Gargantuan ‘Bubbles’ of Radio Energy Spotted at the Center of Our Galaxy. How’d They Get There? | Live Science
This "swirling" of plasma near the core, and above/below both poles is entirely consistent with Peratt's galaxy model, and Scott's Birkeland current paper. I think the key issue is whether or not this current flow pattern leaves concentric rings of oppositely moving plasma at different radii from the core. That's what Scott's model would tend to predict, along with plenty of high (and low) energy radiation from the current threads.
Astronomers discovered these galactic fart bubbles in 2010, while looking toward the center of the galaxy with NASA's Fermi Gamma-ray Space Telescope. Now known as the Fermi Bubbles, these massive, gassy blobs appear only in X-ray and gamma-ray light, teasing at an ancient and extremely powerful origin. How and when this galactic bubble-blowing blast occurred, astronomers can't say. But in a new study published today (Sept. 11) in the journal Nature, an international team of researchers reported some fresh clues found by looking to the opposite end of the electromagnetic spectrum, at radio waves.
This "swirling" of plasma near the core, and above/below both poles is entirely consistent with Peratt's galaxy model, and Scott's Birkeland current paper. I think the key issue is whether or not this current flow pattern leaves concentric rings of oppositely moving plasma at different radii from the core. That's what Scott's model would tend to predict, along with plenty of high (and low) energy radiation from the current threads.