Astronomy and Astrophysics – Astronomy
Scientific paper
May 2009
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009spd....40.3502s&link_type=abstract
American Astronomical Society, SPD meeting #40, #35.02; Bulletin of the American Astronomical Society, Vol. 41, p.867
Astronomy and Astrophysics
Astronomy
Scientific paper
The AIA on SDO will offer arcsecond-resolution coronal imaging at a wide range of temperatures, at 10s cadence, with continuous full-disk coverage, supported by HMI's (vector-)magnetography. These properties can be expected to stimulate advances in particular where large fields of view, continuous coverage, large samples, comprehensive yet differentiating thermal coverage, coronal field modeling, or high cadence are required. In this context, I plan to look forward to the SDO era by focusing on some of the key scientific questions about the solar corona that can be addressed particularly well with SDO, and on their associated problems. These topics include flux emergence and reconnection with pre-existing field, the powering of flares and CMEs, the thermal structure of the active-region corona, quiet-Sun filaments and their field configurations, and coronal seismology.
No associations
LandOfFree
Observing and Modeling the Effects of the Solar Magnetic Field in the Corona does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Observing and Modeling the Effects of the Solar Magnetic Field in the Corona, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Observing and Modeling the Effects of the Solar Magnetic Field in the Corona will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1113420