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  2. Solar zenith angle - Wikipedia

    en.wikipedia.org/wiki/Solar_zenith_angle

    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. [1] [2] 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. [3]

  3. Position of the Sun - Wikipedia

    en.wikipedia.org/wiki/Position_of_the_Sun

    At one date in the year, the Sun would be directly overhead at the North Pole, so its declination would be +90°. For the next few months, the subsolar point would move toward the South Pole at constant speed, crossing the circles of latitude at a constant rate, so that the solar declination would decrease linearly with time. Eventually, the ...

  4. Shadows (software) - Wikipedia

    en.wikipedia.org/wiki/Shadows_(software)

    Drawing of the style to scale 1, ready to be cut out; Tables of coordinates of hour lines and declination lines; Drawing of declination arcs and hour lines (solar or mean time), with or without longitude correction; Moveable, resizable text frames, with list of pre-installed mottoes; Drawing of the curve of equation of time, in various shapes

  5. Sunrise equation - Wikipedia

    en.wikipedia.org/wiki/Sunrise_equation

    The equation above neglects the influence of atmospheric refraction (which lifts the solar disc — i.e. makes the solar disc appear higher in the sky — by approximately 0.6° when it is on the horizon) and the non-zero angle subtended by the solar disc — i.e. the apparent diameter of the sun — (about 0.5°). The times of the rising and ...

  6. Solar longitude - Wikipedia

    en.wikipedia.org/wiki/Solar_longitude

    Solar longitude, commonly abbreviated as Ls, is the ecliptic longitude of the Sun, i.e. the position of the Sun on the celestial sphere along the ecliptic. It is also an effective measure of the position of the Earth (or any other Sun-orbiting body) in its orbit around the Sun, [ 1 ] usually taken as zero at the moment of the vernal equinox . [ 2 ]

  7. Solar eclipse will create Purkinje effect — and red, green ...

    www.aol.com/solar-eclipse-create-purkinje-effect...

    The upcoming total solar eclipse will create the Purkinje effect. Red and green clothes can bring out a greater impact. according to science. Solar eclipse will create Purkinje effect — and red ...

  8. 2024 solar eclipse will create Purkinje effect: Why you ...

    www.aol.com/2024-solar-eclipse-create-purkinje...

    Here's when some Ohio cities along its path can expect the total eclipse to being, and how long it will last: Hamilton -- Begins at 3:09:09 p.m., will last 1 minute, 42 seconds.. Dayton -- 3:09:29 ...

  9. Sun path - Wikipedia

    en.wikipedia.org/wiki/Sun_path

    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. [4] [5] 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. [6]