SKA's higher sensitivity and bandwidth will enable fuller exploitation of radio methods for measuring CME magnetic fields and improving space weather predictions.
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3 Pith papers cite this work. Polarity classification is still indexing.
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TMF simulation of AR 12975 reproduces filament channel formation and energy/helicity injection but shows eruption helicity ratio of 0.23 and torus instability at 0.32 due to complex field configuration.
Varying high-temperature opacity tables in a fixed MESA-RSP delta Cephei model shifts the period by up to 0.037 days and amplitude growth by up to 43 percent, with OPAL-A09 closest to the observed period.
citing papers explorer
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Role of SKA in Advancing Remote Measurements of Magnetic Fields of Solar Coronal Mass Ejections
SKA's higher sensitivity and bandwidth will enable fuller exploitation of radio methods for measuring CME magnetic fields and improving space weather predictions.
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Formation and Eruption of Filament Channel in Solar Active Region 12975: Insights from Observations and Simulations of Magnetic Field Evolution
TMF simulation of AR 12975 reproduces filament channel formation and energy/helicity injection but shows eruption helicity ratio of 0.23 and torus instability at 0.32 due to complex field configuration.
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Native-Opacity Sensitivity of a Fixed Delta Cephei MESA-RSP Pulsation Model
Varying high-temperature opacity tables in a fixed MESA-RSP delta Cephei model shifts the period by up to 0.037 days and amplitude growth by up to 43 percent, with OPAL-A09 closest to the observed period.