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| DC Field | Value | Language |
|---|---|---|
| dc.contributor.author | Aggarwal, Keshav | en_US |
| dc.date.accessioned | 2025-05-06T12:56:05Z | - |
| dc.date.available | 2025-05-06T12:56:05Z | - |
| dc.date.issued | 2023 | - |
| dc.identifier.uri | https://doi.org/10.3847/25c2cfeb.1dbfea1f | - |
| dc.identifier.uri | https://dspace.iiti.ac.in/handle/123456789/16042 | - |
| dc.description.abstract | The coronal magnetic field is the prime driver behind many as-yet unsolved mysteries: solar eruptions, coronal heating, and the solar wind, to name a few. We advocate for new and multi-point co-optimized measurements, sensitive to magnetic field and other plasma parameters, spanning from optical to gamma-ray wavelengths, to bring closure to long-standing and fundamental questions. | en_US |
| dc.language.iso | en | en_US |
| dc.publisher | AAS Publishing | en_US |
| dc.source | Bulletin of the AAS | en_US |
| dc.title | Magnetic Energy Powers the Corona: How We Can Understand its 3D Storage & Release | en_US |
| dc.type | Journal Article | en_US |
| Appears in Collections: | Department of Astronomy, Astrophysics and Space Engineering | |
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