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configuration increases substantially, reaching 94% in the new sample of 31 CMEs. On De ection of Solar Coronal Mass Ejections by the Ambient Coronal Magnetic Field Con guration 1 2 1;3 Jingjing Wang , J. Todd ...
Abstract: Nonlinear force-free (NLFF) modeling is regularly used in order to indirectly infer the 3D geometry of the coronal magnetic field , not accessible on a regular basis by means of direct ...
. Sample results are presented for the numerical computation of the angle of maximum polarization and the degree of maximum polarization to be expected from idealized magnetic field configurations ...
. Our sample includes both confined and eruptive events, with 6 and 15 in each category, respectively. Using the Helioseismic and Magnetic Imager vector magnetic field observations from several hours ...
All stars produce explosive surface events such as flares and coronal mass ejections. These events are driven by the release of energy stored in coronal magnetic fields , generated by the stellar ...
. We conclude that emerging dimming is likely caused by coronal heating episodes, powered by reconnection between the emerging and the ambient magnetic fields . D RAFT VERSION MARCH 17, 2021 Typeset using ...
is first presented where the influence of the magnetic field is demonstrated. The Van Vleck depolarization phenomena is described in these terms. Next, a more precise physical picture of the emission-line ...
Modelling with high accuracy the open magnetic field and the fast solar wind in the heliosphere is essential for space weather forecasting purposes. Primary sources of open magnetic field flux ...
sampled by PSP at 0.11 and 0.26 au from the Sun, in two time intervals almost 5 days apart. The two plasma flows come from two distinct source regions, characterized by different magnetic field polarity ...
to extrapolate a 3D coronal magnetic field for a sample of early-to-mid M dwarfs. During the magnetic reconstruction process it is possible to force a solution towards field geometries that are symmetric ...
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