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Ulf Waves at the Proton Gyrofrequency Upstream of the Martian bow Shock, Based on Mars Global Surveyor's Measurements

机译:基于火星全球测量师的测量,火星弓激波质子陀螺频率上游的短波

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摘要

Small amplitude MHD waves at the proton gyrofrequency were detected and analyzed using the magnetic field measurements obtained by the Mars Global Surveyor, in the region upstream of the Martian bow shock, between days 87 and 255 of 1998. The origin of the observed ULF waves was found to be protons back-streaming from the bow shock and pick-up protons from the planetary hydrogen exosphere, interacting with the incoming solar wind. A small contribution of oxygen ions has also been detected. Furthermore, the spatial distribution of the waves was investigated, using the spacecraft's position during the time the data were obtained.
机译:在1998年第87到255天之间,利用火星全球测量师在火星弓激波上游区域中获得的磁场测量值,检测并分析了质子回旋频率下的小振幅MHD波。观察到的ULF波的起源是被发现是由弓形冲击产生的质子逆流而来,是由行星状氢外层大气吸收的质子,与入射的太阳风相互作用。还检测到少量的氧离子。此外,利用获得数据期间航天器的位置,研究了波的空间分布。

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  • 来源
    《Solar Physics》 |2002年第2期|409-419|共11页
  • 作者

    N. Sergis; X. Moussas;

  • 作者单位

    Department of Astrophysics Astronomy and Mechanics Faculty of Physics National University of Athens;

    Department of Astrophysics Astronomy and Mechanics Faculty of Physics National University of Athens;

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  • 正文语种 eng
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