Not listed THE OSCILLATIONS OF MAGNETOSPHERIC FIELD LINES WITH HIGH AZIMUTHAL WAVENUMBERS (M) ARE CONSIDERED TO BE DRIVEN BY DRIFT OR DRIFT BOUNCE RESONANCE WITH CHARGED PARTICLES. THE IMPORTANCE OF HIGH-M WAVES TO MAGNETOSPHERIC DYNAMICS IS THAT A CHARGED PARTICLE CAN GAIN OR LOSE ENERGY THROUGH DRIFT BOUNCE RESONANT INTERACTION WITH HIGH-M WAVES. HIGH-M WAVES CAN BE DRIVEN BY RING CURRENT IONS AND THESE WAVES IN TURN BECOME POTENTIAL ACCELERATORS FOR RADIATION BELT ELECTRONS THROUGH DRIFT RESONANCE. THEREFORE IT IS IMPORTANT TO ESTABLISH A QUANTITATIVE UNDERSTANDING ABOUT THE OCCURRENCE OF HIGH-M WAVES AND HOW IT RELATES TO THE SOLAR WIND CONDITIONS. WITH A RECENTLY DEVELOPED METHOD FOR IDENTIFYING HIGH-M WAVES IN SPACECRAFT DATA THIS INVESTIGATION AIMS AT ANSWERING THE FOLLOWING FUNDAMENTAL QUESTIONS ABOUT THE OCCURRENCE OF HIGH-M WAVES AS THE SCIENCE OBJECTIVES: A. WHAT IS THE SPATIAL EXTENT OF HIGH-M WAVES IN THE MAGNETOSPHERE IN RELATION TO MAGNETOSPHERIC CONDITIONS? ARE THE OBSERVATIONS CONSISTENT WITH THEORETICAL EXPECTATIONS? B. HOW IS THE OCCURRENCE OF HIGH-M WAVES RELATED TO SOLAR WIND CONDITIONS? THIS INVESTIGATION USES A NEW ANALYSIS METHOD ON THE DATA COLLECTED BY THE NASA ST-5 SATELLITES WHICH RAPIDLY SAMPLED EVENTS OF HIGH -M WAVES AND BUILT UP THE STATISTICS NEEDED. WITH A UNIQUE ORBIT INCLINATION ST-5 IS THE ONLY KNOWN MISSION THAT EFFICIENTLY MEASURED THE DOPPLER-SHIFTED SIGNALS OF HIGH-M WAVES. THIS INVESTIGATION WILL ALSO EXAMINE EVENTS OF POLOIDAL WAVES OBSERVED BY VAN ALLEN PROBES FOR BROADER PERSPECTIVES OF WAVE-PARTICLE INTERACTIONS RELEVANT TO HIGH-M WAVES.BECAUSE OF THE STRICT REQUIREMENTS IN OBSERVATIONS MANY HIGH-M WAVES WERE PRESENT BUT COULD NOT BE OBSERVED OR ED MAKING IT DIFFICULT TO ASSESS THE IMPACT OF THESE WAVES. TODAY THE VAN ALLEN PROBES ARE INVESTIGATING THE DYNAMICS OF THE RADIATION BELT PARTICLES. BY CONDUCTING THE PROPOSED INVESTIGATION NOW WE CAN ESTABLISH A QUANTITATIVE UNDERSTANDING ABOUT THE EXPECTED OCCURRENCE OF THE HIGH-M WAVES IN THE MAGNETOSPHERE AND IMMEDIATELY AID THE INTERPRETATION OF PARTICLE AND WAVE OBSERVATIONS BY THE VAN ALLEN PROBES. TO ADDRESS THE SCIENCE OBJECTIVES WE ANALYZE THE OBSERVATIONS IN THE MAGNETOSPHERE AND IN THE SOLAR WIND MADE BY A NUMBER OF SATELLITE MISSIONS WITH SUPPORTING OBSERVATIONS BY GROUND-BASED MAGNETOMETER NETWORKS. WE ALSO EXAMINE NUMERICAL SIMULATIONS FOR THE THEORETICAL EXPECTATIONS OF THE CHARACTERISTICS OF HIGH-M WAVES AND THEIR INTERACTIONS WITH CHARGED PARTICLES. THE SCIENCE OBJECTIVES OF THIS PROJECT ARE RELEVANT TO GOAL #2 OF THE HELIOPHYSICS DECADAL SURVEY: "DETERMINE THE DYNAMICS AND COUPLING OF EARTH S MAGNETOSPHERE IONOSPHERE AND ATMOSPHERE AND THEIR RESPONSE TO SOLAR AND TERRESTRIAL INPUTS." THE HIGH-M WAVES IN THE OUTER MAGNETOSPHERE ARE INTRINSICALLY RELATED TO THE RESONANT INTERACTIONS WITH CHARGED PARTICLES BUT THE QUANTITATIVE UNDERSTANDING ABOUT THEIR OCCURRENCE AND THE RELATIONSHIP TO SOLAR WIND CONDITIONS ARE STILL INSUFFICIENT. THIS INVESTIGATION CAN BRING IN NEW AND NEEDED KNOWLEDGE IN RESPONSE TO ONE OF THE DECADAL SURVEY GOALS. ($3) 6/22/20 7 THE OSCILLATIONS OF MAGNETOSPHERIC FIELD LINES WITH HIGH AZIMUTHAL WAVENUMBERS (M) ARE CONSIDERED TO BE DRIVEN BY DRIFT OR DRIFT BOUNCE RESONANCE WITH CHARGED PARTICLES. THE IMPORTANCE OF HIGH-M WAVES TO MAGNETOSPHERIC DYNAMICS IS THAT A CHARGED PARTICLE CAN GAIN OR LOSE ENERGY THROUGH DRIFT BOUNCE RESONANT INTERACTION WITH HIGH-M WAVES. HIGH-M WAVES CAN BE DRIVEN BY RING CURRENT IONS, AND THESE WAVES IN TURN BECOME POTENTIAL ACCELERATORS FOR RADIATION BELT ELECTRONS THROUGH DRIFT RESONANCE. THEREFORE, IT IS IMPORTANT TO ESTABLISH A QUANTITATIVE UNDERSTANDING ABOUT THE OCCURRENCE OF HIGH-M WAVES AND HOW IT RELATES TO THE SOLAR WIND CONDITIONS. WITH A RECENTLY DEVELOPED METHOD FOR IDENTIFYING HIGH-M WAVES IN SPACECRAFT DATA, THIS INVESTIGATION AIMS AT ANSWERING THE FOLLOWING FUNDAMENTAL QUESTIONS ABOUT THE OCCURRENCE OF HIGH-M WAVES AS THE SCIENCE OBJECTIVES: A. WHAT IS THE SPATIAL EXTENT OF HIGH-M WAVES IN THE MAGNETOSPHERE IN RELATION TO MAGNETOSPHERIC CONDITIONS? ARE THE OBSERVATIONS CONSISTENT WITH THEORETICAL EXPECTATIONS? B. HOW IS THE OCCURRENCE OF HIGH-M WAVES RELATED TO SOLAR WIND CONDITIONS? THIS INVESTIGATION USES A NEW ANALYSIS METHOD ON THE DATA COLLECTED BY THE NASA ST-5 SATELLITES, WHICH RAPIDLY SAMPLED EVENTS OF HIGH -M WAVES AND BUILT UP THE STATISTICS NEEDED. WITH A UNIQUE ORBIT INCLINATION, ST-5 IS THE ONLY KNOWN MISSION THAT EFFICIENTLY MEASURED THE DOPPLER-SHIFTED SIGNALS OF HIGH-M WAVES. THIS INVESTIGATION WILL ALSO EXAMINE EVENTS OF POLOIDAL WAVES OBSERVED BY VAN ALLEN PROBES FOR BROADER PERSPECTIVES OF WAVE-PARTICLE INTERACTIONS RELEVANT TO HIGH-M WAVES.BECAUSE OF THE STRICT REQUIREMENTS IN OBSERVATIONS, MANY HIGH-M WAVES WERE PRESENT BUT COULD NOT BE OBSERVED OR ED, MAKING IT DIFFICULT TO ASSESS THE IMPACT OF THESE WAVES. TODAY, THE VAN ALLEN PROBES ARE INVESTIGATING THE DYNAMICS OF THE RADIATION BELT PARTICLES. BY CONDUCTING THE PROPOSED INVESTIGATION NOW, WE CAN ESTABLISH A QUANTITATIVE UNDERSTANDING ABOUT THE EXPECTED OCCURRENCE OF THE HIGH-M WAVES IN THE MAGNETOSPHERE AND IMMEDIATELY AID THE INTERPRETATION OF PARTICLE AND WAVE