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1.
This paper describes the pattern of geomagnetic solar quiet day, Sq, variations recorded at the Indian geomagnetic observatories. The extent to which the high and low latitude ionosphere is
interlinked electromagnetically during periods of quiet geomagnetic conditions is a point of debate. The concept of Gabriel
graph is applied to derive the boundaries for the variations of horizontal, vertical, and declination components of the earth’s
magnetic field during geomagnetically quiet periods. Data of the six Indian geomagnetic observatories (Alibag, Hyderabad,
Nagpur, Pondicherry, Visakapatnam, and Trivandrum) are considered for this analysis. This graph theoretical model is complementary
to the classical data analysis techniques. Analytical method and the results of the analysis are presented in the paper. 相似文献
2.
使用华南地区5个国家基准地磁台2008—2018年地磁观测数据,通过对磁偏角D、磁倾角I、总强度F、北向分量X、东向分量Y、水平分量H、垂直分量Z月均值及年变率的分析,研究该区地磁场长期变化特征。结果表明,华南地区5个地磁台近10年来七要素月均值及年变率均呈缓慢变化趋势,且变化量相当,反映了该区域地磁场长期变化的特征。 相似文献
3.
The geomagnetic field components are periodically measured at repeat stations. The main objective of the repeat stations is to provide data for tracing the secular variation of the geomagnetic field components. Secular variation at the repeat station is generally different from that at geomagnetic observatory used in the data reduction. The effect of the secular variation differences on geomagnetic data reduction was estimated for the regions of Europe, North America (below 60°N) and Australia, respectively, during the period of 2000-2010. These estimations were obtained by using the monthly mean values of north, east and vertical components of geomagnetic field, recorded at geomagnetic observatories. The effects were calculated by using observatories pairs, with distances from 350 km (in Europe) to 3100 km (in North America and Australia). The maximal effects were found to be the smallest in east component in Europe and North America, and vertical component in Australia; the effects increase with time from a central reduction epoch and they are not constant during mentioned eleven years; they were less than 1 nT only in Europe, for distances between the observatories up to 1000 km in all three components and for periods spanning ±1 month from a central epoch. It was found that their year to year variability is mostly due to the non-eliminated external field residuals in the observatories monthly means; their effect is up to 3 nT for ±3 months from a central epoch. Further, the real effects were compared to those modeled by IGRF-12 model. The maximal differences between the real and the modeled values are below 4.5 nT in all three components, for ±3 months from a central epoch. 相似文献
4.
At high latitudes, sporadic geomagnetic disturbances associated with geomagnetic storms introduce significant uncertainty in measurements by borehole inclinometers during the directional drilling of deep wells. Variations in the magnetic declination may lead to significant deviations of the actual coordinates of the borehole from the prescribed trajectory. Using the methods for calculating the profile of the actual borehole, we conducted model estimates of the influence of sporadic disturbances in the magnetic declination observed during the magnetic storm of October 28–31, 2003 on the displacement azimuth and intensity of borehole bending at the given locations at the sites of two high-latitude magnetic observatories. It is shown that, unless filtered based on the data of parallel observatory measurements, the geomagnetic disturbances can lead to unacceptably large errors in the borehole inclinometer measurements and cause a borehole deflection exceeding the admissible values. 相似文献
5.
《Journal of Atmospheric and Solar》2007,69(14):1770-1774
Relatively little is known about the effects of geomagnetism on plants. Such fundamental questions as (1) whether or not plants perceive the Earth's magnetic field, (2) the physical nature of the magnetic receptor(s) and (3) whether or not the geomagnetic field has any bearing on the physiology and survival of plants remain largely unanswered. The present review examines the possibility that three classes of unexplained biological rhythms in plants may relate to the sensitivity of plants to variations in the geomagnetic field. The first section examines the possibility that a class of plant rhythms, here termed 0.2–5 Hz rhythms, may be reflections of the sensitivity of plants to Pc1 geomagnetic pulsations. The second section reviews recent evidence that plants are affected by geomagnetic storms. The third section examines the possibility that circa-weekly, circa-fortnightly and circa-monthly rhythms in plants may be reflections of the solar rotation cycle and its sub-harmonics. 相似文献
6.
