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Alfven waves

The Alfven waves are transverse magnetohydrodynamic plasma waves propagating along the magnetic field lines . Caused by low-frequency electromagnetic waves in a plasma propagating along a constant magnetic field [1] . In this case, the plasma also begins to move due to the energy of the electromagnetic field, which leads to a multiple decrease in the wave propagation velocity. Named in honor of the Swedish astrophysicist Hannes Alfven , who predicted their existence in 1942 . The speed of propagation of such waves is given by the formula (in the Gaussian system, [2] ):

v=Hfourπρ{\ displaystyle v = {\ frac {H} {\ sqrt {4 \ pi \ rho}}}} v = \ frac {H} {\ sqrt {4 \ pi \ rho}}

They play an important role in the ionosphere of the Earth , the Sun and other astronomical objects . Their study of the Sun is one of the scientific problems of the Parker solar probe [3] .

Notes

  1. ↑ Elementary plasma physics, 1969 , p. 161.
  2. ↑ Elementary plasma physics, 1969 , p. 162.
  3. ↑ Heliophysicists are encouraging: a “burning” mystery has been revealed, which the Sun has hidden from people for 500 years

Literature

  • W. Gekelman, S. Vincena, B. Van Compernolle, GJ Morales, JE Maggs, P. Pribyl, and TA Carter. The many faces of shear Alfvén waves (Eng.) // Phys. Plasmas . - 2011. - Vol. 18. - P. 055501. - DOI : 10.1063 / 1.3592210 . (inaccessible link)
  • Artsimovich L. A. Elementary plasma physics. - 3rd ed. - M .: Atomizdat , 1969. - 189 p.

Links

  • http://www.astronet.ru/db/msg/1186368
Source - https://ru.wikipedia.org/w/index.php?title=Alvenskie_wolf&oldid=100457411


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