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astro-ph.SR2026

Dual-Perspective Microwave and Hard X-ray Constraints of Asymmetric Nonthermal Loops in an X-class Flare

Ruifei Huang, Yao Chen, Victor Melnikov +9

We report dual-perspective microwave and HXR observations of an X-class flare on 2024 May 15, taking advantage of the unique geometry of a front-side view from the Earth and a back…

astro-ph.SR2025

A Flare-related Decimetric Type-IV Radio Burst Induced by the X2 Radiation of Electron Cyclotron Maser Emission

Maoshui Lv, Ze Zhong, Xiangliang Kong +9

The radiation mechanism of decimetric wideband and pulsating radio bursts from the Sun (in terms of decimetric type-IV (t-IVdm) burst) and other flaring stars is a long-standing pr…

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.SR2024

Electron acceleration and transport in the 2023-03-06 solar flare

Alexey Kuznetsov, Zhao Wu, Sergey Anfinogentov +2

We investigated in detail the M5.8 class solar flare that occurred on 2023-03-06. This flare was one of the first strong flares observed by the Siberian Radioheliograph in the micr…

astro-ph.SR2024

A Multi-Peak Solar Flare with a High Turnover Frequency of The Gyrosynchrotron Spectra from the Loop-Top Source

Zhao Wu, Alexey Kuznetsov, Sergey Anfinogentov +8

The origin of multiple peaks in lightcurves of various wavelengths remains illusive during flares. Here we discuss the flare of SOL2023-05-09T03:54M6.5 with six flux peaks as recor…