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通过不同方法获得的葡萄牙科英布拉中纬度地磁台的地磁场太阳平静(Sq)和太阳扰动(SD)变化的数据集。

Datasets of the solar quiet (Sq) and solar disturbed (SD) variations of the geomagnetic field from the mid latitudinal Magnetic Observatory of Coimbra (Portugal) obtained by different methods.

作者信息

Morozova Anna, Rebbah Rania, Ribeiro Paulo

机构信息

CITEUC, Department of Physics, University of Coimbra, Coimbra, Portugal.

Instituto de Astrofísica e Ciências do Espaço, Department of Physics Coimbra, University of Coimbra, Portugal.

出版信息

Data Brief. 2021 May 28;37:107174. doi: 10.1016/j.dib.2021.107174. eCollection 2021 Aug.

Abstract

The datasets of daily variations is obtained from the geomagnetic field raw observations at the Coimbra Magnetic Observatory (COI, Portugal). The data set was obtained for the 01.01.2007-31.12.2017 time interval and covers almost the entire solar cycle 24. The raw data were processed using two methods to extract daily variability. The first method uses the so-called "geomagnetically quiet days" to calculate S-type variations as daily means resulting in the data sub-set named "IQD Sq and SD". The second method uses the principal component analysis (PCA) to extract main variability modes of the original data. The first three modes produced by PCA and explaining up to 98% of the variability of the raw data are in the data sub-set named "PCA modes". Both methods allow to extract regular geomagnetic field variations related to daily variations (S-type variations) in the ionospheric dynamo region and some magnetospheric currents (e.g., field-aligned currents). The COI location in middle latitudes near the mean latitude of the ionospheric Sq current vortex's focus allows studying its seasonal and decadal variability using the S-type regular variations of the geomagnetic field measured near the ground. The S-type variations for the X and Y components of the geomagnetic field obtained at the COI observatory can also be re-scaled and used to analyze geomagnetic field variations obtained at other European geomagnetic observatories at close latitudes. The S-type variations for the Z component of the geomagnetic field obtained at the COI observatory can be compared to similar variations observed at more continental regions to study the so-called "coastal effect" in the geomagnetic field variations.

摘要

日变化数据集来自葡萄牙科英布拉磁台(COI)的地磁场原始观测数据。该数据集获取的时间区间为2007年1月1日至2017年12月31日,几乎涵盖了整个第24太阳活动周期。原始数据通过两种方法进行处理以提取日变化。第一种方法使用所谓的“地磁平静日”来计算S型变化,将其作为日均值,从而得到名为“IQD Sq和SD”的数据子集。第二种方法使用主成分分析(PCA)来提取原始数据的主要变化模式。PCA产生的前三种模式解释了原始数据高达98%的变化,它们位于名为“PCA模式”的数据子集中。这两种方法都能够提取与电离层发电机区域的日变化(S型变化)以及一些磁层电流(如场向电流)相关的规则地磁场变化。COI位于中纬度地区,靠近电离层Sq电流涡旋中心的平均纬度,这使得利用在地面附近测量的地磁场S型规则变化来研究其季节和年代际变化成为可能。在COI台站获得的地磁场X和Y分量的S型变化也可以重新缩放,并用于分析在相近纬度的其他欧洲地磁台站获得的地磁场变化。在COI台站获得的地磁场Z分量的S型变化可以与在更多大陆地区观测到的类似变化进行比较,以研究地磁场变化中的所谓“海岸效应”。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/5fd9/8182385/4d7de81a3a15/gr1.jpg

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