A Study of Photospheric Vector Magnetic Field Changes During Solar Flares
Abstract. Large amounts of energy are released when magnetic field lines reconnect in the corona during solar flares. Observations have found both transient and irreversible changes in the photospheric magnetic fields during flares, but their origins and mechanisms are yet unclear. To investigate th...
- Autores:
-
Castellanos Durán, Juan Sebastián
- Tipo de recurso:
- Fecha de publicación:
- 2016
- Institución:
- Universidad Nacional de Colombia
- Repositorio:
- Universidad Nacional de Colombia
- Idioma:
- spa
- OAI Identifier:
- oai:repositorio.unal.edu.co:unal/58310
- Acceso en línea:
- https://repositorio.unal.edu.co/handle/unal/58310
http://bdigital.unal.edu.co/55042/
- Palabra clave:
- 52 Astronomía y ciencias afines / Astronomy
El Sol
Fulguraciones Solares
Campos Magnéticos Fotosféricos
The Sun
Solar flares
Photospheric Magnetic fields
- Rights
- openAccess
- License
- Atribución-NoComercial 4.0 Internacional