dc.creatorSalas-Matamoros,Carolina
dc.creatorSánchez-Guevara,Jesús
dc.date2023-12-01
dc.date.accessioned2023-09-25T14:37:30Z
dc.date.available2023-09-25T14:37:30Z
dc.identifierhttp://www.scielo.sa.cr/scielo.php?script=sci_arttext&pid=S1409-24332023000200215
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/8823349
dc.descriptionAbstract In space weather, to study the impact of Earth-directed coronal mass ejections (CME) in our terrestrial environment, one of the most important parameters is the propagation speed of these disturbances. We present an improvement of the 3D CME Geometrical Propagation-Expansion Description (3D-CGPED) model developed in previous work to increase the simple that we can use in CME arrival time predictions. This 3D model estimates the arrival time of Earth-directed CMEs at Earth by including a 3D geometry for the CME propagation and expansion in interplanetary space. Since the 3D-CGPED model computes the expansion of the CME based on the radial distance of the CME front, only travel times for CMEs with welldefined shapes seen by coronographs can be estimated. In the present work, we found an empirical relationship between the expansion angle of CMEs with well-defined shapes and the start-to-peak SXR fluence of their associated flares. We applied this relationship in the 3D-CGPED model to obtain the expansion angle for 8 CMEs with an irregular shape. We found similar window errors in arrival time predictions compared to the previous work. This result allows us to complement the 3D-CGPED model to include not only regular shapes but also irregular ones for CMEs observed by coronographs in future works.
dc.formattext/html
dc.languageen
dc.publisherCentro de Investigaciones en Matemática Pura y Aplicada (CIMPA) y Escuela de Matemática, San José, Costa Rica.
dc.relation10.15517/rmta.v30i2.50449
dc.rightsinfo:eu-repo/semantics/openAccess
dc.sourceRevista de Matemática Teoría y Aplicaciones v.30 n.2 2023
dc.subjectsun
dc.subjectcoronal mass ejections
dc.subjectCME's
dc.subjectsolar flare
dc.subjectradio waves.
dc.titleOn the relationship between expansión angle of earth-directed CMES and soft X-ray emission from their related flare
dc.typeinfo:eu-repo/semantics/article


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