Possible Cause-Effect Relationships Between Vrancea (Romania) Earthquakes and Some Global Geophysical Phenomena

The possibility that the Earth's tides are a triggering factor of Vrancea subcrustal earthquakes is investigated in the first part of this paper. A possible correlation between Vrancea subcrustal earthquakes and geomagnetic jerks is demonstrated in the second part. The last part of the paper presents a number of results concerning a possible relationship between the regularities of strong Vrancea subcrustal seismicity and the Chandler nutation parameters. An attempt is made to integrate all of these phenomena in a more general framework that takes into account physical processes in the Earth mantle and core. A long-term prediction of the next strong Vrancea earthquake is finally attempted.     

地磁匹配导航中几项关键技术研究

地磁匹配导航的实质是数字地图的匹配.地磁数据库的精度和地磁适配区的选择是地磁匹配导航中的2项关键技术.文中把克吕格插值算法引入到地磁图的重构中,仿真结果表明了其有效性;同时把熵选择法和统计特征法引入到地磁适配区的选择中,通过仿真结果对2种方法进行比较,结果表明,熵选择法综合效果更好,更适合于在实际中应用.     

Geomagnetic Pc3 Pulsations During the Total Solar Eclipse on Aug 11, 1999

The solar eclipse on August 11, 1999, observed in the region covered by many geomagnetic observatories, has offered a unique opportunity to look for an effect of the eclipse on geomagnetic pulsations. The pulsation activity digital data have been taken from Budkov Observatory in the Czech Republic (in the X component only), from observatories in Germany (Niemegk, Fürstenfeldbruck, Bad Bergzabern), in Hungary (Nagycenk), and for comparison in South Africa (Hermanus, conjugate-point station), and in Finland (Sodankylä, far from the eclipse zone). At all these stations the field in all three component has been recorded. The pulsation amplitudes in the X component exhibit a long-term minimum near the time of the eclipse. Spectral analysis of selected short intervals confirmed this decrease and also revealed a decrease of the average pulsation period during the eclipse. Such a change in the amplitude or in the period was not observed outside of the eclipse interval or in other days. Investigation in some narrower frequency bands showed that the maximal decrease occurred in the 15–20 s band. All these changes can be found in records from all the stations near the eclipse totality belt, also in records at the conjugate-point station, where no eclipse occurred. No signature has been found in records at the station situated far from the eclipse zone.     

新疆地震活动区的地磁观测与研究

新疆地区是中国最活跃的地震区之一.为了监测新疆地区潜在的强烈地震,2003年在该地区建立了N和S两个地磁测网并进行了地磁三分量测量.在N和S两个测网所选建的51个测点周围环境良好,地磁梯度小,适宜地磁测量.在野外测量中,使用性能稳定可靠的G-856磁力仪、DI磁力仪与GPS仪器,应用GPS测定方位角,DI磁力仪测量地磁偏角D与倾角I,G-856磁力仪测量总强度F.应用新疆地区乌鲁木齐与喀什地磁台站的资料,分别通化了N和S两个测网的地磁测量资料.该地磁通化值的平均标准偏差σ为:F的σf=0.20 nT;D的σd=0.06′;I的σI=0.03′,表明地磁测量资料准确可靠.根据上述地磁测量资料,应用精度高的spline方法,得到了N与S测网地磁场及其异常场的分布.结果表明,该地磁场及其异常场的分布,可以准确地描述N与S测网的地磁场及其地磁异常场.该地磁分布为今后在新疆地区的震磁研究与地震监测提供了良好的地磁参考场.     

京津冀地区地磁场球冠谐分析

2002年在京津冀地区进行了45个测点的地磁三分量测量,对测量资料进行通化处理,通化时间为2002年5月5日16～18时（世界时）. 通化后的观测均方差分别优于1.5nT（地磁场总强度F）,0.5′(磁偏角D和磁倾角I). 将国际参考地磁场（IGRF2000）作为地磁正常场,建立了京津冀地区地磁异常场的球冠谐模型（BTHASCH）. 球冠极的空间位置坐标为39.5°N和117.0°E,球冠半角为4°. 在模型计算过程中,球冠谐函数的截断阶数分别取为1～10. 经综合比较, 最终采用的截断阶数为5. 建立了京津冀地区参考地磁场的球冠谐模型（BTHGRF）.根据模型,绘制了京津冀地区地磁异常场图(ΔX、ΔY、ΔZ、ΔF、ΔD、ΔI)和京津冀地区地磁图(X、Y、Z、F、D、I).     

基于北斗GEO卫星的磁暴期间电离层TEC响应分析

基于亚太地区北斗GEO卫星数据对2017-05发生在中低纬度地区的磁暴现象进行研究,并使用北斗GEO卫星获取的TEC实测数据对全球电离层图的精度进行评估。进一步对磁暴引起的全球电离层TEC变化进行分析发现,电离层TEC对磁暴的响应出现在磁暴主相开始1~4 h之后,最大扰动值达到20 TECu以上。     

地磁太阳黑子周变化起源的讨论

为了避开60年代末和70年代末Jerk(H)、Jerk(Z)的影响,分析了1979～1998年西欧4个台和1979～1999年亚洲东部6个台的H、Z资料,结果表明各台间H(或X)分量的太阳黑子周变化一致性较好.但Z分量的太阳黑子周变化显示出非常特别的现象,Z变化的相位随台站经度变化而变化,东亚地区的Z变化几乎与西欧地区的变化反向.因此,东亚地区的Z变化与H变化的关系不符合P01模式的假设,外源场之说似乎不能解释.     

成都地磁台的观测与评估

通过对成都地磁台的仪器配置、误差来源、资料质量等方面进行综合分析，结果表明．成都地磁台的观测质量稳定，资料连续可靠。成都地磁台的观测能够正确反映成都地区地磁场的变化特征。