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dc.provenanceCONICET-
dc.creatorFrazin, Richard A.-
dc.creatorVasquez, Alberto Marcos-
dc.creatorKamalabadi, Farzad-
dc.date2017-07-14T17:15:12Z-
dc.date2017-07-14T17:15:12Z-
dc.date2009-08-10-
dc.date2017-07-14T14:08:27Z-
dc.date.accessioned2019-04-29T15:45:01Z-
dc.date.available2019-04-29T15:45:01Z-
dc.date.issued2009-08-10-
dc.identifierFrazin, Richard A.; Vasquez, Alberto Marcos; Kamalabadi, Farzad; Quantitative, three dimensional Analysis of the Global Corona with Multi-Spacecraft Differential Emission Measure Tomography; IOP Publishing; Astrophysical Journal; 701; 1; 10-8-2009; 547-560-
dc.identifier0004-637X-
dc.identifierhttp://hdl.handle.net/11336/20574-
dc.identifierCONICET Digital-
dc.identifierCONICET-
dc.identifier.urihttp://rodna.bn.gov.ar:8080/jspui/handle/bnmm/301055-
dc.descriptionA previous paper (Frazin et al.~2005, ApJ, 628, 1070) introduced the concept of differential emission measure tomography (DEMT), which is a three-dimensional (3D) extension of the classical differential emission measure technique for determining the distribution of temperatures in a volume of plasma.  The information for the reconstruction in the three spatial dimensions is provided by solar rotation and/or multi-spacecraft views.  This paper describes, quantitatively,  the procedure for implementing DEMT with data from NASA´s STEREO/EUVI instrument, including the radiometry, line-of-sight geometry, and image preparation steps.  An example of a quantitative, multi-band, 3D reconstruction and local differential emission measure curves are given, and  it is demonstrated that, when applicable, DEMT is simple 3D analysis tool that obviates the need for structure specific modeling.-
dc.descriptionFil: Frazin, Richard A.. University of Michigan; Estados Unidos-
dc.descriptionFil: Vasquez, Alberto Marcos. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina-
dc.descriptionFil: Kamalabadi, Farzad. University of Illinois; Estados Unidos-
dc.formatapplication/pdf-
dc.formatapplication/pdf-
dc.languageeng-
dc.publisherIOP Publishing-
dc.relationinfo:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1088/0004-637X/701/1/547-
dc.relationinfo:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/article/10.1088/0004-637X/701/1/547/meta-
dc.rightsinfo:eu-repo/semantics/restrictedAccess-
dc.rightshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/-
dc.sourcereponame:CONICET Digital (CONICET)-
dc.sourceinstname:Consejo Nacional de Investigaciones Científicas y Técnicas-
dc.sourceinstacron:CONICET-
dc.source.urihttp://hdl.handle.net/11336/20574-
dc.subjectSol: Corona-
dc.subjectSol: Tomografía-
dc.subjectAstronomía-
dc.subjectCiencias Físicas-
dc.subjectCIENCIAS NATURALES Y EXACTAS-
dc.titleQuantitative, three dimensional Analysis of the Global Corona with Multi-Spacecraft Differential Emission Measure Tomography-
dc.typeinfo:eu-repo/semantics/article-
dc.typeinfo:eu-repo/semantics/publishedVersion-
dc.typeinfo:ar-repo/semantics/articulo-
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