A search for mode coupling in magnetic bright points
Context. Magnetic bright points (MBPs) are one of the smallest manifestations of the
magnetic field in the solar atmosphere and are observed to extend from the photosphere up …
magnetic field in the solar atmosphere and are observed to extend from the photosphere up …
[HTML][HTML] Slow Body MHD Waves in Inhomogeneous Photospheric Waveguides
The present study deals with the investigation of the oscillatory morphology of guided slow
body MHD modes in inhomogeneous magnetic waveguides that appear in the solar …
body MHD modes in inhomogeneous magnetic waveguides that appear in the solar …
Poynting flux of MHD modes in magnetic solar vortex tubes
Magnetic flux tubes in the presence of background rotational flows, known as solar vortex
tubes, are abundant throughout the solar atmosphere and may act as conduits for MHD …
tubes, are abundant throughout the solar atmosphere and may act as conduits for MHD …
Resonant Damping and Instability of Propagating Magnetohydrodynamic Body Modes in a Flux Tube with Shear Flow under Photospheric Conditions
DJ Yu - The Astrophysical Journal, 2025 - iopscience.iop.org
The influence of shear flow on resonant absorption is theoretically investigated for
propagating magnetohydrodynamic body modes in cusp (slow) and Alfvén continua in a …
propagating magnetohydrodynamic body modes in cusp (slow) and Alfvén continua in a …
Sausage, kink, and fluting MHD wave modes identified in solar magnetic pores by Solar Orbiter/PHI
Solar pores are intense concentrations of magnetic flux that emerge through the Sun's
photosphere. When compared to sunspots, they are much smaller in diameter and hence …
photosphere. When compared to sunspots, they are much smaller in diameter and hence …