Gombosi Tamas I, Hansen Kenneth C
Center for Space Environment Modeling, Department of Atmospheric, Oceanic and Space Sciences, University of Michigan, Ann Arbor, MI 48109, USA.
Science. 2005 Feb 25;307(5713):1224-6. doi: 10.1126/science.1108226.
Since the Cassini spacecraft reached Saturn's orbit in 2004, its instruments have been sending back a wealth of data on the planet's magnetosphere (the region dominated by the magnetic field of the planet). In this Viewpoint, we discuss some of these results, which are reported in a collection of reports in this issue. The magnetosphere is shown to be highly variable and influenced by the planet's rotation, sources of plasma within the planetary system, and the solar wind. New insights are also gained into the chemical composition of the magnetosphere, with surprising results. These early results from Cassini's first orbit around Saturn bode well for the future as the spacecraft continues to orbit the planet.
自卡西尼号航天器于2004年进入土星轨道以来,其仪器一直在传回有关该行星磁层(由行星磁场主导的区域)的大量数据。在这篇观点文章中,我们讨论其中一些结果,这些结果在本期的一系列报告中有所报道。磁层显示出高度可变,并受到行星自转、行星系统内等离子体源以及太阳风的影响。对磁层的化学成分也有了新的认识,结果令人惊讶。卡西尼号首次环绕土星轨道运行的这些早期结果,对未来航天器继续环绕该行星运行而言是个好兆头。