Abstract
To record the image of a sunset we point the camera toward the setting sun, and the rays diverging from the various elements of the scene fall on the lens and are focused, element by element, on the film. Some people undoubtedly conceive of a camera as a device that reaches out and captures the distant scene, and years ago it was vigorously contended that vision reached out from the eye much as a hand reaches out in a dark room to explore the surroundings. It is, of course, perfectly all right to describe photography as in the introductory sentence above, but with the caveat that the description involves information about certain entities (the source elements and the propagation medium) that are unascertainable by the camera alone. In many branches of science the output of the observing instruments is the only information—astronomy is one example, and seismic exploration of the earth’s interior is another. Both of these endeavors produce images of inaccessible regions of physical space, and they suggest another, more operational, way of describing image formation.
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Literature cited
M. Born AND E. Wolf (1959), Principles of Optics, Pergamon, New York.
R. N. Bracewell (1958), “Radio interferometry of discrete sources,” Proceedings of the Institute of Radio Engineers, vol. 46, pp. 97–105.
R. N. Bracewell (1961), “Interferometry and the spectral sensitivity island diagram,” IRE Transactions on Antennas and Propagation, vol. AP-9, pp. 59–67.
R. N. Bracewell (1984), “Early work on imaging theory in radio astronomy,” in W.T. Sullivan, III, ed., The Early Years of Radio Astronomy, University Press.
R. N. Bracewell (1992), “Planetary influences on electrical engineering,” Proc. IEEE, vol. 80, pp. 230–237.
A. A. Michelson (1902), Light Waves and Their Uses, University of Chicago Press, Chicago.
B. Y. Mills AND A. G. Little (1953), “A resolution aerial system of a new type,” Aust. J. Sci. Res., vol. 6, p. 272–278.
Lord Rayleigh (1892), “On interference bands of approximately homogeneous light; in a letter to Prof. A. Michelson,” Philosophical Magazine, vol. 34, pp. 407–411.
J.A. Roberts (1984), Indirect Imaging, University Press, pp. 177–183.
M. Ryle (1952), “A radio interferometer and its application to the observation of weak radio stars,” Proc. Roy. Soc., A, vol. 211, pp. 351–375.
P. A. G. Scheuer (1984), “The development of aperture synthesis at Cambridge,” in W. T. Sullivan, III, ed., The Early Years of Radio Astronomy, University Press.
A. R. Thompson, J. M. Moran AND G. W. Swenson, Jr. (1986), Interferometry and Synthesis in Radio Astronomy, John Wiley & Sons, New York.
F. Zernicke (1938), “Concept of degree of coherence and its applications to optical problems,” Physika, vol. 5, pp. 785–795.
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Bracewell, R. (2003). Aperture Synthesis and Interferometry. In: Fourier Analysis and Imaging. Springer, Boston, MA. https://doi.org/10.1007/978-1-4419-8963-5_12
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DOI: https://doi.org/10.1007/978-1-4419-8963-5_12
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