Stone E C, Cummings A C, McDonald F B, Heikkila B C, Lal N, Webber W R
California Institute of Technology, Pasadena, CA 91125, USA.
Science. 2005 Sep 23;309(5743):2017-20. doi: 10.1126/science.1117684.
Voyager 1 crossed the termination shock of the supersonic flow of the solar wind on 16 December 2004 at a distance of 94.01 astronomical units from the Sun, becoming the first spacecraft to begin exploring the heliosheath, the outermost layer of the heliosphere. The shock is a steady source of low-energy protons with an energy spectrum approximately E(-1.41 +/- 0.15) from 0.5 to approximately 3.5 megaelectron volts, consistent with a weak termination shock having a solar wind velocity jump ratio r=2.6(-0.2)(+0.4). However, in contradiction to many predictions, the intensity of anomalous cosmic ray (ACR) helium did not peak at the shock, indicating that the ACR source is not in the shock region local to Voyager 1. The intensities of approximately 10-megaelectron volt electrons, ACRs, and galactic cosmic rays have steadily increased since late 2004 as the effects of solar modulation have decreased.
“旅行者1号”于2004年12月16日在距离太阳94.01天文单位处穿过了太阳风超音速流的终端激波,成为首个开始探索日鞘层(即太阳圈最外层)的航天器。该激波是低能质子的稳定来源,其能谱在0.5至约3.5兆电子伏特范围内近似为E(-1.41 +/- 0.15),这与太阳风速度跳跃比r = 2.6(-0.2)(+0.4)的弱终端激波相符。然而,与许多预测相反,反常宇宙射线(ACR)氦的强度并未在激波处达到峰值,这表明ACR源并不在“旅行者1号”所在的激波区域内。自2004年末以来,随着太阳调制效应减弱,约10兆电子伏特电子、ACR和银河宇宙射线的强度稳步上升。