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This work was carried out at the Atmospheric, Oceanic, and Planetary Physics Department at the University of Oxford. The UK authors acknowledge the support of the Science and Technology Facilities Council. We acknowledge the members of the Cassini and CIRS investigation teams involved in the building, testing, and calibration of the instrument, along with the design of imaging sequences, instrument commands, and other vital operational tasks. The authors also thank K. Baines, M. Roos-Serote, A. Aguiar, Y. H. Yamazaki, and R. Wordsworth for their helpful comments and suggestions
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This work was carried out at the Atmospheric, Oceanic, and Planetary Physics Department at the University of Oxford. The UK authors acknowledge the support of the Science and Technology Facilities Council. We acknowledge the members of the Cassini and CIRS investigation teams involved in the building, testing, and calibration of the instrument, along with the design of imaging sequences, instrument commands, and other vital operational tasks. The authors also thank K. Baines, M. Roos-Serote, A. Aguiar, Y. H. Yamazaki, and R. Wordsworth for their helpful comments and suggestions.
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