Radiation Effects on Satellites During Extreme Space Weather Events
Radiation Effects on Satellites During Extreme Space Weather Events
复制标题
DOI:
10.1029/2018sw001913
复制
发表时间:
2018-09-01
影响因子:
3.7
通讯作者:
Horne, R. B.
中科院分区:
文献类型:
--
作者:
Hands, A. D. P.;Ryden, K. A.;Horne, R. B.
High-energy trapped electrons in the Van Allen belts pose a threat to the survivability of orbiting spacecraft. Two key radiation effects are total ionizing dose and displacement damage dose in components and materials, both of which cause cumulative and largely irreversible damage. During an extreme space weather event, trapped electron fluxes in the Van Allen belts can increase by several orders of magnitude in intensity, leading to an enhanced risk of satellite failure. We use extreme environments generated by modeling and statistical analyses to estimate the consequences for satellites in terms of the radiation effects described above. A worst-case event could lead to significant losses in power generating capabilityup to almost 8%and cause up to four years' worth of ionizing dose degradation, leading to component damage and a life-shortening effect on satellites. The consequences of such losses are hugely significant given our increasing reliance on satellites for a vast array of services, including communication, navigation, defense, and critical infrastructure.Plain Language Summary Satellites are exposed to a variety of sources of potentially damaging space radiation. One of the most important of these is the population of high-energy electrons that lies trapped by the Earth's magnetic fieldthe so-called Van Allen belts. During an extreme space weather event, trapped electron fluxes in the Van Allen belts can increase by several orders of magnitude in intensity, leading to an enhanced risk of satellite damage. One example of this damage is degradation in the power-generating capability of satellite solar panels. The threat from space weather in this context has hitherto been associated with solar proton events, that is, bursts of energetic protons that are sporadically emitted from the Sun. However, our analysis shows that enhancements in the Van Allen belt electron population can exceed the solar proton threat, which has implications for the protection of satellites from such phenomena. It is essential that sufficiently robust engineering design measures are put in place, in order to ensure the future reliability of satellite technology, on which our society is increasingly reliant.