Magnetic Energy Powers the Corona: How We Can Understand its 3D Storage & Release
Authors:
- Amir CaspiACAmir Caspi
- Daniel SeatonDSDaniel Seaton
- Roberto CasiniRCRoberto Casini
- Cooper DownsCDCooper Downs
- Sarah GibsonSGSarah Gibson
- Holly GilbertHGHolly Gilbert
- Lindsay GlesenerLGLindsay Glesener
- Silvina GuidoniSGSilvina Guidoni
- J. Marcus HughesJHJ. Marcus Hughes
- David McKenzieDMDavid McKenzie
- Joseph PlowmanJPJoseph Plowman
- Katharine ReevesKRKatharine Reeves
Open Access
- 31 July 2023
- journal article
- research article
- Published by American Astronomical Society
- Vol. 55 (3)
Abstract
Whitepaper #049 in the Decadal Survey for Solar and Space Physics (Heliophysics) 2024-2033. Main topics: basic research. Additional topics: solar physics.Keywords
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This publication has 102 references indexed in Scilit:
- Study of a Prominence Eruption using PROBA2/SWAP and STEREO/EUVI DataSolar Physics, 2012
- The Helioseismic and Magnetic Imager (HMI) Investigation for the Solar Dynamics Observatory (SDO)Solar Physics, 2011
- An Instrument to Measure Coronal Emission Line PolarizationSolar Physics, 2008
- On Solving the Coronal Heating ProblemSolar Physics, 2006
- The magnetic nature of solar flaresThe Astronomy and Astrophysics Review, 2001
- The Solar Oscillations Investigation - Michelson Doppler ImagerSolar Physics, 1995
- Solar flares, microflares, nanoflares, and coronal heatingSolar Physics, 1991
- Numerical study of line-tied magnetic reconnectionSolar Physics, 1982
- The heating of the solar coronaSpace Science Reviews, 1969
- Zur Frage der Deutung der Linien im Spektrum der SonnenkoronaThe Science of Nature, 1939