Ans:
Equation of motion are,
∇ v = 0
ρ dv/dt + ρ (v ∇) v = - ∇p – ρg e + µ ∇2 v,
Where ρ = density, µ = viscosity, g = gravitational acceleration
Let us write
P(r,t) = p0 - ρg z + p1 (r, t)……..(1)
Where p0 = atmospheric pressure
P1 = pressure due to wave,
in the absence of the wave, the water pressure a depth h below the surface is p0 + ρg h
ρdv/dt = - ∇p1 + µ∇2 v
where we have neglected terms that are second order in small quantities,
now neglect viscosity, so our equation becomes,
ρdv/dt = - ∇p1
taking curl of this equation,
ρdw/dt = 0,
where w = ∇ * v
v = -∇ϕ, ϕ = velocity potential
the velocity field is also divergence free. It follows that the velocity potential satisfies Laplace's equation,
∇ϕ2 = 0
p1= ρdϕ/dt
We now need to derive the physical constraints that must be satisfied at the water's upper and lower boundaries. It is assumed that the water is bounded from below by a solid surface located at z=-d
dϕ/dt = 0
take vertical displacement f
df/dt = v = - dϕ/dt
Accourding to above equation (1)
p0 = p0 - ρg z + p1
Now ρgdf/dt = - ρgdϕ/dz = dp1/dt
For a wavelike solution, ϕ(r,t) = F(z)cos(wt – kx)
d2F/dz2 – k2F = 0
solution of this eq. exp(+kz) and exp(-kz)
hence
ϕ(x,z,t) = Aexp(kz)cos(wt – kx) + Bexp(-kz)(wt-kx)
A and B are arbitary constant, B = A exp(-2kd)
Φ(x,z,t) = A(exp(kz) + exp(-k(z+2d))cos(wt-kx)
Ak (1-exp(-2kd)cos(wt-kx) = Aw2/g(1 + exp(-2kd)cos(wt-kx)
Which reduces to be the dispersion relation
w2 = gktanh(kd)
So km = (gρ/T)1/2,
λ = 2π (T/ gρ)1/2
λ = 0.017 m
kd >> 1
d = depth
now w = (gk)1/2
Phase velocity = vp = w/k = (g/k)1/2
Group velocity = vg = dw/dk
vg = ½(g/k)1/2 = 1/2vp,
vg = ½(λ/T)
here λ0/T1 = λ/T2, here λ0 = 0.017m, T1 = 15 s, T2 = 12.5 s
λ = 0.014 m
(30 marks) For water waves with wavelength much longer than Xo, the effect of surface tension...