Sure you are. You guys publish papers all the time about "frozen in magnetic fields". What utter nonsense. The whole thing is moving and flowing and there are no "frozen in" magnetic lines in moving plasma.
What utter nonsense, MM.
The
frozen in magnetic fields are frozen into the flowing plasma

! They flow with the plasma. That is a simple definition of a frozen in magnetic field!
Scientists publish papers about frozen in magnetic fields all the time.
Scientists publish papers about non-frozen in magnetic fields all the time.
Then the magnetic lines you are writing about cannot possibly be 'frozen" either, so all your mathematical models are unrelated to the actual physics inside the moving, spinning, flowing plasma.
Wrong again, MM.
MHD is applied succesfully all the time to the actual physics inside moving, spinning, flowing plasma.
That spaceweather.com video makes it clear that it "heats up" when it 'connects' to the active region. The easiest way to explain that observation is to accept that "current flow" is the "cause" of that heating process.
That spaceweather.com video makes it clear that the not-dark (wow!) filament
- emits more light (heats up) as time passes.
- erupts.
This looks like gev_20101018_1526 that happened on 2010/10/18 15:26:00 17:00:00 at 16:43:00 - a C2.5 flare at S23W60.
- all of the activity seems to happen over active region 11112.
There is no "connect'. There is no "current flow" because you cannot see an electric current flowing in an image of the Sun. You have to measure the electric field (a hard task) or measure the magnetic field (much easier and often done) and deduce the current.
The scientifically verified way to describe that process is a magnetic field reconfiguring and releasing energy that propels plasma away from the Sun. That is a
solar flare
Solar flares affect all layers of the solar atmosphere (photosphere, corona, and chromosphere), heating plasma to tens of millions of kelvins and accelerating electrons, protons, and heavier ions to near the speed of light. They produce radiation across the electromagnetic spectrum at all wavelengths, from radio waves to gamma rays. Most flares occur in active regions around sunspots, where intense magnetic fields penetrate the photosphere to link the corona to the solar interior. Flares are powered by the sudden (timescales of minutes to tens of minutes) release of magnetic energy stored in the corona. If a solar flare is exceptionally powerful, it can cause coronal mass ejections.
Yes, it's called a "Birkeland Current". It has a proper name. You guys keep referring to it in euphemistic magnetic spiral/helix terms rather than it's proper scientific name.
No, its called a feature of plasma that you call a "Birkeland Current" without any evidence that is is a Birkeland current.
Its proper name is a filament (later an flare). You guy keeping referring to it in nonscientific, "I see bunnies in the clouds", unsupported assertion terms rather than it's proper scientific name.
Birkeland currents have (as far my quick research reveals) never been detected in solar events. Strictly speaking they can only happen around the Earth but the term is also used for the same effect around other planets.
I see no helix or spiral in the movie. That is the problem with just looking at pretty picture. You may imagine a spiral filament. I look at the same picture and imagine a randomly twisting filament. Someone else looks at it and sees a bunny

!
No, I see flares and CME's headed our way, hours and actually days before they happen.
No, you do not see them. They are not in the images until they appear in the images. What you have is
- You have an unspecified way of predicting (otherwise known as guessing) that CME's will happen after filament eruptions.
That is in fact a well known fact as this 2004 paper shows:
On the Relation between Filament Eruptions, Flares, and Coronal Mass Ejections.
- You state that there will be a flare from an active region over the next 48 hours.
That is about what the rough average that I worked out is. Astronomers have much better statistics, methodolgies and produce real estimates of the probabilities of flares from an active region:
SolarMonitor (summary for 18 Oct 2010)
Region most likely to flare: NOAA 11112 -- Probabilities: X(1%) M(19%) C(43%)
I've already demonstrated that this process works RC. It's only a matter of time before it will happen again and I will be able to 'predict' the event in advance based on careful observation of those pretty million dollar images that you keep treating like dirt.
Once again: You have not demonstrated that the process works.
You have no process as far as we know except guessing.
The guesses actually happen to be good guesses

eye-poppi) because they fit what astronomers already know about the Sun. However they can produce detailed numeric estimates rather than your guesses. They also have scientific theories about the processes invoved.