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月震特征及与地震的对比

赵娜

赵娜. 月震特征及与地震的对比[J]. 空间科学学报, 2020, 40(2): 264-272. doi: 10.11728/cjss2020.02.264
引用本文: 赵娜. 月震特征及与地震的对比[J]. 空间科学学报, 2020, 40(2): 264-272. doi: 10.11728/cjss2020.02.264
ZHAO Na. Characteristics of Moonquake and Its Comparison with Earthquakeormalsize[J]. Chinese Journal of Space Science, 2020, 40(2): 264-272. doi: 10.11728/cjss2020.02.264
Citation: ZHAO Na. Characteristics of Moonquake and Its Comparison with Earthquakeormalsize[J]. Chinese Journal of Space Science, 2020, 40(2): 264-272. doi: 10.11728/cjss2020.02.264

月震特征及与地震的对比

doi: 10.11728/cjss2020.02.264 cstr: 32142.14.cjss2020.02.264
基金项目: 

浙江省自然科学基金项目(LQ18A030001)和宁波市自然科学基金项目(2019A610090)共同资助

详细信息
    作者简介:
    • 赵娜,E-mail:zhaona@nbufe.edu.cn
  • 中图分类号: P184;P315

Characteristics of Moonquake and Its Comparison with Earthquakeormalsize

  • 摘要: 月球内部结构是月球研究的热点问题,月震是研究月球内部结构的最佳手段之一.对月震数据及震源参数进行了再分析,在分析已有研究结果的基础上,对各类月震的信号特征、震源分布以及震源机制进行讨论,并将其与地震进行对比.研究发现,月震与地震有很多明显差异:月震信号持续时间较长,且深源月震与热月震具有波形匹配特征;探测到的月震多为深源月震,主要分布于月球正面的北东向和南西向;深源月震和热月震的发震时间都具有周期性,深源月震的周期性主要由地球对月球的潮汐引力以及太阳对月球轨道的扰动造成,且其发震位置具有丛集性,即在相同或相近位置重复发生,而热月震的周期性主要由于月球昼夜温度变化造成.

     

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出版历程
  • 收稿日期:  2019-06-20
  • 修回日期:  2020-01-04
  • 刊出日期:  2020-03-15

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