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In this view several white squares of different sizes can be seen on the side of the spacecraft;this side has five of the six MWR antennas. The triang
In this view several white squares of different sizes can be seen on the side of the spacecraft;this side has five of the six MWR antennas. The triangular boom on the right is the Magnetometer (MAG) instrument
The white square is the biggest MWR antenna, and takes up another side of the spacecraft. This antenna is for 600 MHz.
The white square is the biggest MWR antenna, and takes up another side of the spacecraft. This antenna is for 600 MHz.
This visualization released by NASA depicts the layers that MWR will observe below the top visible cloud layer
This visualization released by NASA depicts the layers that MWR will observe below the top visible cloud layer
Layers of the Jovian atmosphere and corresponding MWR channels
Layers of the Jovian atmosphere and corresponding MWR channels
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Humidity and Temperature Profiler (HATPRO-SUNHAT) at the Barbados Clouds Observatory.
Humidity and Temperature Profiler (HATPRO-SUNHAT) at the Barbados Clouds Observatory.
Microwave Radiometer calibration performed by employees of Research Center of R&D in Optoelectronics, Magurele (Romania).
Microwave Radiometer calibration performed by employees of Research Center of R&D in Optoelectronics, Magurele (Romania).
Time series from 14 April 2015 for (a) brightness temperatures measured at 7 different frequencies in the K (right) and V (left) bands, (b) retrieved
Time series from 14 April 2015 for (a) brightness temperatures measured at 7 different frequencies in the K (right) and V (left) bands, (b) retrieved vertically Integrated Water Vapor (IWV) and cloud Liquid Water Path (LWP), (c) temperature profiles from 0 to 5 km, (d) absolute humidity profiles from 0 to 5 km.