activity
20052023
most citedThe first view of Scuti and Doradus stars with the TESS mission

125 citations · 614 across the 35 of their papers we have counts for

collaborators

35 papers

astro-ph.SR2023

Complex Network View of the Sun's Magnetic Patches: I. Identification

Zahra Tajik, Nastaran Farhang, Hossein Safari +1

Solar and stellar magnetic patches (i.e., magnetic fluxes that reach the surface from the interior) are believed to be the primary sources of a star's atmospheric conditions. Hence…

physics.geo-ph2023

Effect of Geomagnetic Storms on a Power Network at Mid Latitudes

Somayeh Tarana, Nasibe Alipoura, Kourosh Roknia +3

Solar activities may disturb the geomagnetic field and impact the power grid via geomagnetically induced currents. We study active and reactive powers as well as the power factor o…

astro-ph.SR2023

Complex network view for Scuti stars

Elham Ziaali, Nasibe Alipour, Hossein Safari

Extraction of characteristics of the complex light curve of pulsating stars is essential for stellar physics. We investigate the complex network (natural and horizontal visibility…

astro-ph.SR2022★ 5 cited

Do Cellular Automaton Avalanche Models Simulate the Quasi-Periodic Pulsations of Solar Flares?

Nastaran Farhang, Farhad Shahbazi, Hossein Safari

Quasi-periodic pulsations (QPPs) with various periods that originate in the underlying magnetohydrodynamic processes of the flaring structures are detected repeatedly in the solar…

astro-ph.SR2022★ 15 cited

Automatic detection of small-scale EUV brightenings observed by the Solar Orbiter/EUI

N. Alipour, H. Safari, C. Verbeeck +23

Context. Accurate detections of frequent small-scale extreme ultraviolet (EUV) brightenings are essential to the investigation of the physical processes heating the corona. Aims. W…

astro-ph.SR2022★ 10 cited

Synchronization of Small-scale Magnetic Features, Blinkers, and Coronal Bright Points

Zahra Shokri, Nasibe Alipour, Hossein Safari +4

We investigate the relationship between different transients such as blinkers detected in images taken at 304~Å, extreme ultraviolet coronal bright points (ECBPs) at 193~Å, X-ray c…