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L. Kitchatinov

61 papers hereh-index 252k citations160 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • sole author13
  • first author26
  • middle author8
  • last author14

Across the 61 of 61 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR48
  • astro-ph10
  • physics.plasm-ph2
  • physics.flu-dyn1
same name
  • L. Kitchatinov — 3 papers, h 1

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20042026
most citedDifferential rotation and meridional flow in the solar convection zone and beneath

79 citations · 1.3k across the 61 of their papers we have counts for

collaborators
Showing 2009Show all

4 papers · 1 filter

astro-ph.SR2009★ 15 cited

Dissipative and nonaxisymmetric standard-MRI in Kepler disks

L. L. Kitchatinov, G. Ruediger

Deviations from axial symmetry are necessary to maintain self-sustained MRI-turbulence. We define the parameters region where nonaxisymmetric MRI is excited and study dependence of…

astro-ph.SR2009★ 19 cited

The kink-type instability of toroidal stellar magnetic fields with thermal diffusion

G. Ruediger, L. L. Kitchatinov

The stability of toroidal magnetic fields in rotating radiative stellar zones is studied for realistic values of both the Prandtl numbers. The two considered models for the magneti…

astro-ph.SR2009★ 12 cited

Stability of latitudinal differential rotation in stars

L. L. Kitchatinov, G. Rüdiger

The question is addressed whether stellar differentially rotating radiative zones (like the solar tachocline) excite nonaxisymmetric r-modes which can be observed. To this end the…

astro-ph.SR2009

Magnetic pinch-type instability in stellar radiative zones

G. Ruediger, L. L. Kitchatinov, M. Gellert

The solar tachocline is shown as hydrodynamically stable against nonaxisymmetric disturbances if it is true that no cos^{4}θterm exists in its rotation law. We also show that the t…

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