Abstract
A least-squares fit method, adapted to the processing of laboratory spectra, was used to analyze spectra of Jupiter ionosphere. A multispectrum fitting procedure was developed to obtain more accurate line parameters from laboratory spectra.
© 2001 Optical Society of America
PDF ArticleMore Like This
J. Vander Auwera
FMC2 Fourier Transform Spectroscopy (FTS) 2001
J. Vander Auwera
FWB1 Fourier Transform Spectroscopy (FTS) 2001
A. Goldman, F. J. Murcray, R. D. Blatherwick, F. H. Murcray, J. J. Kosters, S. J. David, D. G. Murcray, and C. P. Rinsland
FY3 OSA Annual Meeting (FIO) 1992