학술논문

New Atmospheric Remote Sensing Capabilities Demonstrated by the NASA TROPICS Mission
Document Type
Conference
Source
2022 IEEE USNC-URSI Radio Science Meeting (Joint with AP-S Symposium) USNC-URSI Radio Science Meeting (Joint with AP-S Symposium), 2022 IEEE. :15-16 Jul, 2022
Subject
Aerospace
Bioengineering
Communication, Networking and Broadcast Technologies
Components, Circuits, Devices and Systems
Engineered Materials, Dielectrics and Plasmas
Fields, Waves and Electromagnetics
Photonics and Electrooptics
Signal Processing and Analysis
Temperature measurement
Earth
Technological innovation
Absorption
Storms
NASA
Radiometry
Language
Abstract
The Time-Resolved Observations of Precipitation structure and storm Intensity with a Constellation of Smallsats (TROPICS) mission was selected by NASA as part of the Earth Venture--Instrument (EVI-3) program. TROPICS comprises a constellation of six CubeSats in three low-Earth low-inclination orbital planes. Each CubeSat will host a high performance millimeterwave radiometer to provide temperature profiles using seven channels near the 118.75 GHz oxygen absorption line, water vapor profiles using three channels near the 183 GHz water vapor absorption line, imagery in a single channel near 90 GHz for precipitation measurements (when combined with higher resolution water vapor channels), and a single channel at 205 GHz that is more sensitive to precipitation-sized ice particles. Spatial resolution at nadir ranges from approximately 15 km for the G-band channels to 30 km for the W-band channels. The Pathfinder (Qualification Unit) was launched on June 30, 2021, and the six constellation flight units are scheduled to launch in the first half of 2022. The TROPICS Pathfinder mission has provided an opportunity to checkout and optimize all mission elements prior to the primary constellation mission. This paper presents on-orbit results for the successful TROPICS Pathfinder precursor mission and highlights numerous technical innovations that have made the TROPICS mission possible and enabled new capabilities for future Earth observing missions.