Dataset for Sun dynamics from topological features
The present study presents an extensive dataset meticulously curated from solar images sourced from the Solar and Heliospheric Observatory (SOHO), encompassing a range of spectral bands. This collaborative effort spans multiple disciplines and culminates in a robust and automated methodology that tr...
- Autores:
-
Tarazona Alvarado, Miguel
Sierra Porta, David
- Tipo de recurso:
- Fecha de publicación:
- 2023
- Institución:
- Universidad Tecnológica de Bolívar
- Repositorio:
- Repositorio Institucional UTB
- Idioma:
- eng
- OAI Identifier:
- oai:repositorio.utb.edu.co:20.500.12585/12571
- Acceso en línea:
- https://hdl.handle.net/20.500.12585/12571
https://doi.org/10.1016/j.dib.2023.109728
- Palabra clave:
- Sun´s dynamics
Spectral features
Image processing
Space weather
LEMB
- Rights
- openAccess
- License
- http://creativecommons.org/publicdomain/zero/1.0/
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dc.title.spa.fl_str_mv |
Dataset for Sun dynamics from topological features |
title |
Dataset for Sun dynamics from topological features |
spellingShingle |
Dataset for Sun dynamics from topological features Sun´s dynamics Spectral features Image processing Space weather LEMB |
title_short |
Dataset for Sun dynamics from topological features |
title_full |
Dataset for Sun dynamics from topological features |
title_fullStr |
Dataset for Sun dynamics from topological features |
title_full_unstemmed |
Dataset for Sun dynamics from topological features |
title_sort |
Dataset for Sun dynamics from topological features |
dc.creator.fl_str_mv |
Tarazona Alvarado, Miguel Sierra Porta, David |
dc.contributor.author.none.fl_str_mv |
Tarazona Alvarado, Miguel Sierra Porta, David |
dc.subject.keywords.spa.fl_str_mv |
Sun´s dynamics Spectral features Image processing Space weather |
topic |
Sun´s dynamics Spectral features Image processing Space weather LEMB |
dc.subject.armarc.none.fl_str_mv |
LEMB |
description |
The present study presents an extensive dataset meticulously curated from solar images sourced from the Solar and Heliospheric Observatory (SOHO), encompassing a range of spectral bands. This collaborative effort spans multiple disciplines and culminates in a robust and automated methodology that traverses the entire spectrum from solar imaging to the computation of spectral parameters and relevant characteristics. The significance of this undertaking lies in the profound insights yielded by the dataset. Encompassing diverse spectral bands and employing topological features, the dataset captures the multifaceted dynamics of solar activity, fostering interdisciplinary correlations and analyses with other solar phenomena. Consequently, the data's intrinsic value is greatly enhanced, affording researchers in solar physics, space climatology, and related fields the means to unravel intricate processes. To achieve this, an open-source Python library script has been developed, consolidating three pivotal stages: image acquisition, image processing, and parameter calculation. Originally conceived as discrete modules, these steps have been unified into a single script, streamlining the entire process. Applying this script to various solar image types has generated multiple datasets, subsequently synthesized into a comprehensive compilation through a data mining procedures. During the image processing phase, conventional libraries like OpenCV and Python's image analysis tools were harnessed to refine images for analysis. In contrast, image acquisition utilized established URL libraries in Python, facilitating direct access to original SOHO repository images and eliminating the need for local storage. The computation of spectral parameters involved a fusion of standard Python libraries and tailored algorithms for specific attributes. This approach ensures precise computation of a diverse array of attributes crucial for comprehensive analysis of solar images. |
publishDate |
2023 |
dc.date.accessioned.none.fl_str_mv |
2023-11-28T20:34:49Z |