目前,在远海开阔性海域磁测中,尚难以有效设立日变站,致使日变改正仍存在着困难.本文利用地磁台站实测资料对地磁日变的纬度分布特征进行研究,发现日变值随纬度变化具有由Sq电流中心向南北两侧递增的规律,且二者之间的关系可用二次函数近似描述。以此规律为基础我们建立了纬度改正方法,该方法以经度链为基站,利用基站数据得到日变值与磁纬度的拟合函数以进行纬度改正,再调整时差作为经度校正即得到计算站的日变值.实测数据计算结果表明,相较于加权平均法,此方法在远距离(经度差达40°)仍能保持较高的校正精度(4 nT),因而能更好地适用于远海磁测. 相似文献
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地磁急变（jerk）是起源于地球外核并在导电地幔过滤效应后在地球表面观测到的一种地磁现象,其反映了地核内部某些动力学过程.Jerks在空间范围上既可以是区域性的,也可以是全球性的.中国地区地磁台能否检测到2014年jerk？针对这一问题,利用中国大陆10个地磁台的磁静日月均值和CHAOS-6全球磁场模型,分析了X、Y和Z分量2008—2018年期间的长期变化,估算了2014年前、后的长期加速度值,确定了2014年地磁jerk的时间和强度.研究表明中国地磁台Y分量的长期变化为"Λ"型,Z分量存在明显的"V"型,具有典型的jerk特点.Y分量jerk出现的时间大约在2014年6月,比非洲大陆的Algeria TAM台和南美洲French Guiana KOU台时间滞后大约4个月.这暗示着产生jerks的地核流体波动的时序特点.中国西部和东北部地磁台的长期变化形态有明显的差别,主要由非偶极磁场引起.CHAOS-6模型与地面台站的长期变化形态并非始终一致.本文结果有助于更好地理解和解释长期变化的时间演变和地理分布,并为深入探讨jerks的地核起源和驱动机制提供新的观测约束. 相似文献
9.
The IGRF-models for the main field and the secular variation (IGRF 1980 and IGRF-SV 1980–1985) have been compared with geomagnetic ground based data for epoch 1980.5 in the GDR, and also with the secular variation at 34 European observatories. The results for the main magnetic field were much better than for IGRF 1965. With a level-error of ～ 45 nT, the IGRF 1980 included ～ 75% of the magnetic crust field. The structure of the IGRF-field is similar to that of other regional reference fields.The IGRF-SV for 1965, 1975 and 1980–1985 have been compared with analytical SV-models, based on low-degree polynomial approximations. It is shown that the main features of SV in Europe are represented correctly. The mean differences between observatory data and IGRF-SV 1980–1985 are 1.5′/a for declination, and 7 nT/a for total intensity. 相似文献
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Surveys of the geomagnetic declination, inclination and total field intensity were carried out at eight stations of the Croatian
Geomagnetic Repeat Stations Network in 2004 and 2007. The total field time series at repeat stations and observatories were
compared by use of the multi-linear regression and linear correlation coefficients. The surveys’ data were reduced to 2004.5
and 2007.5 epochs by a simple method proposed here, assuming the secular variations at the repeat station and observatory
are equal or different, respectively. These reductions, obtained in reference to L’Aquila, Fürstenfeldbruck and Tihany observatories,
and corresponding weighted as well as non-weighted averages, were compared. The preferred geomagnetic field elements as well
as the corresponding annual changes between 2004.5 and 2007.5 epochs, were compared to the latest International Geomagnetic
Reference Field. Additionally, the Croatian Geomagnetic Normal Reference Fields for 2004.5 and 2007.5 epochs were presented. 相似文献
12.
Summary The ratios of the amplitudes of bay-type variations of the geomagnetic field along the DSS profile VI to the amplitudes of the same phenomena recorded at permanent geomagnetic observatories at Prhonice and Budkov were studied. The relative variations of the values of the horizontal component, declination and, particularly, the vertical component of the geomagnetic field indicate deep fault zones. 相似文献
13.
L. F. Chernogor 《Geomagnetism and Aeronomy》2014,54(5):613-624
An analysis was conducted of time variations in geomagnetic field components on the day of the Chelyabinsk meteorite event (February 15, 2013) and on control days (February 12 and 16, 2013). The analysis uses the data collected by magnetic observatories in Novosibirsk, Almaty, Kyiv, and Lviv. The distance R from the explosion site to the observatories varies in the range 1200–2700 km. The flyby and explosion of the Chelyabinsk cosmic body is found to have been accompanied by variations mainly in the horizontal component of the geomagnetic field. The variations are quasi-periodic with a period of 30–40 min, an amplitude of 0.5–2 nT for R ≈ 2700?1200 km, respectively, and a duration of 2–3 h. The horizontal velocity of the geomagnetic field disturbances is close to 260–370 m/s. A theoretical model of wave disturbances is proposed. According to the model, wave disturbances in the geomagnetic field are caused (a) by the motion of the gravity wave generated in the atmosphere by the falling space body and (b) by traveling ionospheric disturbances, which modulate the ionospheric current at dynamo altitudes. The calculated amplitudes of the wave disturbances are 0.6–1.8 nT for R ≈ 2700?1200 km, respectively. The estimates are in good agreement with the observational data. Disturbances in the geomagnetic field level (geomagnetic pulsations) in the period range 1–1000 s are negligible (less than 1 nT). 相似文献
14.
