Home > Astronomy, Solar System, Sun > Magnetic Turbulence Trumps Collisions To Heat Solar Wind

Magnetic Turbulence Trumps Collisions To Heat Solar Wind


New research led by University of Warwick physicist Dr Kareem Osman has provided significant insight into how the solar wind heats up when it should not. The solar wind rushes outwards from the raging inferno that is our Sun, but from then on the wind should only get cooler as it expands beyond our solar system since there are no particle collisions to dissipate energy. However, the solar wind is surprisingly hotter than it should be, which has puzzled scientists for decades. Two new research papers led by Dr Osman may have solved that puzzle.

The new research led by Dr. Kareem Osman at the University of Warwick’s Centre for Fusion, Space and Astrophysics has revealed how turbulence heats the solar wind. He says:

“Turbulence stretches and bends magnetic field lines, and often two oppositely directed field lines can come together to form a current sheet. These current sheets, which are distributed randomly in space, could be sites where the magnetic field snaps and reconnects transferring energy to particle heating. There are also many more ways that current sheets can heat and accelerate the plasma.”

Full Story: http://www2.warwick.ac.uk/newsandevents/pressreleases/magnetic_turbulence_trumps#

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