星际尘埃和日球层科学之间的协同作用与星际探测器

V. Sterken, S. Hunziker, Kostas Dialynas, K. Herbst, Aigen Li, L. R. Baalmann, K. Scherer, P. Strub, R. Srama, M. Trieloff, M. Blanc, M. Sommer, M. Rowan‐Robinson, Harald Krüger, F. Effenberger, J. Richardson, D. Malaspina, H. Hsu, M. Horányi, Z. Sternovsky, Jonathan Slavin, J. Linsky, S. Redfield, A. Poppe, J. Szalay, Carey Lisse, E. Provornikova, M. Opher, A. Galli, F. Postberg, A. Czechowski, P. Frisch, William S Kurth, M. Shen, Thomas Chen, Zhengwei Hu, G. Stober, Ingrid Mann, N. Ligterink, Jesse A. Miller, B. Fields, J. Baggeley, P. Brandt
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引用次数: 2

摘要

我们讨论了日球层和尘埃科学之间的协同作用,开放的科学问题,技术努力和规划方面是重要的,在未来十年保持或发展。特别是,我们说明了我们如何利用太阳系中的星际尘埃作为(动态)日球层特性的示踪剂,并强调了宇宙尘埃在日球层和天体层物理中的作用这一相当未被探索但潜在重要的科学问题。我们表明,带有专用尘埃套件的星际探测器任务将为星际尘埃研究带来前所未有的进步,并且还可以通过测量尘埃为日球层科学做出贡献。特别是,如果我们与太阳系内的其他任务协同工作,从而利用太空中的多个有利位置来测量尘埃“滚动”进入日球层,这一点就可以做得很好。太阳系内和太阳系外的任务之间的这种协同作用对于解开空间和时间变化的尘埃流至关重要。最后,我们强调了相关的仪器及其适用性,有助于找到研究问题的答案。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Synergies between interstellar dust and heliospheric science with an Interstellar Probe
We discuss the synergies between heliospheric and dust science, the open science questions, the technological endeavors and programmatic aspects that are important to maintain or develop in the decade to come. In particular, we illustrate how we can use interstellar dust in the solar system as a tracer for the (dynamic) heliosphere properties, and emphasize the fairly unexplored, but potentially important science question of the role of cosmic dust in heliospheric and astrospheric physics. We show that an Interstellar Probe mission with a dedicated dust suite would bring unprecedented advances to interstellar dust research, and can also contribute – through measuring dust – to heliospheric science. This can, in particular, be done well if we work in synergy with other missions inside the solar system, thereby using multiple vantage points in space to measure the dust as it ‘rolls’ into the heliosphere. Such synergies between missions inside the solar system and far out are crucial for disentangling the spatially and temporally varying dust flow. Finally, we highlight the relevant instrumentation and its suitability for contributing to finding answers to the research questions.
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