Overview of XRT performance and first results

Details Overview of XRT performance and first results Overview of XRT performance and first results

May 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008iaus..247..326s&link_type=abstract

Waves & Oscillations in the Solar Atmosphere: Heating and Magneto-Seismology, Proceedings of the International Astronomical Unio

Other

Instrumentation: Detectors, Instrumentation: High Angular Resolution, Sun: Corona, Sun: Magnetic Fields

Scientific paper

In this review we present a short introduction to the X-ray Telescope on Hinode. We discuss its capabilities and new features and compare it with Yohkoh SXT. We also discuss some of the first results that include observations of X-ray jets in coronal holes, shear change in flares, sigmoid eruptions and evolution, application of filter ratios and differential emission measure analysis, structure of active regions, fine structure of X-ray bright points, and modeling non-potential fields around filaments. Finally, we describe how XRT works with other ground and space-based instrumentation, in particular with TRACE, EIS, SOT, and SOLIS.

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