Resolving the solar prominence/filament paradox using the magnetic Rayleigh–Taylor instability
J. M. Jenkins, Rony Keppens
Topics & Concepts
Solar prominencePhysicsInstabilityRayleigh–Taylor instabilityAstrophysicsMagnetohydrodynamicsCorona (planetary geology)AstronomyMagnetic fieldMechanicsAstrobiologyVenusQuantum mechanicsSolar and Space Plasma DynamicsAstro and Planetary ScienceIonosphere and magnetosphere dynamics