Shadows (software)

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Shadows is a software package for the calculation and drawing of sundials and astrolabes, available as a freeware in its base level.

Contents

It has been developed by François Blateyron, software developer and amateur astronomer, who made it available on Internet since 1997 and continues to improve it. [1] It is used worldwide by thousands of sundial enthusiasts. [2] It is compatible with Windows 11/10, 8.x and 7. Shadows is available in three levels: Shadows is a freeware; Since version 3.0, it also supports the creation of astrolabes.

Description

Shadows calculates various types of sundials:

as well as astrolabes:

Shadows is software restricted to the Windows operating system. It is simple to use but does not aim to be universal. It draws the sundial on screen and prints it to various scales to act as a template during fabrication. The sundials show solar time and can include longitude correction and equation of time. It also can draw ancient or unequal hours such as Italian and Babylonian and even draw azimuth and altitude curves. It has an animation feature so the shadow of the style can be simulated on the screen. The results can be copied as an image or a vector graphics (metafile or DXF) for use in CAD programs or machine tools.

In 2005, the French astronomical society, Société Astronomique de France (SAF) awarded Blateyron with the Julien Saget prize for the Shadows software. [3]

The Astrolabes are interactive and can be manipulated on screen by rotating the Rete and the Alidade using the mouse.

Several curves and graphs are available: equation of time, solar graph with horizon mask, duration of the day, direction rose. It is now available in French, English, German, Spanish, Italian, Portuguese, Brazilian Portuguese, Dutch, Hungarian, Slovenian, Greek, Polish and Russian- the translation were provided by the users.[ citation needed ]

Features of the three levels of Shadows

Shadows is supplied in three versions.

Vertical sundial drawn by Shadows. Vertical sundial.png
Vertical sundial drawn by Shadows.

Shadows: Freeware version

Shadows Expert: Intermediate version, shareware

Analemmatic sundial drawn by Shadows Expert. Analemmatic sundial.png
Analemmatic sundial drawn by Shadows Expert.

(in addition to standard Shadows features)

Planispheric astrolabe drawn by Shadows Pro. Planispheric astrolabe.png
Planispheric astrolabe drawn by Shadows Pro.

Shadows Pro: Full version, shareware

(in addition to Shadows Expert features)

History of versions

See also

Related Research Articles

<span class="mw-page-title-main">Horizontal coordinate system</span> Type of celestial coordinate system

The horizontal coordinate system is a celestial coordinate system that uses the observer's local horizon as the fundamental plane to define two angles of a spherical coordinate system: altitude and azimuth. Therefore, the horizontal coordinate system is sometimes called the az/el system, the alt/az system, or the alt-azimuth system, among others. In an altazimuth mount of a telescope, the instrument's two axes follow altitude and azimuth.

<span class="mw-page-title-main">Sundial</span> Device that tells the time of day by the apparent position of the Sun in the sky

A sundial is a horological device that tells the time of day when direct sunlight shines by the apparent position of the Sun in the sky. In the narrowest sense of the word, it consists of a flat plate and a gnomon, which casts a shadow onto the dial. As the Sun appears to move through the sky, the shadow aligns with different hour-lines, which are marked on the dial to indicate the time of day. The style is the time-telling edge of the gnomon, though a single point or nodus may be used. The gnomon casts a broad shadow; the shadow of the style shows the time. The gnomon may be a rod, wire, or elaborately decorated metal casting. The style must be parallel to the axis of the Earth's rotation for the sundial to be accurate throughout the year. The style's angle from horizontal is equal to the sundial's geographical latitude.

<span class="mw-page-title-main">Astrolabe</span> Astronomical instrument

An astrolabe is an astronomical instrument dating to ancient times. It serves as a star chart and physical model of visible heavenly bodies. Its various functions also make it an elaborate inclinometer and an analog calculation device capable of working out several kinds of problems in astronomy. In its simplest form it is a metal disc with a pattern of wires, cutouts, and perforations that allows a user to calculate astronomical positions precisely. It is able to measure the altitude above the horizon of a celestial body, day or night; it can be used to identify stars or planets, to determine local latitude given local time, to survey, or to triangulate. It was used in classical antiquity, the Islamic Golden Age, the European Middle Ages and the Age of Discovery for all these purposes.

<span class="mw-page-title-main">Analemma</span> Diagrammatic representation of Suns position over a period of time

In astronomy, an analemma is a diagram showing the position of the Sun in the sky as seen from a fixed location on Earth at the same mean solar time, as that position varies over the course of a year. The diagram will resemble a figure eight. Globes of Earth often display an analemma as a two-dimensional figure of equation of time vs. declination of the Sun.

