On June 1, 2024, NASA's Solar Dynamics Observatory (SDO) captured images of two X-Class solar flares. One flare was an X1.4, peaking at 4:48 a.m. ET, and the other was an X1.0, peaking at 2:36 p.m. Solar flares are intense bursts of radiation caused by the release of built-up magnetic energy on the Sun's surface. These flares can impact Earth's communications, power sources, and navigation systems. The ejected solar energy, known as coronal mass ejections (CMEs), can result in geomagnetic storms and generate northern and southern lights. Understanding solar flares is crucial for forecasting space weather events and protecting Earth's technological systems. The SDO, launched on February 11, 2010, is dedicated to studying the solar atmosphere and provides continuous data for predicting space weather events [8b35db46], [35aedcd1].
The recent solar flares captured by NASA's SDO highlight the ongoing activity and intensity of the Sun's magnetic field. These flares release bursts of radiation and magnetic energy, which can disrupt power grids, communication networks, and navigation systems on Earth. The study of solar flares and their impact on space weather is essential for better preparation and mitigation strategies [7c1b7547].