Manning-Strickler formula

Goals

Write 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

rhone The Rhone River in Switzerland (source: Sebastian Schwindt 2014).

The theory

The Gauckler-Manning-Strickler formula (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 and the continuity equations. Even though one-dimensional (1D) approaches have largely been replaced by at least two-dimensional (2d) numerical models today, the 1d Strickler formula is still frequently used as a first approximation for boundary conditions.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:

u = kst· S1/2 · Rh2/3

where:

  • u is the cross-section-averaged flow velocity in (m/s)

  • kst is the Strickler coefficient in fictional (m1/3/s) corresponding to the inverse of Manning’s n.

    • kst ≈ 20 (n≈0.05) for rough, complex, and near-natural rivers

    • kst ≈ 90 (n≈0.011) for smooth, concrete-lined channels

    • kst ≈ 26/D901/6 (approximation based on the grain size D90, where 90% of the surface sediment grains are smaller, according to Meyer-Peter and Müller 1948)

  • S is the hypothetic energy slope (m/m), which can be assumed to correspond to the channel slope for steady, uniform flow conditions.

  • Rh is the hydraulic radius in (m)

The hydraulic radius Rh 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·h·m (with m being the bank slope as indicated in the figure below).

FlowCrossSection

Thus, A and P result from the following formulas:

  • A = h · 0.5·(b + B) = h · (b + h·m)

  • P = b + 2h·(m² + 1)1/2

Finally, the discharge Q (m³/s) can be calculated as: Q = u · A = kst · S1/2· Rh2/3 · A

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 kst.

Tip

Use import math as m to calculate square roots (m.sqrt). Powers are calculated with the ** operator (e.g., 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 usage of optional keywords arguments (`**kwargs <https://hydro-informatics.github.io/hypy_pyfun.html#keyword-arguments-kwargs>`__) so that a user can optionally either provide the D90 (D90), the Strickler coefficient kst (k_st), or Manning’s n (n_m)

Tip

Internally, use only Manning’s n for the calculations 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 for this purpose. More literature about the Newton-Raphson scheme is provided on ILIAS.

Tip

The absolute value of a parameter can be easily accessed through the built-in abs() method in Python3.

Use a Newton-Raphson solution scheme (Paine 1992) 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

    • a 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 and eps (or calculated discharge Qk)