
- Calibration of a deformable mirror and Strehl ratio measurements by use of phase diversity
- Astronomy & Astrophysics manuscript no. (will be inserted by hand later)
- Image restoration techniques Variations and new developments
- EST: the European Solar Telescope D. Kiselman, M. Lofdahl & G. Scharmer
- Solar image restoration by use of multi-object multi-frame blind deconvolution Michiel van Noort 1 , Luc Rouppe van der Voort 1 & Mats Lofdahl 2
- THE ASTROPHYSICAL JOURNAL, 509:435447, 1998 December 10 1998. The American Astronomical Society. All rights reserved. Printed in U.S.A.(
- In Space Telescopes and Instruments V, Bely & Breckinridge, eds., Proc. SPIE 3356, Kona, HI, March 1998. A Phase Diversity Experiment to Measure Piston Misalignment on
- Seeing effects blurry images Restoration of seeing-degraded solar images
- Solar image restoration by use of multi-frame blind deconvolution with multiple objects and phase diversity
- Astronomy & Astrophysics manuscript no. 0436 September 7, 2004 (DOI: will be inserted by hand later)
- Astronomy & Astrophysics manuscript no. h4462 October 14, 2003 (DOI: will be inserted by hand later)
- An Algorithm for Resolving 2 Ambiguities in Interferometric
- THE ASTROPHYSICAL JOURNAL, 495:965972, 1998 March 10 1998. The American Astronomical Society. All rights reserved. Printed in U.S.A.(
- Modern Solar Facilities Advanced Solar Science, 119126 F. Kneer, K. G. Puschmann, A. D. Wittmann (eds.)
- To appear in Proc. SPIE 4853-54, Innovative Telescopes and Instrumentation for Solar Astrophysics, Keil & Avakyan, eds., Waikoloa, Hawaii, USA, August 2002. Phase diverse speckle inversion applied to data from
- To appear in Proc. SPIE 4792-21, Image Reconstruction from Incomplete Data II, Bones, Fiddy & Millane, eds., Seattle, Washington, USA, July 2002. Multi-frame blind deconvolution with linear equality constraints
- In Proc. SPIE 4007-105, Adaptive Optical Systems Technologies, Wizinowich, ed., Munich, Germany, March 2000. A Workstation Based Solar/Stellar Adaptive Optics System
- To Appear in Proc. Third International Workshop on Solar Polarization, Tenerife, Spain, 2002, Eds. J. Trujillo Bueno & J. Sanchez Almeida., ASP Conference Series
- The Swedish 1-m Solar Telescope D. Kiselman, M. Lofdahl, G. Scharmer & M. van Noort
- Introduction Phase diversity PD/PDS
- In Proc. SPIE 4013-55, UV, Optical, and IR Space Telescopes and Instruments VI, Breckinridge & Jacobsen, eds., Munich, Germany, March 2000. Resolving Piston Ambiguities when Phasing a Segmented Mirror
- THE ASTROPHYSICAL JOURNAL, 495:973983, 1998 March 10 1998. The American Astronomical Society. All rights reserved. Printed in U.S.A.(
- Image Quality Effects from Wavelength Dependent Pupil Apodisation
- Dark cores in sunspot penumbral Goran B. Scharmer, Boris V. Gudiksen, Dan Kiselman, Mats G. Lofdahl
- 0.05.010.015.020.025.0 0.05.010.015.020.025.0
- In Adaptive Optical System Technologies, Bonnaccini & Tyson, eds., Proc. SPIE 3353, Kona, HI, March 1998. Fast Phase Diversity Wavefront Sensing for Mirror Control
- NSO Workshop 23: Solar MHD: Theory and Observations -a High Spatial Resolution Perspective ASP Conference Series, Vol. preprint, 2005
- THE ASTROPHYSICAL JOURNAL, 506:439449, 1998 October 10 1998. The American Astronomical Society. All rights reserved. Printed in U.S.A.(
- submitted to ApJ Rapid Temporal Variability of Faculae: High Resolution
- Astronomy & Astrophysics manuscript no. 2678 March 18, 2005 (DOI: will be inserted by hand later)
- Presented at the 19th NSO/Sac Peak Summer Workshop 1998 Orthogonalization of Basis Functions for Diagonalized
- In Proc. SPIE 4013-51, UV, Optical, and IR Space Telescopes and Instruments VI, Breckinridge & Jacobsen, eds., Munich, Germany, March 2000. A Predictor Approach to Closed-Loop Phase-Diversity
- To appear in Proc. SPIE 4853-52, Innovative Telescopes and Instrumentation for Solar Astrophysics, Keil & Avakyan, eds., Waikoloa, Hawaii, USA, August 2002. Adaptive optics system for the new Swedish solar telescope
- Multi-frame deconvolution with space-variant point spread functions by use of inverse filtering and Fast Fourier Transform