PLASMA NEAR THE HELIOSHEATH: OBSERVATIONS AND MODELING
PLASMA NEAR THE HELIOSHEATH: OBSERVATIONS AND MODELING
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DOI：
10.1088/2041-8205/728/1/l21
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发表时间：
2011-02-10
影响因子：
7.9
通讯作者：
Richardson, John D.
中科院分区：
文献类型：
--
作者：
Borovikov, Sergey N.;Pogorelov, Nikolai V.;Richardson, John D.
可靠的数值模型能够提供有关太阳风与当地星际介质相互作用的重要预测信息。我们的三维模拟结果与 2007 年至 2010 年 Voyager 观测结果非常吻合。我们分析了 Voyager 交叉点的终止激波特性，并将其与观测数据并列。检查内日鞘中的日光层电流片结构。
Sound numerical modeling is capable of providing important predictive information about the solar wind interaction with the local interstellar medium. The results of our three-dimensional simulation show a good agreement with Voyager observations from 2007 to 2010. We analyze the termination shock properties at the Voyager crossing points and juxtapose them with the observed data. The heliospheric current sheet structure in the inner heliosheath is examined.