Not listed THIS IS A "PHASE 3" SUCCESSOR PROPOSAL THAT IS A CONTINUATION OF WORK FUNDED BY THE ASTROPHYSICS RESEARCH AND ANALYSIS (APRA) PROGRAM THROUGH THE SUB-TOPIC "PARTICLE ASTROPHYSICS": CONSIDERABLE ADVANCES IN ASTROPHYSICS OF COSMIC RAYS IN RECENT YEARS HAVE BECOME POSSIBLE DUE TO SUPERIOR INSTRUMENTATION LAUNCHED INTO SPACE AND TO THE TOP OF THE ATMOSPHERE. THE ACE-CRIS AMS-02 FERMI-LAT HAWC PAMELA SUPERTIGER VOYAGER 1 2 WMAP AND MANY OTHER MISSIONS MADE A LOT OF BREAKTHROUGHS AND MORE IS EXPECTED IN THE FOLLOWING YEARS. OTHER HIGH-EXPECTATIONS MISSIONS ARE RECENTLY LAUNCHED (CALET) OR ARE AWAITING FOR LAUNCH (ISS-CREAM). THE CLAIMED PRECISION OF THE AMS-02 DATA REACHES 1-3%. TAKING FULL ADVANTAGE OF THE HIGH QUALITY DATA REQUIRES NUMERICAL MODELS OF COMPARABLE ACCURACY. THE CURRENT STATE-OF-THE-ART COSMIC RAY PROPAGATION MODEL IS GALPROP WHICH HAS BECOME A STANDARD ANALYSIS TOOL IN ASTROPHYSICS OF COSMIC RAYS STUDIES OF THE DIFFUSE EMISSIONS AND RELATED FIELDS. IT PROVIDES A UNIFIED FRAMEWORK FOR THE INTERPRETATION OF DATA COLLECTED BY MANY DIFFERENT KINDS OF EXPERIMENTS AND EMPHASIZES THE INTERRELATIONSHIP BETWEEN DIFFERENT TYPES OF DATA. WE ARE PROPOSING CONSIDERABLE IMPROVEMENTS OF THE GALPROP MODEL AND TOOL THAT INCLUDE GENERALIZATION OF THE DESCRIPTION OF THE COMPONENTS OF THE GALACTIC INTERSTELLAR MEDIUM TO THE FULL 3D AND EXTENSIVE APPLICATION OF THE BAYESIAN TOOLS IN BUILDING SUCH DATA-SETS DEVELOPMENT OF A HELIOSPHERIC PROPAGATION TOOL FULLY COMPATIBLE WITH GALPROP DEVELOPMENT OF A RELIABLE DIFFUSE EMISSION MODEL IN THE KEV-TEV ENERGY RANGE GENERALIZATION OF THE NUCLEAR REACTION NETWORK AND CROSS SECTION ROUTINES TO INCLUDE TRANS-IRON NUCLIDES IMPROVEMENTS IN THE DESCRIPTION OF THE PRODUCTION OF SECONDARY PARTICLES IN COSMIC RAY INTERACTIONS VARIOUS SPEED AND MEMORY OPTIMIZATIONS. WE WILL CONTINUE TO SUPPORT A DEDICATED WEBSITE WHICH HOSTS GALPROP WEBRUN A USER-FRIENDLY INTERFACE FOR RUNNING THE GALPROP CODE ON A DEDICATED CLUSTER TOGETHER WITH THE SOURCE CODE RESULTS OF PUBLISHED MODELS MANUALS A USER FORUM AND OTHER RELEVANT ASTROPHYSICAL INFORMATION. THE IMPROVED GALPROP MODEL WILL BE PUBLICLY AVAILABLE AS WAS THE CASE WITH PREVIOUS VERSIONS OF THE CODE. $0 9/15/21 12 THIS IS A "PHASE 3" SUCCESSOR PROPOSAL THAT IS A CONTINUATION OF WORK FUNDED BY THE ASTROPHYSICS RESEARCH AND ANALYSIS (APRA) PROGRAM THROUGH THE SUB-TOPIC "PARTICLE ASTROPHYSICS": CONSIDERABLE ADVANCES IN ASTROPHYSICS OF COSMIC RAYS IN RECENT YEARS HAVE BECOME POSSIBLE DUE TO SUPERIOR INSTRUMENTATION LAUNCHED INTO SPACE AND TO THE TOP OF THE ATMOSPHERE. THE ACE-CRIS, AMS-02, FERMI-LAT, HAWC, PAMELA, SUPERTIGER, VOYAGER 1,2, WMAP, AND MANY OTHER MISSIONS MADE A LOT OF BREAKTHROUGHS AND MORE IS EXPECTED IN THE FOLLOWING YEARS. OTHER HIGH-EXPECTATIONS MISSIONS ARE RECENTLY LAUNCHED (CALET) OR ARE AWAITING FOR LAUNCH (ISS-CREAM). THE CLAIMED PRECISION OF THE AMS-02 DATA REACHES 1-3%. TAKING FULL ADVANTAGE OF THE HIGH QUALITY DATA REQUIRES NUMERICAL MODELS OF COMPARABLE