[yt-svn] commit/yt: 3 new changesets
commits-noreply at bitbucket.org
commits-noreply at bitbucket.org
Wed Jul 30 12:34:18 PDT 2014
3 new commits in yt:
https://bitbucket.org/yt_analysis/yt/commits/61138e6fa507/
Changeset: 61138e6fa507
Branch: yt-3.0
User: mzingale
Date: 2014-07-30 21:12:16
Summary: update the BoxLib stuff -- in particular, we don't always need inputs
Affected #: 1 file
diff -r cc84ae55b7e867ddf3a951286b83b5ff0d861e3f -r 61138e6fa5078f216eac784c2e71277e1ada8f23 doc/source/examining/loading_data.rst
--- a/doc/source/examining/loading_data.rst
+++ b/doc/source/examining/loading_data.rst
@@ -51,11 +51,13 @@
yt has been tested with Boxlib data generated by Orion, Nyx, Maestro and
Castro. Currently it is cared for by a combination of Andrew Myers, Chris
-Malone, and Matthew Turk.
+Malone, Matthew Turk, and Mike Zingale.
To load a Boxlib dataset, you can use the ``load`` command provided by
-``yt.mods`` and supply to it the directory file name. **You must also have the
-``inputs`` file in the base directory.** For instance, if you were in a
+``yt.mods`` and supply to it the directory file name. In general, you must also have the
+``inputs`` file in the base directory, but Maestro and Castro will get
+all the necessary parameter information from the ``job_info`` file in
+the plotfile directory. For instance, if you were in a
directory with the following files:
.. code-block:: none
@@ -81,6 +83,9 @@
import yt
ds = yt.load("pltgmlcs5600")
+For Maestro and Castro, you would not need the ``inputs`` file, and you
+would have a ``job_info`` file in the plotfile directory.
+
.. _loading-flash-data:
FLASH Data
https://bitbucket.org/yt_analysis/yt/commits/f931f0024323/
Changeset: f931f0024323
Branch: yt-3.0
User: mzingale
Date: 2014-07-30 21:18:25
Summary: yt.mods -> yt.load
Affected #: 1 file
diff -r 61138e6fa5078f216eac784c2e71277e1ada8f23 -r f931f0024323f44200560e6aa5f4aa6555541160 doc/source/examining/loading_data.rst
--- a/doc/source/examining/loading_data.rst
+++ b/doc/source/examining/loading_data.rst
@@ -12,8 +12,8 @@
---------
Enzo data is fully supported and cared for by Matthew Turk. To load an Enzo
-dataset, you can use the ``load`` command provided by ``yt.mods`` and supply to
-it the dataset name. This would be the name of the output file, and it
+dataset, you can use the ``yt.load`` command and provide it the dataset name.
+This would be the name of the output file, and it
contains no extension. For instance, if you have the following files:
.. code-block:: none
@@ -53,8 +53,8 @@
Castro. Currently it is cared for by a combination of Andrew Myers, Chris
Malone, Matthew Turk, and Mike Zingale.
-To load a Boxlib dataset, you can use the ``load`` command provided by
-``yt.mods`` and supply to it the directory file name. In general, you must also have the
+To load a Boxlib dataset, you can use the ``yt.load`` command on
+the plotfile directory name. In general, you must also have the
``inputs`` file in the base directory, but Maestro and Castro will get
all the necessary parameter information from the ``job_info`` file in
the plotfile directory. For instance, if you were in a
@@ -92,8 +92,7 @@
----------
FLASH HDF5 data is *mostly* supported and cared for by John ZuHone. To load a
-FLASH dataset, you can use the ``load`` command provided by ``yt.mods`` and
-supply to it the file name of a plot file or checkpoint file, but particle
+FLASH dataset, you can use the ``yt.load`` command and provide it the file name of a plot file or checkpoint file, but particle
files are not currently directly loadable by themselves, due to the fact that
they typically lack grid information. For instance, if you were in a directory
with the following files:
@@ -130,8 +129,7 @@
In yt-3.0, RAMSES data is fully supported. If you are interested in taking a
development or stewardship role, please contact the yt-dev mailing list. To
-load a RAMSES dataset, you can use the ``load`` command provided by ``yt.mods``
-and supply to it the ``info*.txt`` filename. For instance, if you were in a
+load a RAMSES dataset, you can use the ``yt.load`` command and provide it the ``info*.txt`` filename. For instance, if you were in a
directory with the following files:
.. code-block:: none
@@ -428,8 +426,8 @@
interested in using yt for ART data, or if you are interested in assisting with
development of yt to work with ART data.
