3 THE CONFLUENCE OF THE STEREO AND SDO MISSIONS HAS ALLOWED A LARGE FRACTION OF THE SUN TO BE SIMULTANEOUSLY OBSERVED FOR MANY YEARS AT EXTREME ULTRAVIOLET EUV WAVELENGTHS. WE PROPOSE A COMPREHENSIVE STUDY THAT LEVERAGES THIS DATA TO CHARACTERIZE THE EVOLUTION OF CORONAL HOLES CHS AND IN TURN UNDERSTAND THE DYNAMICS OF THE CORONAL MAGNETIC FIELD RESPONSIBLE FOR THESE CHANGES. OUR RESEARCH WILL ADDRESS THREE PRIMARY SCIENCE TOPICS: 1 - HOW DO CHS EVOLVE ON TIMESCALES FROM SEVERAL WEEKS TO YEARS? 2 - WHAT FRACTION OF THE INTERPLANETARY MAGNETIC FIELD EMANATES FROM CHS? 3 - HOW MUCH OF THE SOLAR WIND ARISES FROM DYNAMIC MAGNETIC FLUX CHANGE AT CH BOUNDARIES? WE WILL EMPLOY A RECENTLY DEVELOPED CH DETECTION PIPELINE DESIGNED WITH THE EXPRESS PURPOSE OF ROBUSTLY TRACKING CHS FOR WEEKS AT A TIME. THE TIMESCALE OF SEVERAL WEEKS IS CRUCIAL FOR CONNECTING THE DYNAMICAL EVOLUTION OF CHS TO THE LARGE SCALE STRUCTURE OF THE CORONA AND THE SOLAR WIND. OUR NOVEL TECHNIQUE ALLOWS US TO CONSISTENTLY MEASURE CH POSITIONS AND PROPERTIES AS THEY EVOLVE AND TRANSITION FROM THE VIEW OF ONE SPACECRAFT TO ANOTHER. WE WILL PRODUCE FULL SUN MAPS OF CH POSITIONS OVER A SUBSTANTIAL DATASET, AND USE THIS TO CHARACTERIZE THE WAY IN WHICH CH BOUNDARIES EVOLVE AND DISTORT WITH TIME. THIS ANALYSIS WILL BE SUPPLEMENTED BY OVERLAYING CH MEASUREMENTS WITH PHOTOSPHERIC FLUXES DERIVED FROM AN OBSERVATION BASED, FREELY AVAILABLE SURFACE FLUX TRANSPORT MODEL. SPECIFICALLY, THIS PROJECT WILL FOCUS ON TWO CLOSELY-RELATED THEMES: 1 - A LONG TERM STUDY OF CH EVOLUTION SPANNING THE LIFETIME OF THE STEREO MISSION. WE WILL PROCESS 195A AND 193A EUV IMAGING DATA FROM THE ENTIRE STEREO EUVI 2007 TO PRESENT AND SDO AIA 2010 TO PRESENT ARCHIVES AT A 2HR CADENCE USING OUR NEW DETECTION PIPELINE. THIS WILL PROVIDE A COMPREHENSIVE ARCHIVE OF CHS DURING THIS TIME PERIOD THAT WILL BE USED TO DERIVE LONG TERM TRENDS THAT TELL US HOW CHS EVOLVE AND HOW THEY RELATE TO THE INTERPLANETARY FLUX DERIVED FROM IN SITU MEASUREMENTS ACE WIND. 2 - DETAILED CASE STUDIES OF CH EVOLUTION AT HIGH CADENCE FOR TWO DISTINCT PERIODS. ONCE FOR A LONG LIVED CH IN EARLY 2011 AND ONCE DURING A PERIOD OF HIGH ACTIVITY IN 2012. THE FIRST CASE STUDY WILL ALLOW US TO CHARACTERIZE HOW CHS EVOLVE DURING THE ABSENCE OF LARGE SCALE FLUX EMERGENCE, WHILE THE LATTER WILL ALLOW US EXAMINE THE ROLE OF FLUX EMERGENCE SPECIFICALLY. THESE STUDIES WILL ALLOW US TO CHARACTERIZE IN DETAIL HOW CHS EVOLVE. OUR CASE STUDY RESULTS WILL ALSO BE USED TO REFINE OUR ANALYSIS AND INTERPRETATION OF THE LONGTERM STUDY. THIS PROJECT IS HIGHLY RELEVANT TO THE