NASA’s Solar Dynamics Observatory captured this image of a solar flare — as seen in the bright flash toward the upper middle area of the Sun — on May 2, 2024. The image shows a subset of extreme ultraviolet light that highlights the extremely hot material in flares and which is colorized in teal. Credit: NASA/SDO
The Sun emitted a strong solar flare, peaking at 10:22 p.m. ET on May 2, 2024. <span class="glossaryLink" aria-describedby="tt" data-cmtooltip="
NASA
Established in 1958, the National Aeronautics and Space Administration (NASA) is an independent agency of the United States Federal Government that succeeded the National Advisory Committee for Aeronautics (NACA). It is responsible for the civilian space program, as well as aeronautics and aerospace research. Its vision is "To discover and expand knowledge for the benefit of humanity." Its core values are "safety, integrity, teamwork, excellence, and inclusion." NASA conducts research, develops technology and launches missions to explore and study Earth, the solar system, and the universe beyond. It also works to advance the state of knowledge in a wide range of scientific fields, including Earth and space science, planetary science, astrophysics, and heliophysics, and it collaborates with private companies and international partners to achieve its goals.
” data-gt-translate-attributes=”[{“attribute”:”data-cmtooltip”, “format”:”html”}]” tabindex=”0″ role=”link”>NASA’s Solar Dynamics Observatory, which watches the Sun constantly, captured an image of the event.
Solar flares are intense bursts of radiation emanating from the release of magnetic energy associated with sunspots. These flares are among the biggest explosive events in our solar system, visible primarily in the ultraviolet range.
Flares impact Earth in a variety of ways: they can disrupt the ionosphere and interfere with <span class="glossaryLink" aria-describedby="tt" data-cmtooltip="
GPS
GPS, or Global Positioning System, is a satellite-based navigation system that provides location and time information anywhere on or near the Earth's surface. It consists of a network of satellites, ground control stations, and GPS receivers, which are found in a variety of devices such as smartphones, cars, and aircraft. GPS is used for a wide range of applications including navigation, mapping, tracking, and timing, and has an accuracy of about 3 meters (10 feet) in most conditions.
” data-gt-translate-attributes=”[{“attribute”:”data-cmtooltip”, “format”:”html”}]” tabindex=”0″ role=”link”>GPS navigation and radio communications. They are also responsible for auroras, the beautiful natural light displays often seen in high-latitude skies.
This flare is classified as an X1.6 flare. X-class denotes the most intense flares, while the number provides more information about its strength.
Solar flares are rated based on their intensity and potential impact on Earth. The classification system consists of five categories: A, B, C, M, and X. Each category has a tenfold increase in energy output compared to the previous one, with A being the weakest and X the strongest. Within each letter class, there is a finer scale from 1 to 9. For example, an X1 flare is weaker than an X2 flare, but significantly stronger than an M5 flare. This classification helps scientists and relevant agencies predict potential impacts and prepare for space weather-related disruptions.
Artist’s concept image of the SDO satellite orbiting Earth. Credit: NASA
NASA’s Solar Dynamics Observatory
NASA’s Solar Dynamics Observatory (SDO) is a mission dedicated to understanding the origins of solar activity and its impacts on Earth. Launched in February 2010, the SDO is a critical part of NASA’s Living With a Star (LWS) program, which aims to develop the scientific understanding necessary to effectively address those aspects of the connected Sun-Earth system that directly affect life and society.
The observatory is equipped with a suite of instruments that provide observations leading to a deeper understanding of the solar atmosphere’s dynamics. These instruments are capable of capturing ultra-high-definition images of the Sun in 13 different wavelengths every few seconds. The key instruments include the Atmospheric Imaging Assembly (AIA), which produces images of the solar corona and chromosphere; the Helioseismic and Magnetic Imager (HMI), which studies the solar surface and magnetic activity; and the Extreme Ultraviolet Variability Experiment (EVE), which measures the Sun’s ultraviolet output.
The data collected by the SDO has been instrumental in improving our ability to forecast space weather events, such as solar flares and coronal mass ejections, which can affect satellite operations, communications, power grids, and navigation systems on Earth. Through continuous monitoring, the SDO plays a pivotal role in our ongoing efforts to understand the complex solar processes that influence our daily lives and technological infrastructure.