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首页> 外文期刊>Space Science Reviews >First Results from ARTEMIS, a New Two-Spacecraft Lunar Mission: Counter-Streaming Plasma Populations in the Lunar Wake
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First Results from ARTEMIS, a New Two-Spacecraft Lunar Mission: Counter-Streaming Plasma Populations in the Lunar Wake

机译:ARTEMIS的初步结果,这是一种新型两航天器的月球任务:月球尾流中的逆流等离子体种群

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摘要

We present observations from the first passage through the lunar plasma wake by one of two spacecraft comprising ARTEMIS (Acceleration, Reconnection, Turbulence, and Electrodynamics of the Moon’s Interaction with the Sun), a new lunar mission that re-tasks two of five probes from the THEMIS magnetospheric mission. On Feb 13, 2010, ARTEMIS probe P1 passed through the wake at ∼3.5 lunar radii downstream from the Moon, in a region between those explored by Wind and the Lunar Prospector, Kaguya, Chandrayaan, and Chang’E missions. ARTEMIS observed interpenetrating proton, alpha particle, and electron populations refilling the wake along magnetic field lines from both flanks. The characteristics of these distributions match expectations from self-similar models of plasma expansion into vacuum, with an asymmetric character likely driven by a combination of a tilted interplanetary magnetic field and an anisotropic incident solar wind electron population. On this flyby, ARTEMIS provided unprecedented measurements of the interpenetrating beams of both electrons and ions naturally produced by the filtration and acceleration effects of electric fields set up during the refilling process. ARTEMIS also measured electrostatic oscillations closely correlated with counter-streaming electron beams in the wake, as previously hypothesized but never before directly measured. These observations demonstrate the capability of the comprehensively instrumented ARTEMIS spacecraft and the potential for new lunar science from this unique two spacecraft constellation.
机译:我们将介绍包括ARTEMIS(加速,重新连接,湍流和月球与太阳的相互作用的电动力学)在内的两个航天器中的一个通过月球等离子尾迹的第一次观测,这是一项新的登月任务,需要重新分配来自五个月球的五个探测器中的两个THEMIS磁层探测任务。 2010年2月13日,ARTEMIS探测器P1在月球下游〜月球半径约3.5处通过了尾迹,该区域位于Wind和探月者,Kaguya,Chandrayaan和Chang'E任务所探测的区域之间。 ARTEMIS观察到互穿的质子,α粒子和电子种群沿着两个侧面的磁力线重新填充了尾流。这些分布的特征符合等离子体膨胀到真空的自相似模型的期望,其不对称特征很可能是由倾斜的行星际磁场和各向异性入射太阳风电子种群共同驱动的。在这次飞越中,ARTEMIS提供了空前的电子和离子互穿射束测量结果,这些电子和离子的互穿射束是通过在填充过程中建立的电场的过滤和加速效应自然产生的。 ARTEMIS还测量了与尾流中逆流电子束紧密相关的静电振荡,这是以前假设的,但从未直接测量过。这些观察结果证明了综合装备的ARTEMIS航天器的能力以及这一独特的两个航天器星座对新月球科学的潜力。

著录项

  • 来源
    《Space Science Reviews》 |2011年第4期|p.93-107|共15页
  • 作者单位

    Space Sciences Laboratory, University of California, Berkeley, CA, 94720, USA;

    Institute of Geophysics and Planetary Physics, UCLA, Los Angeles, CA, 90095, USA;

    NASA Goddard Space Flight Center, Greenbelt, MD, 20771, USA;

    Institute of Geophysics and Planetary Physics, UCLA, Los Angeles, CA, 90095, USA;

    Institute of Geophysics and Planetary Physics, UCLA, Los Angeles, CA, 90095, USA;

    Space Sciences Laboratory, University of California, Berkeley, CA, 94720, USA;

    NASA’s Lunar Science Institute, NASA Ames Research Center, Moffett Field, CA, 94035, USA;

    Space Sciences Laboratory, University of California, Berkeley, CA, 94720, USA;

    Space Sciences Laboratory, University of California, Berkeley, CA, 94720, USA;

    Space Sciences Laboratory, University of California, Berkeley, CA, 94720, USA;

    Laboratory for Atmospheric and Space Physics, University of Colorado, Boulder, CO, 80303, USA;

    Institut für Geo;

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

    Moon; Lunar wake; Counter-streaming distributions;

    机译:月球;月球唤醒;逆流分布;

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