Physics
Scientific paper
Dec 2009
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009agufmsa11a1459s&link_type=abstract
American Geophysical Union, Fall Meeting 2009, abstract #SA11A-1459
Physics
[0310] Atmospheric Composition And Structure / Airglow And Aurora, [0355] Atmospheric Composition And Structure / Thermosphere: Composition And Chemistry, [0394] Atmospheric Composition And Structure / Instruments And Techniques
Scientific paper
OII 7320A line width data were acquired at Arecibo Observatory during the evening and morning twilights since April 2008 using a low resolution single etalon Fabry-Perot Interferometer (FPI). The Arecibo FPI is configured using 0.9cm spacing plate, producing a free spectral range of 0.298A and a spectral resolution of 0.03A, sufficient to sample line width temperatures as low as 500K. A very narrow, 3A FWHM three-cavity interference filter is used to preclude OH contamination from the 7316.3A or 7329.9A. In this work coincident nights of OII 7320A line widths and Incoherent Scatter Radar (ISR) O+ temperatures are compared and analyzed.
Brum C. G.
Garcia Rafael
González Sixto A.
Kerr Robert B.
Migliozzi M.
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