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The camera baseline is the separation between the camera centers of two views. For centers $C_L,C_R$, its length is $B=\Vert C_R-C_L\Vert$. It measures translation, so turning a stationary camera without moving its camera center does not create a nonzero camera baseline. A known camera baseline supplies the length scale in stereoscopic triangulation.^[ref]

In the ideal aligned model with matched coordinate origins, stereo disparity satisfies $d=fB/Z$. For focal length 800 pixels and depth 5 metres, a camera baseline 0.10 metres gives 16 pixels; doubling the camera baseline gives 32 pixels. With unchanged disparity precision, the larger separation improves depth sensitivity. It can also increase occlusion in stereo vision and reduce overlap of the views. Finally, multiplying both $B$ and all reconstructed lengths by the same factor leaves the projections unchanged: a small reprojection error alone cannot certify the metric scale.

Epipolar geometry describes the projective relationship between two camera views. A scene point away from the camera baseline and the two camera centers determine an epipolar plane. Its intersections with the image planes are corresponding epipolar lines. Knowing one image point therefore constrains its partner to a line rather than the whole second image.^[ref]

With image points in homogeneous coordinates, a fundamental matrix $F$ expresses the constraintFor an ideal horizontally rectified pair this reduces to equality of image-row coordinates, while horizontal displacement remains free and carries stereo disparity. A line constraint does not determine depth: many scene points along one viewing ray satisfy the geometry. Correct stereo correspondence selects a partner, and camera calibration then supports metric stereoscopic triangulation.

A reprojection error compares an observed image point with the position predicted by projecting a reconstructed scene point through a camera model. If $q_i$ is an observed position and ${\pi }_i(P)$ its prediction, the residual is $e_i=q_i-{\pi }_i(P)$. One possible aggregate is the per-point root mean square Euclidean norm:Coordinates in pixels give an error in pixels. Least squares instead minimizes the associated sum of squares; normalization conventions should be stated when reporting a summary.^[ref]

For an observation $(100,50)$ and prediction $(103,54)$, the Euclidean norm of the residual is 5 pixels. Camera calibration can adjust model parameters to reduce many such residuals, while stereoscopic triangulation can adjust a reconstructed point with the camera parameters fixed. Low reprojection error tests agreement with observations under that model; incorrect stereo correspondence or an incorrect camera baseline can still produce wrong scene geometry.

Stereo correspondence identifies image positions in two views that depict the same scene point. This is the matching step needed before stereoscopic triangulation can recover that point. Epipolar geometry restricts a candidate match to an epipolar line; after horizontal stereo rectification, that search follows a corresponding image row.^[ref]

For example, matching a corner at horizontal coordinate 120 in the left view with coordinate 96 in the right gives stereo disparity 24 pixels. A repeated window pattern might offer equally plausible candidates at 96 and 72, producing different inferred depths. Geometry alone does not choose the correct window. A foreground object can also hide the feature in one view: occlusion in stereo vision then prevents a visible match. Texture, agreement of nearby matches and explicit rejection of ambiguous locations supply evidence beyond mere proximity along a row. A confident disparity map must represent locations where stereo correspondence failed as well as those where it succeeded.

Stereo disparity is the difference between the image positions of the same scene feature in two views. For an ideal horizontally aligned pair, use signed horizontal coordinates with matched principal points and defineWith the orientation and camera baseline convention of stereoscopic triangulation, a point in front of the cameras has $d=fB/Z$: stereo disparity measures inverse depth, rather than depth itself. Halving $d$ doubles $Z$ when the camera baseline and focal length stay fixed.

A disparity map assigns this difference to matched image locations. Finding the matches is a separate stereo correspondence problem. A repeated pattern can give several plausible matches; a feature hidden from one camera has no visible partner. A small measured stereo disparity is therefore not, by itself, proof of a distant object: the match and calibration must also be credible.^[ref]

The ideal relation also explains why far-away reconstruction becomes sensitive to measurement error. Differentiating $Z=fB/d$ gives $\mathrm{d}Z/\mathrm{d}d=-fB/d^2$; the first-order propagation of uncertainty is ${\sigma }_Z\simeq fB{\sigma }_d/d^2$. Thus equal disparity errors produce larger depth errors at greater depth. The example and curves under stereoscopy quantify this effect.

