activity
20092026
most citedOn the sensitivity of extrasolar mass-loss rate ranges: HD 209458b a case study

54 citations · 236 across the 17 of their papers we have counts for

collaborators

17 papers

astro-ph.SR2026

Nonlinear steepening of a fast magnetoacoustic wave in the vicinity of a coronal magnetic null point

Yu Zhong, Valery M. Nakariakov, Mariana Cécere +1

The interaction of a fast magnetoacoustic wave with a magnetic null point is studied in the context of the sympathetic flare phenomenon. Attention is paid to steepening the wave ca…

astro-ph.SR2022★ 4 cited

Observational and numerical characterization of a recurrent arc-shaped front propagating along a coronal fan

M. V. Sieyra, S. Krishna Prasad, G. Stenborg +5

Recurrent, arc-shaped intensity disturbances were detected by EUV channels in an active region. The fronts were observed to propagate along a coronal loop bundle rooted in a small…

astro-ph.SR2022★ 14 cited

Pseudostreamer influence on flux rope evolution

A. Sahade, M. Cécere, M. V. Sieyra +3

A critical aspect of solar activity is the coupling between eruptions and the surrounding coronal magnetic field, which determines the trajectory and morphology of the eruptive eve…

astro-ph.SR2022

Estimating the coronal supra-arcade downflows radio emission: from centimetre through submillimetre wavelengths

Ernesto Zurbriggen, C. Guillermo Giménez de Castro, Andrea Costa +2

Supra-arcade downflows (SADs) are infrequent, wiggly opaque structures observed to descend through the solar corona, mostly in EUV and soft X-ray frequencies. From their physical c…

astro-ph.SR2020★ 1 cited

Slow and sausage loop mode excitation due to local and global spontaneous perturbations

H. Capettini, M. Cécere, A. Costa +2

We analyse the capability of different type of perturbations -associated with usual environment energy fluctuations of the solar corona- to excite slow and sausage modes in solar f…

astro-ph.SR2020★ 23 cited

Analysis of large deflections of prominence-CME events during the rising phase of solar cycle 24

M. V. Sieyra, M. Cécere, H. Cremades +7

Motivated by the need to improve the ability to forecast whether a certain coronal mass ejection (CME) is to impact Earth, and by the insufficiency of statistical studies that anal…