SunspotCalc: Una aplicación basada en Web y Python para calcular la rotación diferencial del sol y su fotosfera
En este manuscrito presentamos una aplicación web con soporte en lenguaje de programación PYTHON, REACTJS y JAVASCRIPT, libre y abierta, para el desarrollo de una actividad de enseñanza-aprendizaje de la astronomía, específicamente para el cálculo de la rotación diferencial del Sol para estudiantes...
- Autores:
-
Sierra Porta, David
Herrera Acevedo, Daniel
Tarazona-Alvarado, Miguel
Hernández Díaz, Yaleidys
- Tipo de recurso:
- Fecha de publicación:
- 2023
- Institución:
- Universidad Tecnológica de Bolívar
- Repositorio:
- Repositorio Institucional UTB
- Idioma:
- spa
- OAI Identifier:
- oai:repositorio.utb.edu.co:20.500.12585/12483
- Acceso en línea:
- https://hdl.handle.net/20.500.12585/12483
- Palabra clave:
- Rotación diferencial del sol
Manchas solares
Divulgación científica
Ciencia de datos
Differential Sun’s rotation
Sunspots
Scientific outreach
Data science
LEMB
- Rights
- openAccess
- License
- http://creativecommons.org/publicdomain/zero/1.0/
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SunspotCalc: Una aplicación basada en Web y Python para calcular la rotación diferencial del sol y su fotosfera |
| title |
SunspotCalc: Una aplicación basada en Web y Python para calcular la rotación diferencial del sol y su fotosfera |
| spellingShingle |
SunspotCalc: Una aplicación basada en Web y Python para calcular la rotación diferencial del sol y su fotosfera Rotación diferencial del sol Manchas solares Divulgación científica Ciencia de datos Differential Sun’s rotation Sunspots Scientific outreach Data science LEMB |
| title_short |
SunspotCalc: Una aplicación basada en Web y Python para calcular la rotación diferencial del sol y su fotosfera |
| title_full |
SunspotCalc: Una aplicación basada en Web y Python para calcular la rotación diferencial del sol y su fotosfera |
| title_fullStr |
SunspotCalc: Una aplicación basada en Web y Python para calcular la rotación diferencial del sol y su fotosfera |
| title_full_unstemmed |
SunspotCalc: Una aplicación basada en Web y Python para calcular la rotación diferencial del sol y su fotosfera |
| title_sort |
SunspotCalc: Una aplicación basada en Web y Python para calcular la rotación diferencial del sol y su fotosfera |
| dc.creator.fl_str_mv |
Sierra Porta, David Herrera Acevedo, Daniel Tarazona-Alvarado, Miguel Hernández Díaz, Yaleidys |
| dc.contributor.author.none.fl_str_mv |
Sierra Porta, David Herrera Acevedo, Daniel Tarazona-Alvarado, Miguel Hernández Díaz, Yaleidys |
| dc.subject.keywords.spa.fl_str_mv |
Rotación diferencial del sol Manchas solares Divulgación científica Ciencia de datos Differential Sun’s rotation Sunspots Scientific outreach Data science |
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Rotación diferencial del sol Manchas solares Divulgación científica Ciencia de datos Differential Sun’s rotation Sunspots Scientific outreach Data science LEMB |
| dc.subject.armarc.none.fl_str_mv |
LEMB |
| description |
En este manuscrito presentamos una aplicación web con soporte en lenguaje de programación PYTHON, REACTJS y JAVASCRIPT, libre y abierta, para el desarrollo de una actividad de enseñanza-aprendizaje de la astronomía, específicamente para el cálculo de la rotación diferencial del Sol para estudiantes y publicó en general en edad escolar entre 10 y 18 años. El propósito fundamental es la de difundir el conocimiento del Sol y algunas de sus propiedades. La aplicación web es autocontenida y con suficiente guía y ayuda para que cualquiera pueda usarla, además de su dinamismo y diseño innovador, pretende presentar estrategias agradables para la enseñanza y aprendizaje de la ciencia en torno al Sol. |
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2023 |
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2023-09-12T12:05:57Z |
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2023-09-12T12:05:57Z |
| dc.date.issued.none.fl_str_mv |
2023-04-22 |
| dc.date.submitted.none.fl_str_mv |
2023-09-11 |
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http://purl.org/coar/version/c_b1a7d7d4d402bcce |
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http://purl.org/coar/resource_type/c_6501 |
