The effects of driving time scales on heating in a coronal arcade
| Autor: | Lianne Fyfe, Thomas Howson, I. De Moortel |
|---|---|
| Přispěvatelé: | European Research Council, Science & Technology Facilities Council, University of St Andrews. Applied Mathematics |
| Jazyk: | angličtina |
| Rok vydání: | 2020 |
| Předmět: |
010504 meteorology & atmospheric sciences
corona [Sun] T-NDAS FOS: Physical sciences Flux Context (language use) Astrophysics 01 natural sciences 0103 physical sciences QB Astronomy 010303 astronomy & astrophysics Solar and Stellar Astrophysics (astro-ph.SR) QC 0105 earth and related environmental sciences QB Physics Magnetohydrodyanmics (MHD) oscillations [Sun] Astronomy and Astrophysics Mechanics Dissipation Corona Magnetic field Amplitude QC Physics magnetic fields [Sun] Astrophysics - Solar and Stellar Astrophysics 13. Climate action Space and Planetary Science Poynting vector Physics::Space Physics Joule heating |
| Zdroj: | Astronomy & Astrophysics |
| ISSN: | 0004-6361 |
| Popis: | Context. The relative importance of AC and DC heating in maintaining the temperature of the corona is not well constrained. Aims. Investigate the effects of the characteristic time scales of photospheric driving on the injection and dissipation of energy within a coronal arcade. Methods. We have conducted three dimensional MHD simulations of foot point driving imposed on an arcade. We modified the typical driving time scales to understand the efficiency of heating obtained using AC and DC drivers. We considered the implications for the injected Poynting flux and the nature of the energy release in dissipative regimes. Results. For the same driver amplitude and complexity, long time scale motions are able to inject a much greater Poynting flux into the corona. Consequently, in non-ideal regimes, slow stressing motions result in a greater increase in plasma temperature than for wave-like driving. In dissipative simulations, Ohmic heating is found to be much more significant than viscous heating. For all drivers in our parameter space, energy dissipation is greatest close to the base of the arcade where the magnetic field strength is strongest and at separatrix surfaces, where the field connectivity changes. Across all simulations, the background field is stressed with random foot point motions (in a manner typical of DC heating studies) and even for short time scale driving, the injected Poynting flux is large given the small amplitude flows considered. For long time scale driving, the rate of energy injection was comparable to the expected requirements in active regions. The heating rates were found to scale with the perturbed magnetic field strength and not the total field strength. Conclusions. Alongside recent studies which show power within the corona is dominated by low frequency motions, our results suggest that in the closed corona, DC heating is more significant than AC heating. 14 pages, 16 figures |
| Databáze: | OpenAIRE |
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