Commit e60e3163 authored by Janosch Preuß's avatar Janosch Preuß
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......@@ -509,7 +509,7 @@ In these cases we will give specific references to the corresponding reproductio
### Fig. 2.2
* The real and imaginary parts of dtn are contained in the column `zeta` of the files *jump-dtn-kinf16-real.dat* and *jump-dtn-kinf16-imag.dat*, respectively, which are generated while running the script
to reproduce [Fig. 4.6](#figJump).
* The poles of dtn, which are shown in the lower panel of the figure as black crosses, are contained in the file *dtn_hom_poles.dat* which is avaialble after running the reproduction instructions for
* The poles of dtn, which are shown in the lower panel of the figure as black crosses, are contained in the file *dtn_hom_poles.dat* which is available after running the reproduction instructions for
[Fig 2.3](#figdtnHomExp).
### <a name="figdtnHomExp"></a> Fig. 2.3
......@@ -550,6 +550,8 @@ Change to the folder `scripts/6_helio_tbc/2_DtN_sep`. Run `python3 solar_coeff.p
### Fig. 2.8
Change to the directory `scripts/6_helio_tbc/2_DtN_sep`. Run `python3 dcolor-VALC.py`.
Note: Producing the domain coloring plot may take a while. If you only want to obtain the dtn function and its poles (left panel of the figure),
then kill the script after the poles have been computed (the domain coloring plot is produced last).
* The values of the dtn function are available in the file *dtn-VALC-ref-0.007Hz.dat*. The column *l* is the index of the eigenvalue.
The columns *zetaReal* and *zetaImag* contains real and imaginary parts of the dtn function, respectively.
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Subproject commit edff10ce51287287ca4ac4e9245eb48807a88ac3
Subproject commit 1e7121d28903ac0e0fce7b6a44e1bed61405d3dd
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