P
Prasad Varanasi
Researcher at Stony Brook University
Publications - 112
Citations - 7059
Prasad Varanasi is an academic researcher from Stony Brook University. The author has contributed to research in topics: Spectral line & Spectrometer. The author has an hindex of 32, co-authored 111 publications receiving 6923 citations. Previous affiliations of Prasad Varanasi include State University of New York System.
Papers
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Uncertainties of the Intensity of the 1130 nm Band of Water Vapor
Lawrence P. Giver,P. Pilewskie,W. J. Gore,C. Chackerian,Prasad Varanasi,R. Bergstrom,R. S. Freedman +6 more
TL;DR: In this paper, the authors made independent assessments of this proposal using two spectra obtained with the Ames 25 meter base path White cell. And they showed that these spectra are not compatible when the HITRAN line intensities are increased by 38%.
Water Vapor Line Intensity Corrections and Rovibrational Assignment Updates of the Shortwave HITRAN and GEISA Databases
Proceedings ArticleDOI
Laboratory studies of infrared features observed in the atmospheres of the outer planets
Prasad Varanasi,V. Nemtchinov +1 more
TL;DR: In this paper, high-resolution measurements of the halfwidths of several hydrogen-broadened lines in the ν2s-fundamental bands of 14NH3 and 15NH3 at temperatures relevant to the Jovian atmosphere are presented as an illustration of studies in our laboratory of the spectroscopic features observed in the outer planets.
Proceedings ArticleDOI
Infrared absorption cross section data needed for the satellite remote sensing of CFC-14
V. Nemtchinov,Prasad Varanasi +1 more
TL;DR: In this article, high-resolution Fourier transform spectrometer was used to measure the absorption cross-sections of CFC-14 at temperatures between 180 and 296 K. The measured crosssections are free from instrumental distortion, since the spectra were recorded at spectral resolution that was sufficiently high at broadening pressures corresponding to tropospheric and stratospheric layers.
Journal Article
Intensity measurements in the nu4-fundamental of (C-13)H4 at planetary atmospheric temperatures
TL;DR: In this paper, a line-by-line comparison of observed and computed spectral transmittance has yielded line strengths for the nu4-fundamental band of (C-13)H4 at low temperatures of planetary atmospheric interest.