OBSERVATIONS BY THE VAN ALLEN PROBES. TO ADDRESS THE SCIENCE OBJECTIVES, WE ANALYZE THE OBSERVATIONS IN THE MAGNETOSPHERE AND IN THE SOLAR WIND MADE BY A NUMBER OF SATELLITE MISSIONS, WITH SUPPORTING OBSERVATIONS BY GROUND-BASED MAGNETOMETER NETWORKS. WE ALSO EXAMINE NUMERICAL SIMULATIONS FOR THE THEORETICAL EXPECTATIONS OF THE CHARACTERISTICS OF HIGH-M WAVES AND THEIR INTERACTIONS WITH CHARGED PARTICLES. THE SCIENCE OBJECTIVES OF THIS PROJECT ARE RELEVANT TO GOAL #2 OF THE HELIOPHYSICS DECADAL SURVEY: "DETERMINE THE DYNAMICS AND COUPLING OF EARTH S MAGNETOSPHERE, IONOSPHERE, AND ATMOSPHERE AND THEIR RESPONSE TO SOLAR AND TERRESTRIAL INPUTS." THE HIGH-M WAVES IN THE OUTER MAGNETOSPHERE ARE INTRINSICALLY RELATED TO THE RESONANT INTERACTIONS WITH CHARGED PARTICLES, BUT THE QUANTITATIVE UNDERSTANDING ABOUT THEIR OCCURRENCE AND THE RELATIONSHIP TO SOLAR WIND CONDITIONS ARE STILL INSUFFICIENT. THIS INVESTIGATION CAN BRING IN NEW AND NEEDED KNOWLEDGE IN RESPONSE TO ONE OF THE DECADAL SURVEY GOALS. Funding Only Action ($3) 6/22/20 Not listed THE OSCILLATIONS OF MAGNETOSPHERIC FIELD LINES WITH HIGH AZIMUTHAL WAVENUMBERS (M) ARE CONSIDERED TO BE DRIVEN BY DRIFT OR DRIFT BOUNCE RESONANCE WITH CHARGED PARTICLES. THE IMPORTANCE OF HIGH-M WAVES TO MAGNETOSPHERIC DYNAMICS IS THAT A CHARGED PARTICLE CAN GAIN OR LOSE ENERGY THROUGH DRIFT BOUNCE RESONANT INTERACTION WITH HIGH-M WAVES. HIGH-M WAVES CAN BE DRIVEN BY RING CURRENT IONS AND THESE WAVES IN TURN BECOME POTENTIAL ACCELERATORS FOR RADIATION BELT ELECTRONS THROUGH DRIFT RESONANCE. THEREFORE IT IS IMPORTANT TO ESTABLISH A QUANTITATIVE UNDERSTANDING ABOUT THE OCCURRENCE OF HIGH-M WAVES AND HOW IT RELATES TO THE SOLAR WIND CONDITIONS. WITH A RECENTLY DEVELOPED METHOD FOR IDENTIFYING HIGH-M WAVES IN SPACECRAFT DATA THIS INVESTIGATION AIMS AT ANSWERING THE FOLLOWING FUNDAMENTAL QUESTIONS ABOUT THE OCCURRENCE OF HIGH-M WAVES AS THE SCIENCE OBJECTIVES: A. WHAT IS THE SPATIAL EXTENT OF HIGH-M WAVES IN THE MAGNETOSPHERE IN RELATION TO MAGNETOSPHERIC CONDITIONS? ARE THE OBSERVATIONS CONSISTENT WITH THEORETICAL EXPECTATIONS? B. HOW IS THE OCCURRENCE OF HIGH-M WAVES RELATED TO SOLAR WIND CONDITIONS? THIS INVESTIGATION USES A NEW ANALYSIS METHOD ON THE DATA COLLECTED BY THE NASA ST-5 SATELLITES WHICH RAPIDLY SAMPLED EVENTS OF HIGH -M WAVES AND BUILT UP THE STATISTICS NEEDED. WITH A UNIQUE ORBIT INCLINATION ST-5 IS THE ONLY KNOWN MISSION THAT EFFICIENTLY MEASURED THE DOPPLER-SHIFTED SIGNALS OF HIGH-M WAVES. THIS INVESTIGATION WILL ALSO EXAMINE EVENTS OF POLOIDAL WAVES OBSERVED BY VAN ALLEN PROBES FOR BROADER PERSPECTIVES OF WAVE-PARTICLE