Science. 1986 Apr 18;232(4748):377-81. doi: 10.1126/science.232.4748.377.
The plasma wave instrument on the International Cometary Explorer (ICE) detected bursts of strong ion acoustic waves almost continuously when the spacecraft was within 2 million kilometers of the nucleus of comet Giacobini-Zinner. Electromagnetic whistlers and low-level electron plasma oscillations were also observed in this vast region that appears to be associated with heavy ion pickup. As ICE came closer to the anticipated location of the bow shock, the electromagnetic and electrostatic wave levels increased significantly, but even in the midst of this turbulence the wave instrument detected structures with familiar bow shock characteristics that were well correlated with observations of localized electron heating phenomena. Just beyond the visible coma, broadband waves with amplitudes as high as any ever detected by the ICE plasma wave instrument were recorded. These waves may account for the significant electron heating observed in this region by the ICE plasma probe, and these observations of strong wave-particle interactions may provide answers to longstanding questions concerning ionization processes in the vicinity of the coma. Near closest approach, the plasma wave instrument detected broadband electrostatic noise and a changing pattern of weak electron plasma oscillations that yielded a density profile for the outer layers of the cold plasma tail. Near the tail axis the plasma wave instrument also detected a nonuniform flux of dust impacts, and a preliminary profile of the Giacobini-Zinner dust distribution for micrometer-sized particles is presented.
当星际彗星探测器(ICE)的航天器距离 Giacobini-Zinner 彗星核 200 万千米以内时,其上的等离子体波仪器几乎连续探测到强烈的离子声波爆发。在这个似乎与重离子俘获有关的广阔区域中,还观测到了电磁哨声和低水平的电子等离子体振荡。当 ICE 更接近预期的弓形激波位置时,电磁波和静电波的强度显著增加,但即使在这种湍流中,波仪器仍检测到具有熟悉的弓形激波特征的结构,这些结构与局部电子加热现象的观测结果密切相关。在可见彗发之外,记录到了幅度高达 ICE 等离子体波仪器以往任何时候都检测到的宽带波。这些波可能解释了 ICE 等离子体探针在该区域观察到的显著电子加热现象,这些强烈的波粒相互作用的观测结果可能为长期以来关于彗发附近的电离过程的问题提供答案。在最接近的位置附近,等离子体波仪器检测到宽带静电噪声和弱电子等离子体振荡的变化模式,为冷等离子体尾部的外层提供了密度分布。在尾部轴附近,等离子体波仪器还探测到尘埃撞击的非均匀通量,并给出了 Giacobini-Zinner 尘埃分布的初步轮廓,用于测量微米大小的颗粒。