Observation of Alfvén waves heating the Sun's corona

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SUMMARY

The discussion centers on the observation of Alfvén waves and their role in heating the Sun's corona, which is significantly hotter than the solar surface. Researchers, including Samuel D. T. Grant et al., have concluded that the dissipation of Alfvén waves in the solar chromosphere efficiently converts wave energy into heat. This finding addresses a 70-year-old mystery regarding the mechanisms behind the temperature disparity between the solar surface and the corona. Future experiments are anticipated to further elucidate the implications of this heating mechanism on a larger scale.

PREREQUISITES
  • Understanding of Alfvén waves and their properties
  • Familiarity with solar physics and the structure of the Sun
  • Knowledge of plasma dynamics and energy transfer mechanisms
  • Basic comprehension of experimental methods in astrophysics
NEXT STEPS
  • Research the experimental methods used in the study of Alfvén wave dissipation
  • Explore the implications of Alfvén waves on solar atmospheric heating
  • Investigate the upcoming experiments mentioned by Grant et al. for further insights
  • Learn about the broader impacts of solar corona heating on space weather phenomena
USEFUL FOR

Astronomers, astrophysicists, and students of solar physics who are interested in the mechanisms of solar heating and the behavior of plasma in astrophysical contexts.

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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
 
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:
 

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