The most commonly observed sundials are those in which the shadow-casting style is fixed in position and aligned with the Earth's rotational axis, being oriented with
true north and south, and making an angle with the horizontal equal to the geographical latitude. This axis is aligned with the
celestial poles, which is closely, but not perfectly, aligned with the
pole star Polaris. For illustration, the celestial axis points vertically at the true
North Pole, whereas it points horizontally on the
equator. The world's largest axial gnomon sundial is the mast of the
Sundial Bridge at Turtle Bay in
Redding, California. A formerly world's largest gnomon is at
Jaipur, raised 26°55′ above horizontal, reflecting the local latitude. On any given day, the Sun appears to rotate uniformly about this axis, at about 15° per hour, making a full circuit (360°) in 24 hours. A linear gnomon aligned with this axis will cast a sheet of shadow (a half-plane) that, falling opposite to the Sun, likewise rotates about the celestial axis at 15° per hour. The shadow is seen by falling on a receiving surface that is usually flat, but which may be spherical, cylindrical, conical or of other shapes. If the shadow falls on a surface that is symmetrical about the celestial axis (as in an armillary sphere, or an equatorial dial), the surface-shadow likewise moves uniformly; the hour-lines on the sundial are equally spaced. However, if the receiving surface is not symmetrical (as in most horizontal sundials), the surface shadow generally moves non-uniformly and the hour-lines are not equally spaced; one exception is the Lambert dial described below. Some types of sundials are designed with a fixed gnomon that is not aligned with the celestial poles like a vertical obelisk. Such sundials are covered below under the section, "Nodus-based sundials".
Empirical hour-line marking The formulas shown in the paragraphs below allow the positions of the hour-lines to be calculated for various types of sundial. In some cases, the calculations are simple; in others they are extremely complicated. There is an alternative, simple method of finding the positions of the hour-lines which can be used for many types of sundial, and saves a lot of work in cases where the calculations are complex. This is an empirical procedure in which the position of the shadow of the gnomon of a real sundial is marked at hourly intervals. The
equation of time must be taken into account to ensure that the positions of the hour-lines are independent of the time of year when they are marked. An easy way to do this is to set a clock or watch so it shows "sundial time" which is
standard time, plus the equation of time on the day in question. The hour-lines on the sundial are marked to show the positions of the shadow of the style when this clock shows whole numbers of hours, and are labelled with these numbers of hours. For example, when the clock reads 5:00, the shadow of the style is marked, and labelled "5" (or "V" in
Roman numerals). If the hour-lines are not all marked in a single day, the clock must be adjusted every day or two to take account of the variation of the equation of time.
Equatorial sundials , London (1973) an equinoctial dial by
Wendy Taylor , Beijing. The gnomon points
true north and its angle with horizontal equals the local
latitude. Closer inspection of the
full-size image reveals the "spider-web" of date rings and hour-lines. The distinguishing characteristic of the
equatorial dial (also called the
equinoctial dial) is the planar surface that receives the shadow, which is exactly perpendicular to the gnomon's style. This plane is called equatorial, because it is parallel to the equator of the Earth and of the celestial sphere. If the gnomon is fixed and aligned with the Earth's rotational axis, the sun's apparent rotation about the Earth casts a uniformly rotating sheet of shadow from the gnomon; this produces a uniformly rotating line of shadow on the equatorial plane. Since the Earth rotates 360° in 24 hours, the hour-lines on an equatorial dial are all spaced 15° apart (360/24). : H_E = 15^{\circ}\times t\text{ (hours)} ~. The uniformity of their spacing makes this type of sundial easy to construct. If the dial plate material is opaque, both sides of the equatorial dial must be marked, since the shadow will be cast from below in winter and from above in summer. With translucent dial plates (e.g. glass) the hour angles need only be marked on the sun-facing side, although the hour numberings (if used) need be made on both sides of the dial, owing to the differing hour schema on the sun-facing and sun-backing sides. Another major advantage of this dial is that equation of time (EoT) and daylight saving time (DST) corrections can be made by simply rotating the dial plate by the appropriate angle each day. This is because the hour angles are equally spaced around the dial. For this reason, an equatorial dial is often a useful choice when the dial is for public display and it is desirable to have it show the true local time to reasonable accuracy. The EoT correction is made via the relation : \text{Correction}^{\circ} = \frac{\text{EoT (minutes)} + 60 \times \Delta \text{DST (hours)}}{4} ~. Near the
equinoxes in spring and autumn, the sun moves on a circle that is nearly the same as the equatorial plane; hence, no clear shadow is produced on the equatorial dial at those times of year, a drawback of the design. A
nodus is sometimes added to equatorial sundials, which allows the sundial to tell the time of year. On any given day, the shadow of the nodus moves on a circle on the equatorial plane, and the radius of the circle measures the
declination of the sun. The ends of the gnomon bar may be used as the nodus, or some feature along its length. An ancient variant of the equatorial sundial has only a nodus (no style) and the concentric circular hour-lines are arranged to resemble a spider-web.
