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

B. V. Jackson, P. P. Hick, A. Buffington, M. M. Bisi, J. M. Clover, M. Tokumaru, M. Kojima, K. Fujiki

Allbwn ymchwil: Cyfraniad at gyfnodolynErthygladolygiad gan gymheiriaid

51 Dyfyniadau(SciVal)


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 and heliospheric structure. Data from STEREO are proceeded by and contemporaneous with many other types of data and analysis techniques; most of the latter have provided 3-D information by relying on remote-sensing information beyond those of the near corona (outside 10 RS). These include combinations of past data from the Helios spacecraft and the Solwind coronagraphs and, continuing from the past to the present, from observations of interplanetary scintillation (IPS) and the Solar Mass Ejection Imager (SMEI) instrument. In this article we review past and ongoing analyses that have led to a current great wealth of 3-D information. When properly utilized, these analyses can provide not only shapes of CME/ICMEs but also a characterization of any solar wind structure or global outflow.
Iaith wreiddiolSaesneg
Tudalennau (o-i)1214-1227
Nifer y tudalennau14
CyfnodolynJournal of Atmospheric and Solar-Terrestrial Physics
Rhif cyhoeddi10
Dynodwyr Gwrthrych Digidol (DOIs)
StatwsCyhoeddwyd - 20 Meh 2011

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