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Porta, D. S., Acevedo, D. H., Tarazona-Alvarado, M., & Díaz, Y. H. (2023). SunspotCalc: Una aplicación basada en Web y Python para calcular la rotación diferencial del sol y su fotosfera. Revista Mexicana de Física E, 20(2 Jul-Dec), 020208-1. |
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https://hdl.handle.net/20.500.12585/12483 |
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10.31349/RevMexFis.20.020208 |
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Universidad Tecnológica de Bolívar |
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Repositorio Universidad Tecnológica de Bolívar |
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Porta, D. S., Acevedo, D. H., Tarazona-Alvarado, M., & Díaz, Y. H. (2023). SunspotCalc: Una aplicación basada en Web y Python para calcular la rotación diferencial del sol y su fotosfera. Revista Mexicana de Física E, 20(2 Jul-Dec), 020208-1. 10.31349/RevMexFis.20.020208 Universidad Tecnológica de Bolívar Repositorio Universidad Tecnológica de Bolívar |
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12 páginas |
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Sierra Porta, David62fe46fe-2160-4eac-8b0c-89e7fd6ce293Herrera Acevedo, Daniel2f2e14ba-6e9b-4697-a7f7-312414a61c76Tarazona-Alvarado, Miguelef024c8f-0c62-47e6-90e1-9de2e2566b23Hernández Díaz, Yaleidys40e1af31-e516-47da-8ab4-2e14add4bc25Colombia2023-09-12T12:05:57Z2023-09-12T12:05:57Z2023-04-222023-09-11Porta, D. S., Acevedo, D. H., Tarazona-Alvarado, M., & Díaz, Y. H. (2023). SunspotCalc: Una aplicación basada en Web y Python para calcular la rotación diferencial del sol y su fotosfera. Revista Mexicana de Física E, 20(2 Jul-Dec), 020208-1.https://hdl.handle.net/20.500.12585/1248310.31349/RevMexFis.20.020208Universidad Tecnológica de BolívarRepositorio Universidad Tecnológica de BolívarEn este manuscrito presentamos una aplicación web con soporte en lenguaje de programación PYTHON, REACTJS y JAVASCRIPT, libre y abierta, para el desarrollo de una actividad de enseñanza-aprendizaje de la astronomía, específicamente para el cálculo de la rotación diferencial del Sol para estudiantes y publicó en general en edad escolar entre 10 y 18 años. El propósito fundamental es la de difundir el conocimiento del Sol y algunas de sus propiedades. La aplicación web es autocontenida y con suficiente guía y ayuda para que cualquiera pueda usarla, además de su dinamismo y diseño innovador, pretende presentar estrategias agradables para la enseñanza y aprendizaje de la ciencia en torno al Sol.In this manuscript we present a web application with support in PYTHON, REACTJS and JAVASCRIPT programming language, free and open, for the development of a teaching-learning activity of astronomy, specifically for the calculation of the differential rotation of the Sun for students and general public in school age between 10 and 18 years old. The main purpose is to spread the knowledge of the Sun and some of its properties. The web application is self-contained and with enough guidance and help for anyone to use it, in addition to its dynamism and innovative design, it aims to present pleasant strategies for teaching and learning science around the Sun.12 páginasapplication/pdfspahttp://creativecommons.org/publicdomain/zero/1.0/info:eu-repo/semantics/openAccessCC0 1.0 Universalhttp://purl.org/coar/access_right/c_abf2Revista Mexicana de Física ESunspotCalc: Una aplicación basada en Web y Python para calcular la rotación diferencial del sol y su fotosferainfo:eu-repo/semantics/articleinfo:eu-repo/semantics/drafthttp://purl.org/coar/resource_type/c_6501http://purl.org/coar/version/c_b1a7d7d4d402bccehttp://purl.org/coar/resource_type/c_2df8fbb1Rotación diferencial del solManchas solaresDivulgación científicaCiencia de datosDifferential Sun’s rotationSunspotsScientific outreachData scienceLEMBCartagena de IndiasPúblico generalT. Wiegelmann, J. K. Thalmann, and S. K. Solanki, The magnetic field in the solar atmosphere, The Astronomy and Astrophysics Review 22 (2014) 1, https://doi.org/10.1007/ s00159-014-0078-7.M. Georgoulis et al., Solar magnetic helicity injected into the heliosphere: magnitude, balance, and periodicities over solar cycle 23, The Astrophysical Journal 705 (2009) L48, https: //doi.org/10.1088/0004-637X/705/1/L48. P. Demoulin and E. Pariat, Modelling and observations of ´ photospheric magnetic helicity, Advances in Space Research 43 (2009) 1013, https://doi.org/10.1016/j.asr. 2008.12.004.H. Moradi et al., Modeling the subsurface structure of sunspots, Solar Physics 267 (2010) 1, https://doi.org/10. 