Simulations demonstrate that mega-parsec giant radio sources form successfully in normal hot baryonic gas environments within 10^13 to 10^15 solar mass dark matter halos, with radio powers matching observations.
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2 Pith papers cite this work. Polarity classification is still indexing.
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2026 2representative citing papers
A zero-beta MHD simulation of the 2024 May 6 event shows X-point reconnection above two current channels of opposite helicity deflects the erupting filament and forms the observed three-ribbon structure via QSLs in a sandwich magnetic configuration.
citing papers explorer
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Formation of mega-parsec giant radio sources from hosts residing in dark matter halos with normal hot baryonic gas fractions
Simulations demonstrate that mega-parsec giant radio sources form successfully in normal hot baryonic gas environments within 10^13 to 10^15 solar mass dark matter halos, with radio powers matching observations.
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Deflection of a Filament Eruption with Three Parallel Flare Ribbons via Reconnection at an X-Point
A zero-beta MHD simulation of the 2024 May 6 event shows X-point reconnection above two current channels of opposite helicity deflects the erupting filament and forms the observed three-ribbon structure via QSLs in a sandwich magnetic configuration.