Horizontal sundials . June 17, 2007 at 12:21. 44°51′39.3″N, 93°36′58.4″W In the
horizontal sundial (also called a
garden sundial), the plane that receives the shadow is aligned horizontally, rather than being perpendicular to the style as in the equatorial dial. Hence, the line of shadow does not rotate uniformly on the dial face; rather, the hour lines are spaced according to the rule. :\ \tan H_H = \sin L\ \tan \left(\ 15^{\circ} \times t\ \right)\ Or in other terms: : \ H_H = \tan^{-1}\left[\ \sin L\ \tan(\ 15^{\circ} \times t\ )\ \right] where L is the sundial's geographical
latitude (and the angle the gnomon makes with the dial plate), \ H_H\ is the angle between a given hour-line and the noon hour-line (which always points towards
true north) on the plane, and is the number of hours before or after noon. For example, the angle \ H_H\ of the 3 hour-line would equal the
arctangent of since tan 45° = 1. When \ L = 90^\circ\ (at the
North Pole), the horizontal sundial becomes an equatorial sundial; the style points straight up (vertically), and the horizontal plane is aligned with the equatorial plane; the hour-line formula becomes \ H_H = 15^\circ \times t\ , as for an equatorial dial. A horizontal sundial at the Earth's
equator, where \ L = 0^\circ\ , would require a (raised) horizontal style and would be an example of a polar sundial (see below). in London, United Kingdom The chief advantages of the horizontal sundial are that it is easy to read, and the sunlight lights the face throughout the year. All the hour-lines intersect at the point where the gnomon's style crosses the horizontal plane. Since the style is aligned with the Earth's rotational axis, the style points
true north and its angle with the horizontal equals the sundial's geographical latitude . A sundial designed for one
latitude can be adjusted for use at another latitude by tilting its base upwards or downwards by an angle equal to the difference in latitude. For example, a sundial designed for a latitude of 40° can be used at a latitude of 45°, if the sundial plane is tilted upwards by 5°, thus aligning the style with the Earth's rotational axis. Many ornamental sundials are designed to be used at 45 degrees north. Some mass-produced garden sundials fail to correctly calculate the
hourlines and so can never be corrected. A local standard
time zone is nominally 15 degrees wide, but may be modified to follow geographic or political boundaries. A sundial can be rotated around its style (which must remain pointed at the celestial pole) to adjust to the local time zone. In most cases, a rotation in the range of 7.5° east to 23° west suffices. This will introduce error in sundials that do not have equal hour angles. To correct for
daylight saving time, a face needs two sets of numerals or a correction table. An informal standard is to have numerals in hot colors for summer, and in cool colors for winter. Since the hour angles are not evenly spaced, the equation of time corrections cannot be made via rotating the dial plate about the gnomon axis. These types of dials usually have an equation of time correction tabulation engraved on their pedestals or close by. Horizontal dials are commonly seen in gardens, churchyards and in public areas.
