Two eruptive filaments both deflected toward the side with weaker poloidal magnetic field, suggesting inclined filament ejections can result from asymmetric strapping forces.
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The Kinematical Behavior of Solar Eruptive Filaments Affected by the Poloidal Magnetic Field
Two eruptive filaments both deflected toward the side with weaker poloidal magnetic field, suggesting inclined filament ejections can result from asymmetric strapping forces.