Strong magnetic fields have long been suspected to play a major role in heating the corona, something that the Parker Solar Probe was sent to examine in more details. Perhaps in that roiling inferno of the surface hides the enigmatic source of the corona’s high temperature. Granules, sunspots, flares, mass ejections, and more bubble and erupt from the sun’s chaotic exterior. After all, that surface is exposed to the hard, cold, chilling vacuum of outer space, and is separated from the warming core by hundreds of thousands of kilometers of thick, soupy plasma.īut that surface is active, perhaps even more so than the turbulent corona above it. It’s not hard to imagine why the surface of the sun, called the photosphere, is so much cooler than the innermost core. The image above includes an image of Earth to show the size of the CME compared to the size of Earth. The CME did not travel directly toward Earth, but did connect with Earth’s magnetic environment, or magnetosphere, causing aurora to appear on the night of Monday, September 3. The coronal mass ejection, or CME, traveled at over 900 miles per second. On Auga long filament of solar material that had been hovering in the sun’s atmosphere, the corona, erupted out into space at 4:36 p.m.
The conversion leaves a little bit of mass behind, and hence releases a little bit of energy.Įach individual reaction emits just a tiny little bit of energy, but repeat that process countless times and you end up with a fantastic, long-lived, powerful energy source, providing all the light for the entire solar system for billions of years.Īnd since it’s the only power source around, somehow heating up the corona. In the deep, dense, hot core (ironically the only place that bests the temperatures of the corona), the incredible pressures overwhelm the natural repulsion of hydrogen, fusing them together to make helium. There’s only one power source in the sun, and that’s nuclear power. So it’s very obviously a very active and complicated place, which might provide a clue to its hellishly high temperature. Thin wispy filaments, long tenuous loops, and whorls resembling fingerprints dance throughout the sun’s atmosphere.
Detailed examination of the corona reveals very peculiar structures.
0 kommentar(er)
