Seeing the solar corona in three dimensions

The large availability and rich spectral coverage of today's observational data of the solar corona, and the high spatial and temporal resolution provided by many instruments, has enabled the evolution of three-dimensional (3D) physical models to a great level of detail. However, the 3D informa...

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Autor principal:	Vasquez, Alberto Marcos
Publicado:	2016
Materias:	Corona EUV Tomography Stereo image processing Stereo vision Development and applications Differential emission measures Observational data Spatial and temporal resolutions Technical aspects Threedimensional (3-d) Solar radiation
Acceso en línea:	https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_02731177_v57_n6_p1286_Vasquez http://hdl.handle.net/20.500.12110/paper_02731177_v57_n6_p1286_Vasquez
Aporte de:	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

id	paper:paper_02731177_v57_n6_p1286_Vasquez
record_format	dspace
spelling	paper:paper_02731177_v57_n6_p1286_Vasquez2023-06-08T15:25:44Z Seeing the solar corona in three dimensions Vasquez, Alberto Marcos Corona EUV Tomography Stereo image processing Stereo vision Tomography Corona Development and applications Differential emission measures EUV Observational data Spatial and temporal resolutions Technical aspects Threedimensional (3-d) Solar radiation The large availability and rich spectral coverage of today's observational data of the solar corona, and the high spatial and temporal resolution provided by many instruments, has enabled the evolution of three-dimensional (3D) physical models to a great level of detail. However, the 3D information provided by the data is rather limited as every instrument observes from a single angle of vision, or two at the most in the case of the STEREO mission. Two powerful available observational techniques to infer detailed 3D information of the solar corona from empirical data are stereoscopy and tomography. In particular, the technique known as differential emission measure tomography (DEMT) allows determination of the 3D distribution of the coronal electron density and temperature in the inner corona. This paper summarizes the main technical aspects of DEMT, reviews all published work based on it, and comments on its future development and applications. © 2015 COSPAR. Published by Elsevier Ltd. All rights reserved. Fil:Vásquez, A.M. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. 2016 https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_02731177_v57_n6_p1286_Vasquez http://hdl.handle.net/20.500.12110/paper_02731177_v57_n6_p1286_Vasquez
institution	Universidad de Buenos Aires
institution_str	I-28
repository_str	R-134
collection	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
topic	Corona EUV Tomography Stereo image processing Stereo vision Tomography Corona Development and applications Differential emission measures EUV Observational data Spatial and temporal resolutions Technical aspects Threedimensional (3-d) Solar radiation
spellingShingle	Corona EUV Tomography Stereo image processing Stereo vision Tomography Corona Development and applications Differential emission measures EUV Observational data Spatial and temporal resolutions Technical aspects Threedimensional (3-d) Solar radiation Vasquez, Alberto Marcos Seeing the solar corona in three dimensions
topic_facet	Corona EUV Tomography Stereo image processing Stereo vision Tomography Corona Development and applications Differential emission measures EUV Observational data Spatial and temporal resolutions Technical aspects Threedimensional (3-d) Solar radiation
description	The large availability and rich spectral coverage of today's observational data of the solar corona, and the high spatial and temporal resolution provided by many instruments, has enabled the evolution of three-dimensional (3D) physical models to a great level of detail. However, the 3D information provided by the data is rather limited as every instrument observes from a single angle of vision, or two at the most in the case of the STEREO mission. Two powerful available observational techniques to infer detailed 3D information of the solar corona from empirical data are stereoscopy and tomography. In particular, the technique known as differential emission measure tomography (DEMT) allows determination of the 3D distribution of the coronal electron density and temperature in the inner corona. This paper summarizes the main technical aspects of DEMT, reviews all published work based on it, and comments on its future development and applications. © 2015 COSPAR. Published by Elsevier Ltd. All rights reserved.
author	Vasquez, Alberto Marcos
author_facet	Vasquez, Alberto Marcos
author_sort	Vasquez, Alberto Marcos
title	Seeing the solar corona in three dimensions
title_short	Seeing the solar corona in three dimensions
title_full	Seeing the solar corona in three dimensions
title_fullStr	Seeing the solar corona in three dimensions
title_full_unstemmed	Seeing the solar corona in three dimensions
title_sort	seeing the solar corona in three dimensions
publishDate	2016
url	https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_02731177_v57_n6_p1286_Vasquez http://hdl.handle.net/20.500.12110/paper_02731177_v57_n6_p1286_Vasquez
work_keys_str_mv	AT vasquezalbertomarcos seeingthesolarcoronainthreedimensions
_version_	1768543798100492288

Seeing the solar corona in three dimensions

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