E-mail:
aschwanden@lmsal.com -
Markus J.Aschwanden (Lockheed Martin Solar & Astrophysics Lab.)
Introduction into Forward-Fitting of HESSI Images
HESSI Data Analysis Meeting / 1999 Oct 22, NASA/GSFC, Greenbelt/MD
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Forward Fitting: Philosophy and Concept
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How suitable is Forward Fitting for solar HXR images ?
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HXT images of 54 solar flares (Aschwanden et al. 1999, ApJ 517, 977; Fig.1)
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2-D Gaussian Decomposition of 54 solar flares (Aschwanden et al. 1999, ApJ 517, 977; Fig.2)
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1-D Gaussian Fit of 54 solar flares (Aschwanden et al. 1999, ApJ 517, 977; Fig.3)
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Numerical steps of Forward-Fitting Algorithm
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Flow-chart of Forward-Fitting Algorithm
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Back-Projection of a single Gaussian source with 3 iterative decompositions
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Modulation Pattern Profiles (in 9 Collimators) of Backprojection and Model
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Applications of Forward-Fitting: Footpoint motion d(t) and spectral location d(E)