0

Full Content is available to subscribers

Subscribe/Learn More  >
Proceedings Article

Simulation of stellar speckle imaging

[+] Author Affiliations
Erik M. Johansson, Donald T. Gavel

Lawrence Livermore National Lab. (USA)

Proc. SPIE 2200, Amplitude and Intensity Spatial Interferometry II, 372 (June 9, 1994); doi:10.1117/12.177254
Text Size: A A A
From Conference Volume 2200

  • Amplitude and Intensity Spatial Interferometry II
  • James B. Breckinridge
  • Kailua, Kona, HI | March 13, 1994

abstract

Standard FFT-based phase screen generation methods do not accurately model low-frequency turbulence characteristics. This paper introduces a new phase screen generation technique which uses low frequency subharmonic information to correct the problem. We compare our technique to two other subharmonic methods. The structure functions for this new method match very closely the structure functions of Kolmogorov turbulence theory.

© (1994) COPYRIGHT SPIE--The International Society for Optical Engineering. Downloading of the abstract is permitted for personal use only.
Citation

Erik M. Johansson and Donald T. Gavel
"Simulation of stellar speckle imaging", Proc. SPIE 2200, Amplitude and Intensity Spatial Interferometry II, 372 (June 9, 1994); doi:10.1117/12.177254; http://dx.doi.org/10.1117/12.177254


Access This Article
Sign In to Access Full Content
Please Wait... Processing your request... Please Wait.
Sign in or Create a personal account to Buy this article ($15 for members, $18 for non-members).
 

Figures

Tables

NOTE:
Citing articles are presented as examples only. In non-demo SCM6 implementation, integration with CrossRef’s "Cited By" API will populate this tab (http://www.crossref.org/citedby.html).

Some tools below are only available to our subscribers or users with an online account.

Related Content

Customize your page view by dragging & repositioning the boxes below.

Related Book Chapters

Advertisement


Buy this article ($18 for members, $25 for non-members).
Sign In