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    題名: Two-spacecraft observations of an interplanetary slow shock
    作者: Lin,CC;Feng,HQ;Wu,DJ;Chao,JK;Lee,LC;Lyu,LH
    貢獻者: 太空科學研究所
    關鍵詞: EARTHS DISTANT MAGNETOTAIL;PLASMA SHEET BOUNDARY;LARGE MAGNETIC SHEAR;MODE SHOCKS;GEOMAGNETIC TAIL;SOLAR-WIND;AMPTE/IRM OBSERVATIONS;MAGNETOPAUSE;RECONNECTION;REVERSE
    日期: 2009
    上傳時間: 2010-06-29 18:38:19 (UTC+8)
    出版者: 中央大學
    摘要: Slow-mode shocks in space have been identified via one spacecraft observation by many authors since 1970. However, Feng et al. suggested that the analysis using single-spacecraft observation based only on the Rankine-Hugoniot relations could misinterpret a tangential discontinuity as a slow shock. In this paper, we identify a slow-mode shock using a model fitting based on both the Rankine-Hugoniot relations and intraspacecraft timing. As a result, we found a slow-shock solution that, including the local parameters and propagation time, agrees well with the observations. The slow shock may be associated with an asymmetric reconnection exhaust at a heliospheric current sheet.
    關聯: JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS
    顯示於類別:[太空科學研究所 ] 期刊論文

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