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By Seares F.H.

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Extra resources for A Simple Method for Determining the Colors of the Stars (1916)(en)(5s)

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Similarly, the front (FFM) positioner adjusts the FFM signal by moving the photodiode elements in and out (used for FFM, to be described later). The preamp board contains preamplifier circuits for all four photodetecter signals and a laser diode power supply circuit. : (A) front view, (B) optical head, (C) base, and (D) cantilever substrate mounted on cantilever mount (not to scale). 19D, and the deflection beam reflecting mirror is mounted on the upper left in the interior of the head which reflects the deflected beam toward the photodiode.

Thus the friction force was measured by measuring the current that was required to hold the tip stationary. This design was modified later by Kaneko et al. (1991). The major modifications in the design are that (1) the sample is no longer supported by a parallel-leaf spring unit and is directly mounted to a piezotube scanner (which may give more stability while scanning the sample), and the tube scanner is used instead of piezoelectric tripod to move the sample, (2) the friction force (tip motion) is sensed by the voltage difference applied between two parallel electrodes rather than the current passing a coil around a magnet, and (3) the tip is mounted on a single-leaf spring.

22. Either the sample must be larger in diameter than the three support posts or the sample must be rigidly mounted to a larger substrate. Scan lengths of this instrument are 75 and 125 µm. In these units, the sample is stationary. 22A and B. Because the cantilever beam and detector assembly are scanned instead of the sample, some vibration is introduced and lateral resolution of this instrument is reduced. In the stand-alone AFMs, a single photodetector instead of split photodiode detector is used.

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A Simple Method for Determining the Colors of the Stars (1916)(en)(5s) by Seares F.H.

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