This paper presents the coronal ionization state distribution for argon. Th
e calculations include ab initio rate coefficients for collisional excitati
on followed by autoionization (EA), and rates for direct ionization and die
lectronic and radiative recombination. The EA rate coefficients have been f
itted to analytical expressions, and the fitting coefficients are tabulated
. The paper then presents the calculated radiative cooling coefficient for
argon ions in a low-density plasma as a function of temperature. The channe
ls for power loss from argon ions include collisional-radiative (CR) line e
mission, dielectronic and radiative recombination, and bremsstrahlung emiss
ion. The power emitted via CR line emission for each ion is tabulated on a
grid of temperatures and densities. The total power loss coefficient is fit
ted to an analytical expression in powers of the temperature. (C) 1998 Acad
emic Press.