A multi-temperature plasma emission model built from the mekal code. Emission
measures follow a power-law in temperature (ie emission measure from
temperature T is proportional to . The abundance
ratios are set by the abund command. The switch parameter determines
whether the mekal code will be run to calculate the model spectrum for
each temperature or whether the model spectrum will be interpolated from
a pre-calculated table. The former is slower but more accurate.
par1 = index for power-law emissivity functionpar2 = maximum temperature
par3 = nH (cm
)
par4 = Abundance relative Solar
par5 = Redshift
par6 = 0
calculate, 1
interpolate
K = Normalization