Sun Weijia, Tkalčić Hrvoje
Key Laboratory of Earth and Planetary Physics, Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing, China.
Research School of Earth Sciences, The Australian National University, Canberra, Australia.
Nat Commun. 2022 Mar 30;13(1):1695. doi: 10.1038/s41467-022-29329-x.
Marsquakes excite seismic wavefield, allowing the Martian interior structures to be probed. However, the Martian seismic data recorded by InSight have a low signal-to-noise ratio, making the identification of marsquakes challenging. Here we use the Matched Filter technique and Benford's Law to detect hitherto undetected events. Based on nine marsquake templates, we report 47 newly detected events, >90% of which are associated with the two high-quality events located beneath Cerberus Fossae. They occurred at all times of the Martian day, thus excluding the tidal modulation (e.g., Phobos) as their cause. We attribute the newly discovered, low-frequency, repetitive events to magma movement associated with volcanic activity in the upper mantle beneath Cerberus Fossae. The continuous seismicity suggests that Cerberus Fossae is seismically highly active and that the Martian mantle is mobile.
火星地震激发地震波场,从而能够探测火星内部结构。然而,洞察号记录的火星地震数据信噪比很低,使得火星地震的识别具有挑战性。在此,我们使用匹配滤波技术和本福特定律来检测迄今未被发现的事件。基于九个火星地震模板,我们报告了47个新检测到的事件,其中超过90%与位于地狱溪地堑下方的两个高质量事件有关。它们在火星日的任何时间都有发生,因此排除了潮汐调制(例如火卫一)作为其成因。我们将新发现的低频重复事件归因于与地狱溪地堑下方上地幔火山活动相关的岩浆运动。持续的地震活动表明,地狱溪地堑地震活动非常活跃,且火星地幔是可移动的。