OVSA Science Highlights: Difference between revisions
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We welcome submissions for all works that utilize OVSA data. Please see [https://docs.google.com/document/d/1ygn7BrU8IKu-6Q00_MCZTeswLZFXOl9TKU342-u_tCU/edit?usp=sharing the Author Guidelines] for submission guidance. | We welcome submissions for all works that utilize OVSA data. Please see [https://docs.google.com/document/d/1ygn7BrU8IKu-6Q00_MCZTeswLZFXOl9TKU342-u_tCU/edit?usp=sharing the Author Guidelines] for submission guidance. | ||
== | ==All Highlights== | ||
[[OVSA Science Highlight No. 1: Microwave Precursor of a Major Solar Eruption]] | [[OVSA Science Highlight No. 1: Microwave Precursor of a Major Solar Eruption]] | ||
[[File:solar_eruption_nasa.jpeg|left|100px]] | [[File:solar_eruption_nasa.jpeg|left|100px]] | ||
A study by [https://iopscience.iop.org/article/10.3847/2041-8213/adf063 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. [Contributed by Y. Kou; Edited by B. Chen. Posted on August 2, 2025.] | A study by [https://iopscience.iop.org/article/10.3847/2041-8213/adf063 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. [Contributed by Y. Kou; Edited by B. Chen. Posted on August 2, 2025.] | ||
Revision as of 19:01, 2 August 2025
For Authors
We welcome submissions for all works that utilize OVSA data. Please see the Author Guidelines for submission guidance.
All Highlights
OVSA Science Highlight No. 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. [Contributed by Y. Kou; Edited by B. Chen. Posted on August 2, 2025.]