What powers a solar flare? Solar Orbiter is finally giving us answers to this long-standing mystery.The mission caught a 'magnetic avalanche' on the surface of the Sun just before a flare was released
Solar Orbiter Delivers Critical Data Amidst Early 2026 Solar Peak Activity
Edited by: Tetiana Martynovska 17
The joint European Space Agency (ESA) and NASA Solar Orbiter mission continues to provide essential scientific data in January 2026, operating during a period of heightened solar intensity. This collaborative project is tasked with investigating the mechanisms by which the Sun generates and governs the heliosphere, the magnetic envelope surrounding the Solar System. Solar Orbiter's operational profile enables it to capture high-latitude observations from a vantage point closer to the Sun than previously possible, a capability vital for advancing solar and heliospheric physics.
The spacecraft, launched on February 10, 2020, from Cape Canaveral aboard an Atlas V 411 rocket, utilizes a highly elliptical orbit that brings it within one-quarter of Earth's distance to the star. Data acquisition proved particularly significant following a major solar event in early 2026. On January 18, 2026, an X-class solar flare erupted, followed by a powerful Coronal Mass Ejection (CME) that impacted Earth the following day, January 19, 2026. This impact precipitated a severe geomagnetic storm, registered as S4 on the GOES scale, marking one of the most intense radiation events recorded in over two decades, comparable to the October 2003 Halloween storms.
The National Oceanic and Atmospheric Administration's (NOAA) Space Weather Prediction Center (SWPC) confirmed the S4 (severe) status, which carries potential risks for satellite operations, aviation, and power grids. The mission's value is further evidenced by its successful long-term tracking of solar features. An international team combined Solar Orbiter observations with data from NASA's Solar Dynamics Observatory (SDO) to track the evolution of active region NOAA 13664 for 94 continuous days between April and July 2024. This duration allowed researchers to observe the region through more than three full solar rotations, overcoming the typical two-week visibility limitation from Earth-based assets. NOAA 13664, which emerged on April 16, 2024, was responsible for triggering strong geomagnetic storms in May 2024, including a G5 (extreme) event on May 10, 2024.
Solar Orbiter’s unique orbital inclination, which will reach a maximum of 17° latitude this year, is designed to provide the first high-resolution imagery of the Sun's polar regions, areas obscured from Earth-based observation. This capability is essential for understanding the solar dynamo and predicting space weather variability. As the Sun has recently passed the peak of its current solar cycle, these ongoing observations are critical for protecting infrastructure, including supporting crewed endeavors such as the Artemis missions scheduled for 2026.
The Solar Orbiter, which entered service in November 2021 and is currently in an extended mission phase potentially running until 2030, is scheduled to commence a new series of Remote-Sensing Windows beginning in February 2026. Scientific collaboration continues, highlighted by a joint workshop scheduled in Berlin from March 16-19, 2026, where advances in understanding the Sun's magnetic field influence on the heliosphere will be discussed, incorporating data from other missions including India's ISRO and ESA's Proba-3.
Sources
European Space Agency (ESA)
Solar Orbiter Workshop 2026 - MPS - Max-Planck-Gesellschaft
ESA monitoring January 2026 space weather event - European Space Agency
Spacecraft capture the Sun building a massive superstorm - ScienceDaily
Home - SolarNews - American Astronomical Society
Home - Solar Orbiter - ESA - Cosmos
