On the Combination of Differential Emission Measure Analysis and Rotational Tomography for Three‐dimensional Solar EUV Imaging

2005 ◽  
Vol 628 (2) ◽  
pp. 1070-1080 ◽  
Author(s):  
R. A. Frazin ◽  
F. Kamalabadi ◽  
M. A. Weber
Keyword(s):  
Emission Measure ◽  
Three Dimensional ◽  
Differential Emission Measure ◽  
Measure Analysis ◽  
Euv Imaging

scholarly journals The 3D solar minimum with differential emission measure tomography

2011 ◽  
Vol 7 (S286) ◽  
pp. 123-133
Author(s):  
Alberto M. Vásquez ◽  
Richard A. Frazin ◽  
Zhenguang Huang ◽  
Ward B. Manchester ◽  
Paul Shearer
Keyword(s):  
Extreme Ultraviolet ◽  
Emission Measure ◽  
Three Dimensional ◽  
Differential Emission Measure ◽  
Height Range ◽  
Heliospheric Observatory ◽  
Temperature Distributions ◽  
Imaging Telescope ◽  
Electron Density And Temperature ◽  
Comparative Results

AbstractDifferential emission measure tomography (DEMT) makes use of extreme ultraviolet (EUV) image series to deliver two products: a) the three-dimensional (3D) reconstruction of the coronal emissivity in the instrumental bands, and b) the 3D distribution of the local differential emission measure (LDEM). The LDEM allows, in turn, construction of 3D maps of the electron density and temperature distribution. DEMT is being currently applied to the space-based EUV imagers, allowing reconstruction of the inner corona in the height range 1.00 to 1.25 R⊙. In this work we applied DEMT to different Carrington Rotations corresponding to the last two solar Cycle minima. To reconstruct the 2008 minimum we used data taken by the Extreme UltraViolet Imager (EUVI), on board the Solar TErrestrial RElations Observatory (STEREO) spacecraft, and to reconstruct the 1996 minimum we used data taken by the Extreme ultraviolet Imaging Telescope (EIT), on board the Solar and Heliospheric Observatory (SOHO). We show here comparative results, discussing the observed 3D density and temperature distributions in the context of global potential magnetic field extrapolations. We also compare the DEMT results with other observational and modeling efforts of the same periods.

scholarly journals Overview of XRT performance and first results

2007 ◽  
Vol 3 (S247) ◽  
pp. 326-336
Author(s):  
Antonia Savcheva ◽  
Keyword(s):  
Fine Structure ◽  
Coronal Holes ◽  
Emission Measure ◽  
Active Regions ◽  
Potential Fields ◽  
Differential Emission Measure ◽  
Short Introduction ◽  
X Ray ◽  
First Results ◽  
Measure Analysis

AbstractIn this review we present a short introduction to the X-ray Telescope on Hinode. We discuss its capabilities and new features and compare it with Yohkoh SXT. We also discuss some of the first results that include observations of X-ray jets in coronal holes, shear change in flares, sigmoid eruptions and evolution, application of filter ratios and differential emission measure analysis, structure of active regions, fine structure of X-ray bright points, and modeling non-potential fields around filaments. Finally, we describe how XRT works with other ground and space-based instrumentation, in particular with TRACE, EIS, SOT, and SOLIS.

scholarly journals FOXSI-2 Solar Microflares. I. Multi-instrument Differential Emission Measure Analysis and Thermal Energies

2020 ◽  
Vol 891 (1) ◽  
pp. 78 ◽  
Author(s):  
P. S. Athiray ◽  
Juliana Vievering ◽  
Lindsay Glesener ◽  
Shin-nosuke Ishikawa ◽  
Noriyuki Narukage ◽  
...  
Keyword(s):  
Emission Measure ◽  
Differential Emission Measure ◽  
Measure Analysis

scholarly journals Differential emission measure analysis of hot-flare plasma from solar-maximum mission X-ray data

1984 ◽  
Vol 4 (7) ◽  
pp. 203-207 ◽  
Author(s):  
J. Jakimiec ◽  
J. Sylwester ◽  
J.R. Lemen ◽  
R. Mewe ◽  
R.D. Bentley ◽  
...  
Keyword(s):  
Solar Maximum ◽  
Emission Measure ◽  
Differential Emission Measure ◽  
Solar Maximum Mission ◽  
X Ray ◽  
Measure Analysis ◽  
Flare Plasma
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