On 16 Jan 2012, at 23:21, Jose Fiestas Iquira wrote:

Thanks, I am attaching the output file.

The output file looks fine - I can't see any problem with the simulation.  According to the output file, it reached t = 100 M, and in the parameter file that is listed as cctk_final_time, so all looks well!

I did copy the development version. As I can see, it was already
fixed, so I should not get this warning, since I copied the
development version.

Yes, if you are using the current development version, then I don't know why you get the warning.  Can you check which version of Carpet you have by doing

cd repos/carpet
hg tip

to be sure you are using the development version?

Is  the puncture tracker not a better way to plot BH trajectories.

It's cheaper to use the puncture tracker, because computing the horizon centroid is more expensive, but it has to be done every iteration, whereas the horizon can be found less frequently.  For comparison with point-particle results, I don't think it makes much difference; the results are gauge dependent anyway so differences on the order of the horizon size cannot be interpreted physically.  Since the parameter file already has horizon-finding built in, it is easier for you to use that.

If you want to figure out how to add the puncture tracker to the simulation, you can start with these parameters:

ActiveThorns = "PunctureTracker"

PunctureTracker::track                      [0] = yes
PunctureTracker::initial_x                  [0] = $xp
PunctureTracker::which_surface_to_store_info[0] = 0
PunctureTracker::track                      [1] = yes
PunctureTracker::initial_x                  [1] = $xm
PunctureTracker::which_surface_to_store_info[1] = 1

IOASCII::out0D_vars = "PunctureTracker::pt_loc"

Replace $xp and $xm with the initial x coordinates of the +x and -x punctures (this will be \pm TwoPunctures::par_b).  You then need to choose two spherical surfaces (https://docs.einsteintoolkit.org/et-docs/Einstein_Toolkit_standards) which are not being used currently to store the puncture locations in.  If there is already 0D output, just add the puncturetracker variable separated with a space.

I
did some plots, what are really the combinations xx, xy, xz, yy, zz ?
Are they related to the trajectories of one BH (projections)? What
about the second BH?

You should have BH_diagnostics.ah1.gp and BH_diagnostics.ah2.gp.  These correspond to the first and second BHs.  If you look at the top of these files, you will see an explanation of the columns.  More information about each column is available in the AHFinderDirect documentation (http://einsteintoolkit.org/documentation/ThornGuide/ThornGuidech128.html#x144-2264000O4).  Specifically, information about the BH_diagnostics output files is at http://einsteintoolkit.org/documentation/ThornGuide/ThornGuidech128.html#x144-2274000O4.5.5

To plot the trajectory of one of the BHs, you want to plot column 3 and column 4 in a parametric plot.


Cheers,
Jose

On Mon, Jan 16, 2012 at 4:39 AM, Ian Hinder <ian.hinder@aei.mpg.de> wrote:

On 14 Jan 2012, at 00:41, Jose Fiestas Iquira wrote:

Hi Ian,
I did the changes but it started and finished early. I am attaching
the qc0-mclachlan.err file. At the end there is a warning in one of
the Carpet files (mask_test.c)


The warning you see,

WARNING level 1 in thorn CarpetReduce processor 0 host qb517
  (line 120 of
/home/ettest24/Cactus/arrangements/Carpet/CarpetReduce/src/mask_test.c):
  -> Simulation domain volume and reduction weight sum differ

is a known issue (https://trac.einsteintoolkit.org/ticket/434) which was
fixed after the last release and the fix is only available in the
development version.  I believe that the warning is not fatal, and it should
not have terminated the simulation.  Can you also post the qc0-mclachlan.out
file?

Where can I find the puncture tracker?


The PunctureTracker thorn is part of the Einstein Toolkit thornlist, so you
should have it already.  However, I think the best thing for you to do
initially would be to look at the BH_diagnostics files for the apparent
horizon centroid locations for tracking the locations of the BHs.




