Global measurement of temporal signatures of precipitation: Development of the temporal experiment for storms and tropical systems technology demonstration …

SC Reising, TC Gaier, CD Kummerow… - … and Remote Sensing …, 2017 - ieeexplore.ieee.org
SC Reising, TC Gaier, CD Kummerow, S Padmanabhan, BH Lim, C Heneghan, W Berg…
2017 IEEE International Geoscience and Remote Sensing Symposium …, 2017ieeexplore.ieee.org
The Temporal Experiment for Storms and Tropical Systems (TEMPEST) mission concept
consists of a constellation of five identical 6U-Class nanosatellites observing at five
millimeter-wave frequencies with five-minute temporal sampling to observe the time
evolution of clouds and their transition to precipitation. The TEMPEST concept is designed to
improve the understanding of cloud processes, by providing critical information on the time
evolution of cloud and precipitation microphysics and by improving our understanding of the …
The Temporal Experiment for Storms and Tropical Systems (TEMPEST) mission concept consists of a constellation of five identical 6U-Class nanosatellites observing at five millimeter-wave frequencies with five-minute temporal sampling to observe the time evolution of clouds and their transition to precipitation. The TEMPEST concept is designed to improve the understanding of cloud processes, by providing critical information on the time evolution of cloud and precipitation microphysics and by improving our understanding of the largest sources of uncertainty in cloud models. TEMPEST millimeter-wave radiometers are able to perform observations inside the cloud to observe changes as the cloud begins to precipitate or ice accumulates inside the storm. The TEMPEST Technology Demonstration (TEMPEST-D) mission will be deployed to demonstrate measurement capabilities required for a constellation of 6U-Class nanosatellites to directly observe the temporal development of clouds to understand the conditions that control their transition from non-precipitating to precipitating clouds. TEMPEST-D will provide observations at five millimeter-wave frequencies from 89 to 183 GHz using a single compact instrument that is well suited for the 6U-Class architecture.
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