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Finite-modal fluid observation and noise model

Physical scope

Adopted discrete-time model for specified ideal weighted spatial velocity sensors applied to a finite-dimensional modal representation of a three-dimensional fluid velocity field in a fixed nonrelativistic Cartesian inertial chart. Gaussian initial-state, process-noise, and observation-noise assumptions are part of this selected model regime; no actual sensor calibration, universal fluid law, nonlinear or untruncated flow model, or empirical validity is asserted.

Postulate

Let I⊆R be a nonempty open interval and let E be a three-dimensional oriented Euclidean affine space. Fix an orientation-preserving affine isometry x:E→R3 as the Cartesian inertial chart on Newtonian spacetime I×E, with absolute time t in seconds and spatial position in metres. Let D⊂R3 be a bounded Lebesgue-measurable observation region with volume 0<∣D∣<∞, and let H=L2(D;R3) be the space of almost-everywhere equivalence classes of square-integrable vector fields, with norm ∥v∥H=(∫D∣v(x)∣2 d3x)1/2. Write B(H) for the sigma-algebra generated by the norm-open sets. A velocity field has units m s−1.

Choose an integer observation horizon T≥0 and times t0<t1<⋯<tT in I, where observations are taken at t1,…,tT. For each 0≤k≤T, let mk≥1 and choose dimensionless modal fields ϕk,1,…,ϕk,mk∈H. Define the modal map Φk:Rmk→H by Φk(a)=∑j=1mkajϕk,j. The coefficient vector ak∈Rmk has units m s−1, with initial mean μ0 in m s−1, and its represented velocity field is Uk=Φk(ak). This finite-dimensional representation is an adopted approximation for the selected observation times; it does not assert that an untruncated fluid field lies in one of these finite-dimensional spaces.

For each 1≤k≤T, choose pk≥1 sensor weights ψk,1,…,ψk,pk∈H, with units m−3. The ideal sensor on a field v∈H is the weighted spatial average Sψk,i(v)=∫Dv(x)⋅ψk,i(x) d3x; it is not a point evaluation. Define Lk:span⁡{ϕk,1,…,ϕk,mk}→Rpk by (Lkv)i=Sψk,i(v) and define the dimensionless observation matrix by [Hk]ij=(Lkϕk,j)i. Thus Lk(Uk)=Hkak, and each datum and observation-noise component has units m s−1.

On a common probability space (Ω,F,P), adopt the finite linear-Gaussian coefficient model a0∼Nm0(μ0,P0),ak=Fkak−1+qk,yk=Hkak+rk(1≤k≤T), where μ0∈Rm0, P0∈Rm0×m0, Qk∈Rmk×mk, and Rk∈Rpk×pk; Fk∈Rmk×mk−1 is dimensionless, qk∼Nmk(0,Qk) has coefficient units m s−1, and rk∼Npk(0,Rk) has observation units m s−1. The vectors a0,q1,r1,…,qT,rT are mutually independent. Here Nd(μ,C) denotes the d-dimensional Gaussian law with mean μ and covariance C, including singular covariance. A symmetric matrix C is positive semidefinite, written C⪰0, if zTCz≥0 for every vector z of the matching dimension. The covariance matrices P0,Qk,Rk have this property, with entries carrying the corresponding squared units. Assume the Axiom of Choice (AC), meaning every family of nonempty sets has a choice function, for the Gaussian-law construction. The finite-dimensional Gaussian laws and their common probability-space realization use this assumption. For each k, define the field law by μk(B)=P(Uk∈B) for B∈B(H); finite modal fields with finite-second-moment coefficients have finite-second-moment laws.

These linearity, Gaussianity, independence, covariance, finite-mode, and ideal-sensor conditions are adopted physical-model assumptions for this selected regime. The sensor weights and covariance matrices are model inputs; no calibration procedure is asserted. These conditions report no measurements and do not assert that an actual flow, observation system, or noise source satisfies them. Biased or temporally correlated errors, nonlinear observation maps, and untruncated fluid dynamics require separately stated models.

Facts & Assumptions

[A1]

Assume the Axiom of Choice for the Gaussian-law construction of the finite linear-Gaussian model. The Axiom of Choice

[F1]

The classical frame is an adapted Cartesian inertial chart on Newtonian spacetime with absolute time; the fluid velocity is an Eulerian vector field with SI units m s−1. Classical frames, primitive quantities and SI units

[F2]

H=L2(D;R3) is a space of almost-everywhere field classes with its norm topology, and Sψ(v)=∫Dv⋅ψ d3x is a weighted spatial sensor, not a point evaluation. Finite-second-moment random velocity sensor law

[F3]

For every v,ψ∈H, the sensor integral is finite, representative-independent, linear, and bounded by ∣Sψ(v)∣≤∥v∥H∥ψ∥H. The L2 velocity sensor is well-defined

[F4]

A finite linear modal map sends a measurable finite-second-moment coefficient vector to a strongly measurable field with a finite-second-moment pushforward law. Finite modal velocity fields inherit finite second moments

[F5]

The finite coefficient model uses affine state and observation equations with mutually independent Gaussian vectors and positive-semidefinite covariances; its finite observation matrix is defined from the chosen linear observation map. Finite coefficient observation and innovation interface

[F6]

Nd(μ,C) is a d-dimensional Gaussian law with mean μ and positive-semidefinite covariance C, including when C is singular; the independent-noise realization assumes AC. Finite coefficient observation and innovation interface The Axiom of Choice

Depends on

Dependency tree · 2 levels

Sources