Sun Paths

The sun's trajectory in the sky, known as its solar altitude or elevation angle, undergoes variations based on your geographical position relative to the equator and the time of year. This difference can be observed when comparing locations farther from the equator with those closer.

Lattitude Variation

Locations farther from the equator exhibit a distinct sun path compared to places closer to it. For instance, in Los Angeles, which is situated at a higher latitude in the Northern Hemisphere, the sun typically follows a different path than in regions near the equator.

Seasonal Oscillation

In locations farther from the equator, such as Los Angeles, you'll notice more pronounced seasonal changes in the sun's trajectory. During the summer months (around June 21st), the sun takes a higher path, resulting in extended daylight hours and a steeper angle of sunlight. Conversely, during the winter months (around December 21st), the sun follows a lower trajectory, leading to shorter daylight hours and a shallower angle of sunlight. In contrast, areas closer to the equator experience relatively consistent day lengths and solar angles throughout the year.

Solar Noon

The timing of solar noon varies in different regions, with locations closer to the equator experiencing more consistent solar noon times throughout the year.

Twilight Duration

The duration of twilight, the period preceding sunrise and following sunset, also varies depending on your latitude, with regions farther from the equator experiencing shorter twilight periods during certain times of the year.