dasmiller
Just the right amount of cowbell
Actually, the peak was *way* above the Ne+4 energy state. By the time we get to the +2 energy state there's almost no neon emissions.
By the time we got down to +2, the emissions were about 2 orders of magnitude lower. That's still billions of times more Ne+2 than your transparent Ne layer allows.
I'd love to see an NE+3 or +4 image of the sun. I suspect it would look exactly as I predicted, and not as you predict. In other words I would predict that the entire surface of the photosphere is "lit up" in those wavelengths, whereas your theory would suggest that the activity was limited to the coronal loops. One visual test would falsify one of our models.![]()
"My" theory isn't that detailed; I'm not a solar physicist. Ne should be present (at relatively low concentrations) throughout the sun, so I'd expect to see Ne lines from the photosphere. I don't know enough about how the ionization states relate to temperature to have an opinion about whether we'd see much Ne+3 from the photosphere vs. the corona. You'd have to ask one of the others.