Before and after the equinox, the subsolar point migrates north or south. After the March equinox, the subsolar point migrates north as the Northern Hemisphere tilts toward the sun. Around June 21, the subsolar point hits the Tropic of Cancer, (23.5°N). This is the June solstice, after which the subsolar point begins to migrate south.
Full Answer
Before and after the equinox, the subsolar point migrates north or south. After the March equinox, the subsolar point migrates north as the Northern Hemisphere tilts toward the sun. Around June 21, the subsolar point hits the Tropic of Cancer, (23.5°N). This is the June solstice, after which the subsolar point begins to migrate south.
The Equator, at 0° latitude, receives a maximum intensity of the sun’s rays all year. As a result, areas near Earth’s Equator experience relatively constant sunlight and little equinoctial variation.
In the Southern Hemisphere, sun outages occur after the March equinox and before the September equinox. During an equinox, the sun is align ed directly behind satellites in geostationary orbit at the Equator.
Only during an equinox is the Earth's 23.5° axis not tilting toward or away from the sun: the perceived center of the Sun’s disk is in the same plane as the Equator. Before and after the equinox, the subsolar point migrates north or south.
Around June 21, the subsolar point hits the Tropic of Cancer, (23.5°N). This is the June solstice, after which the subsolar point begins to migrate south. After the September equinox, the subsolar point continues to move south as the Southern Hemisphere tilts toward the sun. Around December 21, the subsolar point hits the Tropic ...
Seasonal variation increases with latitude. Atmospheric refraction also increases the disparity in the “equinox” length of day and night. At about 30° latitude, day is about eight minutes longer than night. Polar Regions.
An equinox is an event in which a planet ’s subsolar point passes through its Equator. The equinoxes are the only time when both the Northern and Southern Hemisphere s experience roughly equal amounts of daytime and nighttime.
On Earth, there are two equinoxes every year: one around March 21 and another around September 22. Sometimes, the equinoxes are nicknamed the “ vernal equinox ” (spring equinox) and the “ autumnal equinox ” (fall equinox), although these have different dates in the Northern and Southern Hemispheres.
During the equinoxes, solar declination is 0°. Solar declination describes the latitude of the Earth where the sun is directly overhead at noon. (The Equator, of course, is 0° latitude.) So, equinoxes are the only times of the year when the subsolar point is directly on the Equator.
Around December 21, the subsolar point hits the Tropic of Capricorn (23.5°S). This is the December solstice. As its name suggests, an equinox indicates equally illuminate d hemisphere s, with the solar terminator equally dividing the Earth from north to south.
During an equinox, the sun is align ed directly behind satellites in geostationary orbit at the Equator. Situated directly above the subsolar point, the satellites are flooded with direct solar radiation. This solar radiation can interfere with and even stop satellites from transmit ting signals.