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Inverse relationship between solar corona brightness and velocity of coronal mass ejections discovered

NRL discovers inverse relationship between solar corona brightness and CME velocity
AR11401 on the solar disk as seen by SDO/AIA 193 脜 on 2012 January 24 at 13:00 UT, the bright corona directly above it, and a radial projection from the AR into the corona as seen by LASCO C2. Credit: The Astrophysical Journal (2025). DOI: 10.3847/1538-4357/add3fb

U.S. Naval Research Laboratory (NRL) detailed an inverse relationship between the brightness of the solar corona and the velocity of coronal mass ejections (CMEs) in a paper in The Astrophysical Journal on July 3.

The study, titled "The Relationship Between the Kinematics of Coronal Mass Ejections and the Brightness of the Corona," was authored by Kelly Victor-French, M.S., Karl Battams, Ph.D., and Brian E. Wood, Ph.D., all from NRL's Solar and Heliospheric 糖心视频ics Branch of the Space Science Division.

The team's analysis revealed a significant finding: the brighter the corona overlying active regions on the sun, the less likely high-velocity CMEs were to emerge from those regions.

"This unexpected relationship provides valuable insights into the complex dynamics of the sun and its impact on the ," Victor-French said. "Understanding this connection could significantly improve our ability to forecast ."

Using data from NRL's Large Angle and Spectrometric Coronagraph Experiment (LASCO) on board the joint European Space Agency (ESA)-NASA Solar and Heliospheric Observatory (SOHO), the NRL team compiled nearly three decades of observations of the solar corona. They studied the extensive dataset to investigate trends in the brightness of the sun's corona and compare them to CME velocities over the same period.

Their study found a strong correlation between the two datasets, with bright regions of the solar appearing to relate to substantially slower CME velocities and, in some cases, perhaps entirely precluding CMEs.

An image sequence from the U.S. Naval Research Laboratory's (NRL) Large Angle and Spectrometric Coronagraph Experiment (LASCO) C2 coronagraph observing a fast coronal mass ejection, as mentioned in the study, on September 10, 2017. The Sun is at the center of the visual, hidden by a solid disk that blocks blinding sunlight and enables observations of the much fainter solar corona. (European Space Agency (ESA)-NASA and U.S. Naval Research Laboratory photo). Credit: European Space Agency (ESA)-NASA and U.S. Naval Research Laboratory photo

This research and the associated NRL data have important implications for the space weather community. Advanced knowledge of CME velocity is crucial for improving space weather forecasts, which in turn can lead to more accurate predictions of and solar particle events. These phenomena can disrupt , power grids, and other on Earth.

"Improved space weather forecasting is essential for protecting our technological infrastructure and ensuring the safety of astronauts in space," Victor-French said.

With the publication of these promising results, NRL will continue to explore this relationship and aims to develop a real-time data product for integration into existing space weather models. This ongoing effort promises to further enhance our ability to predict and mitigate the impacts of space weather events.

More information: Kelly Victor-French et al, The Relationship Between the Kinematics of Coronal Mass Ejections and the Brightness of the Corona, The Astrophysical Journal (2025).

Journal information: Astrophysical Journal

Citation: Inverse relationship between solar corona brightness and velocity of coronal mass ejections discovered (2025, July 15) retrieved 22 July 2025 from /news/2025-07-inverse-relationship-solar-corona-brightness.html
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