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Dataset . 2018
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Supplementary data for: Do Images of Biskyrmions Show Type-II Bubbles?

Authors: Cortés-Ortuño, David; Loudon, James; Beg, Marijan; Hovorka, Ondrej; Fangohr, Hans;

Supplementary data for: Do Images of Biskyrmions Show Type-II Bubbles?

Abstract

This repository contains the micromagnetic simulation scripts for the publication Do Images of Biskyrmions Show Type-II Bubbles? by J. C. Loudon, A. C. Harrison, D. Cortes-Ortuno, M. T. Birch, L. A. Turnbull, A. Stefancic, F. Ogrin, E. Burgos-Parra, A. Campbell, H. Popescu, M. Beg, O. Hovorka, H. Fangohr, P. A. Midgley, G. Balakrishnan and P. D. Hatton Simulations are based on the OOMMF code [1] and its Jupyter interface JOOMMF [2] An updated version of this repository can be found here: https://github.com/davidcortesortuno/paper_biskyrmions_bubbles [1] M. J. Donahue and D. G. Porter, OOMMF Users Guide, Version 1.0, Tech. Rep. (National Institute of Standards and Technology, Gaithersburg, MD, 1999). [2] M. Beg, R. A. Pepper, and H. Fangohr, User interfaces for computational science: A domain specific language for OOMMF embedded in python. AIP Advances 7, 056025 (2017), https://doi.org/10.1063/1.4977225.

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Keywords

micromagnetics bubbles magnetism oommf joommf biskyrmions

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This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
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popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
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