Coriolis (satellite)
The Coriolis satellite is a Naval Research Laboratory (NRL) and Air Force Research Laboratory (AFRL) Earth and space observation satellite launched from Vandenberg Air Force Base, on January 6, 2003, at 14:19 GMT.
| Mission type | Earth and Solar observation |
|---|---|
| Operator | NRL, AFRL |
| COSPAR ID | 2003-001A |
| SATCAT no. | 27640 |
| Mission duration | 21 years, 1 month and 25 days (elasped) |
| Spacecraft properties | |
| Manufacturer | Spectrum Astro Inc |
| Launch mass | 395 kilograms (871 lb) |
| Power | 1,174 watts |
| Start of mission | |
| Launch date | January 6, 2003, 14:19 UTC |
| Rocket | Titan II(23)G |
| Launch site | Vandenberg SLC-4W |
| Orbital parameters | |
| Reference system | Geocentric |
| Regime | Low Earth |
| Eccentricity | 0.0013721 |
| Perigee altitude | 826 kilometers (513 mi) |
| Apogee altitude | 846 kilometers (526 mi) |
| Inclination | 98.7 degrees |
| Period | 101.5 minutes |
| Epoch | 14 November 2016, 20:52:53 UTC |
| Instruments | |
| WindSat, SMEI | |
Instruments edit
WINDSAT edit
WINDSAT is a joint Integrated Program Office/Department of Defense demonstration project, intended to measure ocean surface wind speed and wind direction from space using a polarimetric radiometer. WINDSAT was developed and managed by the Space Test Program at Kirtland AFB in New Mexico, designed for a three-year lifetime. It is primarily designed to measure ocean surface wind direction (nonprecipitating conditions) with a 25-km spatial resolution. Secondary measurements are Sea surface temperature, soil moisture, rain rate, ice and snow characteristics and water vapor.
Solar Mass Ejection Imager (SMEI) edit
The Solar Mass Ejection Imager (SMEI) is an instrument intended to detect disturbances in the solar wind by means of imaging scattered light from the free electrons in the plasma of the solar wind. To do this three CCD cameras observe sections of the sky of size 60 by 3 degree.
As the SMEI instrument observes the whole sky, data generated has been used to observe periodic changes in the brightness of stars. This data can be used to detect asteroseismological oscillation in giant stars, and for the detection of large eclipsing extra-solar planets.
External links edit
- Ray, Justin. "Coriolis launched to track ocean winds, solar storms". Spaceflight Now.
Bibliography edit
- WINDSAT site at NRL 2017-04-24 at the Wayback Machine