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هوافضا::
باد خورشیدی
It will operate in a solar polar orbit, to observe, for the first time, the magnetic field in solar-pole regions and its velocity field through spectral and imaging observations, so as to unveil the mechanism of solar activity cycle and understand the origin of high-speed solar wind.
It is capable of continuously observing the solar wind from areas near the Sun to those near the magnetosphere.
KUAFU will: (a) Perform integrated, continuous, multi-layered long-term observation of the origin of solar wind and CME eruptions
SPORT (Fig. 4.9) will observe CMEs, solar high-latitude mag- netism, and the fast solar wind from a polar orbit around the Sun.
vantage point at high latitude, and investigate solar high-latitude magnetism giving rise to eruptions and the fast solar wind.
واژگان شبکه مترجمین ایران