ACCURACY. THE CURRENT STATE-OF-THE-ART COSMIC RAY PROPAGATION MODEL IS GALPROP, WHICH HAS BECOME A STANDARD ANALYSIS TOOL IN ASTROPHYSICS OF COSMIC RAYS, STUDIES OF THE DIFFUSE EMISSIONS, AND RELATED FIELDS. IT PROVIDES A UNIFIED FRAMEWORK FOR THE INTERPRETATION OF DATA COLLECTED BY MANY DIFFERENT KINDS OF EXPERIMENTS AND EMPHASIZES THE INTERRELATIONSHIP BETWEEN DIFFERENT TYPES OF DATA. WE ARE PROPOSING CONSIDERABLE IMPROVEMENTS OF THE GALPROP MODEL AND TOOL THAT INCLUDE GENERALIZATION OF THE DESCRIPTION OF THE COMPONENTS OF THE GALACTIC INTERSTELLAR MEDIUM TO THE FULL 3D AND EXTENSIVE APPLICATION OF THE BAYESIAN TOOLS IN BUILDING SUCH DATA-SETS, DEVELOPMENT OF A HELIOSPHERIC PROPAGATION TOOL FULLY COMPATIBLE WITH GALPROP, DEVELOPMENT OF A RELIABLE DIFFUSE EMISSION MODEL IN THE KEV-TEV ENERGY RANGE, GENERALIZATION OF THE NUCLEAR REACTION NETWORK AND CROSS SECTION ROUTINES TO INCLUDE TRANS-IRON NUCLIDES, IMPROVEMENTS IN THE DESCRIPTION OF THE PRODUCTION OF SECONDARY PARTICLES IN COSMIC RAY INTERACTIONS, VARIOUS SPEED AND MEMORY OPTIMIZATIONS. WE WILL CONTINUE TO SUPPORT A DEDICATED WEBSITE WHICH HOSTS GALPROP WEBRUN, A USER-FRIENDLY INTERFACE FOR RUNNING THE GALPROP CODE ON A DEDICATED CLUSTER, TOGETHER WITH THE SOURCE CODE, RESULTS OF PUBLISHED MODELS, MANUALS, A USER FORUM, AND OTHER RELEVANT ASTROPHYSICAL INFORMATION. THE IMPROVED GALPROP MODEL WILL BE PUBLICLY AVAILABLE AS WAS THE CASE WITH PREVIOUS VERSIONS OF THE CODE. Funding Only Action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ther Administrative Action $0 9/15/21 Not listed THIS IS A "PHASE 3" SUCCESSOR PROPOSAL THAT IS A CONTINUATION OF WORK FUNDED BY THE ASTROPHYSICS RESEARCH AND ANALYSIS (APRA) PROGRAM THROUGH THE SUB-TOPIC "PARTICLE ASTROPHYSICS": CONSIDERABLE ADVANCES IN ASTROPHYSICS OF COSMIC RAYS IN RECENT YEARS HAVE BECOME POSSIBLE DUE TO SUPERIOR INSTRUMENTATION LAUNCHED INTO SPACE AND TO THE TOP OF THE ATMOSPHERE. THE ACE-CRIS AMS-02 FERMI-LAT HAWC PAMELA SUPERTIGER VOYAGER 1 2 WMAP AND MANY OTHER MISSIONS MADE A LOT OF BREAKTHROUGHS AND MORE IS EXPECTED IN THE FOLLOWING YEARS. OTHER HIGH-EXPECTATIONS MISSIONS ARE RECENTLY LAUNCHED (CALET) OR ARE AWAITING FOR LAUNCH (ISS-CREAM). THE CLAIMED PRECISION OF THE AMS-02 DATA REACHES 1-3%. TAKING FULL ADVANTAGE OF THE HIGH QUALITY DATA REQUIRES NUMERICAL MODELS OF COMPARABLE ACCURACY. THE CURRENT STATE-OF-THE-ART COSMIC RAY PROPAGATION MODEL IS GALPROP WHICH HAS BECOME A STANDARD ANALYSIS TOOL IN ASTROPHYSICS OF COSMIC RAYS STUDIES OF THE DIFFUSE EMISSIONS AND RELATED FIELDS. IT PROVIDES A UNIFIED FRAMEWORK FOR THE INTERPRETATION OF DATA COLLECTED BY MANY DIFFERENT KINDS OF EXPERIMENTS AND EMPHASIZES THE INTERRELATIONSHIP BETWEEN DIFFERENT TYPES OF DATA. WE ARE PROPOSING CONSIDERABLE IMPROVEMENTS OF THE GALPROP MODEL AND TOOL THAT INCLUDE GENERALIZATION OF THE DESCRIPTION OF THE COMPONENTS OF THE GALACTIC INTERSTELLAR MEDIUM TO THE FULL 3D AND EXTENSIVE APPLICATION OF THE BAYESIAN TOOLS IN BUILDING SUCH DATA-SETS DEVELOPMENT OF A