1. Proposal: Use AIA data to study wave behavior in atmosphere Requires: Images every 10 (20) seconds Wave studies with AIA

2. I. Travel times provide constraint on magnetic field topology 4 mHz - B inclination angle 7 mHz -  ~1 surface 107 hours of Na & K Data from South Pole

3. II. Seismology Dispersion curves should allow identification of wave type

4. III. Wave contribution to dynamics of upper atmosphere EIT 19.5 nm - “Event” 4 mHz - “wave travel time” Detect magnetic reconnection?

6. “Monitoring the chromospheric energy flux” 107 hours of South Pole data

7. “Monitoring the chromospheric energy flux”

8. “Acoustic Portals” Multi-colored overlay of 3(red), 4(green), & 5(blue) mHz PTTs 3minute running waves leaking from sunspot umbra. Progression to lower frequencies (5minute) visible in the penumbra.  “coronal” wave leakage. “acoustic portals” on SG boundaries. “rainbows” in SG interiors  advected magnetic dipoles? Need: full disk, long duration obs. In B, V and I Potential overlap with Coronal Seismology