HELIOPHYSICS GUEST INVESTIGATORS PROGRAM. OUR OBSERVATIONAL STUDIES WILL LEVERAGE FREELY AVAILABLE MEASUREMENTS AND COMBINE INFORMATION FROM FOUR SEPARATE SPACECRAFT IN HELIOPHYSICS SYSTEM OBSERVATORY. OUR SCIENTIFIC ANALYSIS IS DIRECTLY LINKED TO IMPROVING OUR UNDERSTANDING OF THE DYNAMIC SOLAR ATMOSPHERE AND THE ORIGIN OF THE SOLAR WIND. FURTHERMORE, OUR PRIMARY DATA PRODUCT IS AN ARCHIVE OF SPACE BASED, FULL SUN EUV AND CH MAPS WHICH WILL BE MADE FREELY AVAILABLE TO THE HELIOPHYSICS COMMUNITY. Other Administrative Action $0 4/9/20 Not listed THE CONFLUENCE OF THE STEREO AND SDO MISSIONS HAS ALLOWED A LARGE FRACTION OF THE SUN TO BE SIMULTANEOUSLY OBSERVED FOR MANY YEARS AT EXTREME ULTRAVIOLET EUV WAVELENGTHS. WE PROPOSE A COMPREHENSIVE STUDY THAT LEVERAGES THIS DATA TO CHARACTERIZE THE EVOLUTION OF CORONAL HOLES CHS AND IN TURN UNDERSTAND THE DYNAMICS OF THE CORONAL MAGNETIC FIELD RESPONSIBLE FOR THESE CHANGES. OUR RESEARCH WILL ADDRESS THREE PRIMARY SCIENCE TOPICS: 1 - HOW DO CHS EVOLVE ON TIMESCALES FROM SEVERAL WEEKS TO YEARS? 2 - WHAT FRACTION OF THE INTERPLANETARY MAGNETIC FIELD EMANATES FROM CHS? 3 - HOW MUCH OF THE SOLAR WIND ARISES FROM DYNAMIC MAGNETICFLUX CHANGE AT CH BOUNDARIES?WE WILL EMPLOY A RECENTLY DEVELOPED CH DETECTION PIPELINE DESIGNED WITH THE EXPRESS PURPOSE OF ROBUSTLY TRACKING CHS FOR WEEKS AT A TIME. THE TIMESCALE OF SEVERAL WEEKS IS CRUCIAL FOR CONNECTING THE DYNAMICAL EVOLUTION OF CHS TO THE LARGE SCALE STRUCTURE OF THE CORONA AND THE SOLAR WIND. OUR NOVEL TECHNIQUE ALLOWS US TO CONSISTENTLY MEASURE CH POSITIONS AND PROPERTIES AS THEY EVOLVE AND TRANSITIONFROM THE VIEW OF ONE SPACECRAFT TO ANOTHER. WE WILL PRODUCE FULL SUN MAPS OF CH POSITIONS OVER A SUBSTANTIAL DATASET AND USE THIS TO CHARACTERIZE THE WAY IN WHICH CH BOUNDARIES EVOLVE AND DISTORT WITH TIME. THIS ANALYSIS WILL BE SUPPLEMENTED BY OVERLAYING CH MEASUREMENTS WITH PHOTOSPHERIC FLUXES DERIVED FROM AN OBSERVATION BASED FREELY AVAILABLE SURFACE FLUX TRANSPORT MODEL. SPECIFICALLY THIS PROJECT WILL FOCUS ON TWO CLOSELY-RELATED THEMES:1 - A LONG TERM STUDY OF CH EVOLUTION SPANNING THE LIFETIME OF THE STEREO MISSION. WE WILL PROCESS 195A AND 193A EUV IMAGING DATA FROM THE ENTIRE STEREO EUVI 2007 TO PRESENT AND SDO AIA 2010 TO PRESENT ARCHIVES AT A 2HR CADENCE USING OUR NEW DETECTION PIPELINE. THIS WILL PROVIDE A COMPREHENSIVE ARCHIVE OF CHS DURING THIS TIME PERIOD THAT WILL BE USED TO DERIVE LONG TERM TRENDS THAT TELL US HOW CHS EVOLVE AND HOW THEY RELATE TO THE INTERPLANETARY FLUX DERIVED FROM IN SITU MEASUREMENTS ACE WIND.2 - DETAILED CASE STUDIES OF CH EVOLUTION AT HIGH CADENCE