Estimating external magnetic field differences at high geomagnetic latitudes from a single station 
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下载免费PDF全文 Providing an accurate estimate of the magnetic field on the Earth's surface at a location distant from an observatory has useful scientific and commercial applications, such as in repeat station data reduction, space weather nowcasting or aeromagnetic surveying. While the correlation of measurements between nearby magnetic observatories at low and mid‐latitudes is good, at high geomagnetic latitudes () the external field differences between observatories increase rapidly with distance, even during relatively low magnetic activity. Thus, it is of interest to describe how the differences (or errors) in external magnetic field extrapolation from a single observatory grow with distance from its location. These differences are modulated by local time, seasonal and solar cycle variations, as well as geomagnetic activity, giving a complex temporal and spatial relationship. A straightforward way to describe the differences are via confidence intervals for the extrapolated values with respect to distance. To compute the confidence intervals associated with extrapolation of the external field at varying distances from an observatory, we used 695 station‐years of overlapping minute‐mean data from 37 observatories and variometers at high latitudes from which we removed the main and crustal fields to isolate unmodelled signals. From this data set, the pairwise differences were analysed to quantify the variation during a range of time epochs and separation distances. We estimate the 68.3%, 95.4% and 99.7% confidence levels (equivalent to the 1σ, 2σ and 3σ Gaussian error bounds) from these differences for all components. We find that there is always a small non‐zero bias that we ascribe to instrumentation and local crustal field induction effects. The computed confidence intervals are typically twice as large in the north–south direction compared to the east‐west direction and smaller during the solstice months compared to the equinoxes. 相似文献
15.
Piotr Tucholka 《Earth and Planetary Science Letters》1980,48(2):379-384
A simple method of calculating running means over different intervals within palaeomagnetic records has been used to identify short-period secular variations of the geomagnetic field. The records from Polish lake sediments reveal variations in declination with a period between 290 and 372 years. The periodicity of variations in the inclination has been estimated to be between 522 and 670 years. 相似文献
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《地震科学（英文版）》2010,(4)
By calculating the hourly standard deviation of the first-order differences of the horizontal geomagnetic component minute data,a new index Vr to represent the variation rate of the geomagnetic field was introduced.Vr-indices show similar trends in the temporal change at different observatories and have simultaneous peak values at the observatories covering a large span geographically,which reveals that the source of geomagnetic disturbances represented by Vr is in the magnetosphere.Based on the comparison among Vr,Kp and ap,it is found that generally Vr changes linearly with Kp and ap,which means that the rapid changes of magnetic field usually exist together with magnetic disturbances.But there are exceptions.As Vr can be easily produced by individual observatory in quasi real time and is more sensitive to the variation rate of geomagnetic field rather than the field itself,it can be expected to serve for monitoring or predicting the geomagnetic-induced event in a quick and intuitive way. 相似文献
18.
第11代国际地磁参考场(IGRF-11)是国际地磁学与高空物理学联合会(IAGA)于2009年12月提出的最新与比较准确的IGRF.根据IGRF-11模型,计算了2005-2010年中国地区地磁长期变化(SVC).IGRF-11所描述的2005-2010年中国地区地磁长期变化与实际观测的地磁长期变化(SVO)是基本一致的,但亦有明显差异.分析比较了在中国地区34个台站上的SVO与SVC之间的差异,并得到了它们之间的差值及其均方误差σ,对于地磁偏角和倾角,σ分别为0.35′/a与0.53′/a;对于地磁总强度、水平分量、北向分量、东向分量与垂直分量,σ分别为5.12nT/a,8.91nT/a,8.89nT/a,3.27nT/a与3.59nT/a.引起IGRF-11所描述的2005-2010年中国地区地磁长期变化的误差原因是:中国地区的区域性与局部性的磁异常、IGRF忽略了外源场与IGRF模型的截断阶数、全球台站与测点的分布不均匀、地磁观测误差等因素.由于中国地磁模型(CGM)优于IGRF模型,并能比较准确地描述中国地区地磁场及其长期变化,故在实际应用中应选用CGM. 相似文献
19.
通过对同一台站人工观测的地磁场总强度F与连续记录F,及两套连续记录仪记录的地磁场总强度F夜均值的差值分析,发现同一台站两种差值均存在显著的年变化特征。对其他台站同样可以看到类似变化。而各时段的时均值差值也表现出相似的变化特征。由此说明,同一台站地磁观测区的不同点位,地磁场差异在长时间内不断发生变化,在进行绝对观测时,无法通过选择绝对观测时间消除该差值变化。 相似文献
20.
地磁偏角实时自动修正技术在油田定向钻井中的应用 总被引：2，自引：1，他引：2
在油田定向钻井的磁导向定位系统中，地磁偏角校正是一个不可缺少的基本要素，同时在磁偏角校正值精度直接影响定向井的导向定位精度。因此，作者提出了提高地磁偏角校正值精度的方法，并试图将地磁偏角实时自动修正技术引入我国油田定向钻井领域。 相似文献