grff_from_dem_map

Attributes

start_tim

Functions

getbeam(fitsfile[, showplt])

convolve_eovsabeam(res_tbmap, eofitsfiles[, tbmapcovfile])

make_sub_map(cur_map[, fov, ref_map])

get_pixel(cur_map, x, y)

cal_dem_map(aiafitsfiles[, outfile, fov, scalefactor, ...])

initGET_MW(libname)

Python wrapper for Codes for computing the solar gyroresonance and free-free radio emissions; both the isothermal

ff_gyre_func(dem_res, temps, freq)

calculate_n_plot(demfile[, tbmapfile, freq, showplt, ...])

main()

Module Contents

grff_from_dem_map.start_tim[source]
grff_from_dem_map.getbeam(fitsfile, showplt=False)[source]
grff_from_dem_map.convolve_eovsabeam(res_tbmap, eofitsfiles, tbmapcovfile='tbmaps_convolved.p')[source]
grff_from_dem_map.make_sub_map(cur_map, fov=None, ref_map=None)[source]
grff_from_dem_map.get_pixel(cur_map, x, y)[source]
grff_from_dem_map.cal_dem_map(aiafitsfiles, outfile='demreg.p', fov=[], scalefactor=1.0, overwrite=False)[source]
grff_from_dem_map.initGET_MW(libname)[source]

Python wrapper for Codes for computing the solar gyroresonance and free-free radio emissions; both the isothermal plasma and the sources described by the differential emission measure (DEM) and differential density metric (DDM) are supported. By Alexey Kuznetsov, February 2021. Original code: https://github.com/kuznetsov-radio/GRFF

This is for the single thread version @param libname: path for locating compiled shared library @return: An executable for calling the GS codes in single thread

grff_from_dem_map.ff_gyre_func(dem_res, temps, freq)[source]
grff_from_dem_map.calculate_n_plot(demfile, tbmapfile='', freq=[], showplt=True, overwrite=False, pxy=None)[source]
grff_from_dem_map.main()[source]