  This work utilizes Improved Solar Observing Optical Network (ISOON: Neidig et
al. 2003) continuum (630.2 nm) and H{\alpha} (656.2 nm) data to: 1) detect and
measure intrinsic sunspot rotations occurring in the photosphere and
chromosphere, 2) identify and measure chromospheric filament mass motions, and
3) assess any large-scale photospheric and chromospheric mass couplings.
Significant results from October 27-29, 2003, using the techniques of Brown et
al. (2003), indicate significant counter-rotation between the two large
sunspots in NOAA AR 10486 on October 29, as well as discrete filament mass
motions in NOAA AR 10484 on October 27 that appears associated with at least
one C-class solar flare.
