3 SATURN'S VISIBLE ATMOSPHERIC HAZE SHROUDS A COMPELLING ACTIVE ENVIRONMENT CONTAINING MULTIPLE JET STREAMS, THUNDERSTORMS, AND VORTICES, SIMILAR TO JUPITER'S TROPOSPHERE. CONSIDERABLY MORE IS KNOWN, HOWEVER, ABOUT JUPITER'S ATMOSPHERIC DYNAMICS. 2D WIND MAPS OF JUPITER CONSTRUCTED USING OBSERVATIONS FROM VARIOUS SPACECRAFT MISSIONS BETTER ILLUMINATE THE STRUCTURE AND CHARACTERISTICS OF METEOROLOGICAL FEATURES RESIDING IN ITS ACTIVE ATMOSPHERE. FOR SATURN, ALTHOUGH THE CASSINI MISSION CONTINUES TO RETURN TREMENDOUS VOLUMES OF DATA AND OBSERVATIONS OF THE PLANET, NO COMPLETE 2D WIND MAPS EXIST OF SATURN'S ATMOSPHERE, PREVENTING A FULL UNDERSTANDING OF ITS DYNAMIC METEOROLOGY. WE PROPOSE TO CONSTRUCT 2D WIND MAPS OF THE ATMOSPHERE FROM APPROPRIATE CASSINI ISS AND VIMS DATA SETS. BY UTILIZING ADVANCED CLOUD FEATURE TRACKING SOFTWARE AND ANALYSIS TOOLS, OUR PROPOSED RESEARCH ADDRESSES THIS DECIENCY IN OUR UNDERSTANDING OF SATURN'S DY-NAMIC ATMOSPHERE, AND FURTHERS THE STATE OF KNOWLEDGE. Other Administrative Action $0 5/20/18 Not listed SATURN'S VISIBLE ATMOSPHERIC HAZE SHROUDS A COMPELLING ACTIVE ENVIRONMENT CONTAINING MULTIPLE JET STREAMS THUNDERSTORMS AND VORTICES SIMILAR TO JUPITER'S TROPOSPHERE. CONSIDERABLY MORE IS KNOWN HOWEVER ABOUT JUPITER'S ATMOSPHERIC DYNAMICS. 2D WIND MAPS OF JUPITER CONSTRUCTED USING OBSERVATIONS FROM VARIOUS SPACECRAFT MISSIONS BETTER ILLUMINATE THE STRUCTURE AND CHARACTERISTICS OF METEOROLOGICAL FEATURES RESIDING IN ITS ACTIVE ATMOSPHERE. FOR SATURN ALTHOUGH THE CASSINI MISSION CONTINUES TO RETURN TREMENDOUS VOLUMES OF DATA AND OBSERVATIONS OF THE PLANET NO COMPLETE 2D WIND MAPS EXIST OF SATURN'S ATMOSPHERE PREVENTING A FULL UNDERSTANDING OF ITS DYNAMIC METEOROLOGY. WE PROPOSE TO CONSTRUCT 2D WIND MAPS OF THE ATMOSPHERE FROM APPROPRIATE CASSINI ISS AND VIMS DATA SETS. BY UTILIZING ADVANCED CLOUD FEATURE TRACKING SOFTWARE AND ANALYSIS TOOLS OUR PROPOSED RESEARCH ADDRESSES THIS DECIENCY IN OUR UNDERSTANDING OF SATURN'S DY-NAMIC ATMOSPHERE AND FURTHERS THE STATE OF KNOWLEDGE. $0 5/20/18 2 SATURN'S VISIBLE ATMOSPHERIC HAZE SHROUDS A COMPELLING ACTIVE ENVIRONMENT CONTAINING MULTIPLE JET STREAMS, THUNDERSTORMS, AND VORTICES, SIMILAR TO JUPITER'S TROPOSPHERE. CONSIDERABLY MORE IS KNOWN, HOWEVER, ABOUT JUPITER'S ATMOSPHERIC DYNAMICS. 