University Centre in Svalbard (UNIS)
The instrument is designed to image near-infrared emissions from the OH(6-2) band of airglow. The main objective is to study the morphology of the airglow layer at 90 km of altitude in the mesosphere. We expect to see how gravity waves and meteors interact with the layer in order to get a better understanding of the weather up there. Filter-ratio temperatures will be retrieved and compared to what we measure with the 1m Ebert-Fastie spectrometer (Silver Bullet).
KeoSentry4ix airglow imager. (1) Mamiya RB67 Fish-eye lens, (2) collimator lens, (3) filterwheel, (4) Smart motor system, (5) relay optics, and (6) CCD detector
PIs: Fred Sigernes and Dag Lorentzen
Address: UNIS, P.O. Box 156, N-9171 Longyearbyen, Svalbard, Norway
E-mail: email@example.com and firstname.lastname@example.org
Phones/Fax: +47 79023335(6)/01
Manufacturer: Keo Scientific Ltd.
Front Lens: Mamiya RB67
Spatial coverage: All sky view - FOV 180 deg.
Detector: Back Illuminated eXcellon PI PIXIS CCD 1024x1024 pixels;
Time resolution: 1s - and up!; Cooling: -70 deg.; 16 bits resolution
Filter wheel (6 x 4 inch diameter apertures - temperature stabilized):
[CH1] Blocked (dark images)
[CH2] Notch filter @ 844.6nm; BP 18.5 nm
[CH3] Bandpass filter @ 844.6nm; BP 1.8 nm
[CH4] Bandpass filter @ 856.8nm; BP 1.8 nm
[CH5] Bandpass filter @ 846.5nm; BP 1.8 nm
[CH6] Bandpass filter @ 840.0nm; BP 1.8 nm