The Lamb–Chaplygin dipole model is a mathematical description for a particular inviscid and steady dipolar vortex flow. It is a non-trivial solution to the two-dimensional Euler equations. The model is named after Horace Lamb and Sergey Alexeyevich Chaplygin, who independently discovered this flow structure.[1] This dipole is the two-dimensional analogue of Hill's spherical vortex.
The model
A two-dimensional (2D), solenoidal vector field may be described by a scalar stream function, via , where is the right-handed unit vector perpendicular to the 2D plane. By definition, the stream function is related to the vorticity via a Poisson equation: . The Lamb–Chaplygin model follows from demanding the following characteristics: [citation needed]
The dipole has a circular atmosphere/separatrix with radius : .
The dipole propages through an otherwise irrorational fluid ( at translation velocity .
The flow is steady in the co-moving frame of reference: .
Inside the atmosphere, there is a linear relation between the vorticity and the stream function
where are the zeroth and first Bessel functions of the first kind, respectively. Further, the value of is such that , the first non-trivial zero of the first Bessel function of the first kind.[citation needed]
Usage and considerations
Since the seminal work of P. Orlandi,[2] the Lamb–Chaplygin vortex model has been a popular choice for numerical studies on vortex-environment interactions. The fact that it does not deform make it a prime candidate for consistent flow initialization. A less favorable property is that the second derivative of the flow field at the dipole's edge is not continuous.[3] Further, it serves a framework for stability analysis on dipolar-vortex structures.[4]
^Kizner, Z.; Khvoles, R. (2004). "Two variations on the theme of Lamb–Chaplygin: supersmooth dipole and rotating multipoles". Regular and Chaotic Dynamics. 9 (4): 509. doi:10.1070/rd2004v009n04abeh000293. ISSN1560-3547.