Stereoscopic measurements of coronal Doppler velocities

• Autores: Podladchikova, O.; Harra, L.; Barczynski, K.; Mandrini, Cristina Hemilse; Auchère, F.; Berghmans, D.; Buchlin, É.; Dolla, L.; Mierla, M.; Parenti, S.; Rodriguez, L.
• Año de publicación: 2021
• Idioma: inglés
• Tipo de recurso: artículo
• Materia: INSTRUMENTATION: HIGH ANGULAR RESOLUTION; INSTRUMENTATION: SPECTROGRAPHS; SUN: CORONA; SUN: HELIOSPHERE; SUN: UV RADIATION; TECHNIQUES: IMAGING SPECTROSCOPY
• Institución: Consejo Nacional de Investigaciones Científicas y Técnicas

Context. The Solar Orbiter mission, with an orbit outside the Sun-Earth line and leaving the ecliptic plane, opens up opportunities for the combined analysis of measurements obtained by solar imagers and spectrometers. For the first time different space spectrometers will be located at wide angles to each other, allowing three-dimensional (3D) spectroscopy of the solar atmosphere. Aims. The aim of this work is to prepare a methodology to facilitate the reconstruction of 3D vector velocities from two stereoscopic line of sight (LOS) Doppler velocity measurements using the Spectral Imaging of the Coronal Environment (SPICE) on board the Solar Orbiter and the near-Earth spectrometers, while widely separated in space. Methods. We developed the methodology using the libraries designed earlier for the STEREO mission, but applied to spectroscopic data from the Hinode mission and the Solar Dynamics Observatory. We used well-known methods of static and dynamic solar rotation stereoscopy and the methods of extreme ultraviolet (EUV) stereoscopic triangulation for optically thin coronal EUV plasma emissions. We developed new algorithms using analytical geometry in space to determine the 3D velocity in coronal loops. Results. We demonstrate our approach with the reconstruction of 3D velocity vectors in plasma flows along 'open' and 'closed' magnetic loops. This technique will be applied to an actual situation of two spacecraft at different separations with spectrometers on board during the Solar Orbiter nominal phase: SPICE versus the Interface Region Imaging Spectrograph (IRIS) and Hinode imaging spectrometer. We summarise how these observations can be coordinated.
Fil: Podladchikova, O.. No especifíca;
Fil: Harra, L.. No especifíca;
Fil: Barczynski, K.. No especifíca;
Fil: Mandrini, Cristina Hemilse. Consejo Nacional de Investigaciones 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
Fil: Auchère, F.. Centre National de la Recherche Scientifique; Francia
Fil: Berghmans, D.. Royal Observatory of Belgium; Bélgica
Fil: Buchlin, É.. Centre National de la Recherche Scientifique; Francia
Fil: Dolla, L.. Royal Observatory of Belgium; Bélgica
Fil: Mierla, M.. Royal Observatory of Belgium; Bélgica
Fil: Parenti, S.. Royal Observatory of Belgium; Bélgica
Fil: Rodriguez, L.. Institute of Geodynamics of the Romanian Academy; Rumania