Antisolar point

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A rainbow has 42deg centered around the antisolar point, which always coincides with the shadow of the observer's eye/camera, seen here at the bottom of the frame. Double-alaskan-rainbow.jpg
A rainbow has 42° centered around the antisolar point, which always coincides with the shadow of the observer's eye/camera, seen here at the bottom of the frame.
Centered on the antisolar point, this photo features various antisolar/subhorizon haloes, as viewed from a plane. Subparhelic circle flickr fdecomite.jpg
Centered on the antisolar point, this photo features various antisolar/subhorizon haloes, as viewed from a plane.

The antisolar point is the abstract point on the celestial sphere directly opposite the Sun from an observer's perspective. [1] This means that the antisolar point lies above the horizon when the Sun is below it, and vice versa. On a sunny day, the antisolar point can be easily found; it is located within the shadow of the observer's head. Like the zenith and nadir, the antisolar point is not fixed in three-dimensional space, but is defined relative to the observer. Each observer has an antisolar point that moves as the observer changes position.

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The antisolar point forms the geometric center of several optical phenomena, including subhorizon haloes, rainbows, [2] glories, [3] the Brocken spectre, and heiligenschein. Occasionally, around sunset or sunrise, anticrepuscular rays appear to converge toward the antisolar point near the horizon. [4] However, this is an optical illusion caused by perspective; in reality, the "rays" (i.e. bands of shadow) run near-parallel to each other. [5]

Also around the antisolar point, the gegenschein is often visible in a moonless night sky away from city lights, arising from the backscatter of sunlight by interplanetary dust. In astronomy, the full Moon or a planet in opposition lies near the antisolar point. During a total lunar eclipse, the full Moon enters the umbra of Earth's shadow, which the planet casts onto its atmosphere, into space, and toward the antisolar point.

Anthelic point

The anthelic point is often used as a synonym for the antisolar point, but the two should be differentiated. [1] While the antisolar point is directly opposite the sun, always below the horizon when the sun is up, the anthelic point is opposite but at the same elevation as the sun, and is therefore located on the parhelic circle. There are several halo phenomena that are centered on or converge on the anthelic point, such as the anthelion, Wegener arcs, Tricker arcs and the parhelic circle itself. [6] [7] [8]

See also

Related Research Articles

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A glory is an optical phenomenon, resembling an iconic saint's halo around the shadow of the observer's head, caused by sunlight or moonlight interacting with the tiny water droplets that comprise mist or clouds. The glory consists of one or more concentric, successively dimmer rings, each of which is red on the outside and bluish towards the centre. Due to its appearance, the phenomenon is sometimes mistaken for a circular rainbow, but the latter has a much larger diameter and is caused by different physical processes.

<span class="mw-page-title-main">Sun dog</span> Atmospheric optical phenomenon

A sun dog or mock sun, also called a parhelion in meteorology, is an atmospheric optical phenomenon that consists of a bright spot to one or both sides of the Sun. Two sun dogs often flank the Sun within a 22° halo.

<span class="mw-page-title-main">Halo (optical phenomenon)</span> Optical phenomenon of the sky

A halo is an optical phenomenon produced by light interacting with ice crystals suspended in the atmosphere. Halos can have many forms, ranging from colored or white rings to arcs and spots in the sky. Many of these appear near the Sun or Moon, but others occur elsewhere or even in the opposite part of the sky. Among the best known halo types are the circular halo, light pillars, and sun dogs, but many others occur; some are fairly common while others are extremely rare.

<span class="mw-page-title-main">Anticrepuscular rays</span> Meteorological optical phenomenon

Anticrepuscular rays, or antisolar rays, are meteorological optical phenomena similar to crepuscular rays, but appear opposite the Sun in the sky. Anticrepuscular rays are essentially parallel, but appear to converge toward the antisolar point, the vanishing point, due to a visual illusion from linear perspective.

<span class="mw-page-title-main">Sunbeam</span> Rays of sunlight that appear to radiate from the point in the sky where the sun is located

A sunbeam, in meteorological optics, is a beam of sunlight that appears to radiate from the position of the Sun. Shining through openings in clouds or between other objects such as mountains and buildings, these beams of particle-scattered sunlight are essentially parallel shafts separated by darker shadowed volumes. Their apparent convergence in the sky is a visual illusion from linear perspective. The same illusion causes the apparent convergence of parallel lines on a long straight road or hallway at a distant vanishing point. The scattering particles that make sunlight visible may be air molecules or particulates.

<span class="mw-page-title-main">Heiligenschein</span> Optical phenomenon

Heiligenschein is an optical phenomenon in which a bright spot appears around the shadow of the viewer's head in the presence of dew. In photogrammetry and remote sensing, it is more commonly known as the hotspot. It is also occasionally known as Cellini's halo after the Italian artist and writer Benvenuto Cellini (1500–1571), who described the phenomenon in his memoirs in 1562.

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

An anthelion is a rare optical phenomenon of the halo family. It appears on the parhelic circle opposite to the Sun as a faint white spot, not unlike a sundog, and may be crossed by an X-shaped pair of diffuse arcs.

<span class="mw-page-title-main">Rainbow</span> Meteorological phenomenon

A rainbow is an optical phenomenon that can occur under certain meteorological conditions. It is caused by reflection, refraction and dispersion of light in water droplets resulting in an effect similar to a spectrum of light appearing in the sky. It takes the form of a multicoloured circular arc. Rainbows caused by sunlight always appear in the section of sky directly opposite the Sun.