Vertical sundials (
Norfolk, UK) . The left and right dials face south and east, respectively. Both styles are parallel, their angle to the horizontal equaling the latitude. The east-facing dial is a polar dial with parallel hour-lines, the dial-face being parallel to the style. In the common
vertical dial, the shadow-receiving plane is aligned vertically; as usual, the gnomon's style is aligned with the Earth's axis of rotation. As in the horizontal dial, the line of shadow does not move uniformly on the face; the sundial is not
equiangular. If the face of the vertical dial points directly south, the angle of the hour-lines is instead described by the formula: : \tan H_V = \cos L\ \tan(\ 15^{\circ} \times t\ )\ where is the sundial's geographical
latitude, \ H_V\ is the angle between a given hour-line and the noon hour-line (which always points due north) on the plane, and is the number of hours before or after noon. For example, the angle \ H_V\ of the 3 hour-line would equal the
arctangent of since The shadow moves
counter-clockwise on a south-facing vertical dial, whereas it runs clockwise on horizontal and equatorial north-facing dials. Dials with faces perpendicular to the ground and which face directly south, north, east, or west are called
vertical direct dials. It is widely believed, and stated in respectable publications, that a vertical dial cannot receive more than twelve hours of sunlight a day, no matter how many hours of daylight there are. However, there is an exception. Vertical sundials in the tropics which face the nearer pole (e.g. north facing in the zone between the Equator and the Tropic of Cancer) can actually receive sunlight for more than 12 hours from sunrise to sunset for a short period around the time of the summer solstice. For example, at latitude 20° North, on June 21, the sun shines on a north-facing vertical wall for 13 hours, 21 minutes. Vertical sundials which do
not face directly south (in the northern hemisphere) may receive significantly less than twelve hours of sunlight per day, depending on the direction they do face, and on the time of year. For example, a vertical dial that faces due East can tell time only in the morning hours; in the afternoon, the sun does not shine on its face. Vertical dials that face due East or West are
polar dials, which will be described below. Vertical dials that face north are uncommon, because they tell time only during the spring and summer, and do not show the midday hours except in tropical latitudes (and even there, only around midsummer). For non-direct vertical dials – those that face in non-cardinal directions – the mathematics of arranging the style and the hour-lines becomes more complicated; it may be easier to mark the hour lines by observation, but the placement of the style, at least, must be calculated first; such dials are said to be
declining dials. , Czech Republic; the observer is facing almost due north. Vertical dials are commonly mounted on the walls of buildings, such as town-halls,
cupolas and church-towers, where they are easy to see from far away. In some cases, vertical dials are placed on all four sides of a rectangular tower, providing the time throughout the day. The face may be painted on the wall, or displayed in inlaid stone; the gnomon is often a single metal bar, or a tripod of metal bars for rigidity. If the wall of the building faces
toward the south, but does not face due south, the gnomon will not lie along the noon line, and the hour lines must be corrected. Since the gnomon's style must be parallel to the Earth's axis, it always "points"
true north and its angle with the horizontal will equal the sundial's geographical latitude; on a direct south dial, its angle with the vertical face of the dial will equal the
colatitude, or 90° minus the latitude.
Polar dials (
Spain) In
polar dials, the shadow-receiving plane is aligned
parallel to the gnomon-style. Thus, the shadow slides sideways over the surface, moving perpendicularly to itself as the Sun rotates about the style. As with the gnomon, the hour-lines are all aligned with the Earth's rotational axis. When the Sun's rays are nearly parallel to the plane, the shadow moves very quickly and the hour lines are spaced far apart. The direct East- and West-facing dials are examples of a polar dial. However, the face of a polar dial need not be vertical; it need only be parallel to the gnomon. Thus, a plane inclined at the angle of latitude (relative to horizontal) under the similarly inclined gnomon will be a polar dial. The perpendicular spacing of the hour-lines in the plane is described by the formula : X = H\ \tan(\ 15^{\circ} \times t\ )\ where is the height of the style above the plane, and is the time (in hours) before or after the center-time for the polar dial. The center time is the time when the style's shadow falls directly down on the plane; for an East-facing dial, the center time will be 6 , for a West-facing dial, this will be 6 , and for the inclined dial described above, it will be noon. When approaches ±6 hours away from the center time, the spacing diverges to
+∞; this occurs when the Sun's rays become parallel to the plane.
