activity
20072021
most citedMagnetic Rossby waves in the solar tachocline and Rieger-type periodicities

136 citations · 682 across the 13 of their papers we have counts for

collaborators

13 papers

astro-ph.SR2021★ 7 cited

One dimensional prominence threads: I. Equilibrium models

J. Terradas, M. Luna, R. Soler +3

Threads are the building blocks of solar prominences and very often show longitudinal oscillatory motions that are strongly attenuated with time. The damping mechanism responsible…

astro-ph.SR2021★ 8 cited

Gravitational instability of solar prominence threads I. Curved magnetic fields without dips

A. Adrover-González, J. Terradas, R. Oliver +1

Prominence threads are dense and cold structures lying on curved magnetic fields that can be suspended in the solar atmosphere against gravity. The gravitational stability of threa…

astro-ph.SR2019★ 32 cited

Magneto-Rossby waves in the solar tachocline and the annual variations in solar activity

Tamar Gachechiladze, Teimuraz V. Zaqarashvili, Eka Gurgenashvili +4

Annual oscillations have been detected in many indices of solar activity during many cycles. Recent multi spacecraft observations of coronal bright points revealed slow retrograde…

astro-ph.SR2015★ 41 cited

On the spatial scales of wave heating in the solar chromosphere

Roberto Soler, Marc Carbonell, Jose Luis Ballester

Dissipation of magnetohydrodynamic (MHD) wave energy has been proposed as a viable heating mechanism in the solar chromospheric plasma. Here, we use a simplified one-dimensional mo…

astro-ph.SR2015★ 41 cited

Long-term variation in the Sun's activity caused by magnetic Rossby waves in the tachocline

T. V. Zaqarashvili, R. Oliver, A. Hanslmeier +4

Long-term records of sunspot number and concentrations of cosmogenic radionuclides (10Be and 14C) on the Earth reveal the variation of the Sun's magnetic activity over hundreds and…

astro-ph.SR2013★ 64 cited

Magnetoacoustic waves in a partially ionized two-fluid plasma

Roberto Soler, Marc Carbonell, Jose Luis Ballester

Compressible disturbances propagate in a plasma in the form of magnetoacoustic waves driven by both gas pressure and magnetic forces. In partially ionized plasmas the dynamics of i…

astro-ph.SR2013★ 77 cited

Alfven waves in a partially ionized two-fluid plasma

R. Soler, M. Carbonell, J. L. Ballester +1

Alfvén waves are a particular class of magnetohydrodynamic waves relevant in many astrophysical and laboratory plasmas. In partially ionized plasmas the dynamics of Alfvén waves is…

astro-ph.SR2012★ 34 cited

Cut-off wavenumber of Alfven waves in partially ionized plasmas of the solar atmosphere

T. V. Zaqarashvili, M. Carbonell, J. L. Ballester +1

Alfven wave dynamics in partially ionized plasmas of the solar atmosphere shows that there is indeed a cut-off wavenumber, i.e. the Alfven waves with wavenumbers higher than the cu…

astro-ph.SR2011★ 32 cited

Rossby waves and polar spots in rapidly rotating stars: Implications for stellar wind evolution

T. V. Zaqarashvili, R. Oliver, J. L. Ballester +5

Rapidly rotating stars show short-period oscillations in magnetic activity and polar appearance of starspots. The aim of this paper is to study large-scale shallow water waves in t…

astro-ph.SR2010★ 110 cited

Quasi-biennial oscillations in the solar tachocline caused by magnetic Rossby wave instabilities

T. V. Zaqarashvili, M. carbonell, R. Oliver +1

Quasi-biennial oscillations (QBO) are frequently observed in the solar activity indices. However, no clear physical mechanism for the observed variations has been suggested so far.…

astro-ph.SR2010★ 33 cited

The spatial damping of magnetohydrodynamic waves in a flowing partially ionised prominence plasma

M. Carbonell, P. Forteza, R. Oliver +1

Solar prominences are partially ionised plasmas displaying flows and oscillations. These oscillations show time and spatial damping and, commonly, have been explained in terms of m…

astro-ph.SR2009★ 136 cited

Magnetic Rossby waves in the solar tachocline and Rieger-type periodicities

T. V. Zaqarashvili, M. Carbonell, R. Oliver +1

Apart from the 11-year solar cycle, another periodicity around 155-160 days was discovered during solar cycle 21 in high energy solar flares, and its presence in sunspot areas and…

astro-ph2007★ 67 cited

The statistical significance of the N-S asymmetry of solar activity revisited

M. Carbonell, J. Terradas, R. Oliver +1

The main aim of this study is to point out the difficulties found when trying to assess the statistical significance of the North-South asymmetry (hereafter SSNSA) of the most usua…