Flows and Motions in Moss in the Core of a Flaring Active Region: Evidence for Steady Heating
David H. Brooks, Harry P. Warren

TL;DR
This study uses high-resolution spectroscopic data to show that moss in an active region core is heated in a steady manner, with minimal observed flows or variability despite nearby flaring activity.
Contribution
First high-cadence, spatially resolved measurements of moss velocities, demonstrating steady heating in a flare-active region core.
Findings
Moss intensity varies less than 15% over 16 hours.
No significant Doppler or non-thermal velocity variations detected.
Results support quasi-steady heating in active region moss.
Abstract
We present new measurements of the time variability of intensity, Doppler and non-thermal velocities in moss in an active region core observed by the EUV Imaging Spectrometer on Hinode in 2007, June. The measurements are derived from spectral profiles of the Fe 12 195A line. Using the 2" slit, we repeatedly scanned 150" by 150" in a few mins. This is the first time it has been possible to make such velocity measurements in the moss, and the data presented are the highest cadence spatially resolved maps of moss Doppler and non-thermal velocities ever obtained in the corona. The observed region produced numerous C- and M- class flares with several occurring in the core close to the moss. The magnetic field was therefore clearly changing in the active region core, so we ought to be able to detect dynamic signatures in the moss if they exist. Our measurements of moss intensities agree with…
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