Sunrise

Source: Wikipedia, the free encyclopedia.
For other uses, see Sunrise (disambiguation).
Not to be confused with Dawn.
Sunrise over the ocean in Taiwan

Sunrise (or sunup) is the moment when the upper rim of the Sun appears on the horizon in the morning.[1] The term can also refer to the entire process of the solar disk crossing the horizon.

Terminology

Although the Sun appears to "rise" from the horizon, it is actually the Earth's motion that causes the Sun to appear. The illusion of a moving Sun results from Earth observers being in a

geocentric model, which prevailed until astronomer Nicolaus Copernicus formulated his heliocentric model in the 16th century.[2]

Architect Buckminster Fuller proposed the terms "sunsight" and "sunclipse" to better represent the heliocentric model, though the terms have not entered into common language.[3][4]

Astronomically, sunrise occurs for only an instant: the moment at which the upper limb of the Sun appears tangent to the horizon.[1] However, the term sunrise commonly refers to periods of time both before and after this point:

  • Twilight, the period in the morning during which the sky is brightening, but the Sun is not yet visible. The beginning of morning twilight is called astronomical dawn.
  • The period after the Sun rises during which striking colors and atmospheric effects are still seen.[5] Civil twilight being the brightest, while astronomical twilight being the darkest.

Measurement

Angle with respect to horizon

arcminutes, though this amount varies based on atmospheric conditions.[1]

Also, unlike most other solar measurements, sunrise occurs when the Sun's upper limb, rather than its center, appears to cross the horizon. The apparent radius of the Sun at the horizon is 16 arcminutes.[1]

These two angles combine to define sunrise to occur when the Sun's center is 50 arcminutes below the horizon, or 90.83° from the zenith.[1]

Time of day

See also:
latitude and longitude, altitude, and time zone. These changes are driven by the axial tilt of Earth, daily rotation of the Earth, the planet's movement in its annual elliptical orbit around the Sun, and the Earth and Moon's paired revolutions around each other. The analemma
can be used to make approximate predictions of the time of sunrise.

In late winter and spring, sunrise as seen from temperate latitudes occurs earlier each day, reaching its earliest time near the summer solstice; although the exact date varies by latitude. After this point, the time of sunrise gets later each day, reaching its latest sometime around the winter solstice. The offset between the dates of the solstice and the earliest or latest sunrise time is caused by the eccentricity of Earth's orbit and the tilt of its axis, and is described by the analemma, which can be used to predict the dates.

Variations in atmospheric refraction can alter the time of sunrise by changing its apparent position. Near the poles, the time-of-day variation is exaggerated, since the Sun crosses the horizon at a very shallow angle and thus rises more slowly.[1]

Accounting for atmospheric refraction and measuring from the leading edge slightly increases the average duration of day relative to night. The sunrise equation, however, which is used to derive the time of sunrise and sunset, uses the Sun's physical center for calculation, neglecting atmospheric refraction and the non-zero angle subtended by the solar disc.

Location on the horizon

See also: Sun path and Solar azimuth angle
Timelapse video of twilight and sunrise in
Gjøvik, Norway in February 2021

Neglecting the effects of refraction and the Sun's non-zero size, whenever sunrise occurs, in temperate regions it is always in the northeast quadrant from the March equinox to the September equinox and in the southeast quadrant from the September equinox to the March equinox.[6] Sunrises occur approximately due east on the March and September equinoxes for all viewers on Earth.[7] Exact calculations of the azimuths of sunrise on other dates are complex, but they can be estimated with reasonable accuracy by using the analemma

.

The figure on the right is calculated using the solar geometry routine in Ref.[8] as follows:

  1. For a given latitude and a given date, calculate the declination of the Sun using longitude and
    solar noon
    time as inputs to the routine;
  2. Calculate the sunrise hour angle using the sunrise equation;
  3. Calculate the sunrise time, which is the solar noon time minus the sunrise hour angle in degree divided by 15;
  4. Use the sunrise time as input to the solar geometry routine to get the solar azimuth angle at sunrise.

Hemispheric symmetry

An interesting feature in the figure on the right is apparent hemispheric symmetry in regions where daily sunrise and sunset actually occur.

