1948
DOI: 10.1364/josa.38.000582
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The Preparation and Optical Properties of Gold Blacks*†

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Cited by 123 publications
(40 citation statements)
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“…In films prepared using this procedure, a complex granular structure results from the randomization of atomic velocities before aggregation in the gas phase [8][9][10][11][12] . Such films often but not always resemble the product of diffusion-limited aggregation.…”
Section: Sample Fabrication and Morphologymentioning
confidence: 99%
“…In films prepared using this procedure, a complex granular structure results from the randomization of atomic velocities before aggregation in the gas phase [8][9][10][11][12] . Such films often but not always resemble the product of diffusion-limited aggregation.…”
Section: Sample Fabrication and Morphologymentioning
confidence: 99%
“…Harris 9 indicates that an "80% layer," i.e., one that absorbs 80% of the incident energy (aei = 0.8) has the greatest efficiency. This absorbed energy is dissipated as follows: (1) heating the absorbing layer (QD), (2) heating the membrane (Q2), (3) heating the oil film (Q3), (4) evaporating a portion of the oil film (Q4), (5) reradiation losses (Q5), (6) conduction losses (Q6), and (7) convection losses (Q).…”
Section: Theoretical Sensitivitymentioning
confidence: 99%
“…Pfund deposited metal-blacks on nitrocellulose films in an environment of nitrogen or air. Harris studied gold-black films from the late 1940's into the 1960's [5][6][7][8][9]. The films were prepared similarly to Pfund's (deposited on thin membranes of cellulose nitrate in a partial atmosphere of nitrogen), with emphasis on the pressure of nitrogen and the evaporation rate as prime factors determining the morphology of the films.…”
Section: Introductionmentioning
confidence: 99%
“…The films were prepared similarly to Pfund's (deposited on thin membranes of cellulose nitrate in a partial atmosphere of nitrogen), with emphasis on the pressure of nitrogen and the evaporation rate as prime factors determining the morphology of the films. Optical properties were studied by Harris from the wavelength range of 3 to 15 microns [5], and later from 15 to 110 microns [8]. Deposition by evaporation in an inert gas at tenths to tens of Torr has followed the method of Harris with little change.…”
Section: Introductionmentioning
confidence: 99%