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 abundances
are relative to the Solar abundances 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-par17 = Abundances for He, C, N, O, Ne, Na, Mg, Al, Si, S,
Ar, Ca, Fe, Ni wrt Solar (defined by the abund command)
par18 = Redshift
par19 = 0
calculate, 1
interpolate
K = Normalization