FOR TWO DISTINCT PERIODS. ONCE FOR A LONG LIVED CH IN EARLY 2011 AND ONCE DURING A PERIOD OF HIGH ACTIVITY IN 2012. THE FIRST CASE STUDY WILL ALLOW US TO CHARACTERIZE HOW CHS EVOLVE DURING THE ABSENCE OF LARGE SCALE FLUX EMERGENCE WHILE THE LATTER WILL ALLOW US EXAMINE THE ROLE OF FLUX EMERGENCE SPECIFICALLY. THESE STUDIES WILL ALLOW US TO CHARACTERIZE IN DETAIL HOW CHS EVOLVE. OUR CASE STUDY RESULTS WILL ALSO BE USED TO REFINE OUR ANALYSIS AND INTERPRETATION OF THE LONGTERM STUDY.THIS PROJECT IS HIGHLY RELEVANT TO THE HELIOPHYSICS GUEST INVESTIGATORS PROGRAM. OUR OBSERVATIONAL STUDIES WILL LEVERAGE FREELY AVAILABLE MEASUREMENTS AND COMBINE INFORMATION FROM FOUR SEPARATE SPACECRAFT IN HELIOPHYSICS SYSTEM OBSERVATORY. OUR SCIENTIFIC ANALYSIS IS DIRECTLY LINKED TO IMPROVING OUR UNDERSTANDING OF THE DYNAMIC SOLAR ATMOSPHERE AND THE ORIGIN OF THE SOLAR WIND. FURTHERMORE OUR PRIMARY DATA PRODUCT IS AN ARCHIVE OF SPACE BASED FULL SUN EUV AND CH MAPS WHICH WILL BE MADE FREELY AVAILABLE TO THE HELIOPHYSICS COMMUNITY. $0 4/9/20 Not listed THE CONFLUENCE OF THE STEREO AND SDO MISSIONS HAS ALLOWED A LARGE FRACTION OF THE SUN TO BE SIMULTANEOUSLY OBSERVED FOR MANY YEARS AT EXTREME ULTRAVIOLET EUV WAVELENGTHS. WE PROPOSE A COMPREHENSIVE STUDY THAT LEVERAGES THIS DATA TO CHARACTERIZE THE EVOLUTION OF CORONAL HOLES CHS AND IN TURN UNDERSTAND THE DYNAMICS OF THE CORONAL MAGNETIC FIELD RESPONSIBLE FOR THESE CHANGES. OUR RESEARCH WILL ADDRESS THREE PRIMARY SCIENCE TOPICS: 1 - HOW DO CHS EVOLVE ON TIMESCALES FROM SEVERAL WEEKS TO YEARS? 2 - WHAT FRACTION OF THE INTERPLANETARY MAGNETIC FIELD EMANATES FROM CHS? 3 - HOW MUCH OF THE SOLAR WIND ARISES FROM DYNAMIC MAGNETICFLUX CHANGE AT CH BOUNDARIES?WE WILL EMPLOY A RECENTLY DEVELOPED CH DETECTION PIPELINE DESIGNED WITH THE EXPRESS PURPOSE OF ROBUSTLY TRACKING CHS FOR WEEKS AT A TIME. THE TIMESCALE OF SEVERAL WEEKS IS CRUCIAL FOR CONNECTING THE DYNAMICAL EVOLUTION OF CHS TO THE LARGE SCALE STRUCTURE OF THE CORONA AND THE SOLAR WIND. OUR NOVEL TECHNIQUE ALLOWS US TO CONSISTENTLY MEASURE CH POSITIONS AND PROPERTIES AS THEY EVOLVE AND TRANSITIONFROM THE VIEW OF ONE SPACECRAFT TO ANOTHER. WE WILL PRODUCE FULL SUN MAPS OF CH POSITIONS OVER A SUBSTANTIAL DATASET AND USE THIS TO CHARACTERIZE THE WAY IN WHICH CH BOUNDARIES EVOLVE AND DISTORT WITH TIME. THIS ANALYSIS WILL BE SUPPLEMENTED BY OVERLAYING CH MEASUREMENTS WITH PHOTOSPHERIC FLUXES DERIVED FROM AN OBSERVATION BASED FREELY AVAILABLE SURFACE FLUX TRANSPORT MODEL. SPECIFICALLY THIS PROJECT WILL FOCUS ON TWO CLOSELY-RELATED THEMES:1 - A LONG TERM STUDY OF CH EVOLUTION SPANNING THE