Magnetic Energy Powers the Corona: How We Can Understand its 3D Storage & Release

Please use this identifier to cite or link to this item: https://dspace.iiti.ac.in/handle/123456789/16042

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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.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	en_US
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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