activity
20212026
most citedHarmonic elctron-cyclotron maser emissions driven by energetic electrons of the horseshoe distribution with application to solar radio spikes

14 citations · 48 across the 9 of their papers we have counts for

collaborators

10 papers

astro-ph.SR2026

Plasmoid-Trapped Condensation Associated with a Transient Thermal-Instability-Like Process in Chromospheric Magnetic Reconnection

Abdullah Zafar, Lei Ni, Samrat Sen +4

We perform high-resolution 2.5D single-fluid magnetohydrodynamic (MHD) simulations to explore the development of cool-dense structures within plasmoids during chromospheric magneti…

astro-ph.SR2026

Kinetic Processes to Radio Burst: First Observational-driven Study in Coronal Loops

Mehdi Yousefzadeh, Marian Karlicky, Artem Koval +3

Understanding the origin of coherent solar radio bursts requires linking macroscopic coronal structures with the kinetic processes responsible for wave generation. We investigate e…

cs.CV2026

Coronary Artery Segmentation and Vessel-Type Classification in X-Ray Angiography

Mehdi Yousefzadeh, Siavash Shirzadeh Barough, Ashkan Fakharifar +12

X-ray coronary angiography (XCA) is the clinical reference standard for assessing coronary artery disease, yet quantitative analysis is limited by the difficulty of robust vessel s…

cs.CV2025

GraphDerm: Fusing Imaging, Physical Scale, and Metadata in a Population-Graph Classifier for Dermoscopic Lesions

Mehdi Yousefzadeh, Parsa Esfahanian, Sara Rashidifar +5

Introduction. Dermoscopy aids melanoma triage, yet image-only AI often ignores patient metadata (age, sex, site) and the physical scale needed for geometric analysis. We present Gr…

astro-ph.SR2025★ 1 cited

The Efficiency of Harmonic Emissions Excited by Energetic Electrons in Coronal Loops

Mehdi Yousefzadeh, Alexey Kuznetsov, Yao Chen +1

Magnetic reconnection is a key process that drives the energy release in solar flares. This process can occur at multiple locations along the coronal loop. The reconnection generat…

astro-ph.SR2025★ 2 cited

Emission Characteristics of Energetic Electrons with Crescent-shaped Velocity Distributions

Mehdi Yousefzadeh

Solar flares release magnetic energy through reconnection, accelerating electrons into nonthermal velocity distributions, including crescent-shaped electron populations. These ener…

astro-ph.SR2022★ 7 cited

Harmonic Electron Cyclotron Maser Emission along the Coronal Loop

Mehdi Yousefzadeh, Yao Chen, Hao Ning +1

Efficient radiation at second and/or higher harmonics of Wce has been suggested to circumvent the escaping difficulty of the electron cyclotron maser emission mechanism when it is…

astro-ph.SR2021★ 13 cited

Harmonic maser emissions from electrons with loss-cone distribution in solar active regions

Hao Ning, Yao Chen, Sulan Ni +4

Electron cyclotron maser emission (ECME) is regarded as a plausible source for the coherent radio radiations from solar active regions (e.g., solar radio spikes). In this Letter, w…

astro-ph.SR2021★ 14 cited

Harmonic elctron-cyclotron maser emissions driven by energetic electrons of the horseshoe distribution with application to solar radio spikes

Hao Ning, Yao Chen, Sulan Ni +4

Content. Electron-cyclotron maser emission (ECME) is the favored mechanism for solar radio spikes and has been investigated extensively since the 1980s. Most studies relevant to so…

astro-ph.SR2021★ 11 cited

Harmonic ECME Excited by Energetic Electrons Travelling Inside A Coronal Loop

M. Yousefzadeh, H. Ning, Y. Chen

A complete understanding of solar radio bursts requires developing numerical techniques which can connect large-scale activities with kinetic plasma processes. As a starting point,…