97 citations · 1.3k across the 74 of their papers we have counts for
75 papers
Deriving the Continuous -FPUT Model for Decayless Solar Coronal Oscillations Directly from Resistive MHD
D. Tsiklauri
We present an analytical framework deriving the fluid-continuum -Fermi-Pasta-Ulam-Tsingou (-FPUT) system directly from a third-order resistive magnetohydrodynamics (MHD) expa…
Peristaltic Flow in Compressible, Ideal Magnetohydrodynamics: A Mechanism For Solar Spicules
D. Tsiklauri
We present analytical model for peristaltic transport within compressible, ideal magnetohydrodynamics (MHD). By employing small-amplitude perturbation expansion, under thin-tube lo…
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…
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…
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…
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…