<span class="mw-page-title-main">Scaphe</span> Sundial said to have been invented by Aristarchus

The scaphe was a sundial said to have been invented by Aristarchus of Samos. There are no original works still in existence by Aristarchus, but the adjacent picture is an image of what it might have looked like; only his would have been made of stone. It consisted of a hemispherical bowl which had a vertical gnomon placed inside it, with the top of the gnomon level with the edge of the bowl. Twelve gradations inscribed perpendicular to the hemisphere indicated the hour of the day.

<span class="mw-page-title-main">Equation of time</span> Apparent solar time minus mean solar time

The equation of time describes the discrepancy between two kinds of solar time. The word equation is used in the medieval sense of "reconciliation of a difference". The two times that differ are the apparent solar time, which directly tracks the diurnal motion of the Sun, and mean solar time, which tracks a theoretical mean Sun with uniform motion along the celestial equator. Apparent solar time can be obtained by measurement of the current position of the Sun, as indicated by a sundial. Mean solar time, for the same place, would be the time indicated by a steady clock set so that over the year its differences from apparent solar time would have a mean of zero.

The solar zenith angle is the zenith angle of the sun, i.e., the angle between the sun’s rays and the vertical direction. It is the complement to the solar altitude or solar elevation, which is the altitude angle or elevation angle between the sun’s rays and a horizontal plane. At solar noon, the zenith angle is at a minimum and is equal to latitude minus solar declination angle. This is the basis by which ancient mariners navigated the oceans.

<span class="mw-page-title-main">Ibn al-Shatir</span> Arab astronomer and clockmaker (1304–1375)

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<span class="mw-page-title-main">Analemmatic sundial</span>

Analemmatic sundials are a type of horizontal sundial that has a vertical gnomon and hour markers positioned in an elliptical pattern. The gnomon is not fixed and must change position daily to accurately indicate time of day. Hence there are no hour lines on the dial and the time of day is read only on the ellipse. As with most sundials, analemmatic sundials mark solar time rather than clock time.

Polar alignment is the act of aligning the rotational axis of a telescope's equatorial mount or a sundial's gnomon with a celestial pole to parallel Earth's axis.

<span class="mw-page-title-main">Quadrant (instrument)</span> Navigation instrument

A quadrant is an instrument used to measure angles up to 90°. Different versions of this instrument could be used to calculate various readings, such as longitude, latitude, and time of day. Its earliest recorded usage was in ancient India in Rigvedic times by Rishi Atri to observe a solar eclipse. It was then proposed by Ptolemy as a better kind of astrolabe. Several different variations of the instrument were later produced by medieval Muslim astronomers. Mural quadrants were important astronomical instruments in 18th-century European observatories, establishing a use for positional astronomy.

<span class="mw-page-title-main">Sun path</span> Arc-like path that the Sun appears to follow across the sky

Sun path, sometimes also called day arc, refers to the daily and seasonal arc-like path that the Sun appears to follow across the sky as the Earth rotates and orbits the Sun. The Sun's path affects the length of daytime experienced and amount of daylight received along a certain latitude during a given season.

<span class="mw-page-title-main">Astronomical rings</span> Early astronomical instrument

Astronomical rings, also known as Gemma's rings, are an early astronomical instrument. The instrument consists of three rings, representing the celestial equator, declination, and the meridian.

<span class="mw-page-title-main">History of sundials</span>

A sundial is a device that indicates time by using a light spot or shadow cast by the position of the Sun on a reference scale. As the Earth turns on its polar axis, the sun appears to cross the sky from east to west, rising at sun-rise from beneath the horizon to a zenith at mid-day and falling again behind the horizon at sunset. Both the azimuth (direction) and the altitude (height) can be used to create time measuring devices. Sundials have been invented independently in every major culture and became more accurate and sophisticated as the culture developed.

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<span class="mw-page-title-main">Position of the Sun</span> Calculating the Suns location in the sky at a given time and place

The position of the Sun in the sky is a function of both the time and the geographic location of observation on Earth's surface. As Earth orbits the Sun over the course of a year, the Sun appears to move with respect to the fixed stars on the celestial sphere, along a circular path called the ecliptic.

<span class="mw-page-title-main">Bifilar sundial</span>

A bifilar dial is a type of sundial invented by the German mathematician Hugo Michnik in 1922. It has two non-touching threads parallel to the dial. Usually the second thread is orthogonal-(perpendicular) to the first. The intersection of the two threads' shadows gives the local apparent time.

A schema for horizontal dials is a set of instructions used to construct horizontal sundials using compass and straightedge construction techniques, which were widely used in Europe from the late fifteenth century to the late nineteenth century. The common horizontal sundial is a geometric projection of an equatorial sundial onto a horizontal plane.

<span class="mw-page-title-main">Schema for vertical declining dials</span>

Vertical declining dials are sundials that indicate local apparent time. Vertical south dials are a special case: as are vertical north, vertical east and vertical west dials. The word declining means that the wall is offset from one of these 4 cardinal points. There are dials that are not vertical, and these are called reclining dials.

References