Rover Environmental Monitoring Station (REMS)
Rover Environmental Monitoring Station
The Rover Environmental Monitoring Station monitors atmospheric pressure, humidity, wind currents, and ultraviolet radiation from the sun. Credit: NASA/JPL-Caltech/INTA (Instituto Nacional de Tecnica Aeroespacial)
The Centro de Astrobiologia (CAB), a joint center of Consejo Superior de Investigaciones Cientificas - Instituto Nacional de Tecnica Aeroespacial (CSIC-INTA), is providing a weather monitoring station contributed by the Spanish government and to be carried by the Mars Science Laboratory rover. The Rover Environmental Monitoring Station measures and provides daily and seasonal reports on atmospheric pressure, humidity, ultraviolet radiation at the Martian surface, wind speed and direction, air temperature, and ground temperature around the rover.
Two small booms on the rover mast record the horizontal and vertical components of wind speed to characterize air flow near the Martian surface from breezes, dust devils, and dust storms. A sensor inside the rover's electronic box is exposed to the atmosphere through a small opening and measures changes in pressure caused by different meteorological events such as dust devils, atmospheric tides, and cold and warm fronts. A small filter shields the sensor against dust contamination.
A suite of infrared sensors on one of the booms (Boom 1) measures the intensity of infrared radiation emitted by the ground, which provides an estimate of ground temperature. These data provide the basis for computing ground temperature. A sensor on the other boom (Boom 2) tracks atmospheric humidity. Both booms carry sensors for measuring air temperature.An array of detectors on the rover deck that are sensitive to specific frequencies of sunlight measure ultraviolet radiation at the Martian surface and correlate it with changes in the other environmental variables.