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Linear velocity of sweeping beam on the sensor array can be interpreted as the distance from a beacon based on an equation.
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The beams of the sensors are 200-μm-long approximately.
The object and reference beam are recombined by means of a beam combiner on the CCD sensor that registers the digital holographic interferograms finally stored and processed in a computer.
When SC-DSPI is used for measurement, the three shutters are opened together, resulting in three pairs of object and reference beams emerging on the camera sensor simultaneously.
In Fig. 7 a the telescope triplet efficiency dependence on the sensor threshold is shown for various beam energies and sensor spacings.
Because of the diffuse reflection of the laser beam on the fingertip skin, a part of laser rays is reflected back to sensor.
NEVER push hard on the sensor.
That's right, if you have the sun beaming right onto the sensor bar, it doesn't work.
v=rw where v is the linear velocity of the laser beam projected on sensor array which can be measured, r is the distance from a beacon to the sensor array which we want to know, and ω is the angular velocity of beacon which is constant and known.
With two lenses and one mirror, the beam is directed onto the sensor of a CCD camera (pco.1400).
In its transmission mode, the same microscopy platform changes the position of the CMOS sensor chip and removes the beam-splitter cube (see Fig. 2 ), such that lensfree diffraction holograms of the specimens can be recorded on the sensor-array.
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Justyna Jupowicz-Kozak
CEO of Professional Science Editing for Scientists @ prosciediting.com