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      • In terms of solar time, noon is the moment when the Sun crosses the local meridian and reaches its highest position in the sky, except at the poles. This version of noon is also called solar noon or high noon.
      www.timeanddate.com/astronomy/solar-noon.html
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  2. At true solar noon, the Sun is exactly at the meridian. This means that solar time is the same for all locations on the same meridian. True solar time is obtained from civil time as follows: Civil time - Time zone = UTC (mean solar time on Greenwich meridian) UTC + Longitude shift = Mean solar time Mean solar time + Equation of time = True ...

  3. en.wikipedia.org › wiki › Solar_timeSolar time - Wikipedia

    A tall pole vertically fixed in the ground casts a shadow on any sunny day. At one moment during the day, the shadow will point exactly north or south (or disappear when and if the Sun moves directly overhead). That instant is called local apparent noon, or 12:00 local apparent time. About 24 hours later the shadow will again point north ...

  4. Jul 19, 2017 · Twelve noon local solar time (LST) is defined as when the sun is highest in the sky. Local time (LT) usually varies from LST because of the eccentricity of the Earth's orbit, and because of human adjustments such as time zones and daylight saving.

    • What Is The Meridian?
    • Solar Noon
    • Solar Noon Shadows
    • Clock Noon Versus Solar Noon
    • Here’s How You Do it.

    In the jargon of astronomers and celestial navigators, your local meridian is an imaginary semi-circle that crosses your sky’s dome from due north to due south. The point where the sun crosses that arc – when the sun is highest for that day – is variously called solar noon, or midday, or high noon, or local noon or just plain noon. An astronomer mi...

    At solar noon, the sun can be at one of three places: at zenith (straight overhead), north of zenith or south of zenith. At temperate latitudesin the Northern Hemisphere, the noonday sun is never at zenith but is always found in the southern sky. At temperate latitudes in the Southern Hemisphere, the noonday sun is never at zenith but is always fou...

    The shortest shadow of the day comes at solar noon, or when the sun transits your local meridian. North of the Tropic of Cancer, the noonday shadow always points due north. South of the tropic of Capricorn, the noonday shadow always points due south.

    Generally speaking, noon by the sun and noon by the clock seldom agree. Noon by the sun is a natural phenomenon, based on the sun’s highest point for the day. Noon as defined by the sun long preceded the invention of clocks and the introduction of time zones. Needless to say, noon by the sun also preceded so-called daylight saving time or summer ti...

    Place a plumb or vertical stick into the ground. Note the length of any morning shadow. Then wait until the shadow reaches this same length in the afternoon. Bisect this angle to find due north (or due south). For a fuller explanation, click into MySundial online and scroll down to 4. The “Method of Equal Altitudes.” Don’t want to try this at home?...

  5. Our latitude and longitude page will help you to find the input data you need for our unique Solar Noon Calculator. The time of solar noon depends on the Equation of Time and on the difference in longitude between your location and the standard meridian of the time zone you are in.

  6. The Hour Angle converts the local solar time (LST) into the number of degrees which the sun moves across the sky. By definition, the Hour Angle is 0° at solar noon. Since the Earth rotates 15° per hour, each hour away from solar noon corresponds to an angular motion of the sun in the sky of 15°.

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