James W. Brault Explained
James W. Brault (February 10, 1932 – November 1, 2008) was a 20th-century scientist and a pioneer of Fourier transform spectroscopy.[1] [2] He was a world-leading expert in physical instrument design, numerical methods as applied to spectroscopy, and in atomic and molecular spectroscopy.[3]
He graduated from Princeton University in 1962 as a student of Robert H. Dicke on the gravitational redshift of the sun and worked later at the Kitt Peak National Observatory, where he installed a high-resolution Fourier transform spectrometer used for astronomy, solar physics, and laboratory spectroscopy. In his early years, Brault was involved in the development of the lock-in amplifier, and of differential interference microscopy and phase modulation microscopy with Robert D. Allen.
References
- Sumner P. Davis, Mark C. Abrams, and James W. Brault, Fourier Transform Spectrometry, Academic Press, 2001.
- Ginette Roland, James W. Brault, and Larry Testerman, Photometric Atlas of the Solar Spectrum from 1,850 to 10,000 cm−1, 164 pp., Kitt Peak National Observatory, 1981.
- James W. Brault, "Frequency Responsive Networks", U.S. Patent US3296464, 1967.
- James W. Brault, "Gravitational redshift of solar lines", Bull. Am. Astron. Soc. 8, 28, 1963.
- Photograph during solar eclipse in 1965: http://www.noao.edu/image_gallery/html/im0323.html
Notes and References
- Book: Davis. Sumner P.. Fourier Transform Spectrometry. Abrams. Mark C.. Brault. James W.. 2001-05-30. Elsevier. 978-0-08-050691-3. en.
- Brault. James W.. 1996-06-01. New approach to high-precision Fourier transform spectrometer design. Applied Optics. EN. 35. 16. 2891–2896. 10.1364/AO.35.002891. 21085438. 1996ApOpt..35.2891B. 2155-3165.
- Web site: . Academic Search . James W. Brault . June 6, 2014.