Multi Port Serial - Equinox Systems Inc. - Equinox SST-16P PCI Adapter Computer Driver Updates

Description extracted from Wikipedia:

an astronomical event|the celestial coordinates|Equinox (celestial coordinates)|the article about a specific equinox|March equinox|and|September equinox|other uses Use dmy dates|date=July 2019 solstice-equinox thumb|The Sun at the moment of the March equinox in 2019, when the center of the solar disk contacts the celestial equator (the imaginary line on the celestial sphere above Earth's equator) from south to north. An equinox is commonly regarded as the instant of time when the plane (extended indefinitely in all directions) of Earth's equator passes through the geometric center of the Sun's disk. This occurs twice each year, around 20 March and 23 September. In other words, it is the moment at which the center of the visible Sun is directly above the equator. The word is derived from the Latin/i>, from/i> (equal) and/i> (genitive/i>) (night). On the day of an equinox, daytime and nighttime are of approximately equal duration all over the planet. They are not exactly equal, however, due to the angular size of the Sun, atmospheric refraction, and the rapidly changing duration of the length of day that occurs at most latitudes around the equinoxes. Long before conceiving this equality, primitive equatorial cultures noted the day when the Sun rises due east and sets due west, and indeed this happens on the day closest to the astronomically defined event. In the Northern Hemisphere, the March equinox is called the vernal or spring equinox while the September equinox is called the autumnal or fall equinox. In the Southern Hemisphere, the reverse is true. The dates slightly vary due to leap years and other factors. Since the Moon (and to a lesser extent the planets) causes Earth's orbit to slightly vary from a perfect ellipse, the equinox is officially defined by the Sun's more regular ecliptic longitude rather than by its declination. The instants of the equinoxes are currently defined to be when the apparent geocentric longitude of the Sun is 0° and 180°. thumb|The Sun on the equinox as seen from the site of Pizzo Vento, Fondachelli-Fantina, Sicily

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