Sten Anders

ORCID: 0000-0002-4858-6894
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About
Contact & Profiles
Research Areas
  • Astro and Planetary Science
  • Fluid Dynamics and Mixing
  • Fluid Dynamics and Heat Transfer
  • Metallurgical Processes and Thermodynamics
  • Field-Flow Fractionation Techniques
  • High-pressure geophysics and materials
  • Fluid Dynamics Simulations and Interactions
  • Granular flow and fluidized beds
  • Plant Water Relations and Carbon Dynamics
  • Freezing and Crystallization Processes
  • Bee Products Chemical Analysis
  • Particle Dynamics in Fluid Flows
  • Planetary Science and Exploration
  • Marine and environmental studies
  • Geomagnetism and Paleomagnetism Studies
  • Heat Transfer Mechanisms
  • Micro and Nano Robotics
  • Crystallization and Solubility Studies
  • Global Energy and Sustainability Research

Helmholtz-Zentrum Dresden-Rossendorf
2019-2024

Abstract We introduce a complex image processing scheme for the simultaneous application of liquid crystal thermometry (LCT), in addition to previously established method Anders et al. (Exp Fluids 60(4):68, 2019. 10.1007/s00348-019-2703-8 ) particle tracking velocimetry and velocimetry. This was developed an experimental study on double-diffusive convection aqueous ammonium chloride solution NH 4 Cl(aq) during crystallization. The use thermochromic crystals (TLC) enables visualize flow...

10.1007/s00348-020-2939-3 article EN cc-by Experiments in Fluids 2020-04-01

The lowest swirling wave mode arising in upright circular cylinders as a response to orbital excitation has been widely studied the last decade, largely due its high practical relevance for orbitally shaken bioreactors. Our recent theoretical study (Horstmann et al. , J. Fluid Mech. vol. 891, 2020, A22) revealed damping-induced symmetry breaking mechanism that can cause spiral structures manifested so far disregarded higher rotating modes. Building on this work, we develop linear criterion...

10.1017/jfm.2021.686 article EN cc-by Journal of Fluid Mechanics 2021-08-26

Understanding the crystallization of metallic cores is necessary to constrain structure and thermal evolution terrestrial bodies in our solar system beyond. Core cooling also closely related generation sustainability a magnetic field. The core regime depends primarily on depth intersection temperature with liquidus ([1], refs therein). composition, pressure, profile are major parameters controlling intersection. If gradient across steeper than that liquidus, solidification starts at top,...

10.5194/egusphere-egu24-20752 preprint EN 2024-03-11
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