That's just nonsense Higgsy. There is no "mismatch" with the corona, and it's not required for the entire corona to be as 'hot' as the coronal loops which traverse them.
Great since I prefer Birkeland's cathode model, but even SAFIRE was able to produce an atmosphere around the entire sphere which was hotter than the surface, something your entire industry cannot seem to manage with "magnetic reconnection". You keep sidestepping my difficult questions, like why you're peddling a concept that Alfven called "pseudoscience", and why your entire industry has yet to generate even *basic* atmospheric phenomenon, like *sustained* aurora, and coronas? Your whole industry is a full *century* behind Birkeland and his team *and counting*. Why are you folks so lame in the lab with respect to basic astronomical observation simulations?Secondly, I was originally commenting specifically on how poor a model for the Sun the SAFIRE experiment, so that's what I shall concentrate on, although much of it also applies to Birkeland's terella.
This is also entirely false. In various current carrying scenarios, the temperature of the electrons can exceed the ions by entire orders of magnitude.Your comment doesn't address the issue that to model the plasma, the temperature (mean particle energy) should be the same.
First of all I have very little faith in mainstream density estimates of the sun's atmosphere, so that's not even a serious consideration from my perspective. Secondly, it's simply a scaling issue that is of very little consequence in the final analysis. You folks cannot even generate *simple* features of the solar atmosphere, like a full sphere *hotter* (than the surface), coronal loops, polar jets, sustained solar wind, etc, things Birkeland accomplished in the lab more than a full *century* ago based on circuit theory. Either your entire industry is collectively inept in the lab, or your barking up the wrong pseudo-scientific tree as Alfven suggested.But still, as Eugene pointed out, the density of the gas in the model should scale as L^-1. Across the transition region of the sun, from 1000 to afew thousand km above the photosphere, the number density is 10^14 /cubic cm to 10^9/cubic cm which, if properly modelled would give model densities of 10^23 /cubic cm to 10^18/cubic cm for correct scaling, and this (taking the temperature in the model chamber into account with respect to 20C) is roughly about 0.01 atm to 1000 atm, far away from the actual model pressures.
It matters with respect to answering your question. The amount of current required is critical to answering your question.My opinion doesn't matter to this question.
Don't you already know all this? Am I just wasting my breath or what? Have you read Birkeland's work and/or Alfven's work for yourself yet? You'd already know how both of them expect the sun to be "powered" if you'd read their work for yourself. I have no idea how Juergen's expected to power his anode model, but there's nothing intrinsic about the amount of power an anode model might generate internally, or in it's upper atmosphere.In the electric Sun model(s), how is it powered, what is the process, and what do we observe?
Both Birkeland's cathode model and Alfven's homopolar generator model were powered *internally*. I'm not even required to deviate from the standard solar power process to embrace either of those models, and nothing precludes me from embracing (or at least discussing) an internally powered anode model either.That's not for me to answer, but the proponents of the model(s). In any case, the output has to be 10^26W of radiant power.
Why is that even necessary in the first place? If you're curious enough about this subject to play the role of 'skeptic', I'd expect you to already at least understand the various models.Again - you tell me.
But that is a *blatantly* false statement. SAFIRE *easily* produced a working solar atmosphere which was *hotter* than it's surrounding environment, and covered the whole sphere. That's a feat your entire industry has yet to achieve with your beloved "magnetic reconnection" models.This has all come about because I was responding to someone else's claim that "SAFIRE is the one and ONLY completely viable experimentally proven formation of a Star". You then asked me to say "in what *important* ways does it resemble the sun", and I'm pointing out that it doesn't. At all.
The only way to really know if their model is viable and/or "correct' is to measure all the particle flow patterns around their sphere and compare them to satellite data.
If the mainstream model is "quantified", then yes, such a quantified model exists for all three possible primary solar models. Fusion isn't the exclusive domain of the mainstream solar model Higgsy.So the answer is no. You don't have such a quantified model
There's also a lot of math related to particle flow patterns *around* the sun too. Did you see those calculations?Yes I have read it. However, you are right and I am wrong and there is an extended discussion about the processes in the Sun in those pages of the book.
You did what every astronomer I have ever met has done. You didn't really attempt to study his *whole* body of work. That's the problem with your industry in a nutshell. Had you read his whole book, and studied it carefully, none of your questions would even be required. You'd already have all your answers.I overlooked it, and the claims I made about him not using the terella for studying solar features and not studying the Sun much were wrong. I have no defence other than to say that I was concentrating when reading the book a few years ago on his work on the terrestrial aurora.
It's been 'justified' for more than a full century based on *experimental* data and the comparison of that data to real world in situ measurements, including satellite measurements from space. Birkeland was the first solar physicist to predict that *both* types of particles flowed from the sun, that cathode rays (electron beams) came from the sun, polar jets, coronal loops, etc.I give you the latter (planetary aurora). You'll have to justify the former (solar corona),
You can't even generate and *sustain* a high temperature corona to begin with! Your industry is already a *full century* behind Birkeland in the lab *and counting*.
You have shown *nothing* of the sort, and you're dragging your feet kicking and screaming.as we have seen that these physical models do not scale well to solar conditions;
Actually Alfven confirmed that plasma *does* scale very nicely and he applied circuit theory to every problem where the mainstream uses what Alfven called 'pseudoscience', and "magnetic reconnection" is a complete dud in the lab with respect to solar physics.but then Birkeland's work pre-dated Alfven's by a long time, so he wasn't to know that.
That is *complete* baloney. Birkeland even specifically "scaled" his work with respect to the voltages he expected to see, etc. Birkeland put it at around 600 million volts, whereas Alfven had it closer to a billion volts. Birkeland specifically expected it to scale perfectly, and Alfven's works shows that it does scale perfectly, and demonstrates that circuit theory is superior to MHD theory in explaining high energy plasma like we see in the solar atmosphere.Neither experiment, SAFIRE nor Birkeland's terrella, are good models for the Sun overall, lacking in many important solar features and being improperly scaled.
How it works for starters. I doubt that any of them have read Birkeland's work carefully for themselves. That's what they should do IMO.What exactly do you think today's solar physicists should learn about what solar features from Birkeland's terrella?