ПЛАВУЧЕСТЬ МАГНИТНОГО ПОЛЯ В АККРЕЦИОННЫХ ДИСКАХ МОЛОДЫХ ЗВЕЗД

Translated title of the contribution: MAGNETIC FIELD BUOYANCY IN ACCRETION DISKS OF YOUNG STARS

Research output: Contribution to journalLetterpeer-review

Abstract

Buoyancy of fossil magnetic field in the accretion disks of young stars is investigated. It is assumed that the Parker instability leads to the formation of slender flux tubes of toroidal magnetic field in the regions of effective magnetic field generation. Stationary solution of the induction equation is written in the form in which the buoyancy is treated as the additional mechanism of the magnetic flux escape. We calculate the fossil magnetic field intensity in the accretion disks of young T Tauri stars for the cases when the radius of the magnetic flux tubes amft = 0.1H, 0.5H or 1H, where H is the accretion disk height scale. Calculations show that the buoyancy limits toroidal magnetic field growth, so that its strength is comparable with the vertical magnetic field strength for the case amft = 0.1H.
Translated title of the contributionMAGNETIC FIELD BUOYANCY IN ACCRETION DISKS OF YOUNG STARS
Original languageRussian
Pages (from-to)627
Number of pages1
JournalПисьма в журнал Физика элементарных частиц и атомного ядра
Volume14
Issue number6 (211)
Publication statusPublished - 2022

GRNTI

  • 29.00.00 PHYSICS

Level of Research Output

  • VAK List
  • Russian Science Citation Index

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