FLAG The Solar Fitting at Low Angular degree Group (solarFLAG) FLAG

solarFLAG is an international collaboration of helio- and asteroseismologists. The aims of solarFLAG are to actively develop new, and refine existing, techniques for analysis of low-angular degree solar p-mode data collected by unresolved, Sun-as-a-star observations. The  extraction of accurate and precise estimates of the basic mode parameters (for example frequencies and frequency splittings) is vital for making robust inference on the physical properties of the deep radiative interior and core. solarFLAG provides a forum for co-ordinated development of analysis methods by the leading players in the Sun-as-a-star field
  

 MembersGroup members         Science program    solarFLAG science program

Hare and Hounds #2  New! Hare and Hounds #2     Hare and HoundsOld Hare and Hounds #1    DocumentationDocumentation, papers and data usage

WorkshopFirst solarFLAG Workshop: presentations etc.      asteroFLAG asteroFLAG at ISSI
Dr Bill Chaplin (solarFLAG co-ordinator)
e-mail: wjc@bison.ph.bham.ac.uk

School of Physics & Astronomy
University of Birmingham
Edgbaston, Birmingham B15 2TT, UK
Tel: +44 (0)121 414 4599
Fax: +44 (0)121 414 4601

Last modified 2006 Oct 02 (WJC)