First observations of energetic particles near comet Halley
First observations of energetic particles near comet Halley
复制标题
哈雷彗星附近首次观测到高能粒子
DOI：
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发表时间：
1986
期刊：
影响因子：
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通讯作者：
A. Zarandy
中科院分区：
文献类型：
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作者：
A. Somogyi;K. Gringauz;K. Szego;L. Szabó;G. Kozma;A. Remizov;J. Ero;I. N. Klimenko;I. Szücs;M. Verigin;J. Windberg;T. Cravens;A. Dyachkov;G. Erdős;M. Faragó;T. Gombosi;K. Kecskeméty;E. Keppler;T. Kovács;A. Kondor;Y. Logachev;L. Lohonyai;R. Marsden;R. Redl;A. Richter;V. Stolpovskii;J. Szabó;I. Szentpétery;A. Szepesvary;M. Tátrallyay;A. Varga;G. A. Vladimirova;K. Wenzel;A. Zarandy
Vega 1号航天器上的TÜNDE-M高能粒子仪器在哈雷彗星附近探测到高能（≥40 keV）离子的强通量，从距离最近点107公里处开始。已经确定了三个不同离子特性的区域。一个几百万公里的外部区域包含太阳风中的拾取离子。第二个区域位于弓形激波内部（范围为数十万公里），包含最强的通量，而最里面的区域（数万公里）的特征是强度较低，在最近的地方（距离核约18，900公里）有尖锐的尖峰。
The TÜNDE-M energetic particle instrument aboard the Vega 1 spacecraft detected intense fluxes of energetic (≥40 keV) ions in the vicinity of comet Halley, starting at a distance of 107 km from closest approach. Three regions of differing ion characteristics have been identified. An outer region, several million kilometers in extent, contains pick-up ions in the solar wind. A second region, inside the bow shock (several hundred thousand kilometres in extent), contains the most intense fluxes, whereas the innermost region (several tens of thousands of kilometres) is characterized by lower intensities and sharp spikes near closest approach (∼8,900 km from the nucleus).