activity
20122023
most citedThermodynamic behavior and stability of Polytropic gas

13 citations · 45 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.SR2023★ 1 cited

Concurrent Kink and Sausage Waves in A Crescent Shaped Structure Over A Limb Prominence

Maryam Ghiasi, Neda Dadashi, Hossein Ebadi

A Crescent shaped prominence Structure (CS), over the solar west limb is studied using EIS/HINODE and AIA/SDO. First, the time varying positions of the top and below borders of the…

astro-ph.SR2016★ 2 cited

The period ratio P_1/P_2 of torsional Alfvén waves with steady flows in spicules

H. Ebadi, S. Shahmorad, S. Vasheghani Farahani

The aim here is to model the standing torsional oscillations in solar spicules in the presence of density stratification, magnetic field expansion, and steady flows. By implementin…

physics.gen-ph2015★ 13 cited

Thermodynamic behavior and stability of Polytropic gas

H. Moradpour, A. Abri, H. Ebadi

We focus on the thermodynamic behavior of Polytropic gas as a candidate for dark energy. We use the general arguments of thermodynamics to investigate its properties and behavior.…

astro-ph.SR2015★ 8 cited

The Possibility of Kelvin-Helmholtz Instability in Solar Spicules

A. Ajabshirizadeh, H. Ebadi, R. E. Vekalati +1

Transversal oscillations of spicules axes may be related to the propagation of magnetohydrodynamic waves along them. These waves may become unstable and the instability can be of t…

astro-ph.SR2014

The study of magnetic reconnection in solar spicules

Z. Fazel, H. Ebadi

This work is devoted to study the magnetic reconnection instability under solar spicule conditions. Numerical study of the resistive tearing instability in a current sheet is prese…

astro-ph.SR2014★ 8 cited

Observation of kink waves and their reconnection-like origin in solar spicules

H. Ebadi, M. Ghiassi

We analyze the time series of Ca II H-line obtained from Hinode/SOT on the solar limb. We follow three cases of upwardly propagating kink waves along a spicule and inverted Y-shape…