-To load an ART dataset you can use the ``load`` command provided by
-``yt.mods`` and passing the gas mesh file. It will search for and attempt
+To load an ART dataset you can use the ``yt.load`` command and provide it
+ the gas mesh file. It will search for and attempt
to find the complementary dark matter and stellar particle header and data
files. However, your simulations may not follow the same naming convention.
https://bitbucket.org/yt_analysis/yt/commits/dc039dac15ea/
Changeset: dc039dac15ea
Branch: yt-3.0
User: ngoldbaum
Date: 2014-07-30 21:34:11
Summary: Merged in mzingale/yt/yt-3.0 (pull request #1107)
update the BoxLib stuff -- in particular, we don't always need inputs
Affected #: 1 file
diff -r 9e9340f674c36c5a7cab79640253e01a2ee5cd49 -r dc039dac15eab3e343f2a448c176630d1299f3af doc/source/examining/loading_data.rst
--- a/doc/source/examining/loading_data.rst
+++ b/doc/source/examining/loading_data.rst
@@ -12,8 +12,8 @@
---------
Enzo data is fully supported and cared for by Matthew Turk. To load an Enzo
-dataset, you can use the ``load`` command provided by ``yt.mods`` and supply to
-it the dataset name. This would be the name of the output file, and it
+dataset, you can use the ``yt.load`` command and provide it the dataset name.
+This would be the name of the output file, and it
contains no extension. For instance, if you have the following files:
.. code-block:: none
@@ -51,11 +51,13 @@
yt has been tested with Boxlib data generated by Orion, Nyx, Maestro and
Castro. Currently it is cared for by a combination of Andrew Myers, Chris
-Malone, and Matthew Turk.
+Malone, Matthew Turk, and Mike Zingale.
-To load a Boxlib dataset, you can use the ``load`` command provided by
-``yt.mods`` and supply to it the directory file name. **You must also have the
-``inputs`` file in the base directory.** For instance, if you were in a
+To load a Boxlib dataset, you can use the ``yt.load`` command on
+the plotfile directory name. In general, you must also have the
+``inputs`` file in the base directory, but Maestro and Castro will get
+all the necessary parameter information from the ``job_info`` file in
+the plotfile directory. For instance, if you were in a
directory with the following files:
.. code-block:: none
@@ -81,14 +83,16 @@
import yt
ds = yt.load("pltgmlcs5600")
+For Maestro and Castro, you would not need the ``inputs`` file, and you
+would have a ``job_info`` file in the plotfile directory.
+
.. _loading-flash-data:
FLASH Data
----------
FLASH HDF5 data is *mostly* supported and cared for by John ZuHone. To load a
-FLASH dataset, you can use the ``load`` command provided by ``yt.mods`` and
-supply to it the file name of a plot file or checkpoint file, but particle
+FLASH dataset, you can use the ``yt.load`` command and provide it the file name of a plot file or checkpoint file, but particle
files are not currently directly loadable by themselves, due to the fact that
they typically lack grid information. For instance, if you were in a directory
with the following files:
@@ -125,8 +129,7 @@
In yt-3.0, RAMSES data is fully supported. If you are interested in taking a
development or stewardship role, please contact the yt-dev mailing list. To
-load a RAMSES dataset, you can use the ``load`` command provided by ``yt.mods``
-and supply to it the ``info*.txt`` filename. For instance, if you were in a
+load a RAMSES dataset, you can use the ``yt.load`` command and provide it the ``info*.txt`` filename. For instance, if you were in a
directory with the following files:
.. code-block:: none
@@ -423,8 +426,8 @@
interested in using yt for ART data, or if you are interested in assisting with
development of yt to work with ART data.
-To load an ART dataset you can use the ``load`` command provided by
-``yt.mods`` and passing the gas mesh file. It will search for and attempt
+To load an ART dataset you can use the ``yt.load`` command and provide it
+ the gas mesh file. It will search for and attempt
to find the complementary dark matter and stellar particle header and data
files. However, your simulations may not follow the same naming convention.
Repository URL: https://bitbucket.org/yt_analysis/yt/
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