Light intensity is easily quantified by using calibrated detectors that can directly exploit the energy flux from an incident light. Spatial intensity variations can be imaged using an array of such energy detectors, as in a camera, for instance. On the other hand, light phase is invisible to energy detectors and is usually detected indirectly by exploiting phase-dependent phenomena that affect intensity. For example, intercepting light with a lenslet array would generate an array of spots at the common focal plane of the lenslets and any phase perturbations could be deduced from observed changes in the configuration of the intensity spots. When using coherent illumination, a common method consists of introducing a reference beam and then analyzing the phase-dependent interference pattern to determine the phase perturbation. Working without the benefit of coherent laser sources, Gabor invented the first holograms capable of interferometri-cally recording phase information by adapting Zernike's phase contrast configuration, where the reference and the object beams propagate along a common path to ensure coherence [1]. Aside from coherence, common-path interferometry also surmounts typical experimental hurdles that tend to smear out the interference pattern with its relative tolerance to vibrations and fluctuations in the ambient conditions, which becomes a major problem when the reference beam travels along a different path.
The accuracy of the extracted phase information from the output of an interferometer is dependent on assumptions about the reference wave, and this is no different for a common-path interferometer. Thus it is vital to examine how a phase contrast method models the reference wave in order to understand its limitations. In this chapter, we examine the assumptions employed in Zernike's phase contrast method. Although sufficient for very thin phase objects like biological samples, its limited range of validity necessitates a generalized formulation to encompass a wider range and broaden the horizon for possible applications.
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
Preview
Unable to display preview. Download preview PDF.
References
D. Gabor, “Holography, 1948–1971,” from Nobel Lectures, Physics 1971–1980, Editor Stig Lundqvist, World Scientific Publishing Co., Singapore, 1992
F. Zernike, “How I discovered phase contrast”, Science 121, 345–349 (1955).
F. Zernike, “Phase contrast, a new method for the microscopic observation of transparent objects. Part I,” Physica 9, 686–698 (1942).
F. Zernike, “Phase contrast, a new method for the microscopic observation of transparent objects. Part II,” Physica 9, 974–986(1942).
J. W. Goodman, Introduction to Fourier Optics (McGraw-Hill, San Francisco, 2nd ed., 1996).
H. B. Henning, “A new scheme for viewing phase contrast images”, Electro-optical Systems Design 6, 30–34 (1974).
G. O. Reynolds, J. B. Develis, G. B. Parrent, Jr., B. J. Thompson, The New Physical Optics Notebook: Tutorials in Fourier Optics, (SPIE Optical Engineering Press, New York 1989) Chap. 35.
H. H. Hopkins, “A note on the theory of phase-contrast images”, Proc. Phys. Soc. B., 66, 331–333 (1953).
S. F. Paul, “Dark-ground illumination as a quantitative diagnostic for plasma density”, Appl. Opt., 21, 2531–2537 (1982).
R. C. Anderson and S. Lewis, “Flow visualization by dark central ground interfer-ometry”, Appl. Opt. 24, 3687 (1985).
M. P. Loomis, M. Holt, G. T. Chapman and M. Coon, “Applications of dark central ground interferometry”, Proc. of the 29th Aerospace Sciences Meeting, AIAA 91–0565, 1–8 (1991).
D. Malacara, Optical shop Testing, 302–305 (John Wiley & Sons, New York 2nd ed., 1992).
A. K. Aggarwal and S. K. Kaura, “Further applications of point diffraction interferometer”, J. Optics (Paris) 17, 135–138 (1986).
M. Born and E. Wolf, Principles of Optics, 426–427 (Pergamon Press, 6th ed., 1980).
C. A. Mack, “Phase contrast lithography”, Proc. SPIE 1927, 512–520 (1993).
Y. Arieli, N. Eisenberg and A. Lewis, “Pattern generation by inverse phase contrast”, Opt. Comm. 138, 284–286 (1997).
Rights and permissions
Copyright information
© 2009 Canopus Academic Publishing Limited
About this chapter
Cite this chapter
(2009). Generalized Phase Contrast. In: Generalized Phase Contrast. Springer Series in Optical Sciences, vol 146. Springer, Dordrecht. https://doi.org/10.1007/978-90-481-2839-6_2
Download citation
DOI: https://doi.org/10.1007/978-90-481-2839-6_2
Publisher Name: Springer, Dordrecht
Print ISBN: 978-90-481-2838-9
Online ISBN: 978-90-481-2839-6
eBook Packages: Physics and AstronomyPhysics and Astronomy (R0)