OVSA Science Highlights: Difference between revisions
Jump to navigation
Jump to search
| Line 8: | Line 8: | ||
[[File: | [[File:solar_eruption_nasa.jpeg|left|200px]] | ||
A study by Kou et al. presents the first spatially resolved microwave imaging spectroscopy of the precursor phase of a major solar eruption. The findings reveal that thermal electron emissions dominate during the slow-rise phase, supporting a scenario of moderate magnetic reconnection prior to the flare’s impulsive onset. | A study by Kou et al. presents the first spatially resolved microwave imaging spectroscopy of the precursor phase of a major solar eruption. The findings reveal that thermal electron emissions dominate during the slow-rise phase, supporting a scenario of moderate magnetic reconnection prior to the flare’s impulsive onset. | ||
Revision as of 17:37, 2 August 2025
For Authors
We welcome submissions for all works that utilize OVSA data. Please see the Author Guidelines for submission guidance.
Latest Highlights
OVSA Science Highlight #1: Microwave Precursor of a Major Solar Eruption
A study by Kou et al. presents the first spatially resolved microwave imaging spectroscopy of the precursor phase of a major solar eruption. The findings reveal that thermal electron emissions dominate during the slow-rise phase, supporting a scenario of moderate magnetic reconnection prior to the flare’s impulsive onset.
