Skip to main content

In 2024, the Great Lakes reach historic lows.

 



In late February or early March each year, the Great Lakes typically witness their annual peak in ice coverage. However, the year 2024 marked an anomaly as the lakes were notably devoid of ice during this period. Unusually warm winter conditions and above-average surface water temperatures contributed to this phenomenon, resulting in historically low ice cover. Satellite-based measurements, dating back to 1973, have consistently recorded an average winter extent exceeding 40 percent ice coverage. Yet, by late February 2024, the ice cover reached only about one-tenth of this average maximum.The VIIRS (Visible Infrared Imaging Radiometer Suite) sensor aboard the Suomi NPP satellite captured this striking image of the lakes on February 24, 2024, highlighting the significant departure from the norm.


The freezing patterns of the Great Lakes exhibit considerable variability, with instances like 2014 witnessing coverage exceeding 80 percent. Nevertheless, a discernible trend has emerged since 1973, indicating a decline in ice levels. Data from NOAA's Great Lakes Environmental Research Laboratory (GLERL) reveals an approximate 5 percent decrease per decade in annual maximum ice coverage. This downward trajectory is attributed to warmer winter conditions prevalent in the Great Lakes region, fostering more frequent occurrences of years with lower ice extents.


Great Lakes,from 1973 to 2024.





The provided chart illustrates the ice coverage during the 2023–2024 winter season (depicted in red) in comparison to the patterns observed over the past 50 winters. The line distinctly reflects the unusually warm start to the current ice season. Typically, the first cold air masses sweep over the upper Midwest in December, initiating the cooling of lake water—a process known as "priming." However, in December 2023, this priming did not occur, leading to the lowest January ice cover on record in 2024. Subsequently, when an arctic chill enveloped much of the U.S. in mid-January, the ice cover reached its probable season maximum, peaking at approximately 16 percent, only to dissipate as warmer temperatures returned.


Jia Wang, an ice climatologist at GLERL, highlights the significant correlation between air temperatures and ice cover over the Great Lakes. Exploring the intricate relationship further, Wang identifies four patterns of climate variability influencing temperatures in the region. In the current year, a noteworthy alignment occurs, with three out of the four patterns—El Niño, the Atlantic Multidecadal Oscillation, and the Pacific Decadal Oscillation—simultaneously contributing to warming effects on the Great Lakes, further impacting the observed patterns of ice cover.


The absence of ice on the Great Lakes not only renders shorelines and infrastructure more vulnerable to damage from powerful wind and waves but also exposes certain fish species to increased risk during their spawning season, lacking the protective barrier that ice cover typically provides against predators. Moreover, the repercussions extend to water levels, as diminished ice cover may facilitate heightened evaporation. As of late February, however, NOAA reported no significant impact on water levels. The similarity between lake and air temperatures has contributed to keeping evaporation rates low, mitigating potential consequences on water levels at this point in the season.


As the Great Lakes ice season extends through March, NOAA experts suggest the potential for sporadic bursts of arctic air that could induce periods of ice formation. Despite this possibility, these cold air events are anticipated to be transient, and a significant shift in weather patterns would be necessary to reverse the current below-average trend in ice coverage for this season. The NASA Earth Observatory images, credited to Michala Garrison and Lauren Dauphin, utilize VIIRS data from NASA EOSDIS LANCE, GIBS/Worldview, along with lake ice data from NOAA's Great Lakes Environmental Research Laboratory. The story is credited to Lindsey Doermann.


Comments

Popular posts from this blog

NASA/ESA Hubble Space Telescope Reveals New Details of the Orion Nebula’s Star Formation.

  This NASA/ESA Hubble Space Telescope image captures the Orion Nebula (Messier 42, M42), the nearest star-forming region to Earth, located about 1,500 light-years away. A captivating new image captured by the NASA/ESA Hubble Space Telescope offers an extraordinary look into the Orion Nebula, the nearest massive star-forming region to Earth. Located just 1,500 light-years away, this nebula is visible to the naked eye below the three stars forming Orion's "belt." The region is home to hundreds of newborn stars, including two protostars featured in the image: HOPS 150 and HOPS 153. Named after the Herschel Orion Protostar Survey, conducted with ESA’s Herschel Space Observatory, the protostars HOPS 150 and HOPS 153 provide key insights into the early stages of star formation. HOPS 150, visible in the upper-right corner of the image, is a binary star system, with two young stars orbiting one another. These protostars are surrounded by small dusty disks, where material from th...

New Method Detects Small Asteroids in Main Belt, Offering Insight for Planetary Defense.

  An international team of physicists, led by MIT researchers, has developed a groundbreaking method to detect small asteroids, as small as 10 meters in diameter, within the main asteroid belt. These space rocks, ranging from the size of a bus to several stadiums wide, were previously undetectable using traditional methods. The team's discovery, detailed in a paper published in Nature, could significantly improve tracking of potential asteroid impactors, aiding planetary defense efforts. The main asteroid belt, located between Mars and Jupiter, is home to millions of asteroids, but until now, scientists could only detect objects roughly a kilometer in diameter. The new detection technique, which utilizes the "shift and stack" method, is able to identify much smaller asteroids, even those far from Earth, enabling more precise orbital tracking. This breakthrough is crucial for planetary defense, allowing scientists to spot near-Earth objects that may pose a threat in the fu...

XSPECT Payload Successfully Validates Performance through Cas A Observation.

  The XSPECT instrument captures a detailed spectrum of the supernova remnant Cassiopeia A (Cas A), encompassing both the Galactic Cosmic Ray (GCR) background and the Cosmic X-ray Background (CXB). The flux observed above 8 keV predominantly results from the combined contributions of CXB and GCR. The presented spectrum, depicted in the figure, is derived from a cumulative integration time of 20 ksec, collected across multiple orbits, providing valuable insights into the X-ray emissions associated with Cas A. XPoSat, India's inaugural X-ray polarimetric mission, has achieved a significant as the XSPECT instrument captures its initial observations from the Cassiopeia A (Cas A) supernova remnant. Launched on January 1, 2024, XPoSat is equipped with two co-aligned instruments, namely the POLarimeter Instrument in X-rays (POLIX) and X-ray SPECtroscopy and Timing (XSPECT). This mission is designed to unravel the mysteries of cosmic X-ray sources. While POLIX focuses on examining X-ray po...