Dynamics of the cold solar chromosphere observed with ALMA

ilustraciones, diagramas

Autores:
Ordoñez Araujo, Francisco Javier
Tipo de recurso:
Fecha de publicación:
2024
Institución:
Universidad Nacional de Colombia
Repositorio:
Universidad Nacional de Colombia
Idioma:
eng
OAI Identifier:
oai:repositorio.unal.edu.co:unal/85838
Acceso en línea:
https://repositorio.unal.edu.co/handle/unal/85838
https://repositorio.unal.edu.co/
Palabra clave:
Shock waves
Wave propagation
Solar chromosphere
Formation height
Solar image alignment
Ondas de choque
Propagación de ondas
Cromosfera solar
Altura de formación
Alineación de imágenes solares
Actividad solar
Astrofísica
Ciencias del espacio
Solar activity
Astrophysics
Space sciences
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openAccess
License
Atribución-NoComercial 4.0 Internacional
id UNACIONAL2_432f279b5a18ecbf7282c31ea8b527ea
oai_identifier_str oai:repositorio.unal.edu.co:unal/85838
network_acronym_str UNACIONAL2
network_name_str Universidad Nacional de Colombia
repository_id_str
dc.title.eng.fl_str_mv Dynamics of the cold solar chromosphere observed with ALMA
dc.title.translated.spa.fl_str_mv Dinámica de la cromosfera solar fría observada con ALMA
title Dynamics of the cold solar chromosphere observed with ALMA
spellingShingle Dynamics of the cold solar chromosphere observed with ALMA
Shock waves
Wave propagation
Solar chromosphere
Formation height
Solar image alignment
Ondas de choque
Propagación de ondas
Cromosfera solar
Altura de formación
Alineación de imágenes solares
Actividad solar
Astrofísica
Ciencias del espacio
Solar activity
Astrophysics
Space sciences
title_short Dynamics of the cold solar chromosphere observed with ALMA
title_full Dynamics of the cold solar chromosphere observed with ALMA
title_fullStr Dynamics of the cold solar chromosphere observed with ALMA
title_full_unstemmed Dynamics of the cold solar chromosphere observed with ALMA
title_sort Dynamics of the cold solar chromosphere observed with ALMA
dc.creator.fl_str_mv Ordoñez Araujo, Francisco Javier
dc.contributor.advisor.spa.fl_str_mv Calvo Mozo, Benjamín
dc.contributor.author.spa.fl_str_mv Ordoñez Araujo, Francisco Javier
dc.contributor.referee.spa.fl_str_mv Jafarzadeh, Shahin
Pinzon Estrada, Giovanni
Larrañaga, Eduard
dc.contributor.researchgroup.spa.fl_str_mv Grupo de Astronomía, Astrofísica y Cosmología, línea de Astrofísica Solar, GoSA
dc.contributor.supervisor.spa.fl_str_mv Guevara Gómez, Juan Camilo
dc.contributor.orcid.spa.fl_str_mv Ordoñez Araujo, Francisco Javier [https://orcid.org/0000-0002-7329-4877]
dc.contributor.googlescholar.spa.fl_str_mv Francisco Javier Ordonez Araujo [https://scholar.google.com/citations?user=mxqYk8gAAAAJ&hl=en&authuser=1]
dc.subject.proposal.eng.fl_str_mv Shock waves
Wave propagation
Solar chromosphere
Formation height
Solar image alignment
topic Shock waves
Wave propagation
Solar chromosphere
Formation height
Solar image alignment
Ondas de choque
Propagación de ondas
Cromosfera solar
Altura de formación
Alineación de imágenes solares
Actividad solar
Astrofísica
Ciencias del espacio
Solar activity
Astrophysics
Space sciences
dc.subject.proposal.spa.fl_str_mv Ondas de choque
Propagación de ondas
Cromosfera solar
Altura de formación
Alineación de imágenes solares
dc.subject.unesco.spa.fl_str_mv Actividad solar
Astrofísica
Ciencias del espacio
dc.subject.unesco.eng.fl_str_mv Solar activity
Astrophysics
Space sciences
description ilustraciones, diagramas
publishDate 2024
dc.date.accessioned.none.fl_str_mv 2024-04-02T01:16:53Z
dc.date.available.none.fl_str_mv 2024-04-02T01:16:53Z
dc.date.issued.none.fl_str_mv 2024-04-01
dc.type.spa.fl_str_mv Trabajo de grado - Maestría
dc.type.driver.spa.fl_str_mv info:eu-repo/semantics/masterThesis
dc.type.version.spa.fl_str_mv info:eu-repo/semantics/acceptedVersion
dc.type.content.spa.fl_str_mv Text
dc.type.redcol.spa.fl_str_mv http://purl.org/redcol/resource_type/TM
status_str acceptedVersion
dc.identifier.uri.none.fl_str_mv https://repositorio.unal.edu.co/handle/unal/85838
dc.identifier.instname.spa.fl_str_mv Universidad Nacional de Colombia
dc.identifier.reponame.spa.fl_str_mv Repositorio Institucional Universidad Nacional de Colombia
dc.identifier.repourl.spa.fl_str_mv https://repositorio.unal.edu.co/
url https://repositorio.unal.edu.co/handle/unal/85838