Thanks,
Jose

On Fri, Jan 13, 2012 at 4:38 AM, Ian Hinder <ian.hinder@aei.mpg.de> wrote:


On 13 Jan 2012, at 12:32, Jose Fiestas Iquira wrote:


Yes, trajectories and wave forms would be enough for now. Which are

the names of this files? Many of the .asc files have data like kxx,

kxy, kxz, etc. Is there any description of them?


Not that I am aware of.  Files with extension .x.asc are 1D ascii output of
grid functions from CarpetIOASCII.  kxy is the variable name for the x,y
component of the extrinsic curvature tensor K.  The waveform file should be
in mp_psi4_l2_m2_r*.asc where * corresponds to the radius of the extraction
sphere.  However, looking at the qc0-mclachlan.par file, I see that there is
no wave extraction switched on.  You should be able to enable wave
extraction by adding something like the following to the parameter file:


ActiveThorns = "WeylScal4 CarpetInterp AEILocalInterp Multipole"


Multipole::nradii    = 3

Multipole::radius[0] = 30

Multipole::radius[1] = 40

Multipole::radius[2] = 50

Multipole::variables = "WeylScal4::Psi4r{sw=-2 cmplx=’WeylScal4::Psi4i’}"

Multipole::l_max     = 4

WeylScal4::fdOrder   = 4


(I haven't tested this, so let me know if it doesn't work)


I've just found that the usual PunctureTracker thorn is not enabled in this
example parameter file.  So to look at trajectories you will have to use the
apparent horizon centroids.  These are in the files BH_diagnostics.ah*.gp.
 The meanings of the columns are at the top of the files.  You want the
centroid x and y columns to plot in GnuPlot.






Thanks,

Jose


On Fri, Jan 13, 2012 at 12:41 AM, Ian Hinder <ian.hinder@aei.mpg.de> wrote:


On 12 Jan 2012, at 23:46, Jose Fiestas Iquira wrote:


Dear all,


I run the tutorial and found other interesting examples like the

McLachlan tool for Binary Black Holes.


Regarding the McLachlan tool,

Could somebody help me finding a description of the output? Is all

contained in the .asc files? I would like to visualize it.



Hi Jose,


What sort of output do you want to visualise?  Cactus thorns typically

output "lightweight" information such as BH trajectories and waveforms as

ASCII, and more heavyweight data -- like gridfunctions -- as HDF5.  For the

trajectories (from thorn Puncture Tracker) and waveforms (from Multipole)

you can use gnuplot or anything that can read standard ASCII output to

visualise them.  For gridfunctions in HDF5 format, I think the easiest way

to get started is to use VisIt, for which there is a Carpet plugin (though

installing VisIt is sometimes not so easy!).


Does anyone know if the Carpet plugin is distributed with VisIt yet?  I

believe that was the intention.




Cheers,

Jose



On Wed, Jan 11, 2012 at 7:06 PM, Jose Fiestas Iquira <jafiestas@lbl.gov>

wrote:


Thanks to Erik for advise. ETK example simulation run successfully.




On Wed, Jan 11, 2012 at 11:49 AM, Jose Fiestas Iquira <jafiestas@lbl.gov>

wrote:


Right, it looks good now:



./simfactory/bin/sim list-simulations


  static_tov              [ACTIVE (RUNNING), restart 0000, job id 595490]



Let see how it looks when it finishes. The example was set to 8 hours.



Thanks,


Jose




On Wed, Jan 11, 2012 at 11:45 AM, Erik Schnetter <schnetter@cct.lsu.edu>

wrote:


On Wed, Jan 11, 2012 at 2:42 PM, Jose Fiestas Iquira <jafiestas@lbl.gov>

wrote:



The only thing is that now


$ ./simfactory/bin/sim list-simulations


returns



Error: unknown command list-simulation


Aborting Simfactory.



Did you really type "list-simulations", and the error message says


"list-simulation" (without the final "s")?



-erik



--


Erik Schnetter <schnetter@cct.lsu.edu>   http://www.cct.lsu.edu/~eschnett/


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