dc.date.available.none.fl_str_mv |
2023-11-28T20:34:49Z |
dc.date.issued.none.fl_str_mv |
2023-11-17 |
dc.date.submitted.none.fl_str_mv |
2023-11-27 |
dc.type.coarversion.fl_str_mv |
http://purl.org/coar/version/c_b1a7d7d4d402bcce |
dc.type.coar.fl_str_mv |
http://purl.org/coar/resource_type/c_2df8fbb1 |
dc.type.driver.spa.fl_str_mv |
info:eu-repo/semantics/article |
dc.type.hasversion.spa.fl_str_mv |
info:eu-repo/semantics/draft |
dc.type.spa.spa.fl_str_mv |
http://purl.org/coar/resource_type/c_6501 |
status_str |
draft |
dc.identifier.citation.spa.fl_str_mv |
M. Tarazona-Alvarado, D. Sierra-Porta, Dataset for Sun dynamics from topological features, Data in Brief, Volume 51, 2023, 109728, ISSN 2352-3409, https://doi.org/10.1016/j.dib.2023.109728. https://www.sciencedirect.com/science/article/pii/S2352340923007990 |
dc.identifier.uri.none.fl_str_mv |
https://hdl.handle.net/20.500.12585/12571 |
dc.identifier.doi.none.fl_str_mv |
https://doi.org/10.1016/j.dib.2023.109728 |
dc.identifier.instname.spa.fl_str_mv |
Universidad Tecnológica de Bolívar |
dc.identifier.reponame.spa.fl_str_mv |
Repositorio Universidad Tecnológica de Bolívar |
identifier_str_mv |
M. Tarazona-Alvarado, D. Sierra-Porta, Dataset for Sun dynamics from topological features, Data in Brief, Volume 51, 2023, 109728, ISSN 2352-3409, https://doi.org/10.1016/j.dib.2023.109728. https://www.sciencedirect.com/science/article/pii/S2352340923007990 Universidad Tecnológica de Bolívar Repositorio Universidad Tecnológica de Bolívar |
url |
https://hdl.handle.net/20.500.12585/12571 https://doi.org/10.1016/j.dib.2023.109728 |
dc.language.iso.spa.fl_str_mv |
eng |
language |
eng |
dc.rights.coar.fl_str_mv |
http://purl.org/coar/access_right/c_abf2 |
dc.rights.uri.*.fl_str_mv |
http://creativecommons.org/publicdomain/zero/1.0/ |
dc.rights.accessrights.spa.fl_str_mv |
info:eu-repo/semantics/openAccess |
dc.rights.cc.*.fl_str_mv |
CC0 1.0 Universal |
rights_invalid_str_mv |
http://creativecommons.org/publicdomain/zero/1.0/ CC0 1.0 Universal http://purl.org/coar/access_right/c_abf2 |
eu_rights_str_mv |
openAccess |
dc.format.extent.none.fl_str_mv |
6 paginas |
dc.format.mimetype.spa.fl_str_mv |
application/pdf |
dc.publisher.place.spa.fl_str_mv |
Cartagena de Indias |
dc.source.spa.fl_str_mv |
SciencieDirect |
institution |
Universidad Tecnológica de Bolívar |
bitstream.url.fl_str_mv |
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Tarazona Alvarado, Miguelef024c8f-0c62-47e6-90e1-9de2e2566b23Sierra Porta, David62fe46fe-2160-4eac-8b0c-89e7fd6ce2932023-11-28T20:34:49Z2023-11-28T20:34:49Z2023-11-172023-11-27M. Tarazona-Alvarado, D. Sierra-Porta, Dataset for Sun dynamics from topological features, Data in Brief, Volume 51, 2023, 109728, ISSN 2352-3409, https://doi.org/10.1016/j.dib.2023.109728. https://www.sciencedirect.com/science/article/pii/S2352340923007990https://hdl.handle.net/20.500.12585/12571https://doi.org/10.1016/j.dib.2023.109728Universidad Tecnológica de BolívarRepositorio Universidad Tecnológica de BolívarThe present study presents an extensive dataset meticulously curated from solar images sourced from the Solar and Heliospheric Observatory (SOHO), encompassing a range of spectral bands. This collaborative effort spans multiple disciplines and culminates in a robust and automated methodology that traverses the entire spectrum from solar imaging to the computation of spectral parameters and relevant characteristics. The significance of this undertaking lies in the profound insights yielded by the dataset. Encompassing diverse spectral bands and employing topological features, the dataset captures the multifaceted dynamics of solar activity, fostering interdisciplinary correlations and analyses with other solar phenomena. Consequently, the data's intrinsic value is greatly enhanced, affording researchers in solar physics, space climatology, and related fields the means to unravel intricate processes. To achieve this, an open-source Python library script has been developed, consolidating three pivotal stages: image acquisition, image