That completely depends on your latitude ... where you are on earth north or south relative to the equator.
-- If your latitude is 23.5° south ... on the Tropic of Capricorn ... the noon sun is directly overhead
on December 21.
-- If you are more than 23.5° south of the equator, then the noon sun is (113.5° - your south latitude)
above the northern horizon.
-- If you are between the equator and 23.5° south latitude, the noon sun is (66.5° + your south latitude)
above the southern horizon.
-- If you are north of the equator, the noon sun is (66.5° - your north latitude) above the southern horizon.
Notice that this means that anywhere north of 66.5° north latitude ... the Arctic Circle ... the sun doesn't
rise at all on that day, even at noon.
At noon on June 21st at 41 degrees north latitude, the sun's altitude would be at its highest point of the day, which would be approximately 68.5 degrees above the horizon. This is the highest altitude the sun will reach in the sky during the summer solstice at this latitude.
For an observer at latitude 35 degrees, the highest the sun can ever be in his sky is roughly 31.5 degrees above the horizon.
both september and march because they both contain equinoxes which is when the sun is at the highest altitude
As the altitude of the Sun increases, the Sun appears higher in the sky. This leads to increased intensity of sunlight, shorter shadows, and higher temperatures on the Earth's surface. It also indicates that it is closer to noon.
The seasonal variation in the altitude of the noon sun affects the amount of energy received at the Earth's surface because when the sun is higher in the sky, the energy is more concentrated over a smaller area, leading to more intense heating. Conversely, when the sun is lower in the sky, the energy is more spread out over a larger area, resulting in less intense heating. This variation in intensity of solar radiation influences the temperature and climate patterns on Earth.
the tilt goes towards the sun, the seasons chang from winter to summer
First, we need the "transit altitude" of the celestial equator, at 80 degrees north. That's 90 - 80 degrees = 10 degrees. At noon (local apparent noon) the Sun's altitude will be: 10 degrees + the Sun's declination. That's the altitude of the Sun's "upper culmination". At "midnight" (the Sun's "lower culmination") the Sun's altitude will be: the Sun's declination - 10 degrees. So, the difference in altitude is 20 degrees. The Sun is 20 degrees higher at noon.
Both
The altitude of the sun is the angle between the sun and the observer's horizontal plane. It changes throughout the day as the sun rises and sets. At solar noon, when the sun is at its highest point in the sky, the altitude is its maximum.
At noon on June 21st at 41 degrees north latitude, the sun's altitude would be at its highest point of the day, which would be approximately 68.5 degrees above the horizon. This is the highest altitude the sun will reach in the sky during the summer solstice at this latitude.
For an observer at latitude 35 degrees, the highest the sun can ever be in his sky is roughly 31.5 degrees above the horizon.
3
the sun rises in the west and sets in the east.
i donnt knowww
-The two extremes of angles are on June 21st where the sun is at its highest noon and on December 21st where the sun is at its lowest noon.
The sun's altitude refers to its angle above the horizon, measured in degrees. This angle varies throughout the day and changes with the seasons due to the tilt of the Earth's axis and its orbit around the sun. At solar noon, the sun reaches its highest point in the sky for that day, which is when its altitude is at its maximum. The altitude can be calculated using the observer's latitude, the date, and the time of day.
both september and march because they both contain equinoxes which is when the sun is at the highest altitude