NASA Sun-Solar System Connection Roadmap 1 Targeted Outcome: Phase 2005-2015, Safeguarding our Outbound Journey Determine Extremes of the Variable Radiation.

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Presentation transcript:

NASA Sun-Solar System Connection Roadmap 1 Targeted Outcome: Phase , Safeguarding our Outbound Journey Determine Extremes of the Variable Radiation & Space Environments at Earth, Moon, & Mars J1A: Targeted Outcome to Capabilities to Implementation Measurements of atmospheric, ionospheric, magnetospheric & interplanetary environment enhancements & conditions of occurrence Determine relationships of trapped & SEP fluxes plus atmosphere & ionosphere changes with solar- interplanetary conditions Enabling Capabilities & Measurements Assimilative & theoretical models to provide linkage between observables & near term plus future environmental enhancements Implementation Phase 1: Required Understanding Variability of Space Environments: at & between Earth, Moon & Mars CME Associated Planetary & Interplanetary Radiation Responses Processes That Lead To Extreme Environments High Speed Stream Associated Radiation Responses Causes of Surface, Atmosphere, Ionosphere & Magnetosphere Environment Enhancements Internal Processes of Magnetospheric Radiation Enhancements Current Missions: TIMED, Soho, ACE, Cassini, Cluster, etc.: Extend environment data bases & inform on current environment conditions in support of model development & testing SDO, RBSP, ITSP to provide new environmental measurements and provide the data for new model and theory development relevent to particle acceleratio, ionosphere structure and responses plus measure variability of photonic inputs to Earth and Mars atmospheres. Inner Sentinels at end to start analyses of inner heliosphere SEP acceleration and propagation Model Development: To provide linkage between spatial regions plus source-response relationships Theory Program: To understand responses of planetary (Earth, Moon, Mars) & interplanetary environments to solar and internal drivers LCAS Campaigns: Upper atmosphere & ionosphere responses to energy inputs + determine atmospheric GCR & SEP shielding efficiencies (has direct Mars applications) Measurements needed from planetary atmospheres through interplanetary medium MMS: Additional environmental measurements and data for new model and theory development plus data on SEP magnetotail access DATA MINING Program: Required to determine extreme: Combine all past & current observations to find extreme environments with reasonable probability(Virtual Observatory) Cosmic Rays: Low Earth Orbit Out to Moon & Mars Great Observatory Enabling Contrubuting LWS STP Partner w Exploration Enabling

NASA Sun-Solar System Connection Roadmap 2 MMS Reconnection STEREO CME Propagation Step 5: Known Resources to be applied Low- to mid cost, multi-objective, strategically planned for fundamental space physics and space weather investigations Current Resources: 1 launch per 5 years Low- to mid-cost, multi-objective, strategically targeted for Life and Society Science investigations, Recommended: 1 launch per 3 years SDO Solar Dynamics RBSP Earth->Moon Radiation Explorers, single objective, strategically selected to respond to new knowledge/decision points, Recommendation: 1 launch per 2 years AIM Noctilucent Clouds THEMIS Magnetic Substorms IBEX Interstellar Boundary MIDEXSMEXMIDEXSMEXMIDEXSMEX Important for completion–> Partnership In Development Solar-B Solar Magnetic Fields