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The run directories contain unformatted data files either as data/proc0 (for 128x128x32_20kc_BDMSST93c_Oml) or as data/proc0-3 (for 128x64_20kc_BDMSST93_wind10a), or as bb.sav just for the magnetic field components in the other directories. They can be read directly with the corresponding idl routines that are in the directory (run_directories/run_idl) together with those delivered with the Pencil Code (https://github.com/pencil-code).
{"references": ["Brandenburg, A., & Furuya, R. S.: 2020, ``Application of a helicity proxy to edge-on galaxies,'' Mon. Not. Roy. Astron. Soc., in press (arXiv:2003.07284)"]}
polarization, dynamo, galaxies: magnetic fields, NGC 891
polarization, dynamo, galaxies: magnetic fields, NGC 891
| selected citations These citations are derived from selected sources. 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). | 0 | |
| 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. | Average | |
| influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | Average | |
| impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network. | Average |
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