English

Judgment of paradigms for magnetic reconnection in coronal loops

Plasma Physics 2022-10-06 v1 Solar and Stellar Astrophysics

Abstract

The traditional paradigm for magnetic field lines changing connections ignores magnetic field line chaos and requires an extremely large current density, jmaxRmj_{max}\propto R_m, flowing in thin sheets of thickness 1/Rm1/R_m, where RmR_m is the magnetic Reynolds number. The time required for a general natural evolution to take a smooth magnetic field into such a state is rarely considered. Natural evolutions generally cause magnetic field lines to become chaotic. A fast change in field line connections then arises on the timescale defined by the evolution multiplied by a ln(Rm)\ln(R_m) factor, and the required maximum current density scales as ln(Rm)\ln(R_m). Even when simulations support the new paradigm based on chaos, they have been interpreted as supporting the old. How this could happen is an important example for plasma physics of Kuhn's statements about the acceptance of paradigm change and on Popper's views on the judgment of truth in science.

Keywords

Cite

@article{arxiv.2210.02209,
  title  = {Judgment of paradigms for magnetic reconnection in coronal loops},
  author = {Allen H Boozer},
  journal= {arXiv preprint arXiv:2210.02209},
  year   = {2022}
}