LORAAS
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  A LORAAS/SSULI sensor during testing and calibration. LORAAS

Low Resolution Airglow and Aurora Spectrograph

LORAAS is the first of a series of 6 identical UV limb scanning sensors that will fly during the period 1999-2010 produced by NRL.  The other 5 sensors, named Special Sensor Ultraviolet Limb Imager (SSULI) 1-5, will fly as part of the Defense Meteorological Satellite Program (DMSP).  The combined data retrieved from these UV spectrographs will provide a long-term dataset for studying thermosphere and ionosphere structure, composition, climate, and space weather over the upcoming solar activity cycle.

Schematic of the LORAAS instrument.

Design Features

Summary
f/3 0.25-m near-Wadsworth configuration spectrograph
80-170 nm passband
1.8 nm spectral resolution
Scan mirror
Plane mirror 8.1 cm X 11.7 cm
SiC reflective coating
Motor drive and resolver controlled
Collimator
Mechanical grid collimator
70 mm square aperture
23 stacked grids
Roughly pyramidal effective aperture function
Grating
Spherical concave grating, 250 mm focal length
1600 lines/mm blazed for 110 nm
9.8 cm X 9.4 cm zerodur blank
SiC reflective coating
Detector
Windowless, with clamshell vacuum door mechanism
CsI photocathode
40 mm diameter microchannel plate z-stack
Low sensitivity region in center of detector
photocathode masked, leaving bare microchannel plate
reduces 121.6 and 130.4 nm emission
wedge & strip anode
256 dispersion axis pixels
Field-of-view
0.15-degree (FWHM) vertical resolution (5 km)
2.4 degree (FWHM) horizontal field-of-view (120 km)
Normal scan zenith angles 100-127 degrees (750-50 km)
Extended scan zenith angles 5-140 degrees (800 km - disk)

LORAAS typical dayglow spectrum.LORAAS typical dayglow limb scans.

Scientific Features

Focuses on the F-region of the ionosphere
Measures daytime electron and neutral densities
Measures nighttime electron densities.
Continuous global measurement of space weather
Part of a long-term monitoring monitoring program