Difference between revisions of "Solar radiation"
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*The electromagnetic spectrum is radiated from a near-"Black Body" at 5800K. | *The electromagnetic spectrum is radiated from a near-"Black Body" at 5800K. | ||
| − | *High energy ions can be excited by [[solar wind]] interactions and/or emitted directly from [[solar flares]] or subsequent [[Coronal Mass Ejections]]. A solar proton event (SPE) occurs when the intensity of this radiation temporarily spikes after a solar flare or CME. In an SPE, the intensity of particulate radiation can increase by up to 5 orders of magnitude over the normal level, with radiation returning to the baseline level after several days.<ref>Schimmerling W. (2011, Feb 5). The Space Radiation Environment: An Introduction. <nowiki>https://three.jsc.nasa.gov/concepts/SpaceRadiationEnviron.pdf</nowiki></ref> | + | *High energy ions can be excited by [[solar wind]] interactions and/or emitted directly from [[solar flares]] or subsequent [[Coronal Mass Ejections]]. A solar proton event (SPE) occurs when the intensity of this radiation temporarily spikes after a solar flare or CME. In an SPE, the intensity of particulate radiation can increase by up to 5 orders of magnitude over the normal level, with radiation returning to the baseline level after several days.<ref>Schimmerling W. (2011, Feb 5). The Space Radiation Environment: An Introduction. <nowiki>https://three.jsc.nasa.gov/concepts/SpaceRadiationEnviron.pdf</nowiki></ref> |
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| + | == Protection == | ||
| + | Occasional [[Solar flares|solar flares]] produce particularly high doses. Some SPEs were observed by [[MARIE]] that were not seen by sensors near Earth due to the fact that SPEs are directional. Astronauts on Mars could be warned of SPEs by sensors closer to the Sun and presumably take shelter during these events. This would imply that an [[Early warning system (solar radiation)|Early Warning System]] (possibly a network of sensors in orbit around the sun or a single sensor in [[Lagrangian point]] L1) might be needed to ensure all SPEs threatening Mars were detected early enough. | ||
{{SettlementIndex}} | {{SettlementIndex}} | ||
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[[category:Radiation Protection]] | [[category:Radiation Protection]] | ||
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Revision as of 11:10, 15 March 2020
Sources of solar radiation
Solar radiation can be split into two varieties: electromagnetic and ionized particles.
- The electromagnetic spectrum is radiated from a near-"Black Body" at 5800K.
- High energy ions can be excited by solar wind interactions and/or emitted directly from solar flares or subsequent Coronal Mass Ejections. A solar proton event (SPE) occurs when the intensity of this radiation temporarily spikes after a solar flare or CME. In an SPE, the intensity of particulate radiation can increase by up to 5 orders of magnitude over the normal level, with radiation returning to the baseline level after several days.[1]
Protection
Occasional solar flares produce particularly high doses. Some SPEs were observed by MARIE that were not seen by sensors near Earth due to the fact that SPEs are directional. Astronauts on Mars could be warned of SPEs by sensors closer to the Sun and presumably take shelter during these events. This would imply that an Early Warning System (possibly a network of sensors in orbit around the sun or a single sensor in Lagrangian point L1) might be needed to ensure all SPEs threatening Mars were detected early enough.
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- ↑ Schimmerling W. (2011, Feb 5). The Space Radiation Environment: An Introduction. https://three.jsc.nasa.gov/concepts/SpaceRadiationEnviron.pdf
