TRACE is a single-instrument solar mission that will be put into a Sun
-synchronous polar orbit and will obtain continuous solar observations
for about 8 months per year. It will collect images of solar plasmas
at temperatures from 10(4) to 10(7) K, with 1-arcsec spatial resolutio
n and excellent temporal resolution and continuity. With such data, we
expect to gain a new understanding of many solar and stellar problems
ranging from coronal heating to impulsive magnetohydrodynamic phenome
na.