activity
20092020
most citedSub-second time evolution of Type III solar radio burst sources at fundamental and harmonic frequencies

24 citations · 26 across the 3 of their papers we have counts for

collaborators

9 papers

astro-ph.SR202024 cited

Sub-second time evolution of Type III solar radio burst sources at fundamental and harmonic frequencies

Xingyao Chen, Eduard P. Kontar, Nicolina Chrysaphi +4

Recent developments in astronomical radio telescopes opened new opportunities in imaging and spectroscopy of solar radio bursts at sub-second timescales. Imaging in narrow frequenc…

astro-ph.SR2020

Solar Image Deconvolution by Generative Adversarial Network

Long Xu, Wenqing Sun, Yihua Yan +1

With Aperture synthesis (AS) technique, a number of small antennas can assemble to form a large telescope which spatial resolution is determined by the distance of two farthest ant…

astro-ph.IM2019

Concept of an Experimental Ultra Long-wavelength Radio Array

Linjie Chen, Yihua Yan

The Ultra-Long Wavelength (ULW) regime of longer than 10 m (corresponding to frequencies below 30 MHz), remains as the last virtually unexplored window in radio astronomy, and is p…

astro-ph.SR2018

Chirality and magnetic configuration associated with two-ribbon solar flares: AR 10930 versus AR 11158

Han He, Huaning Wang, Yihua Yan +2

The structural property of the magnetic field in flare-bearing solar active regions (ARs) is one of the key aspects for understanding and forecasting solar flares. In this paper, w…

astro-ph.SR2018

Decimetric emission 500 away from a flaring Site: Possible scenarios from solar radio observations

Susanta Kumar Bisoi, H. S. Sawant, P. Janardhan +5

We present a study of decimetric radio activity, using the first high time cadence (0.5 s) images from the () at 610 M…

astro-ph.IM2018

Antenna Design and Implementation for the Future Space Ultra-Long Wavelength Radio Telescope

Linjie Chen, Amin Aminaei, Leonid I. Gurvits +4

In radio astronomy, the Ultra-Long Wavelengths (ULW) regime of longer than 10 m (frequencies below 30 MHz), remains the last virtually unexplored window of the celestial electromag…