Research on space plasma hurricanes could lead to new sources of energy

September 6, 2016 by James Roddey
An illustration depicting the Cluster spacecraft location with respect to the large scale Kelvin-Helmholtz wave with an approximate 36,000 km wavelength and 3 minute period, and small scale (200 - 2000 km wavelength) Fast Magnetosonic Mode wave packet. Credit: This image was initially published in Nature Physics. Credit: Embry-Riddle Aeronautical University

A new study by researchers at Embry-Riddle Aeronautical University, funded by the National Science Foundation, has identified for the first time a process by which the solar wind is heated along extended regions of the Earth's magnetic shield as it penetrates through this barrier. The process may have parallels to the unsolved problem in astrophysics of how the solar corona is heated. It may also be helpful for understanding the cross-scale transport of energy in man-made plasma devices that may lead to the creation of practical fusion power.

The peer reviewed study; Cross-scale Energy Transport in Space Plasmas is published in Nature Physics.

In 2011, Ph.D. student Thomas W. Moore, at that time a master's student, began working with Dr. Katariina Nykyri, a Professor of Physics in the Physical Sciences Department and member of Embry-Riddle's Center for Space and Atmospheric Research in Daytona Beach, analyzing data gathered from four European Space Agency Cluster spacecraft. The team, including post-doctoral researcher Andrew Dimmock, created numerical simulations that aid in understanding the signatures in the spacecraft data and utilized multi-spacecraft techniques for plasma wave mode identification. For 16 years, these four satellites have been investigating the Earth's magnetic environment and its interaction with the in three dimensions.

"In space, the fast streaming plasma (solar wind) originating from the Sun creates large 'space hurricanes,' called Kelvin-Helmholtz (KH) waves, at the boundary of Earth's magnetic barrier," said Nykyri. "The KH waves typically have wavelengths in range of 20,000-40,000 km and a 1-3 minute period, and as they steepen and roll-up like ocean waves they can transport solar wind plasma into the magnetosphere."

The KH waves are a direct result of the way our planet fits into the larger solar system. Planet Earth is a gigantic magnet and its magnetic influence extends outward in a large bubble called a magnetosphere. A constant flow of particles from the Sun (solar wind) blows by the magnetosphere—not unlike wind blowing over the surface of the ocean. During certain situations, particles and (plasma) from the Sun can breach the magnetosphere, crossing into near-Earth space.

"Within plasma physics, this is a significant discovery," said Moore. "Our understanding of this cross-scale energy transfer process came together gradually. There was not really an 'aha' moment, but the implications of our work became apparent when we realized how all the pieces of our research fit together."

"We found that the giant KH waves can radiate ion-scale waves, or smaller 'space tornadoes,' that have sufficient energy to heat the plasma to the energies we observed," said Nykyri. "This process transfers the kinetic energy from the solar wind into the heat energy of magnetospheric ions, explaining the rapid temperature increase through Earth's magnetic barrier. If we could utilize this mechanism effectively in the high density laboratory plasmas by constructing appropriate transport barriers, we could create energy from water."

Plasma is not a gas, liquid or solid, but the fourth state of matter—a gas that is so hot that some or all its constituent atoms are split up into electrons and ions (charged atoms or molecules), which can move independently of each other. It is estimated that 99.9 percent of the visible universe is made up of plasma.

Technically, the study shows that the Embry-Riddle researchers have described for the first time the process of how energy is transferred from magnetohydrodynamic scale Kelvin-Helmholtz (KH) (with a wavelength of 36,000 km) to ion-scale magnetosonic waves that has sufficient Poynting flux to explain the observed heating from magnetosheath (shocked solar wind) into the magnetosphere. Scaling of this mechanism to typical coronal parameters suggests that it may also help explain the heating of the as well as play role in other astrophysical and laboratory plasmas with a velocity shear.

Moore and Nykyri will be seeking funding to continue research into whether this cross-scale transport of energy continues all the way to the electron scales and how much energy can be transferred to the ion scales in laboratory plasmas.

Explore further: The magnetosphere has a large intake of solar wind energy

More information: T. W. Moore et al. Cross-scale energy transport in space plasmas, Nature Physics (2016). DOI: 10.1038/nphys3869

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Solon
2.2 / 5 (10) Sep 06, 2016
Might have difficulty obtaining further funding, they don't mention dark matter/energy, gravity waves, black holes, AGW, etc.
Kron
4 / 5 (2) Sep 07, 2016
Neat thing is, a bit off topic here so excuse me, if we find that we are underestimating the force of the solar wind (the repulsive force the Sun exudes pushing away the Earth and other planets), it would mean that we are also underestimating the force of gravity. For, if the repulsive forces are higher than previously considered, the force of gravity would have to be stronger than thought to be in order to counterbalance the centrifugal forces from planetary orbits and this stronger than considered repulsion to keep the planets in their orbits. Just some food for thought.

This would definitely have major implications on the dark sector (DM and DE), perhaps eliminating the need for it altogether.

I think further solar wind studies are an excellent route for funding.
antialias_physorg
5 / 5 (3) Sep 07, 2016
it would mean that we are also underestimating the force of gravity.

Satellites are exposed to the solar wind and the effects on their paths is pretty well documented over several decades now (both for satellites close to Earth and those that have ventured farther out/in to the solar system). Not a chance that we're over/underestimating this effect by a large margin.

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