Siphon flow in a cool magnetic loop

Abstract

We investigate the properties of a structure in the solar chromosphere in an active region to find out whether the feature is consistent with a siphon flow in a magnetic loop filled with chromospheric material.

References in corpus (5)

• Intermittent heating in the solar corona employing a 3D MHD model
• Multi-layer study of wave propagation in sunspots
• The influence of coronal EUV irradiance on the emission in the He I 10830 A and D3 multiplets
• The Chromospheric Telescope
• Reversal-free CaIIH profiles: a challenge for solar chromosphere modeling in quiet inter-network

Cited by in corpus (15)

• Flocculent flows in the chromospheric canopy of a sunspot
• He I Vector Magnetometry of Field Aligned Superpenumbral Fibrils
• Sunspot splitting triggering an eruptive flare
• A Steady-state Supersonic Downflow in the Transition Region above a Sunspot Umbra
• The energy of waves in the photosphere and lower chromosphere: IV. Inversion results of Ca II H spectra
• The energy of waves in the photosphere and lower chromosphere: III. Inversion setup for Ca II H spectra in local thermal equilibrium
• A three-dimensional view of the thermal structure in a super-penumbral canopy
• Thermodynamic fluctuations in solar photospheric three-dimensional convection simulations and observations
• Magnetic Properties and Flow Angle of the Inverse Evershed Flow at Its Downflow Points
• Plasma injection into a solar coronal loop
• Magnetic connectivity between the light bridge and penumbra in a sunspot
• Coronal magnetic field and emission properties of small-scale bright and faint loops in the quiet Sun
• Spectropolarimetric evidence for a siphon flow along an emerging magnetic flux tube
• The magnetic topology of the inverse Evershed flow
• Center-to-Limb Variation of the Inverse Evershed Flow