We seek candidates for a post-doctoral position to work in the context of an Odysseus project of the FWO-Vlaanderen (http://www.fwo.be) that aims to perform forward modelling for MHD oscillation models. Forward modelling is the calculation of artificial observations from existing models of the MHD oscillations. The models constructed here are specifically aimed at improving solar atmospheric seismology.
The candidate will be hosted in the Centre for mathematical Plasma Astrophysics (CmPA, http://wis.kuleuven.be/CmPA) in the Mathematics Department of the University of Leuven (KU Leuven, Belgium). The research at the CmPA focusses on plasmas in all astrophysical contexts, ranging from extragalactic jets, over the solar corona, to space weather and the Earth’s magnetosphere.

The tasks in this post-doctoral project are the forward modelling of MHD oscillations, in its broadest sense. This could range from modelling emission features of 3D numerical models, calculating observables from analytical models, to the observational verification of already produced models.

A PhD in Mathematics, Physics or Astrophysics (or closely related subject) is desirable, with preferably a specialisation in solar physics. Experience with numerical modelling and/or forward modelling would be of great benefit. Prior experience with the analysis of oscillatory time series and spectral data is a plus.

You will receive a scholarship for one year, which can be extended after successful evaluation to a total of two years. The position starts March 1, 2014 (or soon thereafter). Applications must include a letter of interest, a CV, a list of publications and the names of two referees. The applications should be sent by e-mail to Tom Van Doorsselaere (tom.vandoorsselaere@wis.kuleuven.be) before 20/11/2013 and should include [postdoc-odysseus] in the subject line.

Deadline:
2013-11-20

Contact:
Tom Van Doorsselaere (tom.vandoorsselaere@wis.kuleuven.be)