Interferometric Imaging with LOFAR Remote Baselines of the Fine Structures of a Solar Type IIIb Radio Burst
PeiJin Zhang, Pietro Zucca, Sarrvesh Seethapuram Sridhar, ChuanBing, Wang, Diana E. Morosan, Bartosz Dabrowski, Andrzej Krankowski, Mario M. Bisi,, Jasmina Magdalenic, Christian Vocks, Gottfried Mann

TL;DR
This study used LOFAR's remote baselines to image and analyze the fine structures of a solar Type IIIb radio burst, revealing distinct source motions and sizes for fundamental and harmonic emissions, advancing understanding of solar radio wave propagation.
Contribution
It provides the first detailed imaging and analysis of a solar Type IIIb-III pair using LOFAR's remote baselines, highlighting differences in source motion and size.
Findings
Fundamental emission source displaces at about 4 times the speed of light.
Harmonic emission source moves at less than 0.02c.
Harmonic source size is smaller than previously observed.
Abstract
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 radio bursts with short time duration may be used as a proxy to understand the wave generation and propagation within the corona. Aims. Complete case studies of the source size, position and kinematics of short term bursts are very rare due to instrumental limitations. A comprehensive multi-frequency spectroscopic and imaging study was carried out of a clear example of a solar type IIIb-III pair. Methods. In this work, the source of the radio burst was imaged with the interferometric mode, using the remote baselines of the LOw Frequency ARray (LOFAR). A detailed analysis of the fine structures in