Gurnett D A, Kurth W S, Scarf F L, Poynter R L
Science. 1986 Jul 4;233(4759):106-9. doi: 10.1126/science.233.4759.106.
Radio emissions from Uranus were detected by the Voyager 2 plasma wave instrument about 5 days before closest approach at frequencies of 31.1 and 56.2 kilohertz. About 10 hours before closest approach the bow shock was identified by an abrupt broadband burst of electrostatic turbulence at a radial distance of 23.5 Uranus radii. Once Voyager was inside the magnetosphere, strong whistler-mode hiss and chorus emissions were observed at radial distances less than about 8 Uranus radii, in the same region where the energetic particle instruments detected intense fluxes of energetic electrons. Various other plasma waves were also observed in this same region. At the ring plane crossing, the plasma wave instrument detected a large number of impulsive events that are interpreted as impacts of micrometer-sized dust particles on the spacecraft. The maximum impact rate was about 30 to 50 impacts per second, and the north-south thickness of the impact region was about 4000 kilometers.
“旅行者2号”的等离子体波仪器在最接近天王星前约5天,于31.1千赫兹和56.2千赫兹的频率探测到了来自天王星的无线电辐射。在最接近天王星前约10小时,在距天王星半径23.5倍的径向距离处,通过静电湍流的突然宽带爆发确定了弓形激波。一旦“旅行者号”进入磁层,在径向距离小于约8个天王星半径的区域内,观测到了强烈的啸声模嘶声和合声辐射,该区域也是高能粒子仪器探测到高能电子强通量的区域。在同一区域还观测到了各种其他等离子体波。在穿越环平面时,等离子体波仪器探测到大量脉冲事件,这些事件被解释为微米级尘埃颗粒对航天器的撞击。最大撞击率约为每秒30至50次撞击,撞击区域的南北厚度约为4000公里。