Scientists at Queen’s university Belfast have led an international team to the ground-breaking discovery that magnetic waves crashing thru the sun may be key to heating its atmosphere and propelling the solar wind.
The sun is the supply of energy that sustains all life on this planet but much stays unknown about it. However, a group of researchers at Queen’s have now unlocked some mysteries in a research paper, which has been published in Nature Physics.
In 1942, Swedish physicist and engineer Hannes Alfven predicted the existence of a new kind of wave due to magnetism acting on a plasma, which led him to obtain the Nobel Prize for Physics in 1970. since his prediction, Alfven waves have been associated with a variety of sources, which includes nuclear reactors, the gas cloud that envelops comets, laboratory experiments, medical MRI imaging and in the atmosphere of our nearest star – the sun.
A sunspot located towards the edge of the Sun, visible here as a dark collection of plasma with magnetic field strengths similar to those found in modern hospital MRI machines. However, it is the size of the sunspot, which is comparable to that of our own Earth (see the scale Earth depicted in the upper-right corner), that gives these structures immense power and energy. Extending upwards from the highly magnetic sunspot are field lines which can guide and direct dynamic motions from within the sun’s private layers.
The latest work published in Nature Physics reveals first-time evidence for how a rare breed of magnetic waves, guided upwards from the surface of the sun, can form shockwaves that heat the surrounding plasma by thousands of degrees. credit: Emma Gallagher
Scientists have suggested for many years that these waves may play an important role in maintaining the sun’s extremely high temperatures however until now had not been able to prove it.
Dr David Jess from the faculty of mathematics and Physics at Queen’s university Belfast explains: “For a long time scientists across the globe have predicted that Alfvén waves travel upwards from the solar surface to break in the higher layers, releasing enormous quantities of energy in the form of heat.
over the last decade scientists have been able to prove that the waves exist however until now there was no direct proof that they had the capability to convert their movement into heat.”
“At Queen’s, we have now led a team to detect and pinpoint the heat produced by means of Alfvén waves in a sunspot. This theory was predicted some seventy five years ago but we now have the evidence for the very first time. Our research opens up a new window to understanding how this phenomenon could potentially work in other areas such as energy reactors and medical gadgets.”
The international team included Queen’s university Belfast; the space research Institute, Austria; Ilia state university, Georgia; the national solar Observatory, usa; Instituto de Astrofísica de Canarias, Spain; Lockheed Martin, united states and California state university Northridge, united states.
The study used advanced high-resolution observations from the Dunn Solar Telescope in New Mexico (USA) alongside complementary observations from NASA’s Solar Dynamics Observatory, to analyse the strongest magnetic fields that appear in sunspots. These sunspots have intense fields similar to modern MRI machines in hospitals and are much bigger than our own planet.
Dr Samuel Grant from Queen’s comments: “By breaking the Sun’s light up into its constituent colours, our international team of researchers were able to examine the behaviour of certain elements from the periodic table within the Sun’s atmosphere, including calcium and iron.”
“Once these elements had been extracted, intense flashes of light were detected in the image sequences. These intense flashes had all the hallmarks of the Alfvén waves converting their energy into shock waves, in a similar way to a supersonic aircraft creating a boom as it exceeds the speed of sound.
The shock waves then ripple through the surrounding plasma, producing extreme heat. Using supercomputers, we were able to analyse the data and show for the first time in history that the Alfvén waves were capable of increasing plasma temperatures violently above their calm background.”
Publication: Samuel D. T. Grant, et al., “Alfvén wave dissipation in the solar chromosphere,” Nature Physics (2018) doi:10.1038/s41567-018-0058-3
Source: Emma Gallagher, Queen’s University Belfast