https://repositorio.unal.edu.co/
identifier_str_mv Universidad Nacional de Colombia
Repositorio Institucional Universidad Nacional de Colombia
dc.language.iso.spa.fl_str_mv eng
language eng
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spelling Atribución-NoComercial 4.0 Internacionalhttp://creativecommons.org/licenses/by-nc/4.0/info:eu-repo/semantics/openAccesshttp://purl.org/coar/access_right/c_abf2Calvo Mozo, Benjamínbddc9d59240df52d624f2ac364ea0804Ordoñez Araujo, Francisco Javier0cde03c608edd6467d8bec99ab895137600Jafarzadeh, ShahinPinzon Estrada, GiovanniLarrañaga, EduardGrupo de Astronomía, Astrofísica y Cosmología, línea de Astrofísica Solar, GoSAGuevara Gómez, Juan CamiloOrdoñez Araujo, Francisco Javier [https://orcid.org/0000-0002-7329-4877]Francisco Javier Ordonez Araujo [https://scholar.google.com/citations?user=mxqYk8gAAAAJ&hl=en&authuser=1]2024-04-02T01:16:53Z2024-04-02T01:16:53Z2024-04-01https://repositorio.unal.edu.co/handle/unal/85838Universidad Nacional de ColombiaRepositorio Institucional Universidad Nacional de Colombiahttps://repositorio.unal.edu.co/ilustraciones, diagramasIn this thesis, a dynamic study of cold regions of the solar chromosphere observed by the Atacama Large Millimeter/submillimeter Array (ALMA) in band 3 is presented. The analysis integrates data from the Solar Dynamics Observatory (SDO) and the Interface Region Imaging Spectrograph (IRIS), focusing specifically on the quiet sun region D06 from the Solar ALMA Science Archive (SALSA) database. In the data processing before the study carried out in the thesis, an alignment method was developed based on the helioprojective coordinates of the SDO, using the Pearson Correlation Coefficient and the Structural Similarity Index to estimate images correlation. The analysis revealed that the cold structures detected in ALMA band 3 are mainly located in internetwork areas, which are characterized by having a weak vertical magnetic field. A total of 44 cold events in ALMA were identified. Through the use of time-distance diagrams in a 6×6 arcsec window, periodic increases and decreases in the temperature were observed. This fluctuation pattern was also observed in IRIS 2796 Å and AIA 1600 Å time-distance diagrams. In these observations, the IRIS 2796 Å and ALMA band 3 data exhibited temporal delays of 20.4 and 100.2 seconds compared to AIA 1600 Å. This suggests the propagation of shock waves from the upper convective zone to chromospheric heights. Using a shock wave speed of 8.0 ± 1.0 km/s and a formation height of 430 ± 185 km for AIA 1600 Å, formation heights of 597 ± 194 km, 1231 ± 230 km for IRIS 2796 Å and ALMA band 3 were estimated. These results are in accordance with formation heights estimated in 3D simulations. Additionally, the distribution of pixels within the cold events corroborated that they are mainly confined to internetwork regions, with typical sizes close to photospheric granulations, suggesting a relationship between the generation of shock waves in intergranular regions and their propagation to upper layers. The distribution of the lifetimes of the events indicated that shock waves pass through the chromosphere approximately every 3 minutes. On the other hand, by measuring the displacement of the center of mass between consecutive frames, we estimated the speed of dark features. Our analysis revealed that the speed distribution peaked at 8.5 km/s, with an average speed of 21 km/s. These speed values were observed in simulations of the propagation of shock waves at chromospheric heights, reinforcing the hypothesis that indeed the dark regions are post-shock regions. This study not only contributes to the understanding of the thermal dynamics of the solar chromosphere but also provides valuable information for future research and the refinement of numerical models in solar astrophysics. However, more detailed statistical analyses are required for a deeper understanding.En esta tesis, se presenta un estudio dinámico de las regiones frías de la cromosfera solar observadas por el Atacama Large Millimeter/submillimeter Array (ALMA) en la banda 3. El análisis integra datos del Solar Dynamics Observatory (SDO) y del Interface Region Imaging Spectrograph (IRIS), enfocándose específicamente en la región del sol