[Yt-svn] commit/yt-doc: MatthewTurk: Fixed some build errors
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Thu Aug 25 19:40:37 PDT 2011
1 new changeset in yt-doc:
http://bitbucket.org/yt_analysis/yt-doc/changeset/fbaff21b4eb5/
changeset: fbaff21b4eb5
user: MatthewTurk
date: 2011-08-26 04:39:17
summary: Fixed some build errors
affected #: 2 files (35 bytes)
--- a/source/analysis_modules/halo_profiling.rst Thu Aug 25 22:00:08 2011 -0400
+++ b/source/analysis_modules/halo_profiling.rst Thu Aug 25 22:39:17 2011 -0400
@@ -16,7 +16,7 @@
your script inside an mpirun call with the --parallel flag at the end.
Configuring the Halo Profiler
-----------------------------
+-----------------------------
A sample script to run the halo profiler can be found in :ref:`cookbook-run_halo_profiler`.
In order to run the halo profiler on a dataset, a halo profiler object must be instantiated
@@ -97,12 +97,9 @@
* **velocity_center** (*list*): the method in which the halo bulk velocity is
calculated (used for calculation of radial and tangential velocities. Valid
options are:
- - ["bulk", "halo"] (Default): the velocity provided in the halo list
- - ["bulk", "sphere"]: the bulk velocity of the sphere centered on the
- halo center.
- - ["max", field]: the velocity of the cell that is the location of
- the maximum of the field specified (used only when halos set to
- single).
+ - ["bulk", "halo"] (Default): the velocity provided in the halo list
+ - ["bulk", "sphere"]: the bulk velocity of the sphere centered on the halo center.
+ - ["max", field]: the velocity of the cell that is the location of the maximum of the field specified (used only when halos set to single).
* **filter_quantities** (*list*): quantities from the original halo list
file to be written out in the filtered list file. Default: ['id','center'].
--- a/source/analysis_modules/running_halofinder.rst Thu Aug 25 22:00:08 2011 -0400
+++ b/source/analysis_modules/running_halofinder.rst Thu Aug 25 22:39:17 2011 -0400
@@ -148,19 +148,18 @@
are the 2D projected distance.
.. _load_haloes:
+
Loading Haloes Off Disk
-----------------------
It is possible to load haloes off disk and use them as if they had just been
-located by the halo finder. This has at least two advantages.
-Quite obviously this
-means that if the halos are properly saved (e.g. ``haloes.dump()``, see above
-and below),
-halo finding does not need to be run again, saving time. Another benefit is
-loaded haloes only use as much memory as needed because the particle data for
-the haloes is loaded off disk on demand. If only a few haloes are being
-examined, a dataset that required parallel analysis for halo finding can be
-analyzed in serial, interactively.
+located by the halo finder. This has at least two advantages. Quite obviously
+this means that if the halos are properly saved (e.g. ``haloes.dump()``, see
+above and below), halo finding does not need to be run again, saving time.
+Another benefit is loaded haloes only use as much memory as needed because the
+particle data for the haloes is loaded off disk on demand. If only a few haloes
+are being examined, a dataset that required parallel analysis for halo finding
+can be analyzed in serial, interactively.
The first step is to save the haloes in a consistent manner, which is made
simple with the ``.dump()`` function:
Repository URL: https://bitbucket.org/yt_analysis/yt-doc/
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