collaborators

5 papers

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

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

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…