Linking the Sun and the Heliosphere with the SPICE Imaging Spectrograph and the Solar Orbiter Missio

来源 :The Fourteenth International Solar Wind Conference (第十四届国际太阳 | 被引量 : 0次 | 上传用户：wangbenny918

【摘要】

：

【作者】

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Don Hassler Robert Wimmer-Schweingruber

【机构】

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Institut d'Astrophysique Spatiale Orsay,France C

【出处】

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The Fourteenth International Solar Wind Conference (第十四届国际太阳

【发表日期】

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2015年5期

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One of the primary objectives of the Solar Orbiter mission is to link remote sensing observations of the solar surface structures with in-situ observations of solar wind streams. The SPICE (Spectral Imaging of the Coronal Environment) instrument will characterize the plasma properties of regions near the Sun to directly compare with in-situ measurements from both Solar Orbiter & Solar Probe+. Specifically, SPICE will map outflow velocities of surface features to solar wind structures with similar composition (FIP, M/q) measured in-situ by the SWA/HIS instrument on Solar Orbiter.

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Linking the Sun and the Heliosphere with the SPICE Imaging Spectrograph and the Solar Orbiter Missio

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