LIFETIME OF THE STEREO MISSION. WE WILL PROCESS 195A AND 193A EUV IMAGING DATA FROM THE ENTIRE STEREO EUVI 2007 TO PRESENT AND SDO AIA 2010 TO PRESENT ARCHIVES AT A 2HR CADENCE USING OUR NEW DETECTION PIPELINE. THIS WILL PROVIDE A COMPREHENSIVE ARCHIVE OF CHS DURING THIS TIME PERIOD THAT WILL BE USED TO DERIVE LONG TERM TRENDS THAT TELL US HOW CHS EVOLVE AND HOW THEY RELATE TO THE INTERPLANETARY FLUX DERIVED FROM IN SITU MEASUREMENTS ACE WIND.2 - DETAILED CASE STUDIES OF CH EVOLUTION AT HIGH CADENCE FOR TWO DISTINCT PERIODS. ONCE FOR A LONG LIVED CH IN EARLY 2011 AND ONCE DURING A PERIOD OF HIGH ACTIVITY IN 2012. THE FIRST CASE STUDY WILL ALLOW US TO CHARACTERIZE HOW CHS EVOLVE DURING THE ABSENCE OF LARGE SCALE FLUX EMERGENCE WHILE THE LATTER WILL ALLOW US EXAMINE THE ROLE OF FLUX EMERGENCE SPECIFICALLY. THESE STUDIES WILL ALLOW US TO CHARACTERIZE IN DETAIL HOW CHS EVOLVE. OUR CASE STUDY RESULTS WILL ALSO BE USED TO REFINE OUR ANALYSIS AND INTERPRETATION OF THE LONGTERM STUDY.THIS PROJECT IS HIGHLY RELEVANT TO THE HELIOPHYSICS GUEST INVESTIGATORS PROGRAM. OUR OBSERVATIONAL STUDIES WILL LEVERAGE FREELY AVAILABLE MEASUREMENTS AND COMBINE INFORMATION FROM FOUR SEPARATE SPACECRAFT IN HELIOPHYSICS SYSTEM OBSERVATORY. OUR SCIENTIFIC ANALYSIS IS DIRECTLY LINKED TO IMPROVING OUR UNDERSTANDING OF THE DYNAMIC SOLAR ATMOSPHERE AND THE ORIGIN OF THE SOLAR WIND. FURTHERMORE OUR PRIMARY DATA PRODUCT IS AN ARCHIVE OF SPACE BASED FULL SUN EUV AND CH MAPS WHICH WILL BE MADE FREELY AVAILABLE TO THE HELIOPHYSICS COMMUNITY. $150.0k 3/1/19 2 THE CONFLUENCE OF THE STEREO AND SDO MISSIONS HAS ALLOWED A LARGE FRACTION OF THE SUN TO BE SIMULTANEOUSLY OBSERVED FOR MANY YEARS AT EXTREME ULTRAVIOLET EUV WAVELENGTHS. WE PROPOSE A COMPREHENSIVE STUDY THAT LEVERAGES THIS DATA TO CHARACTERIZE THE EVOLUTION OF CORONAL HOLES CHS AND IN TURN UNDERSTAND THE DYNAMICS OF THE CORONAL MAGNETIC FIELD RESPONSIBLE FOR THESE CHANGES. OUR RESEARCH WILL ADDRESS THREE PRIMARY SCIENCE TOPICS: 1 - HOW DO CHS EVOLVE ON TIMESCALES FROM SEVERAL WEEKS TO YEARS? 2 - WHAT FRACTION OF THE INTERPLANETARY MAGNETIC FIELD EMANATES FROM CHS? 3 - HOW MUCH OF THE SOLAR WIND ARISES FROM DYNAMIC MAGNETIC FLUX CHANGE AT CH BOUNDARIES? WE WILL EMPLOY A RECENTLY DEVELOPED CH DETECTION PIPELINE DESIGNED WITH THE EXPRESS PURPOSE OF ROBUSTLY TRACKING CHS FOR WEEKS AT A TIME. THE TIMESCALE OF SEVERAL WEEKS IS CRUCIAL FOR CONNECTING THE DYNAMICAL EVOLUTION OF CHS TO THE LARGE SCALE STRUCTURE OF THE CORONA AND THE SOLAR WIND. OUR NOVEL TECHNIQUE ALLOWS US TO CONSISTENTLY MEASURE CH POSITIONS AND PROPERTIES AS THEY EVOLVE AND TRANSITION