iMap is a versatile tool for modeling stellar magnetic fields, polarized radiative transfer calculations and the inversion of spectropolarimetric data. This web-service provides an easy-to-use interface to the iMap code. Without the overhead of compiling various source codes and libraries as well as building platform dependent executables the iMap web-application gives you direct access to most of the basic functionalities of the inversion code.
How to use the iMap web application : Simply login or register and then specify the properties of your stellar target. Choose the analysis and upload your spectra. The resulting surface temperature and/or magnetic field maps as well as the spectral line fits will be sent back to you by Email or can be downloaded via FTP.
PLEASE NOTE, THAT THIS WEB PAGE IS STILL IN ITS EXPERIMENTAL PHASE !
If you have any questions or suggestions do not hesitate to contact me under firstname.lastname@example.org