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Cited by 580

The DOI matches its Crossref record; 3 of the 3 references it cites were found in a registry or an index.

Speckle masking in astronomy: triple correlation theory and applications

Lohmann, Adolf W., Weigelt, Gerd, Wirnitzer, Bernhard·1983·Applied Optics

Abstract

Due to the turbulent atmosphere the resolution of conventional astrophotography is limited to ∼1 sec of arc. However, the speckle-masking method can yield diffraction-limited resolution, i.e., 0.03 sec of arc with a 3.6-m telescope. Speckle masking yields true images of general astronomical objects. No point source is required in the isoplanatic field of the object. We present the theory of speckle masking; it makes use of triple correlations and their Fourier counterparts, the bispectra. We show algorithms for the recovery of the object from genuine astronomical bispectra data.

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Metadata

Authors
Lohmann, A. W., Weigelt, G., & Wirnitzer, B.
Venue
Applied Optics
Published
1983-12-15
Volume
22
Issue
24
Pages
4028
ISSN
  • 0003-6935 (ISSN-L)
  • 1539-4522
OpenAlex
W2041069457
Cited by
580
References
3
FWCI
4.11
Type
journal article
Language
en
Open access
closed

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CoChat. (2026). Citation check: Speckle masking in astronomy: triple correlation theory and applications. https://app.cochat.ai/papers/10.1364/ao.22.004028
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Lohmann, A. W., Weigelt, G., & Wirnitzer, B. (1983). Speckle masking in astronomy: triple correlation theory and applications. Applied Optics. https://doi.org/10.1364/ao.22.004028

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Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.