The major component of the sun's angle at any particular location, at noon, is the season. The sun is at its highest at the summer solstice (about June 21 in the northern hemisphere) and lowest at the winter solstice (about December 21).
Far into the polar areas, the angle of the sun may be so low that even at noon it is still just below the horizon.
In the tropics, the angle of the sun remains very high at noon throughout the year.
The minor component of the sun's angle at noon is caused by Earth's elliptical orbit. Noon may be slightly before or after the sun reaches its highest point for the day. The measurement for this is usually shown by a figure-8 symbol on globes which is traditionally drawn over the Pacific Ocean near Ecuador.
A final component is the alignment of time zones. Few places in the world set noon as the sun's highest point (as was traditional before about 1800) - time zones are used to establish a single time and the sun's highest point may be many minutes before or after noon within a time zone.
Variation in the values of a variable dependent upon the time of the year is seasonal variation. A variable having seasonal variation exhibits a pattern that repeats after exactly one year.
Some ozone is found at all elevations. The ozone layer is in the lower stratosphere, and is still a wide range of elevations, and has latitude and seasonal dependency as well.
The location on Earth with the least seasonal changes is typically found near the equator, particularly in regions like parts of Colombia, Ecuador, and the Democratic Republic of the Congo. These areas experience a tropical climate characterized by consistent temperatures and high humidity throughout the year, with minimal variation in daylight and little to no significant seasonal shifts. Rainfall patterns may vary, but overall, the climate remains relatively stable, avoiding the extreme seasonal changes seen in temperate regions.
Seasonal variations in temperature and day length are greatest at higher latitudes, particularly in polar regions like Antarctica and the Arctic Circle. Here, temperatures can fluctuate dramatically between summer and winter, and day length can vary from 24 hours of sunlight in summer to complete darkness in winter. Conversely, the least seasonal variation occurs near the equator, where temperatures remain relatively consistent year-round, and day length remains fairly constant, resulting in minimal seasonal changes.
The seasonal variations of temperature and day length are least at the equator. Here, temperatures remain relatively constant throughout the year, averaging around 25-30°C (77-86°F), and day length is consistently about 12 hours, with minimal variation. This stability is due to the direct overhead sun and the consistent climate patterns characteristic of tropical regions. Consequently, equatorial areas experience less pronounced seasonal changes compared to higher latitudes.
seasonal variation means seasonal sex variation...... got my dear. sudharu
Variation in the values of a variable dependent upon the time of the year is seasonal variation. A variable having seasonal variation exhibits a pattern that repeats after exactly one year.
secular trend, seasonal variation, cyclical variation, and irregular variation
what is the seasonal variation for amazon rainforest
Planets experience seasonal variation due to the axial tilt. Mars is most like ours and has seasons.
One circumstance in which braided streams form is at the end of a glacier where there is a large seasonal variation in dicharge.
VENUS
yes
cyclical variation: Piece to piece variation. Often used to describe a repeating pattern, such as a seasonal variation in sales that peaks before Christmas.
No, it is not.
Seasonal variation is associated with axial tilt. Mercury, Venus, and Jupiter have very slight inclination, thus nearly erasing any seasonal variation. Mercury also lacks an atmosphere, so it wouldn't experience "seasons" even if it possessed tilt.
The major cause for seasonal temperature variation at any given latitude on Earth is the tilt of the Earth's axis relative to its orbit around the sun. This tilt causes different areas to receive varying amounts of sunlight throughout the year, leading to changes in temperature.