Observation of Alfvén waves heating the Sun's corona

In summary, scientists have recently discovered the mechanism behind the corona being much hotter than the surface of the Sun, which was previously a 70-year-old mystery. They have observed that the conversion of plasma waves to heat is quite efficient, which was not well understood before. This discovery may help explain the significant temperature increase from the solar surface to the corona. Further experiments are planned to gain a better understanding of the implications on a larger scale.
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The corona is much hotter than the surface of the Sun, contrary what you would naively expect from the heat flow. While plasma waves were long suspected as cause, the mechanism was not well understood. How are these waves produced, and how is their energy converted to heat?

Scientists now observed the second part directly, and conclude that the conversion to heat is quite efficient.

phys.org: Scientists crack 70-year-old mystery of how magnetic waves heat the sun

Publication, Samuel D. T. Grant et al: Alfvén wave dissipation in the solar chromosphere
 
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I cannot claim to understand the experimental method, but the interpretation is really interesting. At the end of the paper they indicate an upcoming experiment should help gain understanding of the implications on a larger scale to see if the mechanism (which yields modest heating per wave event) can account for the orders of magnitude temperature increase from the solar surface to the corona. Really cool!

Thanks for pointing us to this article!

jason
 
  • #3
mfb said:
The corona is much hotter than the surface of the Sun, contrary what you would naively expect from the heat flow. While plasma waves were long suspected as cause, the mechanism was not well understood. How are these waves produced, and how is their energy converted to heat?

thanks for that :smile:
 

What are Alfvén waves and how do they heat the Sun's corona?

Alfvén waves are a type of electromagnetic wave that travels through plasma. They are created by the interaction of the Sun's magnetic field with charged particles in the corona. As these waves travel through the corona, they transfer energy to the particles, heating up the corona in the process.

How do scientists observe Alfvén waves heating the Sun's corona?

Scientists use a variety of instruments, such as radio telescopes and satellites, to observe the Sun's corona and study the behavior of Alfvén waves. These instruments can detect the changes in the magnetic field and plasma density caused by the waves.

What impact do Alfvén waves have on the Sun's corona?

The heating caused by Alfvén waves is an important factor in understanding the dynamics of the Sun's corona. This energy input can affect the temperature, density, and structure of the corona, as well as contribute to the solar wind and other phenomena.

Can Alfvén waves be observed on other stars besides the Sun?

Yes, Alfvén waves have been observed on other stars, including red dwarfs and white dwarfs. These observations help scientists better understand the behavior of magnetic fields and plasma in different stellar environments.

How does studying Alfvén waves on the Sun contribute to our understanding of the universe?

Studying Alfvén waves on the Sun not only helps us understand the dynamics of our own star, but also provides insight into the behavior of magnetic fields and plasma in other astrophysical settings. This research can inform our understanding of processes such as star formation, solar flares, and space weather.

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