2D WIND MAPS OF JUPITER CONSTRUCTED USING OBSERVATIONS FROM VARIOUS SPACECRAFT MISSIONS BETTER ILLUMINATE THE STRUCTURE AND CHARACTERISTICS OF METEOROLOGICAL FEATURES RESIDING IN ITS ACTIVE ATMOSPHERE. FOR SATURN, ALTHOUGH THE CASSINI MISSION CONTINUES TO RETURN TREMENDOUS VOLUMES OF DATA AND OBSERVATIONS OF THE PLANET, NO COMPLETE 2D WIND MAPS EXIST OF SATURN'S ATMOSPHERE, PREVENTING A FULL UNDERSTANDING OF ITS DYNAMIC METEOROLOGY. WE PROPOSE TO CONSTRUCT 2D WIND MAPS OF THE ATMOSPHERE FROM APPROPRIATE CASSINI ISS AND VIMS DATA SETS. BY UTILIZING ADVANCED CLOUD FEATURE TRACKING SOFTWARE AND ANALYSIS TOOLS, OUR PROPOSED RESEARCH ADDRESSES THIS DECIENCY IN OUR UNDERSTANDING OF SATURN'S DY-NAMIC ATMOSPHERE, AND FURTHERS THE STATE OF KNOWLEDGE. Funding Only Action $37.3k 2/24/17 Not listed SATURN'S VISIBLE ATMOSPHERIC HAZE SHROUDS A COMPELLING ACTIVE ENVIRONMENT CONTAINING MULTIPLE JET STREAMS THUNDERSTORMS AND VORTICES SIMILAR TO JUPITER'S TROPOSPHERE. CONSIDERABLY MORE IS KNOWN HOWEVER ABOUT JUPITER'S ATMOSPHERIC DYNAMICS. 2D WIND MAPS OF JUPITER CONSTRUCTED USING OBSERVATIONS FROM VARIOUS SPACECRAFT MISSIONS BETTER ILLUMINATE THE STRUCTURE AND CHARACTERISTICS OF METEOROLOGICAL FEATURES RESIDING IN ITS ACTIVE ATMOSPHERE. FOR SATURN ALTHOUGH THE CASSINI MISSION CONTINUES TO RETURN TREMENDOUS VOLUMES OF DATA AND OBSERVATIONS OF THE PLANET NO COMPLETE 2D WIND MAPS EXIST OF SATURN'S ATMOSPHERE PREVENTING A FULL UNDERSTANDING OF ITS DYNAMIC METEOROLOGY. WE PROPOSE TO CONSTRUCT 2D WIND MAPS OF THE ATMOSPHERE FROM APPROPRIATE CASSINI ISS AND VIMS DATA SETS. BY UTILIZING ADVANCED CLOUD FEATURE TRACKING SOFTWARE AND ANALYSIS TOOLS OUR PROPOSED RESEARCH ADDRESSES THIS DECIENCY IN OUR UNDERSTANDING OF SATURN'S DY-NAMIC ATMOSPHERE AND FURTHERS THE STATE OF KNOWLEDGE. $37.3k 2/24/17 1 SATURN'S VISIBLE ATMOSPHERIC HAZE SHROUDS A COMPELLING ACTIVE ENVIRONMENT CONTAINING MULTIPLE JET STREAMS, THUNDERSTORMS, AND VORTICES, SIMILAR TO JUPITER'S TROPOSPHERE. CONSIDERABLY MORE IS KNOWN, HOWEVER, ABOUT JUPITER'S ATMOSPHERIC DYNAMICS. 2D WIND MAPS OF JUPITER CONSTRUCTED USING OBSERVATIONS FROM VARIOUS SPACECRAFT MISSIONS BETTER ILLUMINATE THE STRUCTURE AND CHARACTERISTICS OF METEOROLOGICAL FEATURES RESIDING IN ITS ACTIVE ATMOSPHERE. FOR SATURN, ALTHOUGH THE CASSINI MISSION CONTINUES TO RETURN TREMENDOUS VOLUMES OF DATA AND OBSERVATIONS OF THE PLANET, NO COMPLETE 2D WIND MAPS EXIST OF SATURN'S ATMOSPHERE, PREVENTING A FULL UNDERSTANDING OF ITS DYNAMIC METEOROLOGY. WE PROPOSE TO CONSTRUCT 2D WIND MAPS OF THE ATMOSPHERE FROM APPROPRIATE CASSINI ISS AND VIMS DATA SETS. BY UTILIZING ADVANCED CLOUD FEATURE TRACKING SOFTWARE AND ANALYSIS TOOLS, OUR PROPOSED RESEARCH ADDRESSES THIS DECIENCY IN OUR UNDERSTANDING OF SATURN'S DY-NAMIC ATMOSPHERE, AND FURTHERS THE STATE OF KNOWLEDGE. Funding Only Action $37.1k 3/3/16