ࡱ;  Root Entry  \pCalc Ba=@=Z?N*8X"1Arial1Arial1Arial1Arial1Arial1Symbol1Arial1Symbol1Arial1Arial1& Arial Black#,##0\ "$";\-#,##0\ "$"!#,##0\ "$";[Red]\-#,##0\ "$""#,##0.00\ "$";\-#,##0.00\ "$"'"#,##0.00\ "$";[Red]\-#,##0.00\ "$";*6_-* #,##0\ "$"_-;\-* #,##0\ "$"_-;_-* "-"\ "$"_-;_-@_-8)3_-* #,##0\ _$_-;\-* #,##0\ _$_-;_-* "-"\ _$_-;_-@_-C,>_-* #,##0.00\ "$"_-;\-* #,##0.00\ "$"_-;_-* "-"??\ "$"_-;_-@_-@+;_-* #,##0.00\ _$_-;\-* #,##0.00\ _$_-;_-* "-"??\ _$_-;_-@_- GENERAL                + ) , *  (8 *8 *8 (8 *8 *8 (8 *8 (8 *8 *8 (8 *8 *8  ( "8 !8 8 8  *8   8 8 8  8 8 8  (p (8p "8p 8p 8 8 x  x x 8p 83ffff̙̙3f3fff3f3f33333f33333`@ ChallengesT%Sheet2d0Sheet3  ;jb( 3  @@   2002 Decadal Mag. Rec. Plasma Proc.Plasma/ Neutral Sol. Sys.Mag. Dyn. Solar, Plan., StellarSolar Effects EarthEarth's Mag/ITMSolar Var. Driver Stellar PlanHuman/ Robot Explorers Predict SWPredict Safe Travel SW Explorers Challenges Frontier 1 Frontier 2 Frontier 3 Frontier 4Home 1Home 2Home 3Home 4 Journey 1 Journey 2 Journey 3 Journey 4 Dynamic SunHelioSphere GalaxySolar Wind/ Earth and PlanetsBasic Physical Principles'Predictive Capability/ Human ActivitiesM2005 SSSC Strategic Roadmap Primary Science Objectives & Research Focus Areas>2002 Solar and Space Physics Decadal Survey Science Challenges1. Understanding the structure and dynamics of the Sun's interior, the generation of solar magnetic fields, the origin of solar cycle, the causes of solar activity, and the structure and dynamics of the corona2. Understanding heliospheric structure, the distribution of magnetic fields and matter throughout the solar system, and the interaction of the solar atmosphere with the local interstellar medium3. Understanding the space environments of Earth and other solar system bodies and their dynamical response to external and internal influencesi4. Understanding the basic physical principles manifest to processes observed in solar and space plasmas5. Developing near-real-time predictive capability for understanding and quantifying the impact on human activities of dynamical processes at the Sun, in the interplanetary medium, and in the Earth's magnetosphere;Objective F: Open the Frontier to Space Weather PredictionUnderstand the fundamental physical processes of the space environment - from the Sun to Earth, to other planets, and beyond to the interstellar medium rRFA F1: Understand magnetic reconnection as revealed in solar flares, coronal mass ejections, and geospace stormsF1XXXXXQRFA F2: Understand the plasmas processes that accelerate and transport particlesF2XXX}RFA F3: Understand the role of plasmas and neutral interactions in nonlinear coupling of regions throughout the solar systemF3XXXXRFA F4: Understand the creation and variability of magnetic dynamos and how they drive the dynamics of solar, planetary and stellar environmentsF4XXXX8Objective H: Understand the Nature of Our Home in SpaceUnderstand how human society, technological systems, and the habitability of planets are affected by solar variability and planetary magnetic fields|RFA H1: Understand the causes and subsequent evolution of solar activity that affects Earth's space climate and environmentH1XXXXXRFA H2: Determine changes in the Earth's magnetosphere, ionosphere, and upper atmosphere to enable specification, prediction, and mitigation of their effectsH2XXXRFA H3: Understand the role of the Sun as an energy source to Earth's atmosphere, and in particular the role of solar variability in driving atmospheric and climate changeH3XXXRFA H4: Apply our understanding of space plasmas physics to the role of stellar activity and magnetic shielding in planetary system evolution and habitabilityH4XXXX.Objective J: Safeguarding our Outward JourneyMaximize the safety and productivity of human and robotic explorers by developing the capability to predict the extreme and dynamic conditions in spaceRFA J1: Characterize the variability, extremes, and boundary conditions of the space environments that will be encountered by human and robotic explorersJ1XXRFA J2: Develop the capability to predict the origin and onset of solar activity and disturbances associated with potentially hazardous space weatherJ2XXRFA J3: Develop the capability to predict the propagation and evolution of energetic particles to enable safe travel for human and robotic explorersJ3XXX}RFA Area J4: Understand how space weather affects planetary environments in order to minimize risk in exploration activitiesJ4XXX {   dMbP?*+_%&C&16Comparison of the SSSC 2005 Strategic Roadmap Primary Science Objectives Research Focus Areas Decadal Survey Science Challenges&?'[[?([[?)333333?"Y,,??U} %} n} % }  }  % } ' } % } i } % } %  @;@@ @  @ $                                     $~          $~  !  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