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ROY—A multiscale magnetospheric mission

机译:ROY-多尺度磁层探测任务

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摘要

The scientific rationale of the ROY multi-satellite mission addresses multiscale investigations of plasma processes in the key magnetospheric regions with strong plasma gradients, turbulence and magnetic field annihilation in the range from electron inertial length to MHD scales. The main scientific aims of ROY mission include explorations of: (a) turbulence on a non-uniform background as a keystone for transport processes; (b) structures and jets in plasma flows associated with anomalously large concentration of kinetic energy; their impact on the energy balance and boundary formation; (c) transport barriers: plasma separation and mixing, Alfvenic collapse of magnetic field lines and turbulent dissipation of kinetic energy; (d) self-organized versus forced reconnection of magnetic field lines; (e) collisionless shocks, plasma discontinuities and associated particle acceleration processes. In the case of autonomous operation, 4 mobile spacecrafts of about 200 kg mass with 60 kg payload equipped with electro-reactive plasma engines will provide 3D measurements at the scales of 100-10000 km and simultaneous ID measurements at the scales 10-1000 km. The latter smaller scales will be scanned with the use of radio-tomography (phase-shift density measurements within the cone composed of 1 emitting and 3 receiving spacecrafts). We also discuss different opportunities for extra measurement points inside the ROY mission for simultaneous measurements at up to 3 scales for the common international fleet. Combined influence of intermittent turbulence and reconnection on the geomagnetic tail and on the nonlinear dynamics of boundary layers will be explored in situ with fast techniques including particle devices under development, providing plasma moments down to 30 ms resolution. We propose different options for joint measurements in conjunction with the SCOPE and other missions: simultaneous sampling of low- and high-latitudes magnetopause, bow shock and geomagnetic tail at the same local time;
机译:ROY多卫星飞行任务的科学原理致力于对关键磁层中的等离子体过程进行多尺度研究,这些过程具有很强的等离子体梯度,湍流和磁场an灭,范围从电子惯性长度到MHD尺度。 ROY任务的主要科学目的包括:(a)在非均匀背景下进行湍流作为运输过程的基石; (b)与异常大的动能集中有关的血浆流中的结构和射流;它们对能量平衡和边界形成的影响; (c)运输障碍:血浆分离和混合,磁场线的低空塌陷和动能的湍流耗散; (d)自组织与强制重新连接磁场线; (e)无碰撞冲击,等离子体间断和相关的粒子加速过程。在自主运行的情况下,配备电反应等离子体引擎的4台质量约为200千克,有效载荷为60千克的移动航天器将提供100-10000公里范围内的3D测量和10-1000公里范围内的同时ID测量。后面的较小尺度将使用放射断层扫描(由1个发射航天器和3个接收航天器组成的锥体内的相移密度测量)进行扫描。我们还将讨论ROY任务内部额外的测量点的不同机会,以便为国际通用机队同时进行3级的同时测量。间歇湍流和重新连接对地磁尾部和边界层非线性动力学的综合影响将通过包括粒子设备在内的快速技术在现场进行探索,该技术可提供低至30 ms的等离子矩。我们建议与SCOPE和其他任务一起进行联合测量的不同选择:在同一本地时间同时采样低纬和高纬磁层顶,弓形冲击和地磁尾巴;

著录项

  • 来源
    《Planetary and space science 》 |2011年第7期| p.606-617| 共12页
  • 作者单位

    Space Research Institute, Russian Academy of Sciences, Profsoyuznaya 84/32, Moscow II7977, Russian Federation;

    Space Research Institute, Russian Academy of Sciences, Profsoyuznaya 84/32, Moscow II7977, Russian Federation;

    Interplanetary Space Physics Institute, INAF, Rome, Italy;

    Space Research Institute, Russian Academy of Sciences, Profsoyuznaya 84/32, Moscow II7977, Russian Federation,RRC Kurchatov Institute, 123182, Kurchatov Sq. I, Moscow, Russia;

    Max-Planck Institute for Solar System Research, Katlenburg-Lindau, Germany;

    Space Research Center and Collegium Varsoviense, Warsaw, Poland;

    University of Sheffield, UK;

    Space Research Institute, Russian Academy of Sciences, Profsoyuznaya 84/32, Moscow II7977, Russian Federation;

    Lviv Centre of Institute for Space Research, Ukraine;

    Kyiv University, Ukraine;

    Lavochkin Assosiation, Russia;

    Space Research Institute, Russian Academy of Sciences, Profsoyuznaya 84/32, Moscow II7977, Russian Federation;

    Space Research Institute, Russian Academy of Sciences, Profsoyuznaya 84/32, Moscow II7977, Russian Federation;

    Space Research Institute, Russian Academy of Sciences, Profsoyuznaya 84/32, Moscow II7977, Russian Federation,Space Research Institute, Russian Academy of Sciences, Profsoyuznaya 84/32, Moscow II7977, Russian Federation;

    Space Research Institute, Russian Academy of Sciences, Profsoyuznaya 84/32, Moscow II7977, Russian Federation;

    Space Research Institute, Russian Academy of Sciences, Profsoyuznaya 84/32, Moscow II7977, Russian Federation;

    Space Research Institute, Russian Academy of Sciences, Profsoyuznaya 84/32, Moscow II7977, Russian Federation;

    Space Research Institute, Russian Academy of Sciences, Profsoyuznaya 84/32, Moscow II7977, Russian Federation,;

    Space Research Institute, Russian Academy of Sciences, Profsoyuznaya 84/32, Moscow II7977, Russian Federation;

    Lviv Centre of Institute for Space Research, Ukraine;

    Space Research Institute, Russian Academy of Sciences, Profsoyuznaya 84/32, Moscow II7977, Russian Federation;

    Space Research Institute, Russian Academy of Sciences, Profsoyuznaya 84/32, Moscow II7977, Russian Federation;

    Space Research Institute, Russian Academy of Sciences, Profsoyuznaya 84/32, Moscow II7977, Russian Federation;

    Space Research Institute, Russian Academy of Sciences, Profsoyuznaya 84/32, Moscow II7977, Russian Federation;

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  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

    multiscale observations; turbulence; plasma transport;

    机译:多尺度观测;湍流;等离子体迁移;

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