雅砻江锦屏水电站工程区活动构造研究及地壳稳定性评价

北东向的锦屏山-小金河断裂带从北东到南西斜穿整个锦屏水电站工程区。在它的东南和西北分别有北北西走向的羊坪子-纸厂沟断层组和北西走向的前波、高牛场等断层。锦屏山-小金河断裂带的马山头-周家坪断层组、瓦科断层组和北西向前波断层等晚第四纪继续活动, 但活动强度很弱。工程区新构造运动以整体抬升为主, 兼水平滑移和旋转运动。历史至今, 工程区地震活动微弱, 是地壳相对稳定的地区。     

Study of typical space wave–particle coupling events possibly related with seismic activity

Based on the DEMETER satellite, we found two space wave-particle coupling events during February 2010 that took place in the range of the McIlwain parameter L （1.27-- 1.37）. There are strong spatial and temporal correlation between the particle bursts （PBs） and the electromagnetic disturbances of the coupling events. The two PBs show different energy spectrum characteristics, while the corresponding electromagnetic disturbances concentrated on different frequency ranges. In agreement with the prediction of the theory of wave-particle interaction, we conclude that the two wave-particle inter- actions can be probably explained as follows： one is electron-dominant precipitation with energy of 0.09 MeV,-~0.2 MeV induced by a VLF electromagnetic wave with the frequencies of 14 kHz,-20 kHz, and another is proton-dominant precip- itation with energies of 0.65 MeV--2.85 MeV induced by a VLF electromagnetic wave with the frequency of ≤ 100 Hz. For the first time, these particle bursts＇ origins, from electrons or protons detected by the Instrument for the Detection of Particles （IDP） on board, are inferred by theoretical calculation, although the instrument has no ability to identify the particle species.     

震级频度与古登堡-里克特关系式偏离的实验与震例分析

基于一定时期内区域地震事件的地震震级(M)和频次(N)之间服从古登堡-里克特(G-R)震级频度关系lgN=a-bM的基本原理,本文通过对室内岩石破裂实验及华北地区部分中强以上(M≥5.0)地震震例研究发现,随着在岩石失稳(强地震)的临近,声发射事件能量或地震震级与频度之间不能较好地遵从G-R关系.出现较大偏离.这种偏离可作为强地震发生的前兆指标,对利用区域中小地震活动事件探讨预测强地震具有重要作用.     

Proton loss of inner radiation belt during geomagnetic storm of 2018 based on CSES satellite observation

The proton distribution in inner radiation belt is often affected by strong geomagnetic storm disturbance. Based on the data of the sun-synchronous CSES satellite, which carries with several high energy particle payloads and was launched in February 2018, we analyzed the extensive proton variations in the inner radiation belt in a wide energy range of 2 MeV-220 MeV during 2018 major geomagnetic storm. The result indicates that the loss mechanism of protons was energy dependence which is consistent with some previous studies. For protons at low energy 2 MeV-20 MeV, the fluxes were decreased during main phase of the storm and did not come back quickly during the recovery phase, which is likely to be caused by Coulomb collision due to neutral atmosphere density variation. At higher energy 30 MeV-100 MeV, it was confirmed that the magnetic field line curvature scattering plays a significant role in the proton loss phenomenon during this storm. At highest energies > 100 MeV, the fluxes of protons kept a stable level and did not exhibit a significant loss during this storm.