INTERACTIONS RELEVANT TO HIGH-M WAVES.BECAUSE OF THE STRICT REQUIREMENTS IN OBSERVATIONS MANY HIGH-M WAVES WERE PRESENT BUT COULD NOT BE OBSERVED OR CONFIRMED MAKING IT DIFFICULT TO ASSESS THE IMPACT OF THESE WAVES. TODAY THE VAN ALLEN PROBES ARE INVESTIGATING THE DYNAMICS OF THE RADIATION BELT PARTICLES. BY CONDUCTING THE PROPOSED INVESTIGATION NOW WE CAN ESTABLISH A QUANTITATIVE UNDERSTANDING ABOUT THE EXPECTED OCCURRENCE OF THE HIGH-M WAVES IN THE MAGNETOSPHERE AND IMMEDIATELY AID THE INTERPRETATION OF PARTICLE AND WAVE OBSERVATIONS BY THE VAN ALLEN PROBES. TO ADDRESS THE SCIENCE OBJECTIVES WE ANALYZE THE OBSERVATIONS IN THE MAGNETOSPHERE AND IN THE SOLAR WIND MADE BY A NUMBER OF SATELLITE MISSIONS WITH SUPPORTING OBSERVATIONS BY GROUND-BASED MAGNETOMETER NETWORKS. WE ALSO EXAMINE NUMERICAL SIMULATIONS FOR THE THEORETICAL EXPECTATIONS OF THE CHARACTERISTICS OF HIGH-M WAVES AND THEIR INTERACTIONS WITH CHARGED PARTICLES. THE SCIENCE OBJECTIVES OF THIS PROJECT ARE RELEVANT TO GOAL #2 OF THE HELIOPHYSICS DECADAL SURVEY: "DETERMINE THE DYNAMICS AND COUPLING OF EARTH S MAGNETOSPHERE IONOSPHERE AND ATMOSPHERE AND THEIR RESPONSE TO SOLAR AND TERRESTRIAL INPUTS." THE HIGH-M WAVES IN THE OUTER MAGNETOSPHERE ARE INTRINSICALLY RELATED TO THE RESONANT INTERACTIONS WITH CHARGED PARTICLES BUT THE QUANTITATIVE UNDERSTANDING ABOUT THEIR OCCURRENCE AND THE RELATIONSHIP TO SOLAR WIND CONDITIONS ARE STILL INSUFFICIENT. THIS INVESTIGATION CAN BRING IN NEW AND NEEDED KNOWLEDGE IN RESPONSE TO ONE OF THE DECADAL SURVEY GOALS. $0 3/15/19 6 THE OSCILLATIONS OF MAGNETOSPHERIC FIELD LINES WITH HIGH AZIMUTHAL WAVENUMBERS (M) ARE CONSIDERED TO BE DRIVEN BY DRIFT OR DRIFT BOUNCE RESONANCE WITH CHARGED PARTICLES. THE IMPORTANCE OF HIGH-M WAVES TO MAGNETOSPHERIC DYNAMICS IS THAT A CHARGED PARTICLE CAN GAIN OR LOSE ENERGY THROUGH DRIFT BOUNCE RESONANT INTERACTION WITH HIGH-M WAVES. HIGH-M WAVES CAN BE DRIVEN BY RING CURRENT IONS, AND THESE WAVES IN TURN BECOME POTENTIAL ACCELERATORS FOR RADIATION BELT ELECTRONS THROUGH DRIFT RESONANCE. THEREFORE, IT IS IMPORTANT TO ESTABLISH A QUANTITATIVE UNDERSTANDING ABOUT THE OCCURRENCE OF HIGH-M WAVES AND HOW IT RELATES TO THE SOLAR WIND CONDITIONS. WITH A RECENTLY DEVELOPED METHOD FOR IDENTIFYING HIGH-M WAVES IN SPACECRAFT DATA, THIS INVESTIGATION AIMS AT ANSWERING THE FOLLOWING FUNDAMENTAL QUESTIONS ABOUT THE OCCURRENCE OF HIGH-M WAVES AS THE SCIENCE OBJECTIVES: A. WHAT IS THE SPATIAL EXTENT OF HIGH-M WAVES IN THE MAGNETOSPHERE IN RELATION TO MAGNETOSPHERIC CONDITIONS? ARE THE OBSERVATIONS CONSISTENT WITH THEORETICAL EXPECTATIONS? B. HOW