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RECENT RESULTS FROM THE IMAGE MISSION

机译:图像任务的最新结果

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摘要

The IMAGE satellite was launched on March 25, 2000 into an elliptical polar orbit with apogee of 8.2 Earth radii (geocentric) over the north pole. With this satellite, magnetospheric plasmas are imaged using ultraviolet, energetic neutral atom, and radio plasma imaging techniques. During the first 1.5 years of the mission, IMAGE has obtained new results on the global dynamics of magnetospheric plasmas, including ring current injection and loss, substorm injections, plasmasphere loss and refilling, both subauroral and cusp-region proton auroras, the generation of kilometric continuum radiation, the field-aligned distribution of total plasma density and the global outflow of plasma from the ionosphere. In this paper, some of the new results from IMAGE are presented, and their importance for space weather is assessed.
机译:IMAGE卫星于2000年3月25日发射到椭圆北极轨道,在北极上方的最高点为8.2地球半径(地心)。有了这颗卫星,就可以使用紫外线,高能中性原子和无线电等离子体成像技术对磁层等离子体成像。在执行任务的前1.5年中,IMAGE在磁层等离子体的全球动力学方面取得了新的成果,包括环流注入和损失,亚暴注入,等离子层损失和充填,极光下和尖端区域质子极光,以及千米的产生连续辐射,总血浆密度的场定向分布以及血浆从电离层的整体流出。本文介绍了IMAGE的一些新结果,并评估了它们对空间天气的重要性。

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