gatherresults(filefilter, pol, excludelist, ...) | This function returns a dictionary with selected results from file in the subdirectories (/pol?/*/) of the filedir that are needed for the plotfootprint task. |
obtainvalue(par, key) | This function returns the value from a parameter dict or a default value if the key does not exist |
plotfootprint([ws, parfile]) | Description: |
A tool to plot the footprint of a cosmic ray event with the superterp as background.
Module author: Sander ter Veen <s.terveen@astro.ru.nl>
This function returns a dictionary with selected results from file in the subdirectories (/pol?/*/) of the filedir that are needed for the plotfootprint task.
This function returns the value from a parameter dict or a default value if the key does not exist
Description:
Plots the footprint of the air shower on the ground. It will automatically assign colors to the arrivaltimes and scale the size with the signal power. The footprint is only suitable for stations that have seen a signal. To see also other stations set goodonly = False in the options. But note that then neither colors nor size will make any sense. It can also draw the LORA detector either in static or also with time information (plotlora = True, loracolor=”time”). You need to have LORA data available on your computer. Without the LORA data only the shower geometry can be shown.
Usage:
See example.
Example:
- ::
- polarization=0 filefilter=”/data/VHECR/LORAtriggered/LORA/results/VHECR_LORA-20110716T094509.665Z/” loradir = “/data/VHECR/LORAtriggered/LORA/” crfootprint=cr.trun(“plotfootprint”,filefilter=filefilter,pol=polarization,loradir=loradir)
Input parameters
results
Output parameters