yourthe pseudo forces are:
$$\vec F_p=\underbrace{m\,\left(\vec \Omega\times (\vec \Omega\times \vec R)\right)}_{\text{Centrifugal force}}+ \underbrace{2\,m\,(\vec \Omega\times {\dot{\vec{R}}})}_{\text{Coriolis force}}$$
with:
$$\vec R=\begin{bmatrix} x \\ y \\ z \\ \end{bmatrix}\qquad,{\dot{\vec{R}}}=\begin{bmatrix} v_x \\ v_y \\ v_z \\ \end{bmatrix}\\ \vec \Omega=\Omega\,\begin{bmatrix} 0 \\ \cos(\lambda) \\ \sin(\lambda) \\ \end{bmatrix}$$
$\Rightarrow$
$$\vec F_p=\left[ \begin {array}{c} m{\Omega}^{2}x-2\,m \left( \cos \left( \lambda \right) v_{{z}}-\sin \left( \lambda \right) v_{{y}} \right) \Omega\\ -m\sin \left( \lambda \right) \left( \cos \left( \lambda \right) z-\sin \left( \lambda \right) y \right) { \Omega}^{2}-2\,m\sin \left( \lambda \right) v_{{x}}\Omega \\ m\cos \left( \lambda \right) \left( \cos \left( \lambda \right) z-\sin \left( \lambda \right) y \right) {\Omega}^{2}+2 \,m\cos \left( \lambda \right) v_{{x}}\Omega\end {array} \right] $$
with $~\Omega=7.27\,10^{-5}~[\frac 1s]$ and $~\lambda=\frac{\pi}{2},~\vec\Omega=[0~,0~,\Omega]^T$
$$F_p=\left[ \begin {array}{c} 5.2 \,10^{-9}\,mx+ 1.4 \,10^{-4}\, mv_{{y}}\\ 5.2 \,10^{-9}\,my- 1.4 \,10^{-4}\,mv_{{x}}\\ 0.0\end {array} \right] $$
hence the pseudo force components (unit [N]) are very small and can neglected