When a solar flare, filled with sparse particles ejected from the sun’s insides, its magnetic field is currently not the case, as predicted by the our physics. “Freezing” the magnetic field and thus the magnetic field lines should leak up these particles, but these lines are, however, often broken and then quickly reconnect in a manner that all this has long been introduced in astrophysics paint.
The study, which was undertaken under the guidance of the Gregory Eyink at Johns Hopkins University (USA), presumably, is the keys to understanding why this is happening.
Theorem frozen stream, which is used to explain the behavior of magnetic fields in the plasma, there was 70 years ago thanks to Hannes Alfven. Here is its main idea: magnetic field lines extend along the moving flows of matter and inseparable from it to the same extent that the coasts of the river. It turns out that for the foreseeable future, they can’t be “broken” or reconnection. Continue reading