The Next Generation of Chromospheric Measurements

Details The Next Generation of Chromospheric Measurements The Next Generation of Chromospheric Measurements

May 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005agusmsh12a..06t&link_type=abstract

American Geophysical Union, Spring Meeting 2005, abstract #SH12A-06

Physics

7507 Chromosphere, 7524 Magnetic Fields, 7546 Transition Region, 7594 Instruments And Techniques

Scientific paper

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.

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