File:GOES East Observes the Vernal Equinox As the Seasons Shift (NESDIS 2024-03-20).webm
Original file (WebM audio/video file, VP9, length 12 s, 1,080 × 1,080 pixels, 33.36 Mbps overall, file size: 46.96 MB)
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[edit]DescriptionGOES East Observes the Vernal Equinox As the Seasons Shift (NESDIS 2024-03-20).webm |
English: Spring has officially arrived in the Northern Hemisphere, while the Southern Hemisphere is embracing autumn. The start of astronomical spring, known as the vernal equinox, occurred yesterday, March 19, 2024, at 11:06 p.m. EDT. During equinoxes, which happen twice a year, the Earth's axis is not tilted toward or away from the sun, resulting in nearly equal periods of daylight and darkness worldwide. The term "equinox" is derived from Latin, meaning "equal night," indicating the balance between day and night during these events. At the equator, the sun shines directly overhead at noon during equinoxes due to this alignment. The "nearly" equal hours of day and night is due to refraction of sunlight, or a bending of the light's rays, that causes the sun to appear above the horizon when the actual position of the sun is below the horizon. Additionally, the days become a little longer at higher latitudes farther from the equator, because it takes the sun longer to rise and set. Seasonal changes are driven by the Earth's axial tilt of 23.5 degrees as it orbits the sun, exposing different hemispheres to varying sunlight angles and durations throughout the year. Equinoxes mark the moments when the sun rises due east and sets due west for most places on Earth. In the Northern Hemisphere, meteorological spring is based on temperature cycles and runs from March 1 until May 31, while astronomical spring shifts to summer on the summer solstice, which this year will occur on June 20 at 4:50 p.m. EDT. NOAA's GOES-16 and GOES-18 satellites, positioned above the equator, track the Earth's surface and observe the terminator—the edge between the shadows of nightfall and the sunlight of dusk and dawn—providing insights into seasonal changes throughout the year. The slope of the terminator curve changes with the seasons. During an equinox, the terminator is a straight north-south line over the equator. This animation was created by taking one GeoColor image a day for a year from GOES East, captured at 11:50 UTC each day, and stringing them together. From their position 22,236 miles above the equator, the GOES satellites orbit at the same rate Earth rotates, so they can keep constant watch over the same region. The GOES East geostationary satellite, also known as GOES-16, keeps watch over most of North America, including the contiguous United States and Mexico, as well as Central and South America, the Caribbean, and the Atlantic Ocean to the west coast of Africa. The GOES West satellite, also known as GOES-18, provides geostationary satellite coverage of the Western Hemisphere, including the United States, the Pacific Ocean, Alaska and Hawaii. |
Date | 20 March 2024 (upload date) |
Source | GOES East Observes the Vernal Equinox As the Seasons Shift |
Author | NOAA |
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[edit]Public domainPublic domainfalsefalse |
This image is in the public domain because it contains materials that originally came from the U.S. National Oceanic and Atmospheric Administration, taken or made as part of an employee's official duties.
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current | 23:19, 23 June 2024 | 12 s, 1,080 × 1,080 (46.96 MB) | OptimusPrimeBot (talk | contribs) | Imported media from https://www.nesdis.noaa.gov/s3/2024-03/geocolor_terminator-sways.mp4 |
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