Hot Coronal Plasma Seen by SDO/AIA and Hinode/XRT

Details Hot Coronal Plasma Seen by SDO/AIA and Hinode/XRT Hot Coronal Plasma Seen by SDO/AIA and Hinode/XRT

May 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aas...21640227d&link_type=abstract

American Astronomical Society, AAS Meeting #216, #402.27; Bulletin of the American Astronomical Society, Vol. 41, p.877

Astronomy and Astrophysics

Astronomy

Scientific paper

The normal incidence telescopes on SDO/AIA cover coronal emission from Fe VIII, IX, XII, XIV, XVI, XVIII, XX, XXIII, and XXIV. The grazing incidence soft x-ray telescope on Hinode/XRT covers emission from 4-60A, including the critical Fe XVII L-Shell emission. We will compare the morphology and dynamics of active regions transient brightenings seen with AIA and XRT to understand the complementarity of these two telescopes.

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