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

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

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

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<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

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

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

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<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 actual 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.

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A 22° halo is an atmospheric optical phenomenon that consists of a halo with an apparent diameter of approximately 22° around the Sun or Moon. Around the Sun, it may also be called a sun halo. Around the Moon, it is also known as a moon ring, storm ring, or winter halo. It forms as sunlight or moonlight is refracted by millions of hexagonal ice crystals suspended in the atmosphere. Its radius, as viewed from Earth, is roughly the length of an outstretched hand at arm's length.

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

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

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<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

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