activity
19952026
most citedNon-Newtonian effects in the peristaltic flow of a Maxwell fluid

97 citations · 1.3k across the 74 of their papers we have counts for

collaborators
Showing 2023Show all

5 papers · 1 filter

astro-ph.SR2023★ 3 cited

Particle acceleration by sub-proton cyclotron frequency spectrum of dispersive Alfven waves in inhomogeneous solar coronal plasmas

D. Tsiklauri

The problem of explaining observed soft X-ray fluxes during solar flares, which invokes acceleration of large fraction of electrons, if the acceleration takes places at the solar c…

astro-ph.SR2023★ 3 cited

New cases of super-flares on slowly rotating solar-type stars and large amplitude super-flares in G- and M-type main-sequence stars

A. k. Althukair, D. Tsiklauri

In our previous work, we searched for super-flares on different types of stars while focusing on G-type dwarfs using entire Kepler data to study statistical properties of the occur…

astro-ph.SR2023★ 1 cited

Prediction of short stellar activity cycles using derived and established empirical relations between activity and rotation periods

A. k. Althukair, D. Tsiklauri

In our previous work, we investigated the occurrence rate of super-flares on various types of stars and their statistical properties, with a particular focus on G-type dwarfs, usin…

astro-ph.IM2023★ 3 cited

Magnetic Energy Powers the Corona: How We Can Understand its 3D Storage & Release

Amir Caspi, Daniel B. Seaton, Roberto Casini +12

The coronal magnetic field is the prime driver behind many as-yet unsolved mysteries: solar eruptions, coronal heating, and the solar wind, to name a few. It is, however, still poo…

astro-ph.IM2023★ 5 cited

COMPLETE: A flagship mission for complete understanding of 3D coronal magnetic energy release

Amir Caspi, Daniel B. Seaton, Roberto Casini +12

COMPLETE is a flagship mission concept combining broadband spectroscopic imaging and comprehensive magnetography from multiple viewpoints around the Sun to enable tomographic recon…