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   52011
   ASCA and EUVE spectra of active single stars, RS CVn's and Algol
   binaries show highly active coronae to be depleted in metals relative
   to the photosphere by factors of ~2-10. In contrast, spectra of lower
   activity stars like the Sun exhibit the "FIP Effect" in which elements
   with low first ionization potential (FIP), such as Fe, are enhanced
   relative to the photoshere - a totally opposite effect! Simultaneous
   ASCA and EUVE observations of the X-ray brightest intermediate activity
   star ksi UMa B would provide the first measure of coronal abundance
   anomalies at the missing key intermediate activity level, completing
   the picture of coronal abundance anomalies from low to high activity
   levels and telling us whether or not the metal poor and FIP Effect
   coronae are related.
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