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“嫦娥一號”衛(wèi)星觀測近月太陽風離子特征(英文)

Features of solar wind ions near the Moon observed by spacecraft Chang'E-1

  • 摘要: “嫦娥一號”衛(wèi)星的太陽風離子探測器(SWIDs)的科學目標是研究太陽風與月球的相互作用以及相應的近月空間等離子體環(huán)境。文章利用“嫦娥一號”衛(wèi)星SWIDs探測器在2007年12月30日的觀測數(shù)據(jù)對近月太陽風等離子體環(huán)境,,包括向陽側太陽風離子,、"拾起"離子以及在月球尾跡邊界處的太陽風離子的特征進行分析,得到以下主要觀測結果:1)在慢速太陽風中觀測到雙峰結構,,分別為太陽風中的氫離子和二價氦離子,;2)在行星際磁場具有明顯昏向(+By)分量期間,在月球向陽側持續(xù)觀測到有月表散射或反射后被拾起的太陽風離子,;3)與入射的太陽風離子不同,,這些拾起的太陽風離子具有明顯的角度分布特征;4)在行星際磁場昏向(晨向)期間,,太陽風中的氫離子在月球尾跡北半球的邊界處呈現(xiàn)減速(加速)特征并進入尾跡,;而并未發(fā)現(xiàn)氦離子進入尾跡的特征?!版隙鹨惶枴毙l(wèi)星的這些觀測數(shù)據(jù)對于認識近月空間等離子體環(huán)境有著重要的意義,。

     

    Abstract: The solar wind ions detectors onboard the spacecraft Chang'E-1(CE-1)have made a great contribution in advancing the understanding ofthesolar wind-Moon interaction and the induced near-Moon plasma environment. Several features ofsolar wind ions near the Moon were observed by tlle CE-1 on Dec 30, 2007:1)both protons(H+)and alpha particles(He2+)were identified in the slow solar wind; 2)the accelerated solar wind pickup ions were repeatedly observed on the lunar dayside under the nterplanetary magnetic field(IMF)By dominant conditions; 3)the accelerated pickup ions show being angle-dependent clearly and location-dependent sensitively; 4)under the IMF positive(negative)By conditions, the decelerated (accelerated) solar wind H+ intruded deep into the wake from the wake boundary in the northern hemisphere. while the He2+population intruded less deep than H+. The revelation ofthese features may be of great help to understand the near-Moon plasma environment.

     

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