Korsos, M.B., Yang, S. and Erdelyi, R. (2019) Investigation of pre-flare dynamics using the weighted horizontal magnetic gradient method: From small to major flare classes. Journal of Space Weather and Space Climate, 9. A6. ISSN 2115-7251
Abstract
There is a wide range of eruptions in the solar atmosphere which contribute to space weather, including the major explosions of radiation known as flares. To examine pre-event behavior in δ-spot regions, we use here a method based on the weighted horizontal gradient of magnetic field (WGM), defined between opposite polarity umbrae at the polarity inversion line of active regions (ARs) as measured using from the Debrecen Heliophysical Observatory catalogues. In this work, we extend the previous analysis of high-energy flares to include both medium (M) and low-energy (C and B) flares. First, we found a logarithmic relationship between the log value of highest flare class intensity (from B- to X-class) in a δ-spot AR and the maximum value of WGM of the 127 ARs investigated. We confirm a trend in the convergence-divergence phase of the barycenters of opposite polarities in the vicinity of the polarity inversion line. The extended sample, (i) affirms the linear connection between the durations of the convergence-divergence phases of barycenters of opposite polarities in δ-spot regions up to flare occurrence and (ii) provides a geometric constraint for the location of flare emission around the polarity inversion line. The method provides a tool to possibly estimate the likelihood of a subsequent flare of the same or larger energy.
Metadata
Item Type: | Article |
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Authors/Creators: |
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Copyright, Publisher and Additional Information: | © M.B. Korsœs et al., Published by EDP Sciences 2019. This is an Open Access article distributed under the terms of the Creative Commons Attribution License (http://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited. |
Keywords: | Sun-flares-precursors |
Dates: |
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Institution: | The University of Sheffield |
Academic Units: | The University of Sheffield > Faculty of Science (Sheffield) > School of Mathematics and Statistics (Sheffield) |
Funding Information: | Funder Grant number SCIENCE AND TECHNOLOGY FACILITIES COUNCIL ST/M000826/1 ROYAL SOCIETY IE141493 |
Depositing User: | Symplectic Sheffield |
Date Deposited: | 01 Feb 2019 09:58 |
Last Modified: | 01 Feb 2019 09:58 |
Published Version: | https://doi.org/10.1051/swsc/2019002 |
Status: | Published |
Publisher: | EDP Sciences |
Refereed: | Yes |
Identification Number: | 10.1051/swsc/2019002 |
Open Archives Initiative ID (OAI ID): | oai:eprints.whiterose.ac.uk:141895 |