Identification of nonlinear conservation laws for multiphase flow based on Bayesian inversion
Conservation laws of the generic form c t + f ( c ) x = 0 play a central role in the mathematical description of various engineering related processes. Identification of an unknown flux function f ( c ) from observation data in space and time is challenging due to the fact that the solution c ( x , ...
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Published in | Nonlinear dynamics Vol. 111; no. 19; pp. 18163 - 18190 |
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Main Authors | , , |
Format | Journal Article |
Language | English |
Published |
Dordrecht
Springer Netherlands
01.10.2023
Springer Nature B.V |
Subjects | |
Online Access | Get full text |
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Summary: | Conservation laws of the generic form
c
t
+
f
(
c
)
x
=
0
play a central role in the mathematical description of various engineering related processes. Identification of an unknown flux function
f
(
c
) from observation data in space and time is challenging due to the fact that the solution
c
(
x
,
t
) develops discontinuities in finite time. We explore a Bayesian type of method based on representing the unknown flux
f
(
c
) as a Gaussian random process (parameter vector) combined with an iterative ensemble Kalman filter (EnKF) approach to learn the unknown, nonlinear flux function. As a testing ground, we consider displacement of two fluids in a vertical domain where the nonlinear dynamics is a result of a competition between gravity and viscous forces. This process is described by a multidimensional Navier–Stokes model. Subject to appropriate scaling and simplification constraints, a 1D nonlinear scalar conservation law
c
t
+
f
(
c
)
x
=
0
can be derived with an explicit expression for
f
(
c
) for the volume fraction
c
(
x
,
t
). We consider small (noisy) observation data sets in terms of time series extracted at a few fixed positions in space. The proposed identification method is explored for a range of different displacement conditions ranging from pure concave to highly non-convex
f
(
c
). No a priori information about the sought flux function is given except a sound choice of smoothness for the a priori flux ensemble. It is demonstrated that the method possesses a strong ability to identify the unknown flux function. The role played by the choice of initial data
c
0
(
x
)
as well various types of observation data is highlighted. |
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Bibliography: | ObjectType-Article-1 SourceType-Scholarly Journals-1 ObjectType-Feature-2 content type line 14 |
ISSN: | 0924-090X 1573-269X |
DOI: | 10.1007/s11071-023-08817-9 |