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Coordinated Observations of X-ray and High-Resolution EUV Active Region DynamicsThe recently-launched High-resolution Coronal imager (Hi-C) sounding rocket provided the highest resolution images of coronal loops and other small-scale structures in the 193 Angstrom passband to date. With just 5 minutes of observations, the instrument recorded a variety of dynamic coronal events -- including even a small B-class flare. We will present our results comparing these extreme-ultraviolet (EUV) observations with X-ray imaging from Hinode/XRT as well as EUV AIA data to identify sources of hot plasma rooted in the photosphere and track their affect on the overall topology and dynamics of the active region.
Document ID
20140011666
Acquisition Source
Marshall Space Flight Center
Document Type
Presentation
Authors
Savage, Sabrina (NASA Marshall Space Flight Center Huntsville, AL, United States)
Cirtain, Jonathan (NASA Marshall Space Flight Center Huntsville, AL, United States)
Winebarger, Amy (NASA Marshall Space Flight Center Huntsville, AL, United States)
Kobayashi, Ken (Alabama Univ. Huntsville, AL, United States)
Golub, Leon (Smithsonian Astrophysical Observatory Cambridge, MA, United States)
Korreck, Kelly (Smithsonian Astrophysical Observatory Cambridge, MA, United States)
Date Acquired
September 12, 2014
Publication Date
November 12, 2013
Subject Category
Solar Physics
Spacecraft Instrumentation And Astrionics
Report/Patent Number
M13-3077
Meeting Information
Meeting: Hinode Science Meeting
Location: Takayama
Country: Japan
Start Date: November 12, 2013
End Date: November 15, 2013
Sponsors: National Astronomical Observatory, Japan Aerospace Exploration Agency, Kyoto Univ.
Distribution Limits
Public
Copyright
Public Use Permitted.

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