Role of turbulent dissipation and thermal convection in solar wind's temperature evolution

1996 ◽  
Vol 101 (A12) ◽  
pp. 27549-27554 ◽  
Author(s):  
Mahendra K. Verma
Soil Science ◽  
1994 ◽  
Vol 158 (1) ◽  
pp. 47-55 ◽  
Author(s):  
WEIXING GUO ◽  
RICHARD R. PARIZEK ◽  
ARTHUR W. ROSE

2015 ◽  
Vol 92 (4) ◽  
Author(s):  
Vinodh Bandaru ◽  
Anastasiya Kolchinskaya ◽  
Kathrin Padberg-Gehle ◽  
Jörg Schumacher

2018 ◽  
Vol 180 ◽  
pp. 02097
Author(s):  
Rodion Stepanov ◽  
Peter Frick ◽  
Vladimir Dulin ◽  
Dmitriy Markovich

Important role of helicity was theoretically predicted for the generation of large-scale magnetic fields and atmospheric vortices. Helicity can lead to a reduction of turbulent dissipation in the atmosphere or in a specific constrained flow, e.g. in pipe. We use the TomoPIV data (42 cube of grid points, resolution 0.84 mm) to measure 3D velocity field of turbulent swirling flows. We study spatial distribution of the mean and fluctuating components of energy and helicity. We find that helical turbulence excitation and decay along stream of the jet strongly depend on the inflow swirl. We observe spatial separation of turbulent flow with different sign of helicity while integrated values are conserves. It is shown that large scale swirling flow induces helicity at the small scales. Our results bring valuable materials for benchmark the modern numerical simulations with turbulent closure technique.


Sign in / Sign up

Export Citation Format

Share Document