FROM THE VIEW OF ONE SPACECRAFT TO ANOTHER. WE WILL PRODUCE FULL SUN MAPS OF CH POSITIONS OVER A SUBSTANTIAL DATASET, AND USE THIS TO CHARACTERIZE THE WAY IN WHICH CH BOUNDARIES EVOLVE AND DISTORT WITH TIME. THIS ANALYSIS WILL BE SUPPLEMENTED BY OVERLAYING CH MEASUREMENTS WITH PHOTOSPHERIC FLUXES DERIVED FROM AN OBSERVATION BASED, FREELY AVAILABLE SURFACE FLUX TRANSPORT MODEL. SPECIFICALLY, THIS PROJECT WILL FOCUS ON TWO CLOSELY-RELATED THEMES: 1 - A LONG TERM STUDY OF CH EVOLUTION SPANNING THE LIFETIME OF THE STEREO MISSION. WE WILL PROCESS 195A AND 193A EUV IMAGING DATA FROM THE ENTIRE STEREO EUVI 2007 TO PRESENT AND SDO AIA 2010 TO PRESENT ARCHIVES AT A 2HR CADENCE USING OUR NEW DETECTION PIPELINE. THIS WILL PROVIDE A COMPREHENSIVE ARCHIVE OF CHS DURING THIS TIME PERIOD THAT WILL BE USED TO DERIVE LONG TERM TRENDS THAT TELL US HOW CHS EVOLVE AND HOW THEY RELATE TO THE INTERPLANETARY FLUX DERIVED FROM IN SITU MEASUREMENTS ACE WIND. 2 - DETAILED CASE STUDIES OF CH EVOLUTION AT HIGH CADENCE FOR TWO DISTINCT PERIODS. ONCE FOR A LONG LIVED CH IN EARLY 2011 AND ONCE DURING A PERIOD OF HIGH ACTIVITY IN 2012. THE FIRST CASE STUDY WILL ALLOW US TO CHARACTERIZE HOW CHS EVOLVE DURING THE ABSENCE OF LARGE SCALE FLUX EMERGENCE, WHILE THE LATTER WILL ALLOW US EXAMINE THE ROLE OF FLUX EMERGENCE SPECIFICALLY. THESE STUDIES WILL ALLOW US TO CHARACTERIZE IN DETAIL HOW CHS EVOLVE. OUR CASE STUDY RESULTS WILL ALSO BE USED TO REFINE OUR ANALYSIS AND INTERPRETATION OF THE LONGTERM STUDY. THIS PROJECT IS HIGHLY RELEVANT TO THE HELIOPHYSICS GUEST INVESTIGATORS PROGRAM. OUR OBSERVATIONAL STUDIES WILL LEVERAGE FREELY AVAILABLE MEASUREMENTS AND COMBINE INFORMATION FROM FOUR SEPARATE SPACECRAFT IN HELIOPHYSICS SYSTEM OBSERVATORY. OUR SCIENTIFIC ANALYSIS IS DIRECTLY LINKED TO IMPROVING OUR UNDERSTANDING OF THE DYNAMIC SOLAR ATMOSPHERE AND THE ORIGIN OF THE SOLAR WIND. FURTHERMORE, OUR PRIMARY DATA PRODUCT IS AN ARCHIVE OF SPACE BASED, FULL SUN EUV AND CH MAPS WHICH WILL BE MADE FREELY AVAILABLE TO THE HELIOPHYSICS COMMUNITY. Funding Only Action $150.0k 3/1/19 1 THE CONFLUENCE OF THE STEREO AND SDO MISSIONS HAS ALLOWED A LARGE FRACTION OF THE SUN TO BE SIMULTANEOUSLY OBSERVED FOR MANY YEARS AT EXTREME ULTRAVIOLET EUV WAVELENGTHS. WE PROPOSE A COMPREHENSIVE STUDY THAT LEVERAGES THIS DATA TO CHARACTERIZE THE EVOLUTION OF CORONAL HOLES CHS AND IN TURN UNDERSTAND THE DYNAMICS OF THE CORONAL MAGNETIC FIELD RESPONSIBLE FOR THESE CHANGES. OUR RESEARCH WILL ADDRESS THREE PRIMARY SCIENCE TOPICS: 1 - HOW DO CHS EVOLVE ON TIMESCALES FROM SEVERAL WEEKS TO YEARS? 