processing, and parameter calculation. Originally conceived as discrete modules, these steps have been unified into a single script, streamlining the entire process. Applying this script to various solar image types has generated multiple datasets, subsequently synthesized into a comprehensive compilation through a data mining procedures. During the image processing phase, conventional libraries like OpenCV and Python's image analysis tools were harnessed to refine images for analysis. In contrast, image acquisition utilized established URL libraries in Python, facilitating direct access to original SOHO repository images and eliminating the need for local storage. The computation of spectral parameters involved a fusion of standard Python libraries and tailored algorithms for specific attributes. This approach ensures precise computation of a diverse array of attributes crucial for comprehensive analysis of solar images.6 paginasapplication/pdfenghttp://creativecommons.org/publicdomain/zero/1.0/info:eu-repo/semantics/openAccessCC0 1.0 Universalhttp://purl.org/coar/access_right/c_abf2SciencieDirectDataset for Sun dynamics from topological featuresinfo: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_2df8fbb1Sun´s dynamicsSpectral featuresImage processingSpace weatherLEMBCartagena de IndiasPúblico generalV Domingo, Bernhard Fleck, and AI Poland. Soho: the solar and heliospheric observatory. Space Science Reviews, 72:81–84, 1995.Jørgen Schou, Philip H Scherrer, Rock Irvin Bush, Richard Wachter, Savita Couvidat, Maria Cristina Rabello-Soares, RS Bogart, JT Hoeksema, Y Liu, TL Duvall, et al. Design and ground calibration of the helioseismic and magnetic imager (hmi) instrument on the solar dynamics observatory (sdo). Solar Physics, 275:229–259, 2012Philip Hanby Scherrer, Jesper Schou, RI Bush, AG Kosovichev, RS Bogart, JT Hoeksema, Y Liu, TL Duvall, J Zhao, AM Title, et al. The helioseismic and magnetic imager (hmi) investigation for the solar dynamics observatory (sdo). Solar Physics, 275:207–227, 2012J-P Delaboudiniere, GE Artzner, J Brunaud, Alan H Gabriel, Jean-François Hochedez, F Millier, XY Song, B Au, KP Dere, Russell A Howard, et al. Eit: extreme-ultraviolet imaging telescope for the soho mission. The SOHO Mission, pages 291–312, 1995.John L Kohl, R Esser, Larry D Gardner, Shadia Habbal, Peter S Daigneau, EF Dennis, GU Nystrom, A Panasyuk, JC Raymond, PL Smith, et al. The ultraviolet coronagraph spectrometer for the solar and heliospheric observatory. The SOHO Mission, pages 313–356, 1995Hideyuki Tamura, Shunji Mori, and Takashi Yamawaki. Textural features corresponding to visual perception. IEEE Transactions on Systems, man, and cybernetics, 8(6):460–473, 1978.D Sierra-Porta. On the fractal properties of cosmic rays and sun dynamics cross-correlations. Astrophysics and Space Science, 367(12):116, 2022.David Sierra-Porta and Andy-Rafael Domínguez-Monterroza. Linking cosmic ray intensities to cutoff rigidity through multifractal detrented fluctuation analysis. Physica A: Statistical Mechanics and its Applications, 607:128159, 2022.http://purl.org/coar/resource_type/c_2df8fbb1ORIGINALPaper_SunsTopo_Dataset (1).pdfPaper_SunsTopo_Dataset (1).pdfArtículo principalapplication/pdf3808270https://repositorio.utb.edu.co/bitstream/20.500.12585/12571/1/Paper_SunsTopo_Dataset%20%281%29.pdfa1e2350491711a440d0a3a44807b4c74MD51CC-LICENSElicense_rdflicense_rdfapplication/rdf+xml; charset=utf-8701https://repositorio.utb.edu.co/bitstream/20.500.12585/12571/2/license_rdf42fd4ad1e89814f5e4a476b409eb708cMD52LICENSElicense.txtlicense.txttext/plain; charset=utf-83182https://repositorio.utb.edu.co/bitstream/20.500.12585/12571/3/license.txte20ad307a1c5f3f25af9304a7a7c86b6MD53TEXTPaper_SunsTopo_Dataset (1).pdf.txtPaper_SunsTopo_Dataset (1).pdf.txtExtracted texttext/plain26170https://repositorio.utb.edu.co/bitstream/20.500.12585/12571/4/Paper_SunsTopo_Dataset%20%281%29.pdf.txta717ae097327a0addf803a15eb01e6a3MD54THUMBNAILPaper_SunsTopo_Dataset 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