Proceso de ASC - OBSERVACION Y ANALISIS ESPECTRAL PARA MONITOREO DE LA ACTIVIDAD SOLAR

The Sun is a massive and radiant ball of gas composed of approximately 98% helium and hydrogen and six layers, where nuclear reactions of the aforementioned elements occur. These reactions produce a large amount of energy in the form of short electromagnetic wavelengths called gamma rays, which reac...

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Autores:

Restrepo, René
Álzate, Miguel
Moná, Waira
Mejía, Brandon
Quiñonez, Sergio
Correa, Daniel
Contreras, Andrés
Cano, Manuela

Tipo de recurso:

Investigation report

Fecha de publicación:

2023

Institución:

Universidad EAFIT

Repositorio:

Repositorio EAFIT

Idioma:

spa

OAI Identifier:

oai:repository.eafit.edu.co:10784/34213

Acceso en línea:

https://hdl.handle.net/10784/34213

Palabra clave:

Astronomy
Solar Magnetic Field
Solar Spectrum
Solar Flares
Sunspots
Sun
Astronomía
Campo magnético solar
Espectro solar
Fulguraciones solares
Manchas solares
Sol

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