HR: 11:45h
AN: SH12A-06 INVITED     [Abstracts]
TI: The Next Generation of Chromospheric Measurements
AU: * Tarbell, T D
EM: tarbell@lmsal.com
AF: Lockheed Martin Solar & Astrophysics Lab, Dept ADBS, Bldg 252 3251 Hanover St., Palo Alto, CA 94304 United States
AB: I discuss the new measurements which we know will happen, from missions or observatories which are being developed now, as well as the measurements which should happen for further progress. The future is promising, with new missions such as Solar-B, SDO, and SunRise, and new or upgraded observatories, such as SVST, DOT, GREGOR, ATST, and FASR. I also point out significant needs for the future, such as detailed chromospheric spectroscopy of the type which would have been provided by NEXUS or similar instruments.
DE: 7507 Chromosphere
DE: 7524 Magnetic fields
DE: 7546 Transition region
DE: 7594 Instruments and techniques
SC: SPA-Solar and Heliospheric Physics [SH]
MN: 2005 Joint Assembly