112 citations · 422 across the 7 of their papers we have counts for
9 papers
Hinode/Extreme-Ultraviolet Imaging Spectrometer Observations of the Temperature Structure of the Quiet Corona
David H. Brooks, Harry P. Warren, David R. Williams +1
We present a Differential Emission Measure (DEM) analysis of the quiet solar corona on disk using data obtained by the Extreme-ultraviolet Imaging Spectrometer (EIS) on {\it Hinode…
Flows and Motions in Moss in the Core of a Flaring Active Region: Evidence for Steady Heating
David H. Brooks, Harry P. Warren
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 Hi…
The Temperature and Density Structure of the Solar Corona. I. Observations of the Quiet Sun with the EUV Imaging Spectrometer (EIS) on Hinode
Harry P. Warren, David H. Brooks
Measurements of the temperature and density structure of the solar corona provide critical constraints on theories of coronal heating. Unfortunately, the complexity of the solar at…
Observations of Active Region Loops with the EUV Imaging Spectrometer on Hinode
Harry P. Warren, Ignacio Ugarte-Urra, George A. Doschek +2
Previous solar observations have shown that coronal loops near 1 MK are difficult to reconcile with simple heating models. These loops have lifetimes that are long relative to a ra…
Observations of Solar Doppler Shift Oscillations with the EUV Imaging Spectrometer on Hinode
John T. Mariska, Harry P. Warren, David R. Williams +1
Damped Doppler shift oscillations have been observed in emission lines from ions formed at flare temperatures with the Solar Ultraviolet Measurements of Emitted Radiation spectrome…
Modeling X-ray Loops and EUV "Moss" in an Active Region Core
A. R Winebarger, H. P. Warren, D. A. Falconer
The Soft X-ray intensity of loops in active region cores and corresponding footpoint, or moss, intensity observed in the EUV remain steady for several hours of observation. The ste…