海洋和电离层发电机对佘山台L的影响   总被引：1，自引：0，他引：1  

康国发 《地震地磁观测与研究》1992,13(4):46-50

本文在文献[1]的研究基础上进一步分析海洋和电离层发电机对佘山台L的影响。资料分别按月、季节和年以及太阳活动性分组进行的细致分析,结果表明海洋发电机对Z分量的L有一稳定的影响,L的季节变化主要起源于电离层发电机。L的海洋部分不随太阳活动性改变,太阳活动对L的影响比对S的小。  相似文献   

1945—1995年国际参考地磁场   总被引：1，自引：0，他引：1  

安振昌 《地球物理学进展》1992,(2)

本文回顾了国际参考地磁场(IGRF)的建立和修改过程;介绍了最新的IGRF模型,即第六代国际参考地磁场;综述了国际参考地磁场在地磁学中的应用,并指出了在使用过程中需要注意的一些问题.  相似文献   

1950-1980年中国地区主磁场模型的建立及分析   总被引：3，自引：10，他引：3  

安振昌  徐元芳 《地球物理学报》1991,34(5):585-593

本文根据丰富的地磁资料,用泰勒多项式方法推算出1950.0、1960.0、1970.0和1980.0年中国地区的主磁场模型,绘制出各个年代地磁要素的等值线图,分析研究了局部地区地磁场泰勒多项式模型的特点.  相似文献   

Variations in the strength of recurrent geomagnetic activity in solar cycles 11 to 21     

G. K. Rangarajan 《Journal of Earth System Science》1991,100(1):49-54

From maximum entropy spectral analysis (MESA) of short lengths ofAa indices of geomagnetic activity, the characteristics of the strength of the 27-day and 13.5-day signals for each of the solar cycles 11 to 21 are highlighted. It is shown that the 13.5-day signal is a near permanent feature in geomagnetic activity. The Hale-cycle (22 yr) effect could be seen in the average magnitude of the 27-day signal with greater strengths in the even cycles. No clear annual variation in the strength is noticed, contrary to some earlier known results.  相似文献   

Detector time offset and off-line calibration in EAS experiments     

H.H. He  P. Bernardini  A.K. Calabrese Melcarne  S.Z. Chen 《Astroparticle Physics》2007,27(6):528-532

In extensive air shower (EAS) experiments, the primary direction is reconstructed by the space–time pattern of secondary particles. Thus the equalization of the transit time of signals coming from different parts of the detector is crucial in order to get the best angular resolution and pointing accuracy allowed by the detector. In this paper an off-line calibration method is proposed and studied by means of proper simulations. It allows to calibrate the array repeatedly just using the collected data without disturbing the standard acquisition. The calibration method is based on the definition of a Characteristic Plane introduced to analyze the effects of the time systematic offsets, such as the quasi-sinusoidal modulation on azimuth angle distribution. This calibration procedure works also when a pre-modulation on the primary azimuthal distribution is present.  相似文献   

Geoeffectiveness of magnetic cloud, shock/sheath, interaction region, high-speed stream and their combined occurrence     

Badruddin  Y.P. Singh 《Planetary and Space Science》2009,57(3):318-331

A subset of CMEs, called interplanetary magnetic clouds (MCs), are observed to have systematic rotation [northward to southward (NS) or southward to northward (SN)] in their field structures. These MCs identified in the heliospheric plasma and field data at 1 AU may have different features associated with them. These structures (NS/SN) may be isolated MC moving with the ambient solar wind. MCs (NS/SN) may also be associated with shock/sheath region, formed due to compression of the ambient plasma/field ahead of them. A fraction from each of these four types of MCs have additional features, being ‘pushed’ by fast solar wind streams from coronal holes, forming interaction region (IR) between MCs and high-speed solar wind streams (HSS). Using these different sets of MCs, we have done a detailed study of the geoeffectiveness of NS and SN turning MCs and their associated features (shock/sheath, IR and HSS). To study the process that produces the geomagnetic disturbances and influences its amplitude/duration, we have utilized the interplanetary plasma and field parameters, namely, plasma velocity, density, temperature, pressure, field strength and its north-south component, during the passage of these structures with different associated properties. Differences in the geoeffectiveness of MCs with different structural and dynamical properties have been identified. The possible role of high-speed stream in influencing the recovery time (and hence duration) of geomagnetic disturbance has also been investigated. A best-fit equation representing the relation between level of the geomagnetic activity (due to MCs) and interplanetary plasma/field parameter has been obtained.  相似文献   

Statistical Analysis of the Relationships among Coronal Holes,Corotating Interaction Regions,and Geomagnetic Storms     

Yunhee Choi  Y.-J. Moon  Seonghwan Choi  Ji-Hye Baek  Sungsoo S. Kim  K.-S. Cho  G. S. Choe 《Solar physics》2009,254(2):311-323

