We present results from sunspot observations obtained by SUMER on SOHO. In
sunspot plumes the EUV spectrum differs from the quiet Sun; continua are ob
served with different slopes and intensities; emission lines from molecular
hydrogen and many unidentified species indicate unique plasma conditions a
bove sunspots. Sunspot plumes ale sites of systematic downflow. We also dis
cuss the propel-ties of sunspot oscillations.