Directory Structure and Data Products

Once user started a MeerSOLAR pipeline job, MeerSOLAR assign a unique JobID based on current time in millisecond precision in YYYYMMDDHHMMSSmmm format. Note down the Job ID to view the logger.

The following output will appear in terminal:

########################################
Starting MeerSOLAR Pipeline....
#########################################

###########################
MeerSOLAR Job ID: <YYYYMMDDHHMMSSmmm>
Work directory: <workdir>
Final product directory: <outputdir>
###########################

Directory structure

All data intermediate data products will be saved in <workdir>.

All final data products will be saved in <outputdir>.

Note

In local workstations, it is okay to choose <workdir> and <outputdir>. In HPC environment, generally, high-speed disks are used during data-processing, which may have limited storage life-time, and has seperate long-term storage disks. It is recommended to choose <workdir> path inside the high-speed disk and <outputdir> inside the long-term storage disk. Otherwise, there may be possiblity that final data-products will be removed after certain time.

Data products

Pipeline produces calibrated visibilities as well as several imaging products.

Dynamic spectrum

Dynamic spectra for all (or the ones selected) target scans are available in dynamic_spectra directory inside the output directory <outputdir>.

Diagnostic plots

Diagnostic plots for all measurement sets and calibration tables in pdf format in diagnostic_plots directory inside the output directory <outputdir>.

Calibrated visibilities

Calibrated measurements sets for all (or the ones selected) target scans will be available in work directory <workdir> with naming format, targets_scan_<scan_number>_spw_<channel_range>.ms. Calibrated measurement sets will not be saved in output directory <outputdir> (unless same as <workdir>) to save space.

Imaging products

Imaging products are available in imagedir_f_<freqres>_t_<timeres>_w_<weight>_<robust> directory inside output directory <outputdir>. If imaging is performed with different time and frequency resolutions or different weighting schemes, seperate image directories with corresponding parameters will have the corresponding images.

  1. Image fits in RA/DEC - Fits images in RA/DEC coordinate are available in imagedir_f_<freqres>_t_<timeres>_w_<weight>_<robust>/images directory inside work directory. These are not primary beam corrected.

Note

All fits images have some MeerSOLAR specific metadata in the header and some image statistics.

  1. Primary beam corrected image fits - Primary beam corrected fits images are available in imagedir_f_<freqres>_t_<timeres>_w_<weight>_<robust>/pbcor_images directory inside work directory.

  2. Brightness temperature image fits - Brightness temperature fits images are available in imagedir_f_<freqres>_t_<timeres>_w_<weight>_<robust>/tb_images directory inside work directory.

  3. CLEAN model and residual fits - CLEAN model and residual images are available in imagedir_f_<freqres>_t_<timeres>_w_<weight>_<robust>/models and imagedir_f_<freqres>_t_<timeres>_w_<weight>_<robust>/residuals directory inside work directory. These are not saved only if keep_backup option is switched on.

  4. Radio images in helioprojective coordinates - Directory names hpcs inside directories like, images, pbcor_images, tb_images inside the image directory will have the FITS images in helioprojective coordinates. Images in PNG and PDF formats are also available in pngs and pdfs directories inside the parent directories.

Note

Header of helioprojective maps have wavelength information in unit of centimeter or meter.

  1. Overlays on GOES-SUVI EUV images - Overlays on GOES SUVI EUV (193 Å) images are saved in PNG and PDF formats in imagedir_f_<freqres>_t_<timeres>_w_<weight>_<robust>/overlays_pngs and imagedir_f_<freqres>_t_<timeres>_w_<weight>_<robust>/overlays_pngs, respectively.