activity
20172022
most citedImaging of the Quiet Sun in the Frequency Range of 20-80 MHz

25 citations · 112 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.SR2022★ 25 cited

Imaging of the Quiet Sun in the Frequency Range of 20-80 MHz

PeiJin Zhang, Pietro Zucca, Kamen Kozarev +7

Radio emission of the quiet Sun is considered to be due to thermal bremsstrahlung emission of the hot solar atmosphere. The properties of the quiet Sun in the microwave band have b…

astro-ph.EP2022★ 4 cited

Statistical Study on the Sources of Jovian Decametric Radio Emissions Based on the Radio Observations of Remote Instruments

Ruobing Zheng, Yuming Wang, Xiaolei Li +2

To better understand the physical processes associated with Jovian decametric (DAM) radio emissions, we present the statistical study of DAMs and inferred characteristics of DAM so…

astro-ph.SR2021★ 9 cited

Three-dimensional Reconstruction of Coronal Mass Ejections by CORAR Technique through Different Stereoscopic Angle of STEREO Twin Spacecraft

Shaoyu Lyu, Yuming Wang, Xiaolei Li +3

Recently, we developed the Correlation-Aided Reconstruction (CORAR) method to reconstruct solar wind inhomogeneous structures, or transients, using dual-view white-light images (Li…

astro-ph.SR2021★ 17 cited

Parametric simulation studies on the wave propagation of solar radio emission: the source size, duration, and position

PeiJin Zhang, ChuanBing Wang, Eduard P. Kontar

The observed features of the radio sources indicate complex propagation effects embedded in the waves of solar radio bursts. In this work, we perform ray-tracing simulations on rad…

astro-ph.SR2020★ 22 cited

Interferometric Imaging with LOFAR Remote Baselines of the Fine Structures of a Solar Type IIIb Radio Burst

PeiJin Zhang, Pietro Zucca, Sarrvesh Seethapuram Sridhar +8

Context. Solar radio bursts originate mainly from high energy electrons accelerated in solar eruptions like solar flares, jets, and coronal mass ejections. A subcategory of solar r…

astro-ph.SR2020★ 5 cited

The frequency drift and fine structures of Solar S-bursts in the high frequency band of LOFAR

PeiJin Zhang, Pietro Zucca, ChuanBing Wang +8

Solar S-bursts are short duration ( s at decameter wavelengths) radio bursts that have been observed during periods of moderate solar activity, where S stands for short. The fr…

astro-ph.EP2020★ 3 cited

Locating the Source Field Lines of Jovian Decametric Radio Emissions

Yuming Wang, Xianzhe Jia, Chuanbing Wang +2

Decametric (DAM) radio emissions are one of the main windows through which one can reveal and understand the Jovian magnetospheric dynamics and its interaction with the moons. DAMs…

astro-ph.SR2019★ 15 cited

On the Source Position and Duration of a Solar Type III Radio Burst Observed by LOFAR

PeiJin Zhang, SiJie Yu, Eduard Kontar +1

Solar type III radio bursts are excited by electron beams propagating outward from the Sun. The flux of type III radio burst has a time profile of rising and decay phase at a given…

astro-ph.SR2019★ 7 cited

Forward Modeling of the Type III Radio Burst Exciter

Peijin Zhang, Chuanbing Wang, Lin Ye +1

In this work, we propose a forward-modeling method to study the trajectory and speed of the interplanetary (IP) Type-III radio burst exciter. The model assumes that the source of a…

physics.space-ph2017★ 5 cited

A Parametric Investigation on the Cyclotron Maser Instability Driven by Ring-beam Electrons with Intrinsic Alfvén Waves

Zi-Jin Tong, Chuan-Bing Wang, Pei-Jin Zhang +1

The electron-cyclotron maser is a process that generates intense and coherent radio emission in plasma. In this paper, we present a comprehensive parametric investigation on the el…