This symmetry becomes clear if the hemispheric relation in to the sunrise equation is applied to the x- and y-components of the solar vector presented in Ref.[8]

Appearance

Colors

See also: Sunset § Colors
Further information: Atmospheric optics
Sunrise in Lisbon seen from an airplane. Note refraction of colors by both the atmosphere and clouds.
Sunrise in Marengo and Apollo Bay, Victoria, Australia

Air molecules and airborne particles scatter white sunlight as it passes through the Earth's atmosphere. This is done by a combination of Rayleigh scattering and Mie scattering.[9]

As a ray of white sunlight travels through the atmosphere to an observer, some of the colors are scattered out of the beam by air molecules and

airborne particles, changing the final color of the beam the viewer sees. Because the shorter wavelength components, such as blue and green, scatter more strongly, these colors are preferentially removed from the beam.[9]

At sunrise and sunset, when the path through the atmosphere is longer, the blue and green components are removed almost completely, leaving the longer-wavelength orange and red

forward scattering of white light).[13][14][15]

Sunset colors are typically more brilliant than sunrise colors, because the evening air contains more particles than morning air.

volcanic eruptions, trapped within the troposphere, tends to mute sunset and sunrise colors, while volcanic ejecta that is instead lofted into the stratosphere (as thin clouds of tiny sulfuric acid droplets), can yield beautiful post-sunset colors called afterglows and pre-sunrise glows. A number of eruptions, including those of Mount Pinatubo in 1991 and Krakatoa in 1883
, have produced sufficiently high stratospheric sulfuric acid clouds to yield remarkable sunset afterglows (and pre-sunrise glows) around the world. The high altitude clouds serve to reflect strongly reddened sunlight still striking the stratosphere after sunset, down to the surface.

Optical illusions and other phenomena

parhelion
.
  • Atmospheric refraction causes the Sun to be seen while it is still below the horizon.
  • Light from the lower edge of the Sun's disk is refracted more than light from the upper edge. This reduces the apparent height of the Sun when it appears just above the horizon. The width is not affected, so the Sun appears wider than it is high.
  • The Sun appears larger at sunrise than it does while higher in the sky, in a manner similar to the Moon illusion.
  • The Sun appears to rise above the horizon and circle the Earth, but it is actually the Earth that is rotating, with the Sun remaining fixed. This effect results from the fact that an observer on Earth is in a rotating reference frame.
  • Occasionally a
    parhelion belonging to the optical phenomenon family of halos
    .
  • Sometimes just before sunrise or after sunset, a green flash can be seen. This is an optical phenomenon in which a green spot is visible above the Sun, usually for no more than a second or two.[16]

See also

References

  1. ^
    U.S. Naval Observatory. Archived from the original
    on September 27, 2019.
  2. ^ "The Earth Is the Center of the Universe: Top 10 Science Mistakes". Science Channel. Archived from the original on November 18, 2012.
  3. ^ Griffith, Evan. "Celebrating word making: Buckminster Fuller's take on sunrise and sunset". Notes For Creators. Retrieved 2024-02-04.
  4. ^ Skene, Gordon (22 November 2020). "Buckminster Fuller Has A Few Words For You - 1972 - Ford Hall Forum Lecture". Past Daily. Retrieved 2024-02-04.
  5. Merriam-Webster Dictionary
    . 7 February 2024.
  6. ^ Masters, Karen (October 2004). "How does the position of Moonrise and Moonset change? (Intermediate)". Curious About Astronomy? Ask an Astronomer. Cornell University Astronomy Department. Archived from the original on August 22, 2016. Retrieved 2016-08-11.
  7. ^ "Where Do the Sun and Stars Rise?". Stanford Solar Center. Retrieved 2012-03-20.
  8. ^ a b Zhang, T., Stackhouse, P.W., Macpherson, B., and Mikovitz, J.C., 2021. A solar azimuth formula that renders circumstantial treatment unnecessary without compromising mathematical rigor: Mathematical setup, application and extension of a formula based on the subsolar point and atan2 function. Renewable Energy, 172, 1333-1340. DOI: https://doi.org/10.1016/j.renene.2021.03.047
  9. ^
    ISBN 978-3-540-78426-5
    .
  10. ^ a b B. Guenther, ed. (2005). Encyclopedia of Modern Optics. Vol. 1. Elsevier. p. 186.
  11. ^ "Blue Sky". Hyperphysics, Georgia State University. Archived from the original on April 27, 2012. Retrieved 2012-04-07.
  12. ^ a b Craig Bohren (ed.), Selected Papers on Scattering in the Atmosphere, SPIE Optical Engineering Press, Bellingham, WA, 1989
  13. ^ Corfidi, Stephen F. (February 2009). "The Colors of Twilight and Sunset". Norman, OK: NOAA/NWS Storm Prediction Center.
  14. ^ "Atmospheric Aerosols: What Are They, and Why Are They So Important?". NASA. Aug 1, 1996. Archived from the original on August 5, 2012.
  15. ^
    ISBN 0-321-18878-0
    .
  16. ^ "Red Sunset, Green Flash". HyperPhysics Concepts - Georgia State University. Archived from the original on December 15, 2022.

External links

Wikiquote has quotations related to Sunrise.
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