2026-10-12T16:08:40Z https://www.scidb.cn/oai

10.57760/sciencedb.space.00641 2023-04-18T17:12:40Z

2023-04-18 Analysis data set of XMM-Newton European Photon Imaging Camera (EPIC) during the period of sudden change in solar wind proton flux doi:10.57760/sciencedb.space.00641 en 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. XMM-Newton; solar wind charge exchange; soft X-ray Yingjie Zhang Tianran Sun Jennifer. A. Carter Steve Sembay Dimitra Koutroumpa Li Ji Wenhao Liu Chi Wang PUBLIC https://creativecommons.org/licenses/by/4.0/ dataset http://www.doi.org/10.3847/1538-4357/acc326 Science Data Bank