We have examined the relationships among coronal holes (CHs), corotating interaction regions (CIRs), and geomagnetic storms in the period 1996?–?2003. We have identified 123 CIRs with forward and reverse shock or wave features in ACE and Wind data and have linked them to coronal holes shown in National Solar Observatory/Kitt Peak (NSO/KP) daily He i 10?830 Å maps considering the Sun?–?Earth transit time of the solar wind with the observed wind speed. A sample of 107 CH?–?CIR pairs is thus identified. We have examined the magnetic polarity, location, and area of the CHs as well as their association with geomagnetic storms (Dst≤?50 nT). For all pairs, the magnetic polarity of the CHs is found to be consistent with the sunward (or earthward) direction of the interplanetary magnetic fields (IMFs), which confirms the linkage between the CHs and the CIRs in the sample. Our statistical analysis shows that (1) the mean longitude of the center of CHs is about 8°E, (2) 74% of the CHs are located between 30°S and 30°N (i.e., mostly in the equatorial regions), (3) 46% of the CIRs are associated with geomagnetic storms, (4) the area of geoeffective coronal holes is found to be larger than 0.12% of the solar hemisphere area, and (5) the maximum convective electric field E _y in the solar wind is much more highly correlated with the Dst index than any other solar or interplanetary parameter. In addition, we found that there is also a semiannual variation of CIR-associated geomagnetic storms and discovered new tendencies as follows: For negative-polarity coronal holes, the percentage (59%; 16 out of 27 events) of CIRs associated with geomagnetic storms in the first half of the year is much larger than that (25%; 6 out of 24 events) in the second half of the year and the occurrence percentage (63%; 15 out of 24 events) of CIR-associated storms in the southern hemisphere is significantly larger than that (26%; 7 out of 27 events) in the northern hemisphere. Positive-polarity coronal holes exhibit an opposite tendency.  相似文献   

太原基准地震台地磁转换函数变化与邻区地震的关系     

阎计明  张美仙  刘国俊  王向阳 《山西地震》2001,(4):19-23

利用转换函数方法对太原基准地震台1989年1月至1998年12月的地磁资料进行了计算，用所得到的转换函数A，B的模|A|,|B|及总方差δZ的月变化，来研究地震前后地下电性结构的变化。对1989年以来山西及周边地区的5次Ms5.0以上地震前后太原基准地震台地磁转换函数的变化进行了研究。得出不同周期的转换函数A，B以及总方差δZ在震前有明显变化的结论。  相似文献   

Mid-latitude winds in the mesosphere: a superposed epoch analysis over the geomagnetic storm times     

G. Ma  K. Igarashi  K. Hocke 《Journal of Atmospheric and Solar》2001,63(18):1075

This study aims at looking for the characteristic patterns of mesospheric wind over the geomagnetic storm times. For this purpose, the geomagnetic storms preceded by a sudden commencement (SSC) have been selected from January 1995 to April 1999. By using the onset of SSC as the timing mark, a superposed epoch analysis has been performed on the available neutral wind data measured with medium frequency (MF) radars at Yamagawa (31.2°N, 130.6°E) and Wakkanai (45.4°N, 141.7°E). In doing so, the length of time chosen for the superposed analysis is from 7 days before the SSC onset to 21 days after the onset; subsets of wind data are superimposed for summer and winter months, respectively. Then with harmonic analysis on the superposed winds the mean winds in both summer and winter months have been obtained. Concerning mean wind characteristics, some interesting details are the reversal heights of the summer zonal winds, which is 79–80 km at Yamagawa and 84 km at Wakkanai. Strong wavy structures with 2–4 days period are observed at both Yamagawa and Wakkanai in both summer and winter. As for storm effects, significant enhancement of eastward wind is found 5 days after SSC onset at both Yamagawa and Wakkanai in winter. Moreover, the northward wind turns southward at Wakkanai 2 days after the onset of SSC, and the southward wind lasts for several days thereafter. In summer months, the post-storm enhancement tends to be small and mainly in the eastward wind at both Yamagawa and Wakkanai.  相似文献   

肃南5．3级地震前嘉峪关台地震前兆异常初探     

朱宗德  田文通 《高原地震》2001,13(3):35-39

以嘉峪关台的原始资料为依据，着重探讨了肃南5．3级地震前祁连山西段的地震活动性异常。将本台的地磁Z分量与兰州、天水地磁台进行比较，结果认为：肃南5．3级地震的发生基本符合祁连山西段地震活动的周期性特征，前兆资料无明显的临震异常显示，但本台的自然电场，地磁日幅差和Z分量的日均值资料有明显的短期趋势性异常显示。  相似文献