Visibility functions

The package can be used to calculate visibility and darkening functions for solar and stellar oscillations. So far, only the most dominant mode l = 0 for solar and stellar oscillation has been implemented in the code.

Since the author has moved on to a di erent eld of Helioseismology, the software development of this package has stopped. The user of the package should feel free to use it to its extent and modify the code if applicable.

The code itself is written in IDL and is not a stand-alone code. It has to be used in connection with the radiative transfer code RH by Han Uitenbroek.

The download package includes a manual.



European Helio- and Asteroseismology Network