correo

Mensaje: [<< Primero] [< Prev] [Siguiente >] [Último >>]
Tema: [<< Primero] [< Prev] [Siguiente >] [Último >>]
Autor: [<< Primero] [< Prev] [Siguiente >] [Último >>]

Print Responder
Subject:
Emisor:
Javier Burguete <[log in para visualizar]>
Reply To:
Mecánica de Fluidos <[log in para visualizar]>
Fecha:
Tue, 16 Jun 2020 17:19:08 +0200
Content-Type:
multipart/alternative
Parts/Attachments:
text/plain (4 kB) , text/html (22 kB)
Buenas tardes,

Espero que tanto vosotros como vuestras familias estés lo mejor posible.

Os paso este anuncio de Post-doc, por si a alguien le pudiera interesar. 
Aunque es de MHD, cualquiera con un perfil numérico de Mecánica de 
Fluidos puede aplicar.

Saludos,
Javier



-------- Mensaje reenviado --------
Fecha: 	Tue, 16 Jun 2020 14:59:47 +0200 (CEST)
De: 	Florence Marcotte <[log in para visualizar]>
Responder a: 	Florence Marcotte <[log in para visualizar]>



Dear all,

sorry for the cross posting.
We are hiring an ANR funded postdoctoral research assistant at INRIA in 
Nice, France, to work on optimal control and nonlinear stability of MHD 
flows (more details below).

The postdoc will join the Laboratoire J.A. Dieudonné, located in Parc 
Valrose (Université Nice Sophia-Antipolis) on the French Riviera. The 
campus is in the city-center, at walking distance from the sea and short 
driving distance from the mountains.

Please share this with any recent PhD or postdoc who might be interested.

Best wishes,

Florence


*********************
The considerable diversity of long-lived magnetic fields observed in the 
Universe raises fundamental questions regarding their origin. Although 
it is now widely accepted that such fields are sustained by a dynamo 
instability in the electrically conducting fluid layers of 
celestial bodies, understanding the conditions of nonlinear excitation 
and saturation of a dynamo instability in a swirling MHD flow remains an 
important challenge for the modeling of astrophysical magnetic fields.

The project aims at developing the numerical tools required to 
achieve fully nonlinear optimal control of MHD flows. These tools will 
be used to identify "minimal dynamo seeds" in simple swirling flows 
relevant to stellar systems, i.e. challenge the stability of such flows 
with respect to initial magnetic fields of arbitrary amplitude and 
structure. Furthermore, nonlinear optimisation will be used as a 
physical diagnostic to gain novel understanding of the mechanisms that 
are most favorable to dynamo action in astrophysical systems. Original 
ideas and suggestions from the postdoctoral researcher will be encouraged.

The position requires a PhD in applied maths, fluid mechanics or related 
field, and is available from September, 1st. Funding is already secured 
for two years (one-year position renewable once). Applications will be 
accepted until the position is filled, preferably before July, 10th.
Interested candidates are welcome to contact me 
([log in para visualizar]) for more informations.




Florence Marcotte
Junior researcher at INRIA Sophia Antipolis
Laboratoire J.A. Dieudonné, Université Nice Sophia-Antipolis
Parc Valrose, 06108 Nice, France
  +33 4 89 15 05 47




-- 


*Este mensaje puede contener información confidencial. Si usted no es el 
destinatario del mismo o lo ha recibido por error, por favor, bórrelo de 
sus sistemas y comuníquelo a la mayor brevedad al remitente. Los datos 
personales incluidos en los correos electrónicos que intercambie con el 
personal de la Universidad de Navarra podrán ser almacenados en la libreta 
de direcciones de su interlocutor y/o en los servidores de la Universidad 
durante el tiempo fijado en su política interna de conservación de 
información. La Universidad de Navarra gestiona dichos datos con fines 
meramente operativos, para permitir el contacto por email entre sus 
trabajadores/colaboradores y terceros. Puede consultar la Política de 
Privacidad de la Universidad de Navarra en la dirección: 
**https://www.unav.edu/aviso-legal* <https://www.unav.edu/aviso-legal>****


** **

*This email message may contain confidential information. If you are 
not the intended recipient of this message or their agent, or if this 
message has been addressed to you in error, please immediately alert the 
sender by reply email and then delete this message and any attachments.  
The personal information included in email messages exchanged with 
employees of the University of Navarra may be stored in the database of 
your interlocutor and/or the servers of the University for the time-period 
stipulated by its internal information storage policy. The University 
stores such data for purely administrative purposes, to facilitate e-mail 
contact between its employees and third parties. The University of Navarra 
Privacy Policy may be accessed at https://www.unav.edu/aviso-legal 
<https://www.unav.edu/aviso-legal>      *****

** **

_Antes de imprimir 
este mensaje o sus documentos anexos, asegúrese de que es necesario. 
Proteger el medio ambiente está en nuestras manos.
Before printing this 
e-mail or attachments, be sure it is necessary. _It is in our hands to 
protect the environment.__


ATOM RSS1 RSS2