activity
20112026
most citedAn Observational Overview of Solar Flares

850 citations · 2.3k across the 67 of their papers we have counts for

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Showing 2015Show all

6 papers · 1 filter

astro-ph.SR2015★ 11 cited

Flare Footpoint Regions and a Surge Observed by the Hinode/EUV Imaging Spectrometer (EIS), RHESSI, and SDO/AIA

George A. Doschek, Harry P. Warren, Brian R. Dennis +2

The Extreme-ultraviolet Imaging Spectrometer (EIS) on the Hinode spacecraft observed flare footpoint regions coincident with a surge for a M3.7 flare observed on 25 September 2011…

astro-ph.SR2015★ 41 cited

Benchmark Test of Differential Emission Measure Codes and Multi-Thermal Energies in Solar Active Regions

M. J. Aschwanden, P. Boerner, A. Caspi +3

We compare the ability of 11 Differential Emission Measure (DEM) forward-fitting and inversion methods to constrain the properties of active regions and solar flares by simulating…

astro-ph.IM2015★ 28 cited

Hard X-Ray Imaging of Individual Spectral Components in Solar Flares

Amir Caspi, Albert Y. Shih, James M. McTiernan +1

We present a new analytical technique, combining Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI) high-resolution imaging and spectroscopic observations, to visualize…

astro-ph.IM2015★ 60 cited

Miniature X-Ray Solar Spectrometer (MinXSS) - A Science-Oriented, University 3U CubeSat

James P. Mason, Thomas N. Woods, Amir Caspi +7

The Miniature X-ray Solar Spectrometer (MinXSS) is a 3-Unit (3U) CubeSat developed at the Laboratory for Atmospheric and Space Physics (LASP) at the University of Colorado, Boulder…

astro-ph.SR2015★ 85 cited

Global Energetics of Solar Flares: II. Thermal Energies

M. J. Aschwanden, P. Boerner, D. Ryan +3

We present the second part of a project on the global energetics of solar flares and CMEs that includes about 400 M- and X-class flares observed with AIA/SDO during the first 3.5 y…

astro-ph.SR2015★ 56 cited

New Observations of the Solar 0.5-5 keV Soft X-ray Spectrum

Amir Caspi, Thomas N. Woods, Harry P. Warren

The solar corona is orders of magnitude hotter than the underlying photosphere, but how the corona attains such high temperatures is still not understood. Soft X-ray (SXR) emission…