Vertical declining dials , the hour lines are asymmetrical about noon, with the morning hour-lines ever more widely spaced. , Istanbul, dating back to the late 16th century. It is on the southwest facade with an azimuth angle of 52° N. A
declining dial is any non-horizontal, planar dial that does not face in a cardinal direction, such as (true)
north,
south,
east or
west. As usual, the gnomon's style is aligned with the Earth's rotational axis, but the hour-lines are not symmetrical about the noon hour-line. For a vertical dial, the angle \ H_\text{VD}\ between the noon hour-line and another hour-line is given by the formula below. Note that \ H_\text{VD}\ is defined positive in the clockwise sense w.r.t. the upper vertical hour angle; and that its conversion to the equivalent solar hour requires careful consideration of which quadrant of the sundial that it belongs in. : \tan H_\text{VD} = \frac{\cos L}{\ \cos D\ \cot(\ 15^{\circ} \times t\ ) - s_o\ \sin L\ \sin D\ } where \ L\ is the sundial's geographical
latitude; is the time before or after noon; \ D\ is the angle of declination from true
south, defined as positive when east of south; and \ s_o\ is a switch integer for the dial orientation. A partly south-facing dial has an \ s_o\ value of those partly north-facing, a value of When such a dial faces south (\ D = 0^{\circ}\ ), this formula reduces to the formula given above for vertical south-facing dials, i.e. :\ \tan H_\text{V} = \cos L\ \tan(\ 15^{\circ} \times t\ )\ When a sundial is not aligned with a cardinal direction, the substyle of its gnomon is not aligned with the noon hour-line. The angle \ B\ between the substyle and the noon hour-line is given by the formula
Reclining dials of the
Federal University of Rio de Janeiro, Brazil. The sundials described above have gnomons that are aligned with the Earth's rotational axis and cast their shadow onto a plane. If the plane is neither vertical nor horizontal nor equatorial, the sundial is said to be
reclining or
inclining. Such a sundial might be located on a south-facing roof, for example. The hour-lines for such a sundial can be calculated by slightly correcting the horizontal formula above :\ \tan H_{RV} = \cos(\ L + R\ )\ \tan(\ 15^{\circ} \times t\ )\ where \ R\ is the desired angle of reclining relative to the local vertical, is the sundial's geographical latitude, \ H_{RV}\ is the angle between a given hour-line and the noon hour-line (which always points due north) on the plane, and is the number of hours before or after noon. For example, the angle \ H_{RV}\ of the 3pm hour-line would equal the
arctangent of since When (in other words, a south-facing vertical dial), we obtain the vertical dial formula above. Some authors use a more specific nomenclature to describe the orientation of the shadow-receiving plane. If the plane's face points downwards towards the ground, it is said to be
proclining or
inclining, whereas a dial is said to be
reclining when the dial face is pointing away from the ground. Many authors also often refer to reclined, proclined and inclined sundials in general as inclined sundials. It is also common in the latter case to measure the angle of inclination relative to the horizontal plane on the sun side of the dial. In such texts, since \ I = 90^\circ + R\ , the hour angle formula will often be seen written as : : \tan H_{RV} = \sin(L + I)\ \tan(\ 15^{\circ} \times t\ )\ The angle between the gnomon style and the dial plate, B, in this type of sundial is : : B = 90^{\circ} - (L + R) or : : B = 180^{\circ} - (L + I)
Declining-reclining dials/ Declining-inclining dials Some sundials both decline and recline, in that their shadow-receiving plane is not oriented with a cardinal direction (such as
true north or true south) and is neither horizontal nor vertical nor equatorial. For example, such a sundial might be found on a roof that was not oriented in a cardinal direction. The formulae describing the spacing of the hour-lines on such dials are rather more complicated than those for simpler dials. There are various solution approaches, including some using the methods of rotation matrices, and some making a 3D model of the reclined-declined plane and its vertical declined counterpart plane, extracting the geometrical relationships between the hour angle components on both these planes and then reducing the trigonometric algebra. One system of formulas for Reclining-Declining sundials: (as stated by Fennewick) The angle \ H_\text{RD}\ between the noon hour-line and another hour-line is given by the formula below. Note that \ H_\text{RD}\ advances counterclockwise with respect to the zero hour angle for those dials that are partly south-facing and clockwise for those that are north-facing. :\ \tan H_\text{RD} = \frac{\ \cos