The Link between Nonthermal Velocity and Free Magnetic Energy in Solar Flares
The cause of excess spectral line broadening (nonthermal velocity) is not definitively known, but given its rise before and during flaring, the causal processes hold clues to understanding the triggers for the onset of reconnection and the release of free magnetic energy from the coronal magnetic fi...
Main Authors: | James McKevitt, Robert Jarolim, Sarah Matthews, Deborah Baker, Manuela Temmer, Astrid Veronig, Hamish Reid, Lucie Green |
---|---|
Format: | Article |
Language: | English |
Published: |
IOP Publishing
2024-01-01
|
Series: | The Astrophysical Journal Letters |
Subjects: | |
Online Access: | https://doi.org/10.3847/2041-8213/ad1bee |
Similar Items
-
Response of Global Ionospheric Currents to Solar Flares with Extreme Ultraviolet Late Phases
by: Xuanqing Liu, et al.
Published: (2024-01-01) -
A Model for Gradual-phase Heating Driven by MHD Turbulence in Solar Flares
by: William Ashfield IV, et al.
Published: (2023-01-01) -
Observational Analysis of Lyα Emission in Equivalent-magnitude Solar Flares
by: Harry J. Greatorex, et al.
Published: (2023-01-01) -
Evolution of the Ratio of Mg ii Intensities during Solar Flares
by: Soumya Roy, et al.
Published: (2024-01-01) -
Multistage Reconnection Powering a Solar Coronal Jet
by: David M. Long, et al.
Published: (2023-01-01)