The COSMIC/FORMOSAT-3 Radio Occultation Mission after 12 Years: Accomplishments, Remaining Challenges, and Potential Impacts of COSMIC-2

Author:

Ho Shu-peng1,Anthes Richard A.2,Ao Chi O.3,Healy Sean4,Horanyi Andras4,Hunt Douglas2,Mannucci Anthony J.3,Pedatella Nicholas5,Randel William J.5,Simmons Adrian4,Steiner Andrea6,Xie Feiqin7,Yue Xinan8,Zeng Zhen2

Affiliation:

1. NOAA/Center for Weather and Climate Prediction, College Park, Maryland

2. COSMIC Project Office, University Corporation for Atmospheric Research, Boulder, Colorado

3. Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California

4. European Centre for Medium-Range Weather Forecasts, Reading, United Kingdom

5. National Center for Atmospheric Research, Boulder, Colorado

6. Wegener Center for Climate and Global Change, and Institute for Geophysics, Astrophysics, and Meteorology, Institute of Physics, University of Graz, Graz, Austria

7. Texas A&M University, Corpus Christi, Texas

8. Key Laboratory of Earth and Planetary Physics, Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing, China

Abstract

AbstractLaunched in 2006, the Formosa Satellite Mission 3–Constellation Observing System for Meteorology, Ionosphere and Climate (FORMOSAT-3/COSMIC) was the first constellation of microsatellites carrying global positioning system (GPS) radio occultation (RO) receivers. Radio occultation is an active remote sensing technique that provides valuable information on the vertical variations of electron density in the ionosphere, and temperature, pressure, and water vapor in the stratosphere and troposphere. COSMIC has demonstrated the great value of RO data in ionosphere, climate, and meteorological research and operational weather forecasting. However, there are still challenges using RO data, particularly in the moist lower troposphere and upper stratosphere. A COSMIC follow-on constellation, COSMIC-2, was launched into equatorial orbit in 2019. With increased signal-to-noise ratio (SNR) from improved receivers and digital beam steering antennas, COSMIC-2 will produce at least 5,000 high-quality RO profiles daily in the tropics and subtropics. In this paper, we summarize 1) recent (since 2011 when the last review was published) contributions of COSMIC and other RO observations to weather, climate, and space weather science; 2) the remaining challenges in RO applications; and 3) potential contributions to research and operations of COSMIC-2.

Publisher

American Meteorological Society

Subject

Atmospheric Science

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