R\ \cos L - \sin R\ \sin L\ \cos D - s_o \sin R \sin D \cot(15^{\circ} \times t)\ }{\ \cos D\ \cot(15^{\circ} \times t) - s_o \sin D\ \sin L }\ within the parameter ranges : \ D and -90^{\circ} Or, if preferring to use inclination angle, \ I\ , rather than the reclination, \ R\ , where \ I = (90^{\circ} + R)\ : :\ \tan H_\text{RD} = \frac{\ \sin I\ \cos L + \cos I\ \sin L\ \cos D + s_o \cos I\ \sin D\ \cot(15^{\circ} \times t)\ }{\ \cos D\ \cot(15^{\circ} \times t\ ) - s_o \sin D\ \sin L\ }\ within the parameter ranges : \ D and ~~ 0^{\circ} Here \ L\ is the sundial's geographical latitude; \ s_o\ is the orientation switch integer; is the time in hours before or after noon; and \ R\ and \ D\ are the angles of reclination and declination, respectively. Note that \ R\ is measured with reference to the vertical. It is positive when the dial leans back towards the horizon behind the dial and negative when the dial leans forward to the horizon on the Sun's side. Declination angle \ D\ is defined as positive when moving east of true south. Dials facing fully or partly south have \ s_o = +1\ , while those partly or fully north-facing have an \ s_o = -1 ~. Since the above expression gives the hour angle as an arctangent function, due consideration must be given to which quadrant of the sundial each hour belongs to before assigning the correct hour angle. Unlike the simpler vertical declining sundial, this type of dial does not always show hour angles on its sunside face for all declinations between east and west. When a Northern Hemisphere partly south-facing dial reclines back (i.e. away from the Sun) from the vertical, the gnomon will become co-planar with the dial plate at declinations less than due east or due west. Likewise for Southern Hemisphere dials that are partly north-facing. Were these dials reclining forward, the range of declination would actually exceed due east and due west. In a similar way, Northern Hemisphere dials that are partly north-facing and Southern Hemisphere dials that are south-facing, and which lean forward toward their upward pointing gnomons, will have a similar restriction on the range of declination that is possible for a given reclination value. The critical declination \ D_c\ is a geometrical constraint which depends on the value of both the dial's reclination and its latitude : :\ \cos D_c = \tan R\ \tan L = - \tan L\ \cot I\ As with the vertical declined dial, the gnomon's substyle is not aligned with the noon hour-line. The general formula for the angle \ B\ , between the substyle and the noon-line is given by : :\ \tan B = \frac {\sin D}{\sin R\ \cos D + \cos R\ \tan L} = \frac {\sin D}{\ \cos I\ \cos D - \sin I\ \tan L\ }\ The angle \ G\ , between the style and the plate is given by : :\ \sin G = \cos L\ \cos D\ \cos R - \sin L\ \sin R = - \cos L\ \cos D\ \sin I + \sin L\ \cos I\ Note that for \ G = 0^{\circ}\ , i.e. when the gnomon is coplanar with the dial plate, we have : :\ \cos D = \tan L\ \tan R = - \tan L\ \cot I\ i.e. when \ D = D_c\ , the critical declination value. However, some equiangular sundials – such as the Lambert dial described below – are based on other principles. In the
equatorial bow sundial, the gnomon is a bar, slot or stretched wire parallel to the celestial axis. The face is a semicircle, corresponding to the equator of the sphere, with markings on the inner surface. This pattern, built a couple of meters wide out of temperature-invariant steel
invar, was used to keep the trains running on time in France before World War I. Among the most precise sundials ever made are two equatorial bows constructed of
marble found in
Yantra mandir. This collection of sundials and other astronomical instruments was built by Maharaja
Jai Singh II at his then-new capital of
Jaipur, India between 1727 and 1733. The larger equatorial bow is called the
Samrat Yantra (The Supreme Instrument); standing at 27 meters, its shadow moves visibly at 1 mm per second, or roughly a hand's breadth (6 cm) every minute.
Cylindrical, conical, and other non-planar sundials Other non-planar surfaces may be used to receive the shadow of the gnomon. As an elegant alternative, the style (which could be created by a hole or slit in the circumference) may be located on the circumference of a cylinder or sphere, rather than at its central axis of symmetry. In that case, the hour lines are again spaced equally, but at
twice the usual angle, due to the geometrical
inscribed angle theorem. This is the basis of some modern sundials, but it was also used in ancient times; In another variation of the polar-axis-aligned cylindrical, a cylindrical dial could be rendered as a helical ribbon-like surface, with a thin gnomon located either along its center or at its periphery. ==Movable-gnomon sundials==