Forward Modelling of a Brightening Observed by AIA
dc.citation.firstpage | 1931 | en_US |
dc.citation.issueNumber | 7 | en_US |
dc.citation.journalTitle | Solar Physics | en_US |
dc.citation.lastpage | 1945 | en_US |
dc.citation.volumeNumber | 290 | en_US |
dc.contributor.author | Price, D.J. | en_US |
dc.contributor.author | Taroyan, Y. | en_US |
dc.contributor.author | Innes, D.E. | en_US |
dc.contributor.author | Bradshaw, S.J. | en_US |
dc.date.accessioned | 2017-05-15T21:11:38Z | en_US |
dc.date.available | 2017-05-15T21:11:38Z | en_US |
dc.date.issued | 2015 | en_US |
dc.description.abstract | A comprehensive understanding of the different transient events is necessary for any eventual solution of the coronal heating problem. We present a cold loop whose heating caused a short-lived small-scale brightening that was observed by AIA. The loop was simulated using an adaptive hydrodynamic radiation code that considers the ions to be in a state of non-equilibrium. Forward modelling was used to create synthetic AIA intensity plots, which were tested against the observational data to confirm the simulated properties of the event. The hydrodynamic properties of the loop were determined. We found that the energy released by the heating event is within the canonical energy range of a nanoflare. | en_US |
dc.identifier.citation | Price, D.J., Taroyan, Y., Innes, D.E., et al.. "Forward Modelling of a Brightening Observed by AIA." <i>Solar Physics,</i> 290, no. 7 (2015) Springer: 1931-1945. http://dx.doi.org/10.1007/s11207-015-0722-z. | en_US |
dc.identifier.doi | http://dx.doi.org/10.1007/s11207-015-0722-z | en_US |
dc.identifier.uri | https://hdl.handle.net/1911/94267 | en_US |
dc.language.iso | eng | en_US |
dc.publisher | Springer | en_US |
dc.rights | This article is distributed under the terms of the Creative Commons Attribution 4.0 International License, which permits unrestricted use, distribution, and reproduction in any medium, provided you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons license, and indicate if changes were made. | en_US |
dc.rights.uri | https://creativecommons.org/licenses/by/4.0/ | en_US |
dc.subject.keyword | Corona, structures | en_US |
dc.subject.keyword | Flares, microflares and nanoflares | en_US |
dc.subject.keyword | Heating | en_US |
dc.subject.keyword | Magnetohydrodynamics | en_US |
dc.title | Forward Modelling of a Brightening Observed by AIA | en_US |
dc.type | Journal article | en_US |
dc.type.dcmi | Text | en_US |
dc.type.publication | publisher version | en_US |
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