4 papers
The Sun at millimeter wavelengths V. Magnetohydrodynamic waves in a fibrillar structure
Maryam Saberi, Shahin Jafarzadeh, Sven Wedemeyer +4
Magnetohydrodynamic (MHD) waves, playing a crucial role in transporting energy through the solar atmosphere, manifest in various chromospheric structures. Here, we investigated MHD…
Implementation of thermal conduction energy transfer models in the Bifrost Solar atmosphere MHD code
George Cherry, Boris Gudiksen, Mikolaj Szydlarski
Context: Thermal conductivity provides important contributions to the energy evolution of the upper solar atmosphere, behaving as a non-linear concentration-dependent diffusion equ…
ALMA Memo 628 -- High-cadence observations of the Sun
Sven Wedemeyer, Mikolaj Szydlarski, M. Carmen Toribio +7
The Atacama Large Millimeter/submillimeter Array (ALMA) offers new diagnostic capabilities for studying the Sun, providing complementary insights through high spatial and temporal…
Can we rely on EUV emission to identify coronal waveguides?
P. Kohutova, P. Antolin, M. Szydlarski +1
Traditional models of coronal oscillations rely on modelling the coronal structures that support them as compact cylindrical waveguides. Recently, an alternative model of the struc…