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首页> 外文期刊>Astronomy and astrophysics >Flow pattern of accelerated cometary ions inside and outside the diamagnetic cavity of comet 67P/Churyumov-Gerasimenko
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Flow pattern of accelerated cometary ions inside and outside the diamagnetic cavity of comet 67P/Churyumov-Gerasimenko

机译:彗星67P / Churyumov-Gerasimenko的反磁性腔内外加速彗星离子的流动模式

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Analyzing data from the Ion Composition Analyzer on board the Rosetta spacecraft, we studied a flow pattern of accelerated cometary ions (40–80 eV) inside and outside the diamagnetic cavity of comet 67P/Churyumov-Gerasimenko (67P). We found that the accelerated ions are intermittently observed and are ten times more frequently observed outside the cavity than inside, and they mainly flow tailward with an aberration (~20–40°). We suggest that they are accelerated by the tailward polarization electric field upstream of the comet. Because their occurrence frequency becomes lowest near perihelion where the water production rate is highest at 67P, ion-neutral collisions and/or charge exchange may play a role in controlling the occurrence frequency. The aberration pattern is different inside and outside the cavity in the cometocentric solar equatorial (CSEQ) frame but it is consistent in the comet-Sun electric (CSE) frame; the latter is rotated from the CSEQ frame about the comet-Sun line so that the Z -axis is aligned with the local motional electric field. Because the flow pattern of the accelerated ions inside the cavity in the CSE frame is the same as outside, we suggest that the flow pattern inside is determined by the flow outside, depending on the local plasma and magnetic field. Near the CSE polar plane the aberration is in the opposite direction of the motional electric field, while it is in the anti-cometward direction near the CSE equator plane. The aberration in the anti-electric-field direction near the CSE polar plane suggests that the accelerated ions are mass-loaded by local cold cometary ions, just like the mass-loading of the solar wind by cold cometary ions. The cause of the anti-cometward aberration near the CSE equator plane is still unknown, but this may indicate that the tailward-flowing cometary ions are deflected across the upstream boundaries or by an outward-pointing ambipolar electric field.
机译:分析来自Rosetta航天器上离子组成分析仪的数据,我们研究了彗星67P / Churyumov-Gerasimenko(67P)的反磁腔内部和外部的加速彗星离子(40–80 eV)的流型。我们发现,间歇性观察到加速离子,并且在腔外观察到的频率比内部快十倍,并且它们主要以像差(〜20–40°)向后流动。我们建议通过彗星上游的向后极化电场来加速它们。由于它们的出现频率在近日点附近最高水生产率最高时在67P处变得最低,因此离子中性碰撞和/或电荷交换可能在控制出现频率中起作用。在偏心太阳赤道(CSEQ)框架中,腔内部和外部的像差模式不同,但在彗星-太阳电(CSE)框架中,像差模式是一致的;后者从CSEQ框架绕彗星-太阳线旋转,以使Z轴与局部运动电场对齐。由于CSE框架中腔体内加速离子的流动模式与外部相同,因此我们建议内部流动模式由外部流动确定,具体取决于局部等离子体和磁场。在CSE极平面附近,像差是在运动电场的相反方向上,而在CSE赤道平面附近是在反彗星方向上。 CSE极平面附近的反电场方向上的像差表明,加速离子由局部冷彗星离子负载,就像太阳风对冷彗星离子的负载一样。 CSE赤道面附近反彗形像差的原因仍然未知,但这可能表明向后流动的彗星离子在上游边界或向外指向的双极性电场的作用下发生偏转。

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