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A NUMERICAL SOLUTION TO THE EQUATION OF RADIATIVE TRANSFER FOR PARTICLES IN THE MIE REGIONHerman, Benjamin M. (Benjamin Morris), 1929- January 1964 (has links)
No description available.
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DEVELOPMENT AND APPLICATION OF BISTATIC LIDAR AS A REMOTE ATMOSPHERIC PROBEWebster, Willard Parker, 1941- January 1971 (has links)
No description available.
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An experimental study of atmospheric turbidity using radiometric techniquesShaw, Glenn E. January 1971 (has links)
No description available.
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A survey of methods of sizing and counting water droplets in cloudsAllard, Frederick Charles, 1943- January 1969 (has links)
No description available.
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Improved method for the optical determination of temperature profilesFriend, Arnold Luther, January 1969 (has links)
Thesis (M.S.)--University of Wisconsin--Madison, 1969. / eContent provider-neutral record in process. Description based on print version record. Includes bibliographical references.
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Optical radar detection of scattering layers in the atmosphereFox, Robert Joseph. January 1964 (has links)
Thesis (M.S.)--University of Wisconsin--Madison, 1964. / eContent provider-neutral record in process. Description based on print version record. Bibliography: l. 39-41.
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Calculation of doubly scattered lidar returnsEloranta, Edwin Walter. January 1972 (has links)
Thesis (Ph. D.)--University of Wisconsin--Madison, 1972. / Typescript. Vita. eContent provider-neutral record in process. Description based on print version record. Includes bibliography.
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Stellar scintillation and its use in atmospheric measurements /Campbell, Laurence. January 1991 (has links) (PDF)
Thesis (Ph. D.)--University of Adelaide, Dept. of Physics and Mathematical Physics, 1992. / Includes bibliographical references (leaves ix-xiii).
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Interaction of an Optical System with the Incoming Wavefront in the Presence of Atmospheric TurbulenceShack, R. V. 28 August 1967 (has links)
QC 351 A7 no. 19 / ABSTRACT
The classical properties of an image formed by an optical system
looking through a turbulent medium are scintillation, agitation, and blur.
A simple but adequate statistical model is obtained describing the pupil
function in the presence of random wavefront disturbances in both amplitude
and phase. A measure of scintillation is then obtained in the form
of a normalized, weighted integral in frequency space containing all the
pertinent properties of the optical system. A similar measure of agitation
is then developed, and finally a description of the blur is obtained
in the form of an equivalent transfer function for the turbulent medium
in which the contribution from amplitude variations and the contribution
from phase variations are independent.
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Stellar scintillation and its use in atmospheric measurements / by Laurence CampbellCampbell, Laurence January 1991 (has links)
Bibliography: leaves ix-xiii / viii, 171, ix-xiii leaves : ill. (some col.) ; 30 cm. / Title page, contents and abstract only. The complete thesis in print form is available from the University Library. / Thesis (Ph.D.)--University of Adelaide, Dept. of Physics and Mathematical Physics, 1992
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