Background removal from global auroral images:Data-driven dayglow modeling

作     者：A.Ohma M.Madelaire K.M.Laundal J.P.Reistad S.M.Hatch S.Gasparini S.J.Walker A.Ohma;M.Madelaire;K.M.Laundal;J.P.Reistad;S.M.Hatch;S.Gasparini;S.J.Walker

作者机构：Birkeland Centre for Space ScienceDepartment of Physics and TechnologyUniversity of BergenBergenNorway 

出 版 物：《Earth and Planetary Physics》 (地球与行星物理（英文版）)

年 卷 期：2024年第8卷第1期

页      面：247-257页

核心收录：

学科分类：07[理学] 070802[理学-空间物理学] 0708[理学-地球物理学] 

基　　金：supported by the Research Council of Norway under contracts 223252/F50 and 300844/F50 the Trond Mohn Foundation。 

主　　题：aurora dayglow modeling global auroral images far ultraviolet images dayglow removal 

摘      要：Global images of auroras obtained by cameras on spacecraft are a key tool for studying the near-Earth environment.However,the cameras are sensitive not only to auroral emissions produced by precipitating particles,but also to dayglow emissions produced by photoelectrons induced by sunlight.Nightglow emissions and scattered sunlight can contribute to the background signal.To fully utilize such images in space science,background contamination must be removed to isolate the auroral signal.Here we outline a data-driven approach to modeling the background intensity in multiple images by formulating linear inverse problems based on B-splines and spherical harmonics.The approach is robust,flexible,and iteratively deselects outliers,such as auroral emissions.The final model is smooth across the terminator and accounts for slow temporal variations and large-scale asymmetries in the dayglow.We demonstrate the model by using the three far ultraviolet cameras on the Imager for Magnetopause-to-Aurora Global Exploration(IMAGE)mission.The method can be applied to historical missions and is relevant for upcoming missions,such as the Solar wind Magnetosphere Ionosphere Link Explorer(SMILE)mission.