Transcription of The Radiation Environment - NASA
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J. Barth/Code 562 The Radiation EnvironmentSolar Protons&Heavier IonsGalactic Cosmic RaysTrapped ParticlesNikkei Science, Inc. of Japan, by K. EndoJ. Barth/Code 562 Components of the Natural EnvironmentuTransient Galactic Cosmic Rays Protons & Heavier Ions Solar Particle Events Protons & Heavier IonsuTrapped Electrons, Protons, & Heavier IonsuAtmospheric & Terrestrial Secondaries NeutronsJ. Barth/Code 562 Radiation & EffectsuTotal Ionizing Dose Cumulative long termionizing damage due toprotons & electronsuDisplacement Damage Cumulative long term non-ionizing damage due toprotons, electrons, &neutronsuSingle Event Effects Event caused by a singlecharged particle - heavy ions& protons for some devicesE. Daly/ESAJ. Barth/Code 562 SunYohkoh/SXTS olarFlareuDominates theRadiationEnvironment Source ModulatoruStructure Photosphere Chromosphere CoronaJ. Barth/Code 562 Solar WinduStream of Charged Particles from Sun sCorona Electrons Protons Heavy IonsuMagnetized PlasmauDetected Out to 10 billion km from Earth byPioneer 10uVelocity ~ 300 - 900 km/suEnergy ~.
uStream of Charged Particles from Sun’ s Corona » Electrons » Protons » Heavy Ions uMagnetized Plasma uDetected Out to 10 billion km from Earth by Pioneer 10 uVelocity ~ 300 - 900 km/s uEnergy ~ .5 - 2.0 keV/nuc} Density ~ 1 - 30 / cm3
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