2 - WHAT FRACTION OF THE INTERPLANETARY MAGNETIC FIELD EMANATES FROM CHS? 3 - HOW MUCH OF THE SOLAR WIND ARISES FROM DYNAMIC MAGNETIC FLUX CHANGE AT CH BOUNDARIES? WE WILL EMPLOY A RECENTLY DEVELOPED CH DETECTION PIPELINE DESIGNED WITH THE EXPRESS PURPOSE OF ROBUSTLY TRACKING CHS FOR WEEKS AT A TIME. THE TIMESCALE OF SEVERAL WEEKS IS CRUCIAL FOR CONNECTING THE DYNAMICAL EVOLUTION OF CHS TO THE LARGE SCALE STRUCTURE OF THE CORONA AND THE SOLAR WIND. OUR NOVEL TECHNIQUE ALLOWS US TO CONSISTENTLY MEASURE CH POSITIONS AND PROPERTIES AS THEY EVOLVE AND TRANSITION FROM THE VIEW OF ONE SPACECRAFT TO ANOTHER. WE WILL PRODUCE FULL SUN MAPS OF CH POSITIONS OVER A SUBSTANTIAL DATASET, AND USE THIS TO CHARACTERIZE THE WAY IN WHICH CH BOUNDARIES EVOLVE AND DISTORT WITH TIME. THIS ANALYSIS WILL BE SUPPLEMENTED BY OVERLAYING CH MEASUREMENTS WITH PHOTOSPHERIC FLUXES DERIVED FROM AN OBSERVATION BASED, FREELY AVAILABLE SURFACE FLUX TRANSPORT MODEL. SPECIFICALLY, THIS PROJECT WILL FOCUS ON TWO CLOSELY-RELATED THEMES: 1 - A LONG TERM STUDY OF CH EVOLUTION SPANNING THE LIFETIME OF THE STEREO MISSION. WE WILL PROCESS 195A AND 193A EUV IMAGING DATA FROM THE ENTIRE STEREO EUVI 2007 TO PRESENT AND SDO AIA 2010 TO PRESENT ARCHIVES AT A 2HR CADENCE USING OUR NEW DETECTION PIPELINE. THIS WILL PROVIDE A COMPREHENSIVE ARCHIVE OF CHS DURING THIS TIME PERIOD THAT WILL BE USED TO DERIVE LONG TERM TRENDS THAT TELL US HOW CHS EVOLVE AND HOW THEY RELATE TO THE INTERPLANETARY FLUX DERIVED FROM IN SITU MEASUREMENTS ACE WIND. 2 - DETAILED CASE STUDIES OF CH EVOLUTION AT HIGH CADENCE FOR TWO DISTINCT PERIODS. ONCE FOR A LONG LIVED CH IN EARLY 2011 AND ONCE DURING A PERIOD OF HIGH ACTIVITY IN 2012. THE FIRST CASE STUDY WILL ALLOW US TO CHARACTERIZE HOW CHS EVOLVE DURING THE ABSENCE OF LARGE SCALE FLUX EMERGENCE, WHILE THE LATTER WILL ALLOW US EXAMINE THE ROLE OF FLUX EMERGENCE SPECIFICALLY. THESE STUDIES WILL ALLOW US TO CHARACTERIZE IN DETAIL HOW CHS EVOLVE. OUR CASE STUDY RESULTS WILL ALSO BE USED TO REFINE OUR ANALYSIS AND INTERPRETATION OF THE LONGTERM STUDY. THIS PROJECT IS HIGHLY RELEVANT TO THE HELIOPHYSICS GUEST INVESTIGATORS PROGRAM. OUR OBSERVATIONAL STUDIES WILL LEVERAGE FREELY AVAILABLE MEASUREMENTS AND COMBINE INFORMATION FROM FOUR SEPARATE SPACECRAFT IN HELIOPHYSICS SYSTEM OBSERVATORY. OUR SCIENTIFIC ANALYSIS IS DIRECTLY LINKED TO IMPROVING OUR UNDERSTANDING OF THE DYNAMIC SOLAR ATMOSPHERE AND THE ORIGIN OF THE SOLAR WIND. FURTHERMORE, OUR PRIMARY DATA PRODUCT IS AN ARCHIVE OF SPACE BASED, FULL SUN EUV AND CH MAPS WHICH WILL BE MADE FREELY AVAILABLE TO THE HELIOPHYSICS COMMUNITY. Funding Only Action $145.0k 3/1/18