Supplementary Dataset: "Polar ionospheric currents and high temporal resolution geomagnetic field models"

READMEData and model parameter files supplement the paper:Title: "Polar ionospheric currents and high temporal resolution geomagnetic field models"Authors: Kloss, C. and Finlay, C. and Laundal, K.M. and Olsen, N.DOI: 10.1093/gji/ggad325Supplementary software that investigates the divergence and curl of the estimated poloidal ionospheric field is available at https://doi.org/10.11583/DTU.24542374.Files DescriptionThe following files are available:Model-A_datafile.h5Reference.matModel-A.matModel-B.matreadme.txt(1) Model-A_datafile.h5:The file stores the processed magnetic data used to estimate our geomagnetic field model called Model-A. Data is organized as HDF-datasets within the HDF-group "vector". Each HDF-dataset comes with the attributes "UNITS", "DESCRIPTION" and "FORMAT", which provide additional information on the HDF-dataset.Python code example (using h5py Python package):>>> import h5py as h5>>> file = h5.File('Model-A_datafile.h5', 'r')>>> print(list(file['vector'].keys())) # list all data variables>>> print(file["vector/Time"].attrs["UNITS"].decode()) # units of "Time">>> file.close()References to the original databases:(i) Swarm and CryoSat2 data are available through ESA at https://swarm-diss.eo.esa.int/#.(ii) CHAMP data are available from GFZ Data Services at https://www.doi.org/10.5880/GFZ.2.3.2019.004.(iii) Ground magnetic observatory data from INTERMAGNET are available via the virtual research platform VirES https://vires.services/.(iv) RC index is available at http://www.spacecenter.dk/files/magnetic-models/RC/.(v) SML index is available at https://supermag.jhuapl.edu/info/.(vi) Solar wind speed, interplanetary magnetic field and Kp index are available through the GSFC/SPDF OMNIWeb interface at https://omniweb.gsfc.nasa.gov/ow.html.(vii) CHAOS-7 model and its updates are available at http://www.spacecenter.dk/files/magnetic-models/CHAOS-7/.(2-4) Reference.mat (similarly for Model-A.mat, Model-B.mat):Model parameter file of our estimated model in mat-format, following the style of the CHAOS model releases.Chaosmagpy (documentation, doi: https://doi.org/10.5281/zenodo.3352398 ) can be used to load the mat-formatted file and evaluate the non-ionospheric parts of the model. The ionospheric part of our model is unfortunately not supported at the moment. However, we have plans to make this possible in a future version of chaosmagpy.Python code example (using ChaosMagPy Python package):>>> import chaosmagpy as cp>>> model_a = cp.CHAOS.from_mat('Model-A.mat) # load model file>>> B_int = model_a.synth_values_tdep(...) # evaluate time-dependent internal field(5) Readme.txt:Copy of this document.Changelog2023-11-10 Added link to supplementary software.2023-08-16 Initial preparation of this document and the files by Clemens Kloss.

README数据与模型参数文件补充了该论文：
标题：
《极区电离层电流与高时间分辨率地磁场模型》
作者：Kloss, C. 和 Finlay, C. 和 Laundal, K.M. 和 Olsen, N.
DOI：10.1093/gji/ggad325
可供查询的补充软件用于研究估算的极向电离层场的散度和旋度，可在以下链接找到：https://doi.org/10.11583/DTU.24542374。
文件描述
以下文件可供使用：
Model-A_datafile.h5
Reference.mat
Model-A.mat
Model-B.mat
readme.txt
（1）Model-A_datafile.h5：
该文件存储了用于估算我们所称的Model-A地磁场模型的处理后的磁数据。数据按HDF-datasets组织在HDF-group "vector"内。每个HDF-dataset都附带"UNITS"、"DESCRIPTION"和"FORMAT"属性，这些属性提供了有关HDF-dataset的附加信息。
Python代码示例（使用h5py Python包）：
>>> import h5py as h5
>>> file = h5.File('Model-A_datafile.h5', 'r')
>>> print(list(file['vector'].keys())) # 列出所有数据变量
>>> print(file["vector/Time"].attrs["UNITS