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Turbulence profiling using extended objects for slope detection and ranging (SLODAR)

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Turbulence properties along the Solar Probe trajectory

Computer Science
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Turbulence Regimes of the Solar Wind in the Region of its Acceleration and Initial Stage of Supersonic Motion

Computer Science – Sound
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Turbulence-induced fluctuations in ionization and application to PMSE

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Turbulent collective processes of new ions at Venus and Mars: problems of numerical models for the interaction between the solar wind and these planets. II. A two-fluid MHD model.

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Turbulent collectivization processes of new ions near Venus and Mars, and problems of numerical modeling of solar wind interaction with these planets. II - A two-fluid MHD model

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Turbulent convection in rapidly rotating spherical shells: A model for equatorial and high latitude jets on Jupiter and Saturn

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Turbulent Diffusion of Large-Scale Magnetic Fields in the Presence of Ambipolar Drift.

Computer Science
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Turbulent Dynamics in the Solar Convection Zone

Computer Science – Performance
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Turbulent Flames in SNe Ia

Computer Science – Sound
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Turbulent flow microstructures observed by sonar

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Turbulent fluctuations of plasma and magnetic field parameters in the magnetosheath and the low-latitude boundary layer formation: Multisatellite observations on March 2, 1996

Computer Science
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Turbulent heat fluxes by profile and inertial dissipation methods: analysis of the atmospheric surface layer from shipboard measurements during the SOFIA/ASTEX and SEMAPHORE experiments

Computer Science – Sound
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Turbulent heating in solar cosmic ray theory

Computer Science
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Turbulent heating of the interplanetary plasma at large heliocentric distances

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Turbulent kinetic energy dissipation rates in the polar mesosphere measured by a 3-MHz-Doppler radar

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Turbulent mixing in the Amazon River: The isotopic memory of confluences

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Turbulent mixing of metal and silicate during planet accretion — And interpretation of the Hf-W chronometer

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Turbulent pick-up of new-born ions near Venus and Mars and problems of numerical modelling of the solar wind interaction with these planets. II - Two-fluid HD model

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Turbulent pick-up processes for new ions at Venus and Mars and problems of numerical modeling of the solar wind interaction with these planets. 1. Features of the solar wind flow around the planets.

Computer Science
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