Solar Prominence Formation and Equilibrium:
New Data, New Models

Purpose

Our International Team spans a wide range of expertise in order to make progress in the understanding of solar prominences, and in particular the mechanisms capable of explaining their formation and their equilibrium. The Team consists of 11 members whose research interests combine data analysis and interpretation, spectro-polarimetry, radiative transfer modelling (including polarised radiative transfer), and modelling of the magnetic field and plasma. We will meet at ISSI to discuss the latest developments in these fields, interpret existing space observations, set up and propose new observational programmes using space instrumentation, and decide modelling strategies to be carried out between the meetings. The outcome of the proposed research is a better understanding of the formation processes of solar prominences and of the physical conditions necessary for the stability of quiescent prominences.

This project builds on the success of the International Team on Spectroscopy and Imaging of Quiescent and Eruptive Solar Prominences from Space.

Team members

José Luis Ballester, Universitat de les Illes Balears, SP
Rick DeVore, Naval Research Laboratory, USA
Holly Gilbert, NASA/GSFC, USA
Petr Heinzel, Astronomical Institute, Academy of Sciences of the Czech Republic, CZ
Nicolas Labrosse, University of Glasgow, UK (Leader)
Arturo López Ariste, THEMIS, CNRS, SP
Duncan Mackay, University of St. Andrews, Scotland, UK
Zoran Mikic, Predictive Science, Inc., USA
Frédéric Paletou, Observatoire Midi-Pyrénées, Université de Toulouse, FR
Susanna Parenti, Royal Observatory of Belgium, BE
Brigitte Schmieder, LESIA, Observatoire de Paris Meudon, FR
Jean-Claude Vial, Institut d'Astrophysique Spatiale, FR

Young scientists

Stanislav Gunar, Astronomical Institute, Academy of Sciences of the Czech Republic, CZ
Manuel Luna Bennasar, NASA/GSFC, USA
Roberto Soler, Universitat de les Illes Balears, SP

Publications

The team members have a strong expertise in the physics of solar prominences. You can find a list of relevant publications on this ADS page.

This project contributed to the publication of the following papers acknowledging the support from ISSI:

Schedule

Three meetings are planned. The first meeting took place between 29th March and 1st April 2010. The second meeting took place between 3rd and 5th November 2010. The last meeting was held between 5 and 8 September 2011.

Contact

Nicolas Labrosse
School of Physics and Astronomy
University of Glasgow
University Avenue
Glasgow G12 8QQ
Scotland
Direct line: +44 (0)141 330 3817
Fax: +44 (0)141 330 8600
Web: http://www.astro.gla.ac.uk/?p=171

Subsistence

A great deal of work is done thanks to the fine restaurants accepting groups of 10 or more people in the evening! Here are a few that we tried and liked, for future reference for ourselves and other teams...

News

16/07/2012

New publications with acknowledgement to ISSI.

04/10/2011

Presentations and pictures of third meeting now available

23/09/2011

New publications with acknowledgement to ISSI.

01/09/2011

Agenda of third meeting now available

New publications with acknowledgement to ISSI.

16/02/2011

The dates of the third meeting: 5-8 September 2011

26/12/2010

Pictures taken by Jean-Claude are now available

6/11/2010

Presentations and pictures of second meeting now available

26/10/2010

Agenda of second meeting now available

New publications with acknowledgement to ISSI.

23/10/2010

Arturo López Ariste (THEMIS/CNRS) is now a member of our Team.

16/09/2010

The second meeting will take place between 3-5 November 2010.

06/04/2010

Presentations and pictures of first meeting now available

16/03/2010

Agenda of first meeting now available

06/12/2009

The first meeting will take place between 29th March and 1st April, 2010. Agenda to follow!