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https://dspace.iiti.ac.in/handle/123456789/16042
| Title: | Magnetic Energy Powers the Corona: How We Can Understand its 3D Storage & Release |
| Authors: | Aggarwal, Keshav |
| Issue Date: | 2023 |
| Publisher: | AAS Publishing |
| Citation: | Caspi, A., Seaton, D., Casini, R., Downs, C., Gibson, S., Gilbert, H., Glesener, L., Guidoni, S., Hughes, J. M., McKenzie, D., Plowman, J., Reeves, K., Saint-Hilaire, P., Shih, A. Y., West, M., Alaoui, M., Alexander, D., Allred, J. C., Antiochos, S., � Zimovets, I. V. (2023). Magnetic Energy Powers the Corona: How We Can Understand its 3D Storage & Release. Bulletin of the AAS, 55(3). https://doi.org/10.3847/25c2cfeb.1dbfea1f |
| 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. |
| URI: | https://doi.org/10.3847/25c2cfeb.1dbfea1f https://dspace.iiti.ac.in/handle/123456789/16042 |
| Type of Material: | Journal Article |
| Appears in Collections: | Department of Astronomy, Astrophysics and Space Engineering |
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