activity
20002026
most citedRossby waves in "shallow water" magnetohydrodynamics

107 citations · 401 across the 28 of their papers we have counts for

collaborators

28 papers

astro-ph.SR2026

Evidence of global periodicity in PSP data: can they be linked to long-period oscillations in solar active regions?

G. Dumbadze, B. M. Shergelashvili, M. Khodachenko +4

The presence of coherent oscillatory signatures in Parker Solar Probe SWEAP datasets, identified through a series of spectral analyses, is addressed, and their possible connection…

astro-ph.SR2026

Polytropic stellar wind models with strongly localized heating

L. Westrich, B. Shergelashvili, H. Fichtner +1

Polytropic models of stellar winds remain to be useful tools because they allow for a simple description of the energy balance of the expanding plasma without explicitly specifying…

astro-ph.SR2024

Wide-band fluctuations of solar active regions probed with SHARP magnetograms

G. Dumbadze, B. M. Shergelashvili, M. L. Khodachenko +1

The power spectra of the fluctuation noise of the solar active region (AR) areas and magnetic fluxes sequentially observed in time contain information about their geometrical featu…

astro-ph.SR2022★ 1 cited

Categorization model of moving small-scale intensity enhancements in solar active regions

B. M. Shergelashvili, E. Philishvili, S. Buitendag +2

The small-scale moving intensity enhancements remotely observed in the extreme ultraviolet images of the solar active regions, which we refer to as active region moving campfires (…

astro-ph.SR2021★ 3 cited

Eigenspectra of solar active region long-period oscillations

G. Dumbadze, B. M. Shergelashvili, S. Poedts +3

We studied the low-frequency h (long-period h) oscillations of active regions (ARs). The investigation is based on an analysis of a time series…

astro-ph.SR2020★ 2 cited

Case study on the identification and classification of small-scale flow patterns in flaring active region

E. Philishvi, B. M. Shergelashvili, S. Buitendag +3

We propose a novel methodology to identity flows in the solar atmosphere and classify their velocities as either supersonic, subsonic, or sonic. The proposed methodology consists o…