First a general remark: no experiment can achieve an exact null result, as there is always some noise. In case of Michelson and Morley experiment, the arm lengths were not exactly equal, the light rays hit each mirror at different angles, etc. What matters is whether the result is zero within the experimental uncertainty.
Then, Michelson and Morley experiment was designed to test the dragged Ether hypothesis of Fresnel. The result they found did falsify that as @Ruslan pointed out. But since the outcome was zero within experimental limits, it became seen as a null result.
More importantly, the only relevance of Michelson-Morley type of experiment is to test Special Relativity (SR) but then they are not the only type of such experiments. You also have the Kennedy-Thorndyke type, the Ives–Stilwell type, the Mössbauer type, Doppler, etc. Thus one needs a meaningful way to compare them all. Looking at fringe shifts is not general enough: first some experiments don't measure that and then even among all the optical experiments, the fringe shifts depend on the experimental setup and they cannot directly be compared to each other. As a result, physicists have developed so-called test theories, allowing for departure from SR, within which one can model any experiment. The most used one is that of Mansouri and Sexl [1,2,3]. This is conceptually so simple that I will describe it here before I can then go an compare Michelson-Morley and Joos. I haven't studied all your other references.
One assumes that there is an inertial frame $\Sigma$ in which the speed of light is isotropic, and in which clocks are synchronised with Einstein's procedure, the Ether frame, usually chosen to be the "CMBR frame". Let $X$, $Y$, $Z$ and $T$ be the space and time coordinates in $\Sigma$. Then one considers another frame $S$ moving at a speed $v$ along the x-axis, where coordinates are $x$, $y$, $z$ and $t$ (thus $v\approx 300\, \mathrm{km}/\mathrm{s}$). Finally one assumes the following transformations:
$$\begin{aligned}
t &= aT+\epsilon x + \epsilon_2 y + \epsilon_3 z\\
x &= b(X - vT)\\
y &= dY\\
z &= dZ
\end{aligned}$$
where $a$, $b$, $d$, $\epsilon$, $\epsilon_2$, and $\epsilon_3$ are functions of the speed $v$. Those last 3 functions define the synchronisation used in $S$ and they are therefore spurious: only $a$, $b$, and $d$ can be probed experimentally. This is done by expanding them in series of $v$ (one can prove that $a$, $b$ and $d$ must be even, so the first-order term has to be zero):
$$\begin{aligned}
a &= 1 + \alpha v^2+\cdots\\
b &= 1 + \beta v^2 +\cdots\\
d &= 1 + \delta v^2+\cdots
\end{aligned}$$
Then any experimental test of special relativity can be analysed in this framework, and this results on upper bounds on combinations of $\alpha$, $\beta$ and $\delta$, as SR corresponds to $\alpha=\beta=+1/2$ and $\delta=0$.
For Michelson-Morley experiments, the difference $\delta\tau$ in the optical path between the two arms reads
$$\delta\tau = (l_1 + l_2)(2\beta + 2\delta -1)v^2\cos2\theta,$$
where $l_1$ and $l_2$ are the lengths of the arms, and $\theta$ is the orientation of one of the arm. For example, for the original Michelson-Morley experiment, taking $\delta\tau < 0.005\lambda$,
$$\beta + \delta = 0.5\pm10^{-3}$$
whereas for Joos experiment
$$\beta + \delta = 0.5\pm3\times10^{-5},$$
a two-order of magnitude improvement.
[1] Reza Mansouri and Roman U. Sexl. A test theory of special relativity: I. simultaneity and clock synchronization. General Relativity and Gravitation, 8(7):497–513, 1977.
[2] Reza Mansouri and Roman U. Sexl. A test theory of special relativity: II. first order tests. General Relativity and Gravitation, 8(7):515–524, 1977.
[3] Reza Mansouri and Roman U. Sexl. A test theory of special relativity: III. Second-order tests. General Relativity and Gravitation, 8(10):809–814, 1977.
