The Solar Clock
The solar clock is a fascinating excursion into the use of interplanetary energy, being essentially a variant of a cyclic type of mechanical motion using the elastic vibrations of pure epidosite crystals whose oscillation frequencies are more sharply defined and higher than quartz crystals-some 800,000 vibrations per second. That is to say, instead of electrical gearing of any kind of cathode ray, the amplification was of hendiadysiac sympathy or episeismic contact emanating from the constellations of the southern hemisphere or, more specifically, the azimuthal use of Eridanus and Reticulum in crossing the Llhuroscian meridian tentatively identified as New Corwale. As a matter of fact the reconstructed mechanism of this Llhuroscian clock was strikingly similar to present day use of the quartz crystal oscillator: the perforations in the radial dial of the Llhuroscian clock were coated with an alloy similar to elinvar in modulus of elasticity, an arrangement which provided a feedback from a kind of anode circuit much like an old wireless radio. Synchronized with electrical discharges alternately from Eridanus and Reticulum, the temple clock behaved like a tuned grid circuit without the necessity of a valve amplifier and was completely unaffected by either changes of temperature or barometric pressure. In short, the occasion of random error was reduced to less than one part in one trillion. Today we must content ourselves, from the horological point of view, with random error reduction of one part in one thousand million. Ancient horometry offers few examples as bizarre as this clock that signalized the openings of the notorious sexual feasts of the Lokust sect. The erotic figures on the radial dial actually functioned as an ingenious electric gravity escapement, rocking with increasing scope at appointed times for orgiastic rituals. (12)
Another noteworthy Llhuroscian measuring instrument was the combination planispherical astrolabic torquetum. It bears a remarkable resemblance to the earliest working models made by Nasir ad-din at-Tûsi, the thirteenth century Islamic astronomer. In both the Llhuroscian and the Islamic torquetums, the plane projection of the sphere required the observer’s eye to be placed at the South Pole.
This complex Llhuroscian scientific device had many purposes: when the horizontal plate was oriented, it was possible to make measurements at azimuth (angles measured along the horizon); on the eastern rim of this plate one equitorial plate is hinged so that it could be raised to an angle equal to the complement of the latitude of the place where one was working; the curved phrenlix (a type of gnomon) threw shadows which were read in multiples of twenty-seven degrees, fifteen seconds. This complex division permitted a time measurement far more accurate than our prime meridian of Greenwich allows, because it was not limited to the plane of the ecliptic but measured finite convexities versus finite concavities in determining celestial latitudes. All other known astrolabes (sundials) use the singular solar reference.
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