\section{Cartesian spaces and a common constrained approximation family} \label{sec:spaces} \subsection{A concrete two-level conforming construction} Let $h=1/M$, where $M$ is a positive integer, and let $\mathcal T_h$ be the uniform partition of $\Omega$ into squares of side $h$. On a rectangle, write $\mathbb Q_3$ for polynomials of degree at most three in each variable. Let $S_h\subset H^2_0(\Omega)$ be the clamped Cartesian bicubic Hermite space. Its local degrees of freedom at each vertex are the value, the two first derivatives, and the mixed derivative $\partial_{xy}$. Matching these degrees of freedom gives a globally $C^1$ function. The boundary degrees of freedom are set to zero, so that both the function and its normal derivative vanish on $\partial\Omega$. This is the standard Cartesian Bogner--Fox--Schmit construction; see, for example, \citet{bfs2020} for its tensor-product description and interpolation estimates. For a coarse cell $K\in\mathcal T_h$, divide $K$ into four squares of side $h/2$. Define $B_h(K)$ to consist of the $C^1$ piecewise bicubics on this subdivision whose value and gradient vanish on $\partial K$. Extending such a function by zero gives an element of $H^2_0(\Omega)$. Equivalently, all Hermite degrees of freedom at the eight boundary vertices are zero and the four degrees of freedom at the center vertex are free. Hence $\dim B_h(K)=4$. For any set $\mathcal A\subset\mathcal T_h$, put \begin{equation}\label{eq:cartesian-spaces} S_{h,\mathcal A}=S_h+\sum_{K\in\mathcal A}B_h(K),\qquad X_{h,\mathcal A}=\curl S_{h,\mathcal A},\qquad \curl\psi=(\partial_y\psi,-\partial_x\psi). \end{equation} Every $X_{h,\mathcal A}$ is a finite-dimensional subspace of $U$. Incompressibility holds exactly, since $\divg\curl\psi=0$ in distributions for $\psi\in H^2$. The zero boundary gradient of the streamfunction gives the outer homogeneous velocity condition. This construction retains the full coarse space and adds local fine-grid degrees of freedom. All the spaces are contained in the uniform $h/2$ master space, but only cells in $\mathcal A$ carry the additional center degrees of freedom. Adding or deleting an arbitrary cell from $\mathcal A$ is a genuine local refinement or coarsening of this specified conforming space. The zero value and gradient of each local enrichment on the coarse-cell boundary prevent a conformity defect at a coarse--fine interface. We do not identify this space with the full space of every possible hanging-node implementation. For a regularization width $\eps$ and a panel space $\Lambda_\mathcal P$, define \begin{equation}\label{eq:spatial-Z} Z_{h,\mathcal A,\eps,\mathcal P} =\{v_h\in X_{h,\mathcal A}:b_\eps(v_h,\mu)=0 \text{ for every }\mu\in\Lambda_\mathcal P\}. \end{equation} These are exact surface-moment constraints. Linear independence of their rows is neither assumed nor needed for the velocity approximation arguments below. \subsection{A family present in every configuration} Let $\bar\eps$ be an upper bound for every regularization width in one run. Define the union of coarse cells \begin{equation}\label{eq:collar-cells} \begin{aligned} D_{h,\bar\eps} &=\bigcup\{K\in\mathcal T_h: K\cap\{x:\dist(x,\Gamma)\le\bar\eps\}\ne\varnothing\},\\ K_{h,\bar\eps} &=\{v_h\in\curl S_h:v_h=0\text{ on }D_{h,\bar\eps}\}. \end{aligned} \end{equation} The equalities defining $K_{h,\bar\eps}$ are polynomial identities on specified coarse cells, and therefore define a finite-dimensional linear space. They impose zero \emph{velocity}; they do not impose zero streamfunction on the immersed collar. The latter would unnecessarily exclude circulation modes. If $0<\eps\le\bar\eps$, every kernel support centered on $\Gamma$ lies inside $D_{h,\bar\eps}$. Thus \begin{equation}\label{eq:common-inclusion} K_{h,\bar\eps}\subset V, \qquad K_{h,\bar\eps}\subset Z_{h,\mathcal A,\eps,\mathcal P} \quad\text{for every }\mathcal A,\mathcal P, \quad 0<\eps\le\bar\eps. \end{equation} In particular, an orthogonal transfer onto any of these constraint spaces fixes every element of $K_{h,\bar\eps}$. The next result shows that this common family is large enough to approximate the physical solution space. \begin{lemma}[Common recovery family]\label{lem:recovery} Let $h_m\to0$ and $\bar\eps_m\to0$. For each $w\in V$ there exist $w_m\in K_{h_m,\bar\eps_m}$ such that \begin{equation}\label{eq:recovery} \norm{w_m-w}_U\longrightarrow0. \end{equation} The sequence $w_m$ is independent of the refinement sets, the panel partitions, and the individual regularization widths used during run $m$, provided those widths do not exceed $\bar\eps_m$. No relation between $h_m$ and $\bar\eps_m$ is required. \end{lemma} \begin{proof} The restrictions of $w$ to $B$ and $F$ belong to the zero-trace solenoidal $H^1$ spaces on these domains. The standard solenoidal density theorem on bounded Lipschitz domains, applied separately in the two domains, gives smooth divergence-free fields compactly supported in $B$ and $F$ that converge to these restrictions in $H^1$; see \citet[Section III.4]{galdi2011}. Their zero extensions and sums form a sequence $w^{(j)}\in C_c^\infty(\Omega)^2$ converging to $w$ in $U$. For each $j$, $w^{(j)}$ vanishes on a neighborhood of $\Gamma$ and is globally divergence free. This domainwise construction is valid in the multiply connected exterior region; it does not assert that the streamfunction has the same constant on its different boundary components. For a fixed such field $w^{(j)}$, define explicitly \[ \psi^{(j)}(x,y)=\int_0^y w^{(j)}_1(x,s)\,ds. \] Since $\divg w^{(j)}=0$ and $w^{(j)}_2(x,0)=0$, one has $\partial_y\psi^{(j)}=w^{(j)}_1$ and $\partial_x\psi^{(j)}=-w^{(j)}_2$. The zero outer velocity implies $\psi^{(j)}=0$ and $\nabla\psi^{(j)}=0$ on the outer square. On the connected collar of $\Gamma$, $\psi^{(j)}$ is a constant, which need not be zero. Thus $\psi^{(j)}$ is a smooth clamped streamfunction. Let $I_h\psi^{(j)}\in S_h$ be its bicubic Hermite interpolant. The Cartesian Hermite interpolation estimate, for example \citet[equation (52), with $m=2$]{bfs2020}, gives \begin{equation}\label{eq:BFS-interpolation} \norm{I_h\psi^{(j)}-\psi^{(j)}}_{H^2(\Omega)} \le C h^2\norm{\psi^{(j)}}_{H^4(\Omega)}. \end{equation} If $w^{(j)}$ vanishes whenever $\dist(x,\Gamma)0$, depending only on the fixed geometry, such that the following holds. If $h+\bar\eps