An overview of the recent results from the H-alpha and OII 7320A observations at Arecibo Observatory using the new low resolution Fabry-Perot Interferometer

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[0310] Atmospheric Composition And Structure / Airglow And Aurora, [2415] Ionosphere / Equatorial Ionosphere, [2419] Ionosphere / Ion Chemistry And Composition, [2494] Ionosphere / Instruments And Techniques

Scientific paper

The low resolution single etalon Fabry-Perot interferometer (FPI) in the Optical Laboratory at the Arecibo Observatory has been upgraded to permit remote operation, to improve FPI sensitivity, and to permit FPI response in the near infrared. Integration of a 2048 x 2048 Andor CCD array into the existing low-resolution FPI with a new optical system is complete and in continuous operation since 2006. In this work an overview of the recent results using two distinct configurations for the new resolution FPI in order to study the Geocoronal Balmer-Alpha airglow at 6563A and the OII 7320A twilight emission is presented.

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