activity
20072023
most citedSoliton Turbulence in Shallow Water Ocean Surface Waves

126 citations · 152 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.SR2023★ 1 cited

Modulation depth of the gyrosynchrotron emission as identifier of fundamental sausage modes

M. Cécere, A. Costa, T. Van Doorsselaere

We study the intensity, the modulation depth and the mean modulation depth of the gyrosynchrotron (GS) radiation as a function of the frequency and the line of sight (LOS) in fast…

astro-ph.SR2021★ 5 cited

An MHD Study of Large-Amplitude Oscillations in Solar Filaments

Ernesto Zurbriggen, Mariana Cécere, María Valeria Sieyra +3

Quiescent filaments are usually affected by internal and/or external perturbations triggering oscillations of different kinds. In particular, external large-scale coronal waves can…

astro-ph.SR2021★ 10 cited

Polarity relevance in flux rope deflections triggered by coronal holes

Abril Sahade, Mariana Cécere, Andrea Costa +1

Many observations show that coronal holes (CHs) deviate coronal mass ejections (CMEs) away from them. However, there are some peculiar events reported where the opposite occurs. To…

nlin.PS2014★ 126 cited

Soliton Turbulence in Shallow Water Ocean Surface Waves

Andrea Costa, Alfred R. Osborne, Donald T. Resio +5

We analyze shallow water wind waves in Currituck Sound, North Carolina and experimentally confirm, for the first time, the presence of in ocean waves. Solito…

cond-mat.stat-mech2014★ 4 cited

Maintenance of order in a moving strong condensate

Justin Whitehouse, André Costa, Richard A Blythe +1

We investigate the conditions under which a moving condensate may exist in a driven mass transport system. Our paradigm is a minimal mass transport model in which particles m…

astro-ph2007★ 6 cited

Stability and mode analysis of solar coronal loops using thermodynamic irreversible energy principles

Andrea Costa, Rafael Gonzalez

We study the modes and stability of non - isothermal coronal loop models with different intensity values of the equilibrium magnetic field. We use an energy principle obtained via…