Solutions to BAS-PRO model runs for Modelling 1-10MeV Proton Phase Space Density

This dataset contains solution data produced by the BAS-PRO proton radiation belt model for the study "Modelling Inner Proton Belt Variability at Energies 1 to 10MeV using BAS-PRO". The solution data is in the form of 3D grids describing phase space density computed during dynamic simulations of Earth's proton belt over the modelling period 2014 to 2018. Three model runs are included: SA19, J81 and S16. Files were produced in May 2021. This work was funded by the Natural Environment Research Council (NERC) via Doctoral Training Programme NE/R009457/1. Richard B. Horne and Sarah A. Glauert were supported by NERC National Capability grants NE/R016038/1 and NE/R016445/1, and by NERC grant NE/V00249X/1 (Sat-Risk), and by Highlight Topic Grant NE/P01738X/1 (Rad-Sat). Giulio Del Zanna acknowledges support from STFC (UK) via the consolidated grants to the atomic astrophysics group (AAG) at DAMTP, University of Cambridge (ST/P000665/1 and ST/T000481/1). Seth G. Claudepierre acknowledges support from NASA Grant no. NNX17AF10G and from RBSP-ECT funding provided by JHU/APL Contract 967399 under NASA's Prime Contract NAS5-01072.

本数据集包含由BAS-PRO质子辐射带模型生成的解算数据，用于研究论文《使用BAS-PRO对1至10MeV能量下内质子带变化性进行建模》。该解算数据以三维网格形式呈现，描述了2014年至2018年建模周期内，地球质子带动态模拟过程中计算得到的相空间密度。数据集包含三组模型运行结果：SA19、J81与S16。所有数据文件均于2021年5月生成。
本研究由自然环境研究委员会（Natural Environment Research Council, NERC）通过博士培训项目NE/R009457/1资助。Richard B. Horne与Sarah A. Glauert获得了NERC国家能力项目拨款NE/R016038/1与NE/R016445/1、NERC专项拨款NE/V00249X/1（Sat-Risk项目）以及重点主题拨款NE/P01738X/1（Rad-Sat项目）的支持。Giulio Del Zanna感谢英国科学与技术设施委员会（Science and Technology Facilities Council, STFC）通过剑桥大学DAMTP原子天体物理组（AAG）的综合研究拨款（ST/P000665/1与ST/T000481/1）提供的资助。Seth G. Claudepierre感谢NASA拨款编号NNX17AF10G，以及由约翰·霍普金斯大学应用物理实验室（JHU/APL）依据NASA主合同NAS5-01072签订的合同967399提供的RBSP-ECT项目资助。