At either of the tropics the sun's rays are most directly overhead at mid-day in mid summer.
The sun's rays strike Earth most directly at the equator, where sunlight is more concentrated due to the curvature of the Earth and the angle of incidence. The sun's rays strike Earth least directly at the poles, where sunlight is spread out over a larger surface area and travels through a thicker layer of atmosphere, resulting in lower intensity.
The temperature rises most from direct rays because they are more concentrated than slanted rays. Direct rays hit the Earth's surface more directly, leading to more heat absorption compared to slanted rays that are spread over a larger area.
Directly is near the equator. Least directly is at the poles.
The rays of the Sun fall more directly on the equator because the Sun shines more on the center of the Earth.
The rays of the sun strike most directly on the equator, resulting in more intense heat and sunlight in that region. As you move towards the poles, the angle of the sun's rays becomes more oblique, leading to less direct sunlight and lower temperatures. In the temperate zone, the angle of the sun's rays varies seasonally, leading to differences in sunlight intensity. Over oceans, the angle of the sun's rays can also vary but tends to be more consistent compared to over land areas.
the equater A+ 90 degrees
90 degrees
The sun's rays are always directly overhead somewhere on earth. Twice a year,at the moment of each equinox, that place is somewhere on the equator.
The rays of the sun strike the Earth most directly at the equator, where sunlight is nearly perpendicular to the surface. This results in more concentrated heat and higher temperatures in these regions.
The Sun's rays strike least directly at the poles.
The sun is most directly overhead near the equator. This happens during the equinoxes where the sun is directly above the equator, resulting in near-vertical rays at noon.
During an equinox, the sun's rays are most direct at the Earth's equator. This is because during an equinox, the tilt of the Earth's axis is such that the sun is directly over the equator, leading to equal day and night lengths at all latitudes.