Difference between revisions of "Solar radiation"
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Revision as of 15:52, 17 December 2018
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]
| Concepts: | Greenhouse · Settlements · Locations · General |
| Hazards: | Space Weather · Climate · General |
| Technology: | Hi-Tech · Lo-Tech · Energy · Spaceflight science · Communication · General |
| Human Considerations: | Economics · Health · Governance · Trade · Law · Social |
| This article is a stub. You can help Marspedia by expanding it. |
- ↑ Schimmerling W. (2011, Feb 5). The Space Radiation Environment: An Introduction. https://three.jsc.nasa.gov/concepts/SpaceRadiationEnviron.pdf