A stereomicroscope is an optical microscope that sends distinct views of the same specimen to the two eyes through separate viewing channels. The views originate at slightly different directions, producing stereo disparity that supports stereoscopy. Two microscope eyepieces alone do not establish stereo imaging: splitting one image into identical copies supplies no second viewpoint.

A two-objective arrangement uses separate microscope objective assemblies whose viewing directions converge on the specimen. A shared-objective arrangement can instead preserve two distinct viewing bundles through one main objective. The distinction concerns how the two perspectives are formed, rather than the number of eyepieces. A primary manufacturer manual gives a concrete two-path example: its S-series optics have a10° convergence angle and a compact lower assembly providing access around the specimen.^[ref]

For an original geometric illustration, take two viewing rays inclined by $\pm \alpha$ to the normal of a reference plane. A feature at height $h$ above that plane has ray intersections displaced in opposite directions by $h\tan \alpha$, so their separation isWith total convergence angle $2\alpha =10^{\circ }$ and $h=1\mathrm{mm}$, the separation is about0.175mm. This back-projected reference-plane geometry illustrates stereoscopic triangulation; it is not a specification of human depth accuracy or a universal pixel-to-height calibration. Actual image coordinates also depend on each channel's optics and alignment.

The distinct viewpoints are useful when positioning a fine tool near a surface, inspecting a small mechanical assembly or distinguishing raised features from flat markings. Illumination reflected from an opaque surface makes many such specimens accessible without preparing a thin transmitting section. The microscope working distance determines how much physical room remains between the instrument and the focused specimen, which matters when a probe or tool must enter that space.

For measurement, retain the magnification setting and calibrate the relevant channel with a stage micrometer. A scale calibration in a reference plane does not automatically convert stereo displacement into height; that requires the viewing geometry or a separate height calibration. Increasing magnification also does not guarantee improved diffraction-limited resolution. The purpose of the second view is geometric information, alongside the instrument's ability to resolve and magnify structure.

Stereoscopic triangulation reconstructs a scene point from corresponding image positions and known camera geometry. Each image position determines a viewing direction. Two correctly matched views constrain the point to lie on both viewing rays; one view alone leaves its position along a ray undetermined.

For an ideal aligned pair, put the left camera at the origin and the right one at $(B,0,0)$ in a Cartesian coordinate system, with their axes pointing in the positive $Z$ direction. Assume a common focal length $f$, square pixels, corrected distortion and image coordinates measured from aligned principal points. Forward perspective projection givesThe stereo disparity $d=u_L-u_R$ therefore determines all three coordinates:Here $Z$ is depth along the camera axis; the Euclidean distance from the left camera is instead $\sqrt{X^2+Y^2+Z^2}$. If $f,u_L,v_L,d$ use pixels and the camera baseline $B$ uses metres, the recovered coordinates use metres. Without a known length scale, the images alone do not determine metric size.^[ref]

Real cameras require calibration before these simplified equations apply. Stereo rectification transforms the images to an aligned geometry. With noisy measurements, viewing rays need not intersect exactly; minimizing reprojection error instead seeks a point whose projected positions agree as closely as possible with the observations. Reconstruction also depends on stereo correspondence: a mathematically precise intersection of mismatched viewing directions can still describe the wrong scene point.^[ref]

Stereoscopy uses images from different viewpoints to convey or recover depth. In scientific photography, identifying the same feature in two calibrated views permits stereoscopic triangulation: intersecting the directions inferred from the two images.^[ref]

Consider ideal cameras with parallel axes, separated by a baseline $B$. With matching forward-projection coordinates and common focal length $f$ in image-coordinate units, a point at $(X,Z)$ projects toSubtracting gives the stereo disparity $d=x_L-x_R=fB/Z$, hence $Z=fB/d$. If $f$ and $d$ are measured in pixels, $Z$ has the same length unit as $B$.

For an original example, $B=0.12\mathrm{m}$, $f=800$ pixels and $d=24$ pixels give $Z=4\mathrm{m}$. First-order propagation of uncertainty gives ${\sigma }_Z\simeq fB{\sigma }_d/d^2$. Thus fixed disparity precision produces increasing depth uncertainty for more distant objects. Correctly matching the same feature is also essential; ambiguous or hidden features can defeat the reconstruction even when the geometry is known.