The HIRDLS instrument can obtain profiles over most of the globe, both day and night. Complete Earth coverage can be obtained in twelve hours. Observations of the lower stratosphere and upper troposphere are possible through the use of special narrow and more-transparent spectral channels.
After launch, activation of the HIRDLS instrument revealed that the optical path was blocked so that 20% of the aperture could view the earth's atmosphere. Engineering studies suggest that a piece of thermal blanketing material ruptured from the back of the instrument during the explosive decompression of launch. Attempts to remove this material mirror failed. However, even with the 80% blockage, measurements at high vertical resolution can be made at one scan angle.
Overall science goals of HIRDLS are to observe the global distributions of temperature and several trace species in the stratosphere and upper troposphere at high vertical and horizontal resolution. Specific issues to be investigated include:
Although HIRDLS lost is azimuth scanning capability, much of the science can be retained through the use of chemical transport and data assimilation models.
| Item | Parameter |
|---|---|
| Spectral Range: | 6 to 18 mm |
| Standard profile spacing: | 5o longitude x 5o latitude, and 1-km vertical resolution; programmable to other modes and resolutions |
| Spatial resolution: | Profile spacing 500 km horizontally (5o lat) x 1 km vertically; averaging volume for each data sample 1 km vertical x 10 km across x 300 km along line-of-sight |
| Mass: | 220 kg |
| Duty cycle: | 100% |
| Power: | 220 W (average), 239 W (peak) |
| Data rate: | 65 kbps |
| Thermal control: | Stirling cycle cooler, heaters, sun baffle, radiator panel |
| Thermal operating range: | 20o-30o C |
| Scan range: | Elevation, 22.1o to 27.3o below horizontal, Azimuth, -21o (sun side) to +43o (anti-sun side) |
| Detector IFOV: | 1 km vertical x 10 km horizontal |
| Pointing requirements (platform+instrument, 3s): | |
| Control & Knowledge: | Such that scan range will allow all channels to observe from 0.25o below the hard horizon to 3.25o above it |
| Stability: | 30 arcsec/sec per axis |
| Jitter: | 84-Hz sample spacing uniform to ±7 arcsec |
+ Observes aerosols in the upper troposphere, stratosphere, and mesosphere
Scan mirror rotating inside optical assembly
Internal components of the optical assembly