``sctrack.x`` - Interpolate ``kaiju`` results along a spacecraft trajectory =========================================================================== Introduction ------------ ``sctrack.x`` is a compiled tool that interpolates ``kaiju`` results onto a user-specified trajectory, typically representing a spacecraft. This is used when comparing ``kaiju`` results to measured data. Before you start ---------------- In order to use ``sctrack.x``, you need the following: * A set of output files from a ``kaiju`` magnetosphere run. * An HDF5 file containing the spacecraft trajectory, with variables ``T``, ``X``, ``Y``, and ``Z``. * An XML file describing the magnetosphere results and the settings for ``sctrack.x``. ``kaiju`` magnetosphere result files ------------------------------------ Any set of ``kaiju`` magnetosphere results can be used. This documentation assumes you used the MPI version the the ``kaiju`` software, e.g. ``gamera_mpi.x``. This should generate a number of HDF5 files which contain the model results from each MPI rank. Assume all result files are in the current directory. The XML file for ``sctrack.x`` ------------------------------ The XML file read by ``chop.x`` should look something like this (file ``chop.xml``): .. code-block:: xml The elements and attributes of the XML file are described below. .. note:: Standard XML is *case-sensitive*. However, the XML parser used by the Fortran code in ``kaiju`` is *case-insensitive*. Therefore, all of the XML tags and attributes described below can be written with any combintion of upper and lower case. * ```` (required): Specifies XML version. * ```` (required): Outer element for all ``kaiju`` elements. * ```` (required): Inner element for CHIMP-specific elements. * ```` (optional): Specify identifying information for the ``kaiju`` results to use, * ``runid`` (optional, default ``"Sim"``): String specifying the runid for the ``kaiju`` results to use as the basis for the extraction. * ```` (required): Describes the results from a MAGE model run. * ``doMHD`` (optional, default ``"F"``): Set to ``"T"`` to pass the full set of magnetohydrodynamic variables to ``sctrack.x``, rather than just the electric and magnetic fields. Includes velocity vector, density and pressure in the output file. See ``ebtypes.F90``. * ``grType`` (optional, default ``"EGG"``): String specifying grid type used by the MAGE output files. Valid values are ``"EGG"``, ``"LFM"``, ``"SPH"``. If the string is not one of the supported grid types, the default value (``"EGG"``) is used, and a warning message is printed. Note that for a magnetosphere simulation, the ``grType`` is nearly always ``"LFM"``. * ``ebfile`` (optional, default ``"ebdata"``): Root name for HDF5 files containing the results produced by a MAGE model run. This is usually the same as the runid. * ``isMPI`` (optional): If ``"T"``, the MAGE results are from an MPI run. * ```` (optional): Data on units system used in the model run. * ``uid`` (optional, default ``"EARTH"``): Name of units system used in the model run. See ``chmpunits.F90``. Valid values are ``"EARTH"``, ``"EARTHCODE"``, ``"JUPITER"``, ``"JUPITERCODE"``, ``"SATURN"``, ``"SATURNCODE"``, ``"HELIO"``, ``"LFM"``, ``"LFMJUPITER"``.. * ```` (required): Options specific to the spacecraft trajectory. ``H5Traj`` (required): Name of HDF5 file containing spacecraft trajectory. The interpolated data will be written back to this file. ``doSmooth`` (required): Set to ``"T"`` to smooth the trajectory, ``F`` otherwise. Running ``sctrack.x`` --------------------- You can now run ``sctrack.x`` with the following command: .. code-block:: bash sctrack.x sctrack.xml The extracted data will be in the file defined in the ``H5Traj`` attribute.