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Zeeman splitting of the 61 Gigahertz oxygen ( O 2 ) line in the mesosphere
Author(s) -
Hartmann G. K.,
Degenhardt W.,
Richards M. L.,
Liebe H. J.,
Hufford G. A.,
Cotton M. G.,
Bevilacqua R. M.,
Olivero J. J.,
Kämpfer N.,
Langen J.
Publication year - 1996
Publication title -
geophysical research letters
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.007
H-Index - 273
eISSN - 1944-8007
pISSN - 0094-8276
DOI - 10.1029/96gl01043
Subject(s) - zeeman effect , atmosphere (unit) , mesosphere , physics , spectrometer , atmosphere of earth , spectral line , radiometer , satellite , airglow , line (geometry) , stratosphere , remote sensing , environmental science , atmospheric sciences , optics , magnetic field , meteorology , astronomy , geology , geometry , mathematics , quantum mechanics
Zeeman splitting of O 2 molecular states in the Earth's upper atmosphere leads to polarized emission spectra. A 61 GHz radiometer operated as part of the Millimeter‐wave Atmospheric Sounder (MAS), a core payload instrument of the NASA Space Shuttle ATLAS missions, observed such emissions. This instrument's high resolution spectrometer (200 kHz) allows us to verify for the first time Zeeman effect model calculations for the upper atmosphere in some detail. The results suggest some interesting new aspects for the research of the upper atmosphere.