HELIOSPHERIC PROPAGATION TOOL FULLY COMPATIBLE WITH GALPROP DEVELOPMENT OF A RELIABLE DIFFUSE EMISSION MODEL IN THE KEV-TEV ENERGY RANGE GENERALIZATION OF THE NUCLEAR REACTION NETWORK AND CROSS SECTION ROUTINES TO INCLUDE TRANS-IRON NUCLIDES IMPROVEMENTS IN THE DESCRIPTION OF THE PRODUCTION OF SECONDARY PARTICLES IN COSMIC RAY INTERACTIONS VARIOUS SPEED AND MEMORY OPTIMIZATIONS. WE WILL CONTINUE TO SUPPORT A DEDICATED WEBSITE WHICH HOSTS GALPROP WEBRUN A USER-FRIENDLY INTERFACE FOR RUNNING THE GALPROP CODE ON A DEDICATED CLUSTER TOGETHER WITH THE SOURCE CODE RESULTS OF PUBLISHED MODELS MANUALS A USER FORUM AND OTHER RELEVANT ASTROPHYSICAL INFORMATION. THE IMPROVED GALPROP MODEL WILL BE PUBLICLY AVAILABLE AS WAS THE CASE WITH PREVIOUS VERSIONS OF THE CODE. ($11) 9/15/21 Not listed THIS IS A "PHASE 3" SUCCESSOR PROPOSAL THAT IS A CONTINUATION OF WORK FUNDED BY THE ASTROPHYSICS RESEARCH AND ANALYSIS (APRA) PROGRAM THROUGH THE SUB-TOPIC "PARTICLE ASTROPHYSICS": CONSIDERABLE ADVANCES IN ASTROPHYSICS OF COSMIC RAYS IN RECENT YEARS HAVE BECOME POSSIBLE DUE TO SUPERIOR INSTRUMENTATION LAUNCHED INTO SPACE AND TO THE TOP OF THE ATMOSPHERE. THE ACE-CRIS AMS-02 FERMI-LAT HAWC PAMELA SUPERTIGER VOYAGER 1 2 WMAP AND MANY OTHER MISSIONS MADE A LOT OF BREAKTHROUGHS AND MORE IS EXPECTED IN THE FOLLOWING YEARS. OTHER HIGH-EXPECTATIONS MISSIONS ARE RECENTLY LAUNCHED (CALET) OR ARE AWAITING FOR LAUNCH (ISS-CREAM). THE CLAIMED PRECISION OF THE AMS-02 DATA REACHES 1-3%. TAKING FULL ADVANTAGE OF THE HIGH QUALITY DATA REQUIRES NUMERICAL MODELS OF COMPARABLE ACCURACY. THE CURRENT STATE-OF-THE-ART COSMIC RAY PROPAGATION MODEL IS GALPROP WHICH HAS BECOME A STANDARD ANALYSIS TOOL IN ASTROPHYSICS OF COSMIC RAYS STUDIES OF THE DIFFUSE EMISSIONS AND RELATED FIELDS. IT PROVIDES A UNIFIED FRAMEWORK FOR THE INTERPRETATION OF DATA COLLECTED BY MANY DIFFERENT KINDS OF EXPERIMENTS AND EMPHASIZES THE INTERRELATIONSHIP BETWEEN DIFFERENT TYPES OF DATA. WE ARE PROPOSING CONSIDERABLE IMPROVEMENTS OF THE GALPROP MODEL AND TOOL THAT INCLUDE GENERALIZATION OF THE DESCRIPTION OF THE COMPONENTS OF THE GALACTIC INTERSTELLAR MEDIUM TO THE FULL 3D AND EXTENSIVE APPLICATION OF THE BAYESIAN TOOLS IN BUILDING SUCH DATA-SETS DEVELOPMENT OF A HELIOSPHERIC PROPAGATION TOOL FULLY COMPATIBLE WITH GALPROP DEVELOPMENT OF A RELIABLE DIFFUSE EMISSION MODEL IN THE KEV-TEV ENERGY RANGE GENERALIZATION OF THE NUCLEAR REACTION NETWORK AND CROSS SECTION ROUTINES TO INCLUDE TRANS-IRON NUCLIDES IMPROVEMENTS IN THE DESCRIPTION OF THE PRODUCTION OF SECONDARY PARTICLES IN COSMIC RAY INTERACTIONS VARIOUS SPEED AND MEMORY OPTIMIZATIONS. WE WILL CONTINUE TO SUPPORT A DEDICATED WEBSITE WHICH HOSTS GALPROP WEBRUN A USER-FRIENDLY INTERFACE FOR RUNNING THE GALPROP CODE ON A DEDICATED CLUSTER TOGETHER WITH THE SOURCE CODE RESULTS OF PUBLISHED MODELS MANUALS A USER FORUM AND OTHER RELEVANT ASTROPHYSICAL INFORMATION. THE IMPROVED GALPROP MODEL WILL BE PUBLICLY AVAILABLE AS WAS THE CASE WITH PREVIOUS VERSIONS OF THE CODE. $343.6k 9/23/20