...
首页> 外文期刊>Planetary and space science >Ulysses jovian latitude scan of high-velocity dust streams originating from the jovian system
【24h】

Ulysses jovian latitude scan of high-velocity dust streams originating from the jovian system

机译:尤利西斯·朱维安纬度扫描源自木星系统的高速尘埃流

获取原文
获取原文并翻译 | 示例

摘要

In February 2004 the Ulysses spacecraft had its second flyby at Jupiter at 0.8 AU distance from the planet. Twenty-eight dust streams emanating from the jovian system were measured between November 2002 and August 2005 while the spacecraft was within 4 AU of the planet, scanning jovigraphic latitudes from +75° to -25°. The highest dust fluxes were measured in mid 2004 at the passage of the equatorial plane of the planet when more than 2000 impacts per day were measured. The grain impact direction is correlated with the polarity and strength of the interplanetary magnetic field. At high jovigraphic latitudes, the impact rates show a periodicity of 26 days, closely matching the solar rotation period, while at the jovian equator the streams fluctuate with twice this period. The 14-day subharmonic streams alternate in arrival direction and are correlated with the pointing of the interplanetary magnetic field. Dust fluxes measured above and below the equatorial plane roughly decrease with the inverse square of the distance from the planet while along the equatorial plane dust fluxes are enhanced by up to 2 orders of magnitude.
机译:2004年2月,尤利西斯号飞船在木星上进行了第二次飞越,距离木星0.8 AU。在2002年11月至2005年8月期间,当航天器位于行星4 AU以内时,测量了来自木星系统的28条尘埃流,扫描了从+ 75°到-25°的纬向纬度。在2004年年中,当每天测得2000多次撞击时,尘埃通量最高。晶粒冲击方向与行星际磁场的极性和强度相关。在较高的纬度纬度下,撞击率的周期为26天,与太阳的旋转周期非常匹配,而在赤道赤道,水流的波动是该周期的两倍。 14天的次谐波流在到达方向上交替变化,并与行星际磁场的指向相关。在赤道平面上方和下方测得的尘埃通量与距行星距离的平方成反比,而沿赤道平面的尘埃通量最多可增加2个数量级。

著录项

相似文献

  • 外文文献
  • 中文文献
  • 专利
获取原文

客服邮箱:kefu@zhangqiaokeyan.com

京公网安备:11010802029741号 ICP备案号:京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有
  • 客服微信

  • 服务号