{ "id": "1907.08013", "version": "v1", "published": "2019-07-18T12:24:33.000Z", "updated": "2019-07-18T12:24:33.000Z", "title": "Wave heating in simulated multi-stranded coronal loops", "authors": [ "Mingzhe Guo", "Tom Van Doorsselaere", "Konstantinos Karampelas", "Bo Li" ], "comment": "8 figures, accepted for publication in ApJ", "categories": [ "astro-ph.SR" ], "abstract": "It has been found that the Kelvin-Helmholtz instability (KHI) induced by both transverse and torsional oscillations in coronal loops can reinforce the effects of wave heating. In this study, we model a coronal loop as a system of individual strands, and we study wave heating effects by considering a combined transverse and torsional driver at the loop footpoint. We deposit the same energy into the multi-stranded loop and an equivalent monolithic loop, and then observe a faster increase in the internal energy and temperature in the multi-stranded model. Therefore, the multi-stranded model is more efficient in starting the heating process. Moreover, higher temperature is observed near the footpoint in the multi-stranded loop and near the apex in the monolithic loop. The apparent heating location in the multi-stranded loop agrees with the previous predictions and observations. Given the differences in the results from our multi-stranded loop and monolithic loop simulations, and given that coronal loops are suggested to be multi-stranded on both theoretical and observational grounds, our results suggest that the multi-strandedness of coronal loops needs to be incorporated in future wave-based heating mechanisms.", "revisions": [ { "version": "v1", "updated": "2019-07-18T12:24:33.000Z" } ], "analyses": { "keywords": [ "simulated multi-stranded coronal loops", "multi-stranded loop", "equivalent monolithic loop", "coronal loops needs", "multi-stranded model" ], "note": { "typesetting": "TeX", "pages": 0, "language": "en", "license": "arXiv", "status": "editable" } } }