1007/s11207-010-9630-4.. J. H. Thomas and N. O. Weiss, The theory of sunspots, Sunspots: Theory and Observations (1992) 3, https://doi. org/10.1007/978-94-011-2769-1 1.. G. E. Hale, Solar vortices (contributions from the Mt. Wilson Solar Observatory, no. 26), Astrophysical Journal, 28 (1908) 100G. E. 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Sierra-Porta, Cross correlation and time-lag between cosmic ray intensity and solar activity during solar cycles 21, 22 and 23, Astrophysics and Space Science 363 (2018) 1, https: //doi.org/10.1007/s10509-018-3360-8D. Sierra-Porta, On the fractal properties of cosmic rays and Sun dynamics cross-correlations, Astrophysics and Space Science 367 (2022) 1, https://doi.org/10.1007/ s10509-022-04151-5.6. D. Sierra-Porta, M. Tarazona-Alvarado, and J. Villalba- Acebedo, Quantitatively relating cosmic rays intensities from solar activity parameters based on structural equation modeling, Advances in Space Research (2023), https://doi.org/10. 1016/j.asr.2023.02.044.I. Sammis, F. Tang, and H. Zirin, The dependence of large flare occurrence on the magnetic structure of sunspots, The Astrophysical Journal 540 (2000) 583, https://doi.org/ 10.1086/309303.J. M. Borrero and K. Ichimoto, Magnetic structure of sunspots, Living Reviews in Solar Physics 8 (2011) 1, https: //doi.org/10.12942/lrsp-2011-4.S. 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Immel, et al., The ionospheric connection explorer mission: Mission goals and design, Space Science Reviews 214 (2018) 1, https://doi.org/10.1007/ s11214-017-0449-2.R. Howard, P. Gilman, and P. Gilman, Rotation of the sun measured from Mount Wilson white-light images, The Astrophysical Journal 283 (1984) 373.E. Schroter, The solar differential rotation: present status of ob- ¨ servations, Solar Physics 100 (1985) 141.J. G. Beck, A comparison of differential rotation measurements-(Invited Review), Solar physics 191 (2000) 47, https://doi.org/10.1023/A:1005226402796P. Scherrer, J. Wilcox, and L. Svalgaard, Rotation of the sun: observations at Stanford, Astrophys. J.; (United States) 241 (1980)R. Howard, J. E. Boyden, and B. J. Labonte, Solar rotation measurements at Mount Wilson: I. Analysis and instrumental effects, Solar Physics 66 (1980) 167.R. K. Ulrich et al., Solar rotation measurements at MountWilson: V. Reanalysis of 21 years of data, Solar Physics 117 (1988) 291.. J. Beck, T. Duvall Jr, and P. Scherrer, Long-lived giant cells detected at the surface of the Sun, Nature 394 (1998) 653.R. Ulrich, Identification of very large scale velocity structures on the solar surface using Mt Wilson synoptic observations, In Structure and Dynamics of the Interior of the Sun and Sun-like Stars, 418 (1998) 851.. D. A. Lamb, Measurements of solar differential rotation and meridional circulation from tracking of photospheric magnetic features, The Astrophysical Journal 836 (2017) 10, https: //doi.org/10.3847/1538-4357/836/1/10.B. Shneiderman, Science 2.0, Science 319 (2008) 1349T. Bucheler and J. H. Sieg, Understanding science 2.0: Crowd- ¨ sourcing and open innovation in the scientific method, Procedia Computer Science 7 (2011) 327, https://doi.org/10. 1016/j.procs.2011.09.014.. R. Bonney et al., Can citizen science enhance public understanding of science?, Public understanding of science 25 (2016) 2, https://doi.org/10.1177/0963662515607406.J. P. Cohn, Citizen science: Can volunteers do real research?, BioScience 58 (2008) 192, https://doi.org/10.1641/ B580303.P. J. Marshall, C. J. Lintott, and L. N. Fletcher, Ideas for citizen science in astronomy, Annual Review of Astronomy and Astrophysics 53 (2015) 247.The SunPy Community et al., The SunPy Project: Open Source Development and Status of the Version 1.0 Core Package, The Astrophysical Journal 890 (2020) 68, https://doi.org/ 10.3847/1538-4357/ab4f7a.. J. Meeus, Astronomical algorithms, Richmond, VA:WillmannBell (1998).C. 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