The COronal Solar Magnetism Observatory (COSMO) K-coronagraph (K-Cor) is one of three proposed instruments in the COSMO facility suite. It is specifically designed to study the formation and dynamics of coronal mass ejections and the evolution of the density structure of the low corona. The K-Cor records the polarization brightness (pB) formed by Thomson scattering of photospheric light by coronal free electrons. The National Center for Atmospheric Research (NCAR), via the National Science Foundation (NSF), provided full funding for the COSMO K-Cor, which was deployed to the Mauna Loa Solar Observatory (MLSO) in Hawaii in September 2013, replacing the aging MLSO Mk4 K-coronameter.
This pipeline produces level 1 and level 2 data products from the raw data from the instrument. The level 1 product contains polarization brightness (pB) images of the corona and sky, pB of the sky only, and total intensity, while the level 2 product contains pB images with sky polarization removed.
There is a near real-time component of the pipeline which produces fully calibrated level 2 pB images along with an end-of-day component which produces averages, differences, and many engineering products.
- IDL 8 or later
- cmake 3.1.3 or later
- MySQL developer installation
- Python 2.7+ (including 3.x) in order to run command line utility script including the simulators, the production pipeline does not strictly require Python
To build the KCor pipeline code, your system must have IDL, the MySQL client development package, and CMake 3.1.3 or later. Make sure these are installed on your system before continuing.
These instructions will work on Linux and Mac systems. It should be possible to install the KCor pipeline on Windows systems, but it is not described here.
To configure the KCor pipeline for your system, do the following from the top-level of the pipeline source code (change the location of your IDL installation and the location where you want the pipeline to your needs):
cd kcor-pipeline
mkdir build
cmake \
-DCMAKE_INSTALL_PREFIX:PATH=~/software/kcor-pipeline \
-DIDL_ROOT_DIR:PATH=/opt/share/idl8.5/idl85 \
..
There are example configuration scripts, linux_configure.sh and mac_configure.sh, in the pipeline source code that are more detailed examples of the above configuration command.
Next, to build and install the KCor pipeline, run:
cd build
make install
The options of the pipeline are specified via a configuration file. See the configuration specification file kcor.spec.cfg in the config directory of the distribution for all the options and their documentation. The filename of the config file must match the pattern kcor.[NAME].cfg with a name such as "production", "latest", or "geometry-fix". These configuration files must be placed in the config/ directory.
All files with the cfg extension in the config directory will be copied into the installation during a make install.
For example, to process the data from 20220712 with the kcor.latest.cfg configuration file use the kcor utility script in the bin/ directory of the installation:
kcor process -f latest 20220712
Creating the configuration file, in this case kcor.latest.cfg, is the main work in running the pipeline.
- analysis for routines to perform various analyses of KCor data
- bin for shell and Python scripts
- cmake for CMake modules
- cme_detection for code for the automated CME detection pipeline
- config for configuration files
- gen for non-KCor-specific MLSO IDL routines used in the KCor pipeline
- hv for helioviewer specific IDL code
- lib for 3rd party IDL routines used in KCor pipeline
- observing for KCor-related observing code
- resources for data files such as color tables used in KCor pipeline
- scripts for various scripts to be run on processed data
- src for KCor pipeline IDL code
- ssw for SSW IDL routines used in KCor pipeline
- stream for code to remove aerosols in real-time from stream data
- unit for unit tests