Hydrodynamical helicity
In
Let be the velocity field and the corresponding vorticity field. Under the following three conditions, the vortex lines are transported with (or 'frozen in') the flow: (i) the fluid is inviscid; (ii) either the flow is incompressible (), or it is compressible with a barotropic relation between pressure p and density ρ; and (iii) any body forces acting on the fluid are conservative. Under these conditions, any closed surface S whose normal vectors are orthogonal to the vorticity (that is, ) is, like vorticity, transported with the flow.
Let V be the volume inside such a surface. Then the helicity in V, denoted H, is defined by the volume integral
For a localised vorticity distribution in an unbounded fluid, V can be taken to be the whole space, and H is then the total helicity of the flow. H is invariant precisely because the vortex lines are frozen in the flow and their linkage and/or knottedness is therefore conserved, as recognized by
For two linked unknotted vortex tubes having circulations and , and no internal twist, the helicity is given by , where n is the Gauss linking number of the two tubes, and the plus or minus is chosen according as the linkage is right- or left-handed. For a single knotted vortex tube with circulation , then, as shown by Moffatt & Ricca (1992), the helicity is given by , where and are the writhe and twist of the tube; the sum is known to be invariant under continuous deformation of the tube.
The invariance of helicity provides an essential cornerstone of the subject topological fluid dynamics and magnetohydrodynamics, which is concerned with global properties of flows and their topological characteristics.
Meteorology
In
where
- is the altitude,
- is the horizontal velocity,
- is the horizontal vorticity.
According to this formula, if the horizontal wind does not change direction with altitude, H will be zero as and are
This notion is used to predict the possibility of
where is the cloud motion relative to the ground.
Critical values of SRH (Storm Relative Helicity) for tornadic development, as researched in North America,[3] are:
- SRH = 150-299 ... tornadoes according to Fujita scale
- SRH = 300-499 ... very favourable to supercells development and strong tornadoes
- SRH > 450 ... violent tornadoes
- When calculated only below 1 km (4,000 feet), the cut-off value is 100.
Helicity in itself is not the only component of severe
This incorporates not only the helicity but the energy of the air parcel and thus tries to eliminate weak potential for thunderstorms even in strong SRH regions. The critical values of EHI:
- EHI = 1 ... possible tornadoes
- EHI = 1-2 ... moderate to strong tornadoes
- EHI > 2 ... strong tornadoes
Notes
- ^ Moreau, J. J. (1961). Constantes d'un îlot tourbillonnaire en fluide parfait barotrope. Comptes Rendus hebdomadaires des séances de l'Académie des sciences, 252(19), 2810.
- UKMET. "Definitions of terms in meteorology". Archived from the originalon 2006-05-16. Retrieved 2006-07-15.
- NOAA. Archivedfrom the original on December 29, 2022. Retrieved February 13, 2023.
- ^ "Storm Relative Helicity". NOAA. Retrieved 8 August 2014.
References
- Batchelor, G.K., (1967, reprinted 2000) An Introduction to Fluid Dynamics, Cambridge Univ. Press
- Ohkitani, K., "Elementary Account Of Vorticity And Related Equations". Cambridge University Press. January 30, 2005. ISBN 0-521-81984-9
- ISBN 0-387-94197-5
- ISBN 0-521-63948-4
- ISBN 0-19-854493-6
- Arfken, G., "Mathematical Methods for Physicists", 3rd ed. Academic Press, Orlando, FL. 1985. ISBN 0-12-059820-5
- Moffatt, H.K. (1969) The degree of knottedness of tangled vortex lines. J. Fluid Mech. 35, pp. 117–129.
- Moffatt, H.K. & Ricca, R.L. (1992) Helicity and the Cǎlugǎreanu Invariant. Proc. R. Soc. Lond. A 439, pp. 411–429.
- Thomson, W. (Lord Kelvin)(1868) On vortex motion. Trans. Roy. Soc. Edin. 25, pp. 217–260.