Solar Physics

, Volume 187, Issue 2, pp 347–356

Resolution Improvement of Solar Images

  • Noriaki Miura
  • Naoshi Baba
  • Takashi Sakurai
  • Kiyoshi Ichimoto
  • Dirk Soltau
  • Peter Brandt
Article

DOI: 10.1023/A:1005107223372

Cite this article as:
Miura, N., Baba, N., Sakurai, T. et al. Sol Phys (1999) 187: 347. doi:10.1023/A:1005107223372

Abstract

A method for the improvement of resolution in an observed solar image is proposed. A blind deconvolution method is used for restoration of an atmospherically-degraded solar image, and a super-resolution method is applied to its restored image to improve the resolution. It is confirmed that a blind deconvolution process can restore fine structures that are blurred in an observed image, and that the super-resolution process can make a cutoff frequency in a blind-deconvolved image higher. A time series of super-resolved images of a sunspot observed with the 70-cm Vacuum Tower Telescope at Teide Observatory is presented.

Copyright information

© Kluwer Academic Publishers 1999

Authors and Affiliations

  • Noriaki Miura
    • 1
  • Naoshi Baba
    • 2
  • Takashi Sakurai
    • 3
  • Kiyoshi Ichimoto
    • 3
  • Dirk Soltau
    • 4
  • Peter Brandt
    • 4
  1. 1.Department of Computer SciencesKitami Institute of TechnologyKitamiJapan
  2. 2.Department of Applied Physics, Faculty of EngineeringHokkaido UniversitySapporoJapan
  3. 3.National Astronomical Observatory of JapanMitakaJapan
  4. 4.Kiepenheuer-Institut für SonnenphysikFreiburg i. Br.Germany