These rings can be the basis of a mechanism that causes severe and ordinary explosions of the sun, according to the .
“This is a historical moment in solar science,” said Cole Tomburi of the University of Colorado Boulder. We finally see the sun on the scale in which it works.
Solar flames are created when the magnetic field lines pass through the outer atmosphere of the sun, ie the crown of the sun, are pulled and torn, thus releaseing the magnetic lines of energy and then reconnecting. This has been known for a while, but details of magnetic re -connection and solar eruptions still need further research.
The telescope is now photographing hundreds of solar crown rings, with an average of only 1.5 kilometers wide, and some may be 2 kilometers narrow. These sizes are at the boundary of the telescope.
The role of these small rings in the magnetic re -connection process is still not clear, but now that scientists have been assured that these rings are available, they can introduce them in their models of how the sun works. These small rings may be the basic blocks of the magnetic structure of the sun that cause solar eruptions.
The role of these small rings in the magnetic re -connection process is still not clear, but now that the researchers have been assured that these rings are available, they can introduce them in their models of how the sun works. These small rings may be the basic blocks of the magnetic structure of the sun that cause solar eruptions.
(tagstotranslate) Sun (T) Scientific Research (T) Photo (T) Telescope
RCO NEWS




