http://adsabs.harvard.edu/full/1958IAUS....6..135DHiggsy wrote: ↑Thu Dec 24, 2020 3:47 pmBut these pulsed facilities aren't designed for studying topological magnetic field changes, so are not intended for and do not study reconnection.Michael Mozina wrote: ↑Thu Dec 24, 2020 12:21 amThis particular paragraph bears further examination.Higgsy wrote: ↑Tue Dec 15, 2020 12:07 am
This is all very well, but it is important to keep in mind that theoretical models need to be grounded in empirical work. There are two sources for empirical studies, natural phenomena themselves such as solar flares, studies by satellite missions such as YOKOH, SOHO, TRACE, Hinode etc, where the observations of the geometry and UV, soft and hard X-rays confirms that the reconnection models are progressing on the right lines, and laboratory experiments. With regard to the latter, the problem of scaling arises, in that many of the naturally occurring processes occur on linear scales and at temperatures, densities, pressures and magnetic field strengths that are difficult or impossible to reach in the lab.
https://phys.org/news/2006-03-machine-b ... otter.html
https://www.sandia.gov/z-machine/
Actually such temperatures, pressures and field strengths are routinely reached in labs on Earth,
As far back as the 1950's, James Dungey was using the term "magnetic reconnection" and "electrical discharge" to describe solar flares. What *exactly* can't you study in the lab, and why on God's green Earth can't you even simulate a sustained planetary aurora yet in a real lab experiment based on "magnetic reconnection'?
This sounds suspiciously like "the dog ate my 3D homework for the last 100 years". How do you figure that strong fields and high temperatures are *sustained* in MRx, and why can't you show us such a process in a real lab experiment yet?The scale change from coronal loops (say 10^8 m) to typical high temperature pressure and magnetic field dimensions (say 10^-3 m to be generous), means that L scales as 10^-11. As temperature scales as L^0, 2-3MK is fine, but plasma pressure and magnetic field strength scales as L^-1, and the latter scaled is 10^5 T and is particularly difficult to achieve simultaneously along with the other conditions, even though it is critical.
You're welcome to "scale' your models to any size that you like so long as you can get a "scaled down" version to produce a few sustained working simulations as has been true for circuit theory for more than a full century and counting.