activity
20022023
most citedTemporal aspects and frequency distributions of solar soft X-ray flares

242 citations · 1.4k across the 35 of their papers we have counts for

collaborators

35 papers

astro-ph.EP2023★ 4 cited

Protective Effects of Halite to Vacuum and Vacuum-Ultraviolet Radiation: A Potential Scenario During a Young Sun Superflare

Ximena C. Abrevaya, Douglas Galante, Paula M. Tribelli +16

Halite (NaCl mineral) has exhibited the potential to preserve microorganisms for millions of years on Earth. This mineral was also identified on Mars and in meteorites. In this stu…

astro-ph.SR2021★ 10 cited

Kink instability of triangular jets in the solar atmosphere

T. V. Zaqarashvili, S. Lomineishvili, P. Leitner +3

It is known that hydrodynamic triangular jets are unstable to antisymmetric kink perturbations. The inclusion of magnetic field may lead to the stabilisation of the jets. Jets and…

astro-ph.SR2020★ 29 cited

The UV surface habitability of Proxima b: first experiments revealing probable life survival to stellar flares

Ximena C. Abrevaya, Martin Leitzinger, Oscar oppezzo +5

We use a new interdisciplinary approach to study the UV surface habitability of Proxima under quiescent and flaring stellar conditions. We assumed planetary atmospheric composi…

astro-ph.SR2019★ 85 cited

Mapping the magnetic field of flare coronal loops

D. Kuridze, M. Mathioudakis, H. Morgan +9

Here we report on the unique observation of flaring coronal loops at the solar limb using high resolution imaging spectropolarimetry from the Swedish 1-meter Solar Telescope. The v…

astro-ph.SR2018★ 12 cited

Numerical Simulation of Coronal Waves Interacting with Coronal Holes: III. Dependence on Initial Amplitude of the Incoming Wave

Isabell Piantschitsch, Bojan Vrsnak, Arnold Hanslmeier +4

We performed 2.5D magnetohydrodynamic (MHD) simulations showing the propagation of fast-mode MHD waves of different initial amplitudes and their interaction with a coronal hole (CH…

astro-ph.SR2018★ 13 cited

Numerical Simulation of Coronal Waves Interacting with Coronal Holes: II. Dependence on Alfvén Speed Inside the Coronal Hole

Isabell Piantschitsch, Bojan Vrsnak, Arnold Hanslmeier +4

We used our newly developed magnetohydrodynamic (MHD) code to perform 2.5D simulations of a fast-mode MHD wave interacting with coronal holes (CH) of varying Alfvén speed which res…