173 citations · 2.3k across the 52 of their papers we have counts for
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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…
Observation and Modeling of Coronal "Moss" With the EUV Imaging Spectrometer on Hinode
Harry P. Warren, Amy R. Winebarger, John T. Mariska +2
Observations of transition region emission in solar active regions represent a powerful tool for determining the properties of hot coronal loops. In this Letter we present the anal…
The Magnetic Topology of Coronal Mass Ejection sources
I. Ugarte-Urra, H. P. Warren, A. R. Winebarger
In an attempt to test current initiation models of coronal mass ejections (CMEs), with an emphasis on the magnetic breakout model, we inspect the magnetic topology of the sources o…
Static and Dynamic Modeling of a Solar Active Region. I: Soft X-Ray Emission
Harry P. Warren, Amy R. Winebarger
Recent simulations of solar active regions have shown that it is possible to reproduce both the total intensity and the general morphology of the high temperature emission observed…
Hydrostatic Modeling of the Integrated Soft X-Ray and EUV Emission in Solar Active Regions
Harry P. Warren, Amy R. Winebarger
Many studies of the solar corona have shown that the observed X-ray luminosity is well correlated with the total unsigned magnetic flux. In this paper we present results from the e…
Cooling Active Region Loops Observed With SXT and TRACE
Amy R. Winebarger, Harry P. Warren
An Impulsive Heating Multiple Strand (IHMS) Model is able to reproduce the observational characteristics of EUV (~ 1 MK) active region loops. This model implies that some of the lo…