gyre
The gyre frontend calculates the free-oscillation
modes of a stellar model. The general flow of execution is outlined in
the chart to the right. After reading the namelist input file and the model,
gyre loops over &mode namelist groups,
processing each in turn.
For a given group, gyre searches over a range of
oscillation frequencies for modes with a specific harmonic degree
\(\ell\) and azimuthal order \(m\). With each mode found, the
eigenfrequency, eigenfunctions and other data are optionally written
to a detail file. At the end of the run,
response data from all modes found (across all &mode groups)
are optionally written to a summary file.
The table below lists which namelist groups, and in what number, should appear in namelist input files for gyre.
Description |
Namelist group name |
Count |
|---|---|---|
1 |
||
\(\geq 1\)[1] |
||
\(\geq 1\) |
||
1 |
||
\(\geq 1\)[1] |
||
\(\geq 1\)[1] |
||
1 |
||
1 |
||
\(\geq 1\)[1] |
||
\(\geq 1\) |
Footnotes