IS THE OCCURRENCE OF HIGH-M WAVES RELATED TO SOLAR WIND CONDITIONS? THIS INVESTIGATION USES A NEW ANALYSIS METHOD ON THE DATA COLLECTED BY THE NASA ST-5 SATELLITES, WHICH RAPIDLY SAMPLED EVENTS OF HIGH -M WAVES AND BUILT UP THE STATISTICS NEEDED. WITH A UNIQUE ORBIT INCLINATION, ST-5 IS THE ONLY KNOWN MISSION THAT EFFICIENTLY MEASURED THE DOPPLER-SHIFTED SIGNALS OF HIGH-M WAVES. THIS INVESTIGATION WILL ALSO EXAMINE EVENTS OF POLOIDAL WAVES OBSERVED BY VAN ALLEN PROBES FOR BROADER PERSPECTIVES OF WAVE-PARTICLE INTERACTIONS RELEVANT TO HIGH-M WAVES.BECAUSE OF THE STRICT REQUIREMENTS IN OBSERVATIONS, MANY HIGH-M WAVES WERE PRESENT BUT COULD NOT BE OBSERVED OR CONFIRMED, MAKING IT DIFFICULT TO ASSESS THE IMPACT OF THESE WAVES. TODAY, THE VAN ALLEN PROBES ARE INVESTIGATING THE DYNAMICS OF THE RADIATION BELT PARTICLES. BY CONDUCTING THE PROPOSED INVESTIGATION NOW, WE CAN ESTABLISH A QUANTITATIVE UNDERSTANDING ABOUT THE EXPECTED OCCURRENCE OF THE HIGH-M WAVES IN THE MAGNETOSPHERE AND IMMEDIATELY AID THE INTERPRETATION OF PARTICLE AND WAVE OBSERVATIONS BY THE VAN ALLEN PROBES. TO ADDRESS THE SCIENCE OBJECTIVES, WE ANALYZE THE OBSERVATIONS IN THE MAGNETOSPHERE AND IN THE SOLAR WIND MADE BY A NUMBER OF SATELLITE MISSIONS, WITH SUPPORTING OBSERVATIONS BY GROUND-BASED MAGNETOMETER NETWORKS. WE ALSO EXAMINE NUMERICAL SIMULATIONS FOR THE THEORETICAL EXPECTATIONS OF THE CHARACTERISTICS OF HIGH-M WAVES AND THEIR INTERACTIONS WITH CHARGED PARTICLES. THE SCIENCE OBJECTIVES OF THIS PROJECT ARE RELEVANT TO GOAL #2 OF THE HELIOPHYSICS DECADAL SURVEY: "DETERMINE THE DYNAMICS AND COUPLING OF EARTH S MAGNETOSPHERE, IONOSPHERE, AND ATMOSPHERE AND THEIR RESPONSE TO SOLAR AND TERRESTRIAL INPUTS." THE HIGH-M WAVES IN THE OUTER MAGNETOSPHERE ARE INTRINSICALLY RELATED TO THE RESONANT INTERACTIONS WITH CHARGED PARTICLES, BUT THE QUANTITATIVE UNDERSTANDING ABOUT THEIR OCCURRENCE AND THE RELATIONSHIP TO SOLAR WIND CONDITIONS ARE STILL INSUFFICIENT. THIS INVESTIGATION CAN BRING IN NEW AND NEEDED KNOWLEDGE IN RESPONSE TO ONE OF THE DECADAL SURVEY GOALS. Other Administrative Action $0 3/15/19 Not listed THE OSCILLATIONS OF MAGNETOSPHERIC FIELD LINES WITH HIGH AZIMUTHAL WAVENUMBERS (M) ARE CONSIDERED TO BE DRIVEN BY DRIFT OR DRIFT BOUNCE RESONANCE WITH CHARGED PARTICLES. THE IMPORTANCE OF HIGH-M WAVES TO MAGNETOSPHERIC DYNAMICS IS THAT A CHARGED PARTICLE CAN GAIN OR LOSE ENERGY THROUGH DRIFT BOUNCE RESONANT INTERACTION WITH HIGH-M WAVES. HIGH-M WAVES CAN BE DRIVEN BY RING CURRENT IONS AND THESE WAVES IN TURN BECOME POTENTIAL ACCELERATORS FOR RADIATION BELT ELECTRONS THROUGH DRIFT RESONANCE. THEREFORE