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Imaging the Interaction of the Heliosphere with the Interstellar Medium from Saturn with Cassini

机译:用卡西尼号成像土星与星际介质相互作用的日光层

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摘要

We report an all-sky image of energetic neutral atoms (ENAs) >6 kilo-electron volts produced by energetic protons occupying the region (heliosheath) between the boundary of the extended solar atmosphere and the local interstellar medium (LISM). The map obtained by the Ion and Neutral Camera (INCA) onboard Cassini reveals a broad belt of energetic protons whose nonthermal pressure is comparable to that of the local interstellar magnetic field. The belt, centered at ~260° ecliptic longitude extending from north to south and looping back through ~80°, appears to be ordered by the local interstellar magnetic field. The shape revealed by the ENA image does not conform to current models, wherein the heliosphere resembles a cometlike figure aligned in the direction of Sun's travel through the LISM.
机译:我们报告了高能中性原子(ENA)> 6千电子伏特的全天候图像,这些能量由高能质子占据扩展的太阳大气边界和当地星际介质(LISM)之间的区域(heliosheath)产生。卡西尼号上的离子和中性照相机(INCA)获得的地图显示了高能质子带,其非热压力可与局部星际磁场相媲美。该带的中心是从北向南延伸至约260°的黄道经,并向后绕回约80°,似乎是由局部星际磁场所命令的。 ENA图像显示的形状与当前模型不符,其中的日光层类似于彗星状的图形,其沿太阳穿过LISM的行进方向对齐。

著录项

  • 来源
    《Science》 |2009年第5955期|971-973|共3页
  • 作者单位

    Applied Physics Laboratory, Johns Hopkins University, Laurel, MD 20723, USA Office for Space Research and Technology, Academy of Athens, 106 79 Athens, Greece;

    Applied Physics Laboratory, Johns Hopkins University, Laurel, MD 20723, USA;

    Applied Physics Laboratory, Johns Hopkins University, Laurel, MD 20723, USA;

    Department of Physics, University of Arizona, Tucson, AZ 85721, USA;

    Southwest Research Institute, San Antonio, TX 78228, USA University of Texas, San Antonio, TX 78249, USA;

  • 收录信息 美国《科学引文索引》(SCI);美国《工程索引》(EI);美国《生物学医学文摘》(MEDLINE);美国《化学文摘》(CA);
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
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  • 入库时间 2022-08-18 02:55:15

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