seasmith wrote:Following the general rule that "magnetic lines of force" are preceded by an electric impetus, it seems reasonable to ask if magnetic formations like coronal loops and 'flux tubes' are preceded by an electric event?
Yes. IMO the extremely powerful magnetic fields associated with sunspots are generated by Birkeland currents on steroids.
Rotating current produces a toroidal magnetic field:
http://charles-chandler.org/Geophysics/ ... lenoid.png
But unlike the "open field lines" in flux tubes coming out of granules, the field lines of sunspots close locally, in a classic toroidal form. The reasons are complex, but essentially, the photosphere is cooler, and thus allows more electron uptake than the hotter plasma beneath. As a consequence, the photosphere has a higher electrical resistance. This resistance slows the current down, meaning weaker magnetic fields, and less of a pinch. With less pinch, the electrons are dispersed, which further relaxes the magnetic field. If the dispersed current isn't capable of keeping the axial lines of force in the magnetic field consolidated, they will close locally, instead of following the current out into space.
At this point, the current is braked even further. When the magnetic field lines close in a local toroidal form, the current that was spiraling around them would then have to cross those lines of force to get out into space. But this generates a Lorentz force that deflects the currents in the direction of the magnetic field lines. So look again at the previous image, and imagine that the spiraling current is trying to keep heading upward, but then it encounters those toroidal lines. If the current is deflected by the lines of force that it created, the current splays outward.
http://qdl.scs-inc.us/2ndParty/Images/C ... on_wbg.png
We know that this outward splaying of electric currents happens, because we can see -- and measure -- the electric currents inside the penumbral filaments. In addition to the overall toroidal field of the sunspot itself, each filament generates its own field, and which follows the left-hand rule for electrons flowing out of the sunspot. We can also observe that the penumbral filaments have no footpoints where they splay outward -- they taper down to nothing in mid-flight. The sunspot's magnetic field dives back down into the photosphere, but the currents inside the penumbral filaments don't follow the magnetic lines. This is because the current is motivated by the attraction of electrons to the positive charge in the heliosphere, which won't allow the electrons to turn the corner and dive back down into the Sun. Instead, the E-field brings the current to a halt as soon as the filaments start heading back down. The deceleration relaxes the electrodynamic behaviors of the currents, and the electrons are dispersed by their electrostatic repulsion from each other. Then they are once again free to head straight out into space, responding to their attraction to the positive charge in the heliosphere.
seasmith wrote:We know that solar flares reach Earth's magnetosphere in about 8 minutes, while CME's usually take a matter of days.
Photons from a flare travel at the speed of light, taking a little over 8 minutes to get to the Earth. The maximum speed for the particles in a CME was 1/3 the speed of light. This was from an extremely rare proton storm, and it hit in less than an hour. More typically the particles take several or many hours to arrive, and sometimes take days.
As concerns solar flares, these are an extremely tough theoretical problem, since massive electrostatic discharges shouldn't be possible in the excellent conductivity of 6000 K hydrogen plasma -- arc discharges require
resistance to preserve the charge separation until the breakdown voltage is achieved. What's the breakdown voltage inside an excellent conductor? Next to nothing. So what develops the potential for a flare? IMO, the key is the sudden disappearance of the toroidal magnetic field. Assuming that there is a high negative charge density inside the sunspot shaft, where the electric current is, and where +ions are getting evacuated by electron drag, +ions from the surrounding photosphere will get drawn toward the sunspot shaft. But this lateral flow of +ions is impeded by that extremely powerful magnetic field, which doesn't like charged particles crossing perpendicular to it. So we can expect a build-up of +ions outside of the magnetic field (shown as a green gradient in the following image), with a powerful E-field between the electrons inside the sunspot shaft, and the +ions outside of it.
http://qdl.scs-inc.us/2ndParty/Images/C ... ut_wbg.png
But what if that magnetic field suddenly goes away? Then there is nothing preventing an arc in that powerful E-field. Thus a flare is produced. This is consistent with the fact that there is an extremely high concentration of heavy elements that are highly ionized in CMEs (e.g., Fe XV). So flares don't occur in the typical 75% hydrogen, 25% helium mix of the photosphere -- something is attracting highly ionized heavy elements. This makes sense if the sunspot shaft is negatively charged, and if the magnetic field prevents +ions from entering the negative charge stream.