IT IS IMPORTANT TO ESTABLISH A QUANTITATIVE UNDERSTANDING ABOUT THE OCCURRENCE OF HIGH-M WAVES AND HOW IT RELATES TO THE SOLAR WIND CONDITIONS. WITH A RECENTLY DEVELOPED METHOD FOR IDENTIFYING HIGH-M WAVES IN SPACECRAFT DATA THIS INVESTIGATION AIMS AT ANSWERING THE FOLLOWING FUNDAMENTAL QUESTIONS ABOUT THE OCCURRENCE OF HIGH-M WAVES AS THE SCIENCE OBJECTIVES: A. WHAT IS THE SPATIAL EXTENT OF HIGH-M WAVES IN THE MAGNETOSPHERE IN RELATION TO MAGNETOSPHERIC CONDITIONS? ARE THE OBSERVATIONS CONSISTENT WITH THEORETICAL EXPECTATIONS? B. HOW IS THE OCCURRENCE OF HIGH-M WAVES RELATED TO SOLAR WIND CONDITIONS? THIS INVESTIGATION USES A NEW ANALYSIS METHOD ON THE DATA COLLECTED BY THE NASA ST-5 SATELLITES WHICH RAPIDLY SAMPLED EVENTS OF HIGH -M WAVES AND BUILT UP THE STATISTICS NEEDED. WITH A UNIQUE ORBIT INCLINATION ST-5 IS THE ONLY KNOWN MISSION THAT EFFICIENTLY MEASURED THE DOPPLER-SHIFTED SIGNALS OF HIGH-M WAVES. THIS INVESTIGATION WILL ALSO EXAMINE EVENTS OF POLOIDAL WAVES OBSERVED BY VAN ALLEN PROBES FOR BROADER PERSPECTIVES OF WAVE-PARTICLE INTERACTIONS RELEVANT TO HIGH-M WAVES.BECAUSE OF THE STRICT REQUIREMENTS IN OBSERVATIONS MANY HIGH-M WAVES WERE PRESENT BUT COULD NOT BE OBSERVED OR CONFIRMED MAKING IT DIFFICULT TO ASSESS THE IMPACT OF THESE WAVES. TODAY THE VAN ALLEN PROBES ARE INVESTIGATING THE DYNAMICS OF THE RADIATION BELT PARTICLES. BY CONDUCTING THE PROPOSED INVESTIGATION NOW WE CAN ESTABLISH A QUANTITATIVE UNDERSTANDING ABOUT THE EXPECTED OCCURRENCE OF THE HIGH-M WAVES IN THE MAGNETOSPHERE AND IMMEDIATELY AID THE INTERPRETATION OF PARTICLE AND WAVE OBSERVATIONS BY THE VAN ALLEN PROBES. TO ADDRESS THE SCIENCE OBJECTIVES WE ANALYZE THE OBSERVATIONS IN THE MAGNETOSPHERE AND IN THE SOLAR WIND MADE BY A NUMBER OF SATELLITE MISSIONS WITH SUPPORTING OBSERVATIONS BY GROUND-BASED MAGNETOMETER NETWORKS. WE ALSO EXAMINE NUMERICAL SIMULATIONS FOR THE THEORETICAL EXPECTATIONS OF THE CHARACTERISTICS OF HIGH-M WAVES AND THEIR INTERACTIONS WITH CHARGED PARTICLES. THE SCIENCE OBJECTIVES OF THIS PROJECT ARE RELEVANT TO GOAL #2 OF THE HELIOPHYSICS DECADAL SURVEY: "DETERMINE THE DYNAMICS AND COUPLING OF EARTH S MAGNETOSPHERE IONOSPHERE AND ATMOSPHERE AND THEIR RESPONSE TO SOLAR AND TERRESTRIAL INPUTS." THE HIGH-M WAVES IN THE OUTER MAGNETOSPHERE ARE INTRINSICALLY RELATED TO THE RESONANT INTERACTIONS WITH CHARGED PARTICLES BUT THE QUANTITATIVE UNDERSTANDING ABOUT THEIR OCCURRENCE AND THE RELATIONSHIP TO SOLAR WIND CONDITIONS ARE STILL INSUFFICIENT. THIS INVESTIGATION CAN BRING IN NEW AND NEEDED KNOWLEDGE IN RESPONSE TO ONE OF THE DECADAL SURVEY GOALS. $0 5/3/18