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Supporting files for "Interchange reconnection as the source of the fast solar wind within coronal holes"

descriptionPublicationkeyboard_double_arrow_right Article 23 Jan 2023Publisher:Zenodo
Authors: Bale, S.D.; Drake, J.F.; McManus, M.D.; Desai, M.I.; Badman, S.T.; Larson, D.E.; Swisdak, M.; +9 Authors

doi: 10.5281/zenodo.7562034 , 10.5281/zenodo.7562035

Supporting files for "Interchange reconnection as the source of the fast solar wind within coronal holes"

Abstract

IDL data files and code for generating the plots from the PIC simulations in the paper "Interchange reconnection as the source of the fast solar wind within coronal holes". The full data set from the simulations is too large to upload, so only relevant snapshots are included here. The complete data set is stored at the supercomputing centers at which the runs were performed and access can be arranged upon request.

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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).
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impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
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