Three-dimensional reconstruction of heliospheric structure using iterative tomography: A review

摘要: Abstract Current perspective and in-situ analyses using data from NASA’s twin Solar TErrestrial RElations Observatory (STEREO) spacecraft have focused studies on ways to provide three-dimensional (3-D) reconstructions of coronal heliospheric structure. Data STEREO are proceeded by contemporaneous with many other types analysis techniques; most the latter provided 3-D information relying remote-sensing beyond those near corona (outside 10 RS). These include combinations past Helios Solwind coronagraphs and, continuing present, observations interplanetary scintillation (IPS) Mass Ejection Imager (SMEI) instrument. In this article we review ongoing that led a current great wealth information. When properly utilized, these can not only shapes CME/ICMEs but also characterization any solar wind structure or global outflow.