<span class="mw-page-title-main">Belt of Venus</span> Atmospheric phenomenon

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<span class="mw-page-title-main">Circumhorizontal arc</span> Optical phenomenon

A circumhorizontal arc is an optical phenomenon that belongs to the family of ice halos formed by the refraction of sunlight or moonlight in plate-shaped ice crystals suspended in the atmosphere, typically in cirrus or cirrostratus clouds. In its full form, the arc has the appearance of a large, brightly spectrum-coloured band running parallel to the horizon, located far below the Sun or Moon. The distance between the arc and the Sun or Moon is twice as far as the common 22-degree halo. Often, when the halo-forming cloud is small or patchy, only fragments of the arc are seen. As with all halos, it can be caused by the Sun as well as the Moon.

<span class="mw-page-title-main">Circumzenithal arc</span> Optical phenomenon arising from refraction of sunlight through ice crystals

The circumzenithal arc, also called the circumzenith arc (CZA), upside-down rainbow, and the Bravais arc, is an optical phenomenon similar in appearance to a rainbow, but belonging to the family of halos arising from refraction of sunlight through ice crystals, generally in cirrus or cirrostratus clouds, rather than from raindrops. The arc is located at a considerable distance above the observed Sun and at most forms a quarter of a circle centered on the zenith. It has been called "a smile in the sky", its first impression being that of an upside-down rainbow. The CZA is one of the brightest and most colorful members of the halo family. Its colors, ranging from violet on top to red at the bottom, are purer than those of a rainbow because there is much less overlap in their formation.

<span class="mw-page-title-main">Subparhelic circle</span>

The subparhelic circle is a rare halo, an optical phenomenon, located below the horizon. It passes through both the subsun and the antisolar point. The subparhelic circle is the subhorizon counterpart to the parhelic circle, located above the horizon.

A subhelic arc is a rare halo, formed by internal reflection through ice crystals, that curves upwards from the horizon and touches the tricker arc above the anthelic point. Subhelic arcs are a result of ray entrance and exit through prism end faces with two intermediate internal reflections.

<span class="mw-page-title-main">Aureole effect</span>

The aureole effect or water aureole is an optical phenomenon similar to Heiligenschein, creating sparkling light and dark rays radiating from the shadow of the viewer's head. This effect is seen only over a rippling water surface. The waves act as lenses to focus and defocus sunlight: focused sunlight produces the lighter rays, while defocused sunlight produces the darker rays. Suspended particles in the water help make the aureole effect more pronounced. The effect extends a greater angular distance from the viewer's shadow when the viewer is higher above the water, and can sometimes be seen from a plane.

<span class="mw-page-title-main">Atmospheric optics</span> Study of the optical characteristics of the atmosphere or products of atmospheric processes

Atmospheric optics is "the study of the optical characteristics of the atmosphere or products of atmospheric processes .... [including] temporal and spatial resolutions beyond those discernible with the naked eye". Meteorological optics is "that part of atmospheric optics concerned with the study of patterns observable with the naked eye". Nevertheless, the two terms are sometimes used interchangeably.

<span class="mw-page-title-main">Earth's shadow</span> Shadow that Earth itself casts through its atmosphere and into outer space

Earth's shadow is the shadow that Earth itself casts through its atmosphere and into outer space, toward the antisolar point. During the twilight period, the shadow's visible fringe – sometimes called the dark segment or twilight wedge – appears as a dark and diffuse band just above the horizon, most distinct when the sky is clear.

<span class="mw-page-title-main">Optical phenomena</span> Observable events that result from the interaction of light and matter

Optical phenomena are any observable events that result from the interaction of light and matter.

The Sevenfold Sun Miracle was an atmospheric phenomenon witnessed in Gdańsk in 1661. It was a complex halo phenomenon, and was described by Georg Fehlau, the pastor of the St Marien church, in a sermon two weeks later, which was then published under the title Siebenfältiges Sonnenwunder oder sieben Nebensonnen, so in diesem 1661 Jahr den 20. Februar neuen Stils am Sonntage Sexagesima um 11 Uhr bis nach 12 am Himmel bei uns sind gesehen worden The same event was also described by the astronomer Johan Hevelius the following year in his book Mercurius in Sole visus Gedani.

References

  1. 1 2 Herd, Tim (2007). "Angular Measurements in the sky" . Kaleidoscope Sky. Abrams. p.  27. ISBN   081099397X.
  2. Cowley, Les. "Primary rainbows". atoptics.co.uk. Retrieved 13 September 2013.
  3. Cowley, Les. "The Glory". atoptics.co.uk.
  4. Cowley, Les. "Anticrepuscular rays". atoptics.co.uk. Retrieved 13 September 2013.
  5. Cowley, Les. "Antisolar or anticrepuscular rays". atoptics.co.uk.
  6. Alexander Wünsche; Jim Foster, Anthelion and anthelic arcs, 2006
  7. Walter Tape, Atmospheric Halos, ISSN   0066-4634, ISBN   0875908349, American Geophysical Union, 1994, p. 27
  8. Les Cowley. South Pole Halos – Anthelic View – Atmospheric Optics Archived 2015-09-23 at the Wayback Machine , accessed 13 September 2013