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High-Resolution Solar Imaging Using Blind Deconvolution

  • K. Hartkorn
Conference paper
Part of the Astrophysics and Space Science Library book series (ASSL, volume 259)

Abstract

In every imaging system, there are certain effects that modify the initial intensity distribution of the observed object into the measured intensity distribution.

Keywords

Reconstruction Algorithm Solar Phys Pointspread Function Iteration Number Conjugate Gradient Method 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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References

  1. Christou, J., http://www.eso.org/jchristo/bd/bd.html.Google Scholar
  2. Jefferies, S. and Christou, J.: 1993, ApJ 415, 862.ADSCrossRefGoogle Scholar
  3. Miura, N., Baba, N., Sakurai, T., Ichimoto, K, Soltau, D., and Brandt, P.: 1999, Solar Phys. 187, 347.ADSCrossRefGoogle Scholar
  4. Tsumuraya, F., Miura, N., and Baba, N.: 1994, A&A 282, 699.ADSGoogle Scholar

Copyright information

© Springer Science+Business Media Dordrecht 2001

Authors and Affiliations

  • K. Hartkorn
    • 1
  1. 1.Kiepenheuer-Institut für SonnenphysikFreiburgGermany

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