activity
20072026
most citedThe Magnetic Response of the Solar Atmosphere to Umbral Flashes

47 citations · 458 across the 21 of their papers we have counts for

collaborators

21 papers

astro-ph.SR2026★ 2 cited

Inference of horizontal velocity fields from the induction equation in the solar atmosphere. I. Analytical and numerical solutions in 2D

H. Vila Crespo, J. M. Borrero, I. Milić +2

Spectroscopic and spectropolarimetric observations, which rely on the Doppler effect, only provide access to the line-of-sight component of the solar plasma velocity (vz). However,…

astro-ph.SR2024★ 3 cited

SiO maser polarization and magnetic field in evolved cool stars

L. Marinho, F. Herpin, H. Wiesemeyer +6

Both magnetic fields and photospheric/atmospheric dynamics can be involved in triggering the important mass loss observed in evolved cool stars. Previous works have revealed that t…

astro-ph.SR2018★ 3 cited

High-resolution spectroscopy of Boyajian's star during optical dimming events

M. J. Martínez González, C. González-Fernández, A. Asensio Ramos +13

Boyajian's star is an apparently normal main sequence F-type star with a very unusual light curve. The dipping activity of the star, discovered during the Kepler mission, presents…

astro-ph.SR2018★ 47 cited

The Magnetic Response of the Solar Atmosphere to Umbral Flashes

S. J. Houston, D. B. Jess, A. Asensio Ramos +4

Chromospheric observations of sunspot umbrae offer an exceptional view of magneto-acoustic shock phenomena and the impact they have on the surrounding magnetically-dominated plasma…

astro-ph.SR2016★ 17 cited

On the magnetism and dynamics of prominence legs hosting tornadoes

M. J. Martinez Gonzalez, A. Asensio Ramos, I. Arregui +3

Solar tornadoes are dark vertical filamentary structures observed in the extreme ultraviolet associated with prominence legs and filament barbs. Their true nature and relationship…

astro-ph.SR2015★ 27 cited

Model comparison for the density structure across solar coronal waveguides

I. Arregui, R. Soler, A. Asensio Ramos

The spatial variation of physical quantities, such as the mass density, across solar atmospheric waveguides governs the timescales and spatial scales for wave damping and energy di…