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土星的磁层、光环和内卫星。

Saturn's Magnetosphere, Rings, and Inner Satellites.

作者信息

VAN Allen J A, Thomsen M F, Randall B A, Rairden R L, Grosskreutz C L

出版信息

Science. 1980 Jan 25;207(4429):415-21. doi: 10.1126/science.207.4429.415.

Abstract

Our 31 August to 5 September 1979 observations together with those of the other Pioneer 11 investigators provide the first credible discovery of the magnetosphere of Saturn and many detailed characteristics thereof. In physical dimensions and energetic charged particle population, Saturn's magnetosphere is intermediate between those of Earth and Jupiter. In terms of planetary radii, the scale of Saturn's magnetosphere more nearly resembles that of Earth and there is much less inflation by entrapped plasma than in the case at Jupiter. The orbit of Titan lies in the outer fringes of the magnetosphere. Particle angular distributions on the inbound leg of the trajectory (sunward side) have a complex pattern but are everywhere consistent with a dipolar magnetic field approximately perpendicular to the planet's equator. On the outbound leg (dawnside) there are marked departures from this situation outside of 7 Saturn radii (Rs), suggesting an equatorial current sheet having both longitudinal and radial components. The particulate rings and inner satellites have a profound effect on the distribution of energetic particles. We find (i) clear absorption signatures of Dione and Mimas; (ii) a broad absorption region encompassing the orbital radii of Tethys and Enceladus but probably attributable, at least in part, to plasma physical effects; (iii) no evidence for Janus (1966 S 1) (S 10) at or near 2.66 Rs; (iv) a satellite of diameter greater, similar 170 kilometers at 2.534 R(s) (1979 S 2), probably the same object as that detected optically by Pioneer 11 (1979 S 1) and previously by groundbased telescopes (1966 S 2) (S 11); (v) a satellite of comparable diameter at 2.343 Rs (1979 S 5); (vi) confirmation of the F ring between 2.336 and 2.371 Rs; (vii) confirmation of the Pioneer division between 2.292 and 2.336 Rs; (viii) a suspected satellite at 2.82 Rs (1979 S 3); (ix) no clear evidence for the E ring though its influence may be obscured by stronger effects; and (x) the outer radius of the A ring at 2.292 Rs. Inside of 2.292 Rs there is a virtually total absence of magnetospheric particles and a marked reduction in cosmic-ray intensity. All distances are in units of the adopted equatorial radius of Saturn, 60,000 kilometers.

摘要

我们在1979年8月31日至9月5日期间的观测结果,与其他“先驱者11号”研究人员的观测结果一起,首次可靠地发现了土星的磁层及其许多详细特征。在物理尺寸和高能带电粒子数量方面,土星的磁层介于地球和木星的磁层之间。以行星半径衡量,土星磁层的尺度更接近地球,与木星相比,被捕获等离子体导致的膨胀要小得多。土卫六的轨道位于磁层的外缘。在轨迹的入轨段(朝向太阳一侧),粒子的角分布呈现出复杂的模式,但在各处都与大致垂直于行星赤道的偶极磁场一致。在出轨段(黎明一侧),在7个土星半径(Rs)之外明显偏离这种情况,这表明存在一个具有纵向和径向分量的赤道电流片。颗粒环和内侧卫星对高能粒子的分布有深远影响。我们发现:(i)土卫二和土卫一有明显的吸收特征;(ii)一个宽广的吸收区域,涵盖了土卫三与土卫二的轨道半径,但至少部分可能归因于等离子体物理效应;(iii)在2.66 Rs处或其附近没有发现雅努斯(1966 S 1)(S 10)的证据;(iv)在2.534 R(s)(1979 S 2)处有一颗直径更大、约170千米的卫星,可能与“先驱者11号”光学探测到的(1979 S 1)以及之前地面望远镜探测到的(1966 S 2)(S 11)是同一物体;(v)在2.343 Rs处有一颗直径相当的卫星(1979 S 5);(vi)证实了在2.336至2.371 Rs之间存在F环;(vii)证实了在2.292至2.336 Rs之间存在“先驱者环缝”;(viii)在2.82 Rs处(1979 S 3)有一颗疑似卫星;(ix)没有明确证据表明存在E环,尽管其影响可能被更强的效应掩盖;(x)A环的外半径在2.292 Rs处。在2.292 Rs以内,几乎完全没有磁层粒子,宇宙射线强度也显著降低。所有距离均以土星采用的赤道半径60,000千米为单位。

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