Connection between proto-neutron star Tayler-Spruit dynamos and low-field magnetars: dataset

Raw scientific data for Nature Astronomy publication

Andrei Igoshev, Paul Barrere, Raphael Raynaud, Jerome Guilet, Toby Wood and Rainer Hollerbach

Connection between proto-neutron star Tayler-Spruit dynamos and low-field magnetars

The folder contains the following files:

Figure1.vtu stores crust-confined magnetic fields at the beginning of simulations.

We provide Python Notebook Figure2_NA.ipynb to produce Figure 2 using custom output files produced with Parody code.

This script extract surface magnetic fields from snapshoots Gt=0.00064.HD2, Gt=0.00256.HD2 and Gt=0.01016.HD2.

These files contains dimensionless magnetic fields and temperatures everywhere in the crust of neutron star.

Figure3.vtu contains surface temperature and external magnetic fields.

Figure4.vtu contains crust confined magnetic fields and cracks structure.

Folder Figure5 contains .npy files used to produce Figure 5.

*.vtu files can be opened using open source data visualisation software ParaView https://www.paraview.org/

用于《自然·天文学》（Nature Astronomy）刊发的原始科研数据

安德烈·伊戈舍夫（Andrei Igoshev）、保罗·巴雷尔（Paul Barrere）、拉斐尔·雷诺（Raphael Raynaud）、热罗姆·吉莱（Jerome Guilet）、托比·伍德（Toby Wood）与赖纳·霍勒巴赫（Rainer Hollerbach）

原中子星泰勒-斯普鲁特（Tayler-Spruit）发电机与低场磁星的关联

本文件夹包含以下文件：

Figure1.vtu 存储了模拟初始时刻地壳约束的磁场。

我们提供Python Notebook文件Figure2_NA.ipynb，可依托Parody代码生成的自定义输出文件绘制图2。该脚本可从快照文件Gt=0.00064.HD2、Gt=0.00256.HD2及Gt=0.01016.HD2中提取表面磁场。

上述文件包含中子星星壳全域的无量纲磁场与温度数据。

Figure3.vtu 存储了表面温度与外部磁场数据。

Figure4.vtu 存储了地壳约束的磁场与裂纹结构。

Figure5文件夹内包含用于绘制图5的.npy格式文件。

所有*.vtu格式文件均可通过开源数据可视化软件ParaView（https://www.paraview.org/）打开。