most citedMagnetically Structured Oscillatory Power Along an Active-Region Transect in Near-UV Sunrise-III/SUSI Spectroscopy

3 citations · 4 across the 5 of their papers we have counts for

collaborators

7 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…

hep-ex2026

Final Report on the Measurement of the Positive Muon Anomalous Magnetic Moment at Fermilab to 127 ppb

2 Collaboration, D. P. Aguillard, T. Albahri +192

This report details the final measurement of the muon magnetic anomaly, , by the Muon experiment at Fermi National Accelerator Laboratory (FNAL), using posit…

astro-ph.SR20263 cited

Magnetically Structured Oscillatory Power Along an Active-Region Transect in Near-UV Sunrise-III/SUSI Spectroscopy

Shahin Jafarzadeh, David B. Jess, Marco Stangalini +33

We present a multi-line characterisation of how oscillatory power is organised across distinct magnetic environments in an active region using seeing-free, stratospheric near-ultra…

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…