tranquilo D06 del Solar ALMA Science Archive (SALSA). En el procesamiento de datos antes del estudio realizado en la tesis, se desarrolló un método de alineación basado en las coordenadas helioproyectivas del SDO, utilizando el Coeficiente de Correlación de Pearson y el Índice de Similitud Estructural para estimar la correlación de las imágenes. El análisis reveló que las estructuras frías detectadas en la banda 3 de ALMA están principalmente ubicadas en áreas de internetwork, las cuales se caracterizan por tener un campo magnético vertical débil. Se identificaron un total de 44 eventos fríos en ALMA. Mediante el uso de diagramas de tiempo-distancia en una ventana de 6×6 arcsec, se observaron aumentos y disminuciones periódicas en la temperatura. Este patrón de fluctuación también se observó en los diagramas de tiempo-distancia de IRIS 2796 Å y AIA 1600 Å. En estas observaciones, los datos de IRIS 2796 Å y ALMA banda 3 exhibieron retrasos temporales de 20.4 y 100.2 segundos comparados con AIA 1600 Å. Esto sugiere la propagación de ondas de choque desde la zona convectiva superior hacia alturas cromosféricas. Utilizando una velocidad de onda de choque de 8.0 ± 1.0 km/s y una altura de formación de 430 ± 185 km para AIA 1600 Å, se estimaron alturas de formación de 597 ± 194 km, 1231 ± 230 km para IRIS 2796 Å y ALMA banda 3. Estos resultados están en acuerdo con las alturas de formación estimadas en simulaciones 3D. Adicionalmente, la distribución de píxeles dentro de los eventos fríos corroboró que están principalmente confinados a regiones de internetwork, con tamaños típicos cercanos a las granulaciones fotosféricas, sugiriendo una relación entre la generación de ondas de choque en regiones intergranulares y su propagación a capas superiores. La distribución de las duraciones de los eventos indicó que las ondas de choque pasan por la cromosfera aproximadamente cada 3 minutos. Por otro lado, al medir el desplazamiento del centro de masa entre cuadros consecutivos, estimamos la velocidad de las características oscuras. Nuestro análisis reveló que la distribución de la velocidad alcanzó un pico de 8.5 km/s, con una velocidad promedio de 21 km/s. Estos valores de velocidad se observaron en simulaciones de la propagación de ondas de choque en alturas cromosféricas, reforzando la hipótesis de que, de hecho, las regiones oscuras son regiones post-choque. Este estudio no solo contribuye a la comprensión de la dinámica térmica de la cromosfera solar, sino que también proporciona información valiosa para investigaciones futuras y el refinamiento de modelos numéricos en astrofísica solar. Sin embargo, se requieren análisis estadísticos más detallados para una comprensión más profunda. (Texto tomado de la fuente).MaestríaMagíster en Ciencias - AstronomíaFísica solarxxiv, 79 páginasapplication/pdfengUniversidad Nacional de ColombiaBogotá - Ciencias - Maestría en Ciencias - AstronomíaFacultad de CienciasBogotá, ColombiaUniversidad Nacional de Colombia - Sede BogotáDynamics of the cold solar chromosphere observed with ALMADinámica de la cromosfera solar fría observada con ALMATrabajo de grado - Maestríainfo:eu-repo/semantics/masterThesisinfo:eu-repo/semantics/acceptedVersionTexthttp://purl.org/redcol/resource_type/TMD. G. Altman and J. M. Bland. Standard deviations and standard errors. 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Provided by the SAO/NASA Astrophysics Data SystemShock wavesWave propagationSolar chromosphereFormation heightSolar image alignmentOndas de choquePropagación de ondasCromosfera solarAltura de formaciónAlineación de imágenes solaresActividad solarAstrofísicaCiencias del espacioSolar activityAstrophysicsSpace sciencesEstudiantesInvestigadoresMaestrosPúblico generalORIGINALfranciscoordonezaraujo.2024.pdffranciscoordonezaraujo.2024.pdfTesis de Maestría en Ciencias - Astronomíaapplication/pdf55457666https://repositorio.unal.edu.co/bitstream/unal/85838/4/franciscoordonezaraujo.2024.pdf911e9211abda2589a1b9bf8b393fc0d9MD54LICENSElicense.txtlicense.txttext/plain; charset=utf-85879https://repositorio.unal.edu.co/bitstream/unal/85838/5/license.txteb34b1cf90b7e1103fc9dfd26be24b4aMD55THUMBNAILfranciscoordonezaraujo.2024.pdf.jpgfranciscoordonezaraujo.2024.pdf.jpgGenerated 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