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- W1630508353 abstract "The magnetic field permeating the solar atmosphere governs much of the structure, morphology, brightness, and dynamics observed on the Sun. The magnetic field, especially in active regions, is thought to provide the power for energetic events in the solar corona, such as solar flares and Coronal Mass Ejections (CME) and is believed to energize the hot coronal plasma seen in extreme ultraviolet or X-rays. The question remains what specific aspect of the magnetic flux governs the observed variability. To directly understand the role of the magnetic field in energizing the solar corona, it is necessary to measure the free magnetic energy available in active regions. The grant now expiring has demonstrated a new and valuable technique for observing the magnetic free energy in active regions as a function of time." @default.
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- W1630508353 date "2001-09-15" @default.
- W1630508353 modified "2023-09-26" @default.
- W1630508353 title "The Magnetic Free Energy in Active Regions" @default.
- W1630508353 hasPublicationYear "2001" @default.
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