首页> 外文会议>Proceedings of ESA living planet symposium >COMPARISON OF THE GLOBAL ANALYTICAL MODELS OF THE MAIN GEOMAGNETIC FIELD WITH THE STRATOSPHERIC BALLOON MAGNETIC DATA
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COMPARISON OF THE GLOBAL ANALYTICAL MODELS OF THE MAIN GEOMAGNETIC FIELD WITH THE STRATOSPHERIC BALLOON MAGNETIC DATA

机译:主要地磁场的全球解析模型与平流球囊磁数据的比较

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Three global analytical models of a main geomagneticrnfield constructed by satellite data are used: model IGRF,rnDaily Mean Spherical Harmonic Models (DMSHM),rnand model EMM/2010, and also scalar data ofrngeomagnetic field and its gradients, received inrnstratospheric balloon gradient magnetic surveys atrnaltitudes of ~30 km. At these altitudes the regionalrnmagnetic field is formed from all sources of the Earth'srncrust. It enables to receive along lengthy routes ofrnsurveys the fullest data on regional and longwave-lenghtrnmagnetic anomalies. Model DMSHM is used atrnextracting of magnetic anomalies for elimination of arnsecular variation up to significant value 0,2 nT. Thernmodel can be constructed within the limits of ± 1rnmonths from the moment stratospheric balloon surveysrnwith beneficial day terms with magnetic activity up tornKp <20, that leads to an error of representation of mainrnMFE equal ±5 нТл. It is possible at presence acting forrnthe period of stratospheric balloon magnetic survey ofrnthe satellite, for example, Swarm. On stratosphericrnballoon data it is shown, that model EMM/2010rnunsatisfactorily displays MFE at altitude of 30 km.rnHence, the qualitative model of the constant (main andrnanomaly) magnetic field cannot be constructed onlyrnwith use of satellite and ground data. The improvedrnmodel constant MFE, constructed according to satelliternand stratospheric balloon magnetic surveys, developedrnup to a degree and the order m=n=720, will have arnreliable data about regional crust magnetic field, hence,rnand about deep magnetic structure of the Earth's crust.rnThe use gradient magnetic surveys aboard stratosphericrnballoons allows to find the places alternatingrnapproximately through 3000 km in which there are nornmagnetic anomalies. In these places probably tornsupervise satellite magnetic models for a range ofrnaltitude of 20-40 km, timed to stratospheric balloonrnmagnetic surveys.
机译:使用了由卫星数据构建的主要地磁场的三个全局分析模型:IGRF模型,每日平均球谐模型(DMSHM),EMM / 2010模型以及地磁场和其梯度的标量数据,在平流层气球内进行了磁梯度勘测约30公里。在这些高度上,区域磁场是由地壳的所有来源形成的。它使您能够沿着漫长的测量路径接收有关区域和长波电磁异常的最完整数据。 DMSHM模型用于磁性异常的提取,以消除高达0.2 nT的显着值的神经变异。可以在平流层球囊勘测开始的±1rnmonth范围内构建模型,其中有利的天数项的磁活动高达tornKp <20,这会导致mainrnMFE的表示误差等于±5Ω。在存在的情况下,可能会在例如Swarm的卫星的平流层气球磁测期间内起作用。从平流层气球的数据可以看出,EMM / 2010模型在30 km的高度上不能令人满意地显示MFE。因此,仅使用卫星和地面数据就不能建立恒定(主磁异常)磁场的定性模型。根据卫星和平流层气球磁测量法构造的改进模型常数MFE,发展到一定程度,阶数m = n = 720,将具有关于区域地壳磁场的可靠数据,因此,将具有关于地壳深层磁性结构的可靠数据。使用平流层气球上的梯度磁测量法,可以找到大约3000 km内有正磁异常的位置。在这些地方,可能会破坏监测卫星磁模型的高度,范围为20-40 km,以平流层球囊磁测量为定时。

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  • 会议地点 Edinburgh(GB)
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    Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation Russian Academy of Sciences (IZMIRAN) 142190, Moscow, Troitsk, Kaluzhskoe shosse d.4, Russia. Email: tsvetkov@izmiran.ru;

    Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation Russian Academy of Sciences (IZMIRAN)142190, Moscow, Troitsk, Kaluzhskoe shosse d.4, Russia;

    Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation Russian Academy of Sciences (IZMIRAN)142190, Moscow, Troitsk, Kaluzhskoe shosse d.4, Russia;

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