Paper
11 February 2003 Diverse phase speckle inversion applied to data from the Swedish 1-meter solar telescope
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Abstract
We report on the use of a new joint phase diverse speckle code, an implementation of a method where a single object and individual phases are estimated from several pairs of phase diverse data. The code was used on 430.5 nm G-band data collected with the newly installed Swedish 1-meter solar telescope in La Palma, equipped with a low-order adaptive optics system. We describe the algorithm briefly, show wavefront statistics and object estimates from the processing and discuss the results. We demonstrate a resolution of 0.12 arc seconds for a time sequence and a large field of view, which is a break-through for ground based solar telescopes.
© (2003) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Mats G. Lofdahl and Goran B. Scharmer "Diverse phase speckle inversion applied to data from the Swedish 1-meter solar telescope", Proc. SPIE 4853, Innovative Telescopes and Instrumentation for Solar Astrophysics, (11 February 2003); https://doi.org/10.1117/12.460285
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CITATIONS
Cited by 12 scholarly publications.
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KEYWORDS
Wavefronts

Adaptive optics

Solar telescopes

Speckle

Image restoration

Telescopes

Signal to noise ratio

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