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.
Keith Arnaud (kaa@genji.gsfc.nasa.gov)
Mon Sep 18 14:36:38 EDT 1995
. The
abundance ratios are set by the abund command.
