Analysis data set of XMM-Newton European Photon Imaging Camera (EPIC) during the period of sudden change in solar wind proton flux
收藏科学数据银行2023-04-18 更新2026-04-23 收录
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资源简介：
The sudden change in solar wind proton flux was defined as: (1) the ratio of high-flux to low-flux ≥ 1.5, (2) the duration of high-flux ≥ 1 hour.XMM-Newton's line of sight passed through the sun-side magnetosheath.XMM-Newton original data files were acquired from the XMM-Newton science archive. The Science Analysis System (SAS) software (version 20.0.0) and the Current Calibration Files (CCFs) released on September 20, 2021, were used for the XMM-Newton data analysis.
提供机构：
College of Earth and Planetary Sciences, The University of Chinese Academy of Sciences, Beijing, China; State Key Laboratory of Space Weather, National Space Science Center, Chinese Academy of Sciences, Beijing, China; LATMOS/IPSL, CNRS, UVSQ Université Paris-Saclay, Sorbonne Université, Guyancourt, France; Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing, China; Yingjie Zhang; Wenhao Liu; Tianran Sun; School of Physics and Astronomy, The University of Leicester, Leicester, UK; Jennifer. A. Carter
创建时间：
2023-04-18
