Paulo J. A

Nov 22, 2023 | mdpi.com | Mariela M. Nolasco |Stewart Parker |Pedro D. Vaz |Paulo J. A

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Jul 31, 2023 | eprints.gla.ac.uk | Juan Camilo |Juan Martinez |Juan Martínez |Paulo J. A

Authors: Glesener, L., Shih, A. Y., Caspi, A., Milligan, R., Hudson, H., Oka, M., Buitrago-Casas, J. C., Guo, F., Ryan, D., Kontar, E., Veronig, A., Hayes, L. A., Inglis, A., Golub, L., Vilmer, N., Gary, D., Reid, H., Hannah, I., Kerr, G. S., Reeves, K. K., Allred, J., Guidoni, S., Yu, S., Christe, S., Musset, S., Dennis, B., Oliveros, J. C. M., Athiray, P. S., Vievering, J., White, S., Winebarger, A., Drake, J., Jeffrey, N., Antiochos, S., Duncan, J., Zhang, Y., Alaoui, M., Simões, P. J.

May 24, 2023 | eprints.gla.ac.uk | Paulo J. A

Carlsson, M., Fletcher, L. , Allred, J., Heinzel, P., Kašparová, J., Kowalski, A., Mathioudakis, M., Reid, A. and Simoes, P. J. A. (2023) The F-CHROMA grid of 1D RADYN flare models. Astronomy and Astrophysics, 673, A150. (doi: 10.1051/0004-6361/202346087) Text318484.pdf - Published Version Available under License Creative Commons Attribution. 1MBAbstractContext: Solar flares are the result of the sudden release of magnetic energy in the corona.