太阳风对火星感应磁场的影响:MAVEN观测

IF 4 3区地球科学 Q2 ENGINEERING, ELECTRICAL & ELECTRONIC

IEEE Geoscience and Remote Sensing Letters Pub Date : 2023-01-01 DOI:10.23977/geors.2023.060102

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引用次数: 0

摘要

自古以来，人类对外太空的探索从未停止过。火星作为八大行星之一，自然成为我们的重点研究对象之一。本文主要研究火星空间环境的特点及其影响因素。利用MAVEN多年的观测数据，发现在高太阳风压条件下，感应磁场强度增强，并利用基于MHD方程的分析方法对这一现象进行了解释。

本文章由计算机程序翻译，如有差异，请以英文原文为准。

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Solar Wind Influences on the Induced Magnetic Field of Mars: MAVEN Observations

Since ancient times, human beings have never stopped exploring outer space. As one of the eight planets, Mars has naturally become one of our key research objects. This paper mainly studies the characteristics and influencing factors of the Martian space environment. By using MAVEN's observation data for many years, we found that the intensity of the induced magnetic field is enhanced under the condition of high solar wind pressure, and this phenomenon is explained by the analysis method based on MHD equation.

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来源期刊

IEEE Geoscience and Remote Sensing Letters 工程技术-地球化学与地球物理

CiteScore

7.60

自引率

12.50%

发文量

1113

审稿时长

3.4 months

期刊介绍： IEEE Geoscience and Remote Sensing Letters (GRSL) is a monthly publication for short papers (maximum length 5 pages) addressing new ideas and formative concepts in remote sensing as well as important new and timely results and concepts. Papers should relate to the theory, concepts and techniques of science and engineering as applied to sensing the earth, oceans, atmosphere, and space, and the processing, interpretation, and dissemination of this information. The technical content of papers must be both new and significant. Experimental data must be complete and include sufficient description of experimental apparatus, methods, and relevant experimental conditions. GRSL encourages the incorporation of "extended objects" or "multimedia" such as animations to enhance the shorter papers.