Low Altitude Solar Magnetic Reconnection, Type III Solar Radio Bursts, and X-ray Emissions

Type III solar radio bursts are the Sun’s most intense and frequent nonthermal radio emissions. They involve two critical problems in astrophysics, plasma physics, and space physics: how collective processes produce nonthermal radiation and how magnetic reconnection occurs and changes magnetic energ...

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Detalles Bibliográficos
Autores principales: Cairns, I. H., Lobzin, V. V., Donea, A., Tingay, S. J., McCauley, P. I., Oberoi, D., Duffin, R. T., Reiner, M. J., Hurley-Walker, N., Kudryavtseva, N. A., Melrose, D. B., Harding, J. C., Bernardi, G., Bowman, J. D., Cappallo, R. J., Corey, B. E., Deshpande, A., Emrich, D., Goeke, R., Hazelton, B. J., Johnston-Hollitt, M., Kaplan, D. L., Kasper, J. C., Kratzenberg, E., Lonsdale, C. J., Lynch, M. J., McWhirter, S. R., Mitchell, D. A., Morales, M. F., Morgan, E., Ord, S. M., Prabu, T., Roshi, A., Shankar, N. Udaya, Srivani, K. S., Subrahmanyan, R., Wayth, R. B., Waterson, M., Webster, R. L., Whitney, A. R., Williams, A., Williams, C. L.
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Nature Publishing Group UK 2018
Materias:
Article
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC5786056/
https://www.ncbi.nlm.nih.gov/pubmed/29374211
http://dx.doi.org/10.1038/s41598-018-19195-3

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