Science. 1965 Sep 10;149(3689):1233-9. doi: 10.1126/science.149.3689.1233.
The Mariner IV spacecraft on 14-15 July 1965 passed within 9850 kilometers of Mars, carrying a solid-state charged-particle telescope which could detect electrons greater than 40 kiloelectron volts and protons greater than 1 million electron volts. The trajectory could have passed through a bow shock, a transition region, and a magnetospheric boundary where particles could be stably trapped for a wide range of Martian magnetic moments. No evidence of charged-particle radiation was found in any of these regions. In view of these results, an upper limit is established for the Martian magnetic moment provided it is assumed that the same physical processes leading to acceleration and trapping of electrons in Earth's magnetic field would be found in a Martian magnetic field. On this basis, the upper limit for the Martian magnetic moment is 0.1 percent that of Earth for a wide range of postulated orientations with respect to the rotational axis of Mars. The implications of these results for the physical and biological environment of Mars are briefly discussed.
水手四号飞船于 1965 年 7 月 14 日至 15 日飞掠火星,携带一台固态带电粒子望远镜,可探测大于 40 千电子伏特的电子和大于 100 万电子伏特的质子。该轨迹可能穿过弓形激波、过渡区和磁层边界,在这些区域内,粒子可以在很宽的火星磁矩范围内稳定捕获。在这些区域中都没有发现带电粒子辐射的证据。鉴于这些结果,如果假设导致地球磁场中电子加速和捕获的相同物理过程也会在火星磁场中找到,那么就为火星磁矩建立了一个上限。在此基础上,对于火星相对于火星自转轴的各种假定取向,火星磁矩的上限为地球的 0.1%。简要讨论了这些结果对火星物理和生物环境的影响。