High-frequency torsional Alfvén waves as an energy source for coronal heating

The existence of the Sun’s hot atmosphere and the solar wind acceleration continues to be an outstanding problem in solar-astrophysics. Although magnetohydrodynamic (MHD) modes and dissipation of magnetic energy contribute to heating and the mass cycle of the solar atmosphere, yet direct evidence of...

Descripción completa

Detalles Bibliográficos
Autores principales: Srivastava, Abhishek Kumar, Shetye, Juie, Murawski, Krzysztof, Doyle, John Gerard, Stangalini, Marco, Scullion, Eamon, Ray, Tom, Wójcik, Dariusz Patryk, Dwivedi, Bhola N.
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Nature Publishing Group 2017
Materias:
Article
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC5335648/
https://www.ncbi.nlm.nih.gov/pubmed/28256538
http://dx.doi.org/10.1038/srep43147

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC5335648/
https://www.ncbi.nlm.nih.gov/pubmed/28256538
http://dx.doi.org/10.1038/srep43147

Ejemplares similares