activity
20242026
most citedMulti-line Wave Signatures in a Sunspot from Near-UV Sunrise III/SUSI Observations

2 citations · 3 across the 4 of their papers we have counts for

collaborators

9 papers

astro-ph.SR20261 cited

Standing oscillations in a resonant sunspot atmosphere captured by integral field spectroscopy

Glen Chambers, David B. Jess, Shahin Jafarzadeh +8

The solar atmosphere is replete with magnetohydrodynamic wave activity, with magnetic structures such as sunspots channelling wave energy flux efficiently into the outer atmosphere…

astro-ph.SR20262 cited

Multi-line Wave Signatures in a Sunspot from Near-UV Sunrise III/SUSI Observations

Shahin Jafarzadeh, David B. Jess, Marco Stangalini +32

Magnetohydrodynamic waves redistribute energy in magnetic structures of the lower solar atmosphere, yet constraints on how wave power and dominant frequencies are organised above s…

astro-ph.SR2026

The Influence of Opacity on Inferred MHD Wave Signatures in the Lower Solar Atmosphere

Samuel J. Skirvin, Samuel D. T. Grant, David B. Jess +8

Magnetohydrodynamic wave activity in small-scale magnetic structures, such as solar pores, provides key insights into energy transport in the lower solar atmosphere. This study pre…

astro-ph.SR2026

Adaptive multi-line fitting for stable line-core intensity and Doppler velocity

Shahin Jafarzadeh, David B. Jess, Marco Stangalini +5

Next-generation solar spectrographs increasingly record dense wavelength windows in which tens to hundreds of spectral lines are sampled at each spatial location and time step. Thi…

astro-ph.SR2026

Can instrumental effects obscure the true photospheric wave spectrum?

M. Berretti, M. Stangalini, D. B. Jess +6

Optical aberrations and instrument resolution can affect the observed morphological properties of features in the solar atmosphere. However, little work has been done to study the…

astro-ph.SR2025

Umbral oscillations in the photosphere. A comprehensive statistical study

M. Berretti, M. Stangalini, G. Verth +4

It is well-known that the global acoustic oscillations of the Sun's atmosphere can excite resonance modes within large-scale magnetic concentrations. These structures are conduits…