Paper
14 February 2003 Solar polarimetry close to the diffraction limit
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Abstract
Much progress has been made during the last years in obtaining polarimetric observations of the Sun close to the diffraction limit. Here I summarize the problems one encounters when observing close to the diffraction limit of a large solar telescope, review techniques, present examples of recent observations, and discuss the need for further developments of instruments and image reconstruction techniques.
© (2003) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Christoph U. Keller "Solar polarimetry close to the diffraction limit", Proc. SPIE 4843, Polarimetry in Astronomy, (14 February 2003); https://doi.org/10.1117/12.459286
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Cited by 8 scholarly publications.
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KEYWORDS
Polarimetry

Diffraction

Adaptive optics

Speckle imaging

Solar telescopes

Signal to noise ratio

Speckle

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