1d Hydraulics (Manning-Strickler Formula)#
Goals
Write a basic script and use loops. Write a function and parse optional keyword arguments (**kwargs
).
Requirements
Python libraries: math (standard library). Read and understand how loops and Functions work in Python.
Get ready by cloning the exercise repository:
git clone https://github.com/Ecohydraulics/Exercise-ManningStrickler.git
Theoretical background#
The Gauckler-Manning-Strickler formula [KC08] (or Strickler formula in Europe) relates water depth and flow velocity of open channel flow based on the assumption of one-dimensional (cross-section-averaged) flow characteristics. The Strickler formula results from a heavy simplification of the Navier-Stokes equations and the Continuity equation [KC08]. Even though one-dimensional (1d) approaches have largely been replaced by at least two-dimensional (2d) numerical models today, the 1d Strickler formula is still frequently used as a first approximation for boundary conditions.
The basic shape of the Strickler formula is:
where:
\(u\) is the cross-section-averaged flow velocity in (m/s)
\(k_{st}\) is the Strickler coefficient in fictional (m\(^{1/3}\)/s) corresponding to the inverse of Manning’s \(n_m\).
\(k_{st}\) \(\approx\) 20 (\(n_m \approx\) 0.05) for rough, complex, and near-natural rivers
\(k_{st}\) \(\approx\) 90 (\(n_m \approx\) 0.011) for smooth, concrete-lined channels
\(k_{st}\) \(\approx\) 26/\(D_{90}^{1/6}\) (approximation based on the grain size \(D_{90}\), where 90% of the surface sediment grains are smaller, according to Meyer-Peter and Müller [MPM48]
\(S\) is the hypothetic energy slope (m/m), which can be assumed to correspond to the channel slope for steady, uniform flow conditions.
\(R_{h}\) is the hydraulic radius in (m)
The hydraulic radius \(R_{h}\) is the ratio of wetted area \(A\) and wetted perimeter \(P\). Both \(A\) and \(P\) can be calculated as a function of the water depth \(h\) and the channel base width \(b\). Many channel cross-sections can be approximated with a trapezoidal shape, where the water surface width \(B=b+2\cdot h\cdot m\) (with \(m\) being the bank slope as indicated in the figure below).
Thus, \(A\) and \(P\) result from the following formulas:
Finally, the discharge \(Q\) (m³/s) can be calculated as:
Calculate the discharge#
Write a script that prints the discharge as a function of the channel base width \(b\), bank slope \(m\), water depth \(h\), the slope \(S\), and the Strickler coefficient \(k_{st}\).
Tip
Use import math as m
to calculate square roots (m.sqrt
). Powers are calculated with the **
operator (e.g., \(m^2\) corresponds to m**2
).
Functionalize#
Cast the calculation into a function (e.g., def calc_discharge(b, h, k_st, m, S): ...
) that returns the discharge \(Q\).
Flexibilize#
Make the function more flexible through the implementation of (optional) keyword arguments so that a user can optionally either provide the \(D_{90}\) (D90
), the Strickler coefficient \(k_{st}\) (k_st
), or Manning’s \(n_m\) (n_m
).
Tip
In the code, only use Manning’s \(n_m\) and parse kwargs.items()
to find out the kwargs
provided by a user.
Invert the function#
The backward solution to the Manning-Strickler formula is a non-linear problem if the channel is not rectangular. This is why an iterative approximation is needed and here, we use the Newton-Raphson scheme [AK87] for this purpose (see also the the University of Stuttgart’s ILIAS platform).
Absolute Values
The absolute value of a parameter can be easily accessed through the built-in abs()
method in Python3.
Use a Newton-Raphson solution scheme [Pai92] to interpolate the water depth h
for a given discharge Q
of a trapezoidal channel.
Write a new function
def interpolate_h(Q, b, m, S, **kwargs):
Define an initial guess of
h
(e.g.,h = 1.0
) and an initial error margin (e.g.,eps = 1.0
)Use a
while
loop until the error margin is negligible small (e.g.,while eps > 10**-3:
) and calculate the :wetted area
A
(see above formula)wetted perimeter
P
(see above formula)current discharge guess (based on
h
):Qk = A ** (5/3) * sqrt(S) / (n_m * P ** (2 / 3))
error update
eps = abs(Q - Qk) / Q
derivative of
A
:dA_dh = b + 2 * m * h
derivative of
P
:dP_dh = 2 * m.sqrt(m ** 2 + 1)
function that should become zero
F = n_m * Q * P ** (2 / 3) - A ** (5 / 3) * m.sqrt(S)
its derivative:
dF_dh = 2/3 * n_m * Q * P ** (-1 / 3) * dP_dh - 5 / 3 * A ** (2 / 3) * m.sqrt(S) * dA_dh
water depth update
h = abs(h - F / dF_dh)
Implement an emergency stop to avoid endless iterations - the Newton-Raphson scheme is not always stable!
Return
h
andeps
(or calculated dischargeQk
)