  We report the analysis of the high-resolution soft X-ray spectrum of the
nearby F-type star Procyon in the wavelength range from 5 to 175 Angstrom
obtained with the Low Energy Transmission Grating Spectrometer (LETGS) on board
Chandra and with the Reflection Grating Spectrometers (RGS) and the EPIC-MOS
CCD spectrometers on board XMM-Newton. Line fluxes have been measured
separately for the RGS and LETGS. Spectra have been fitted globally to obtain
self-consistent temperatures, emission measures, and abundances. The total
volume emission measure is ~4.1 x 10e50/cm3 with a peak between 1 and 3 MK. No
indications for a dominant hot component (T > 4 MK) were found. We present
additional evidence for the lack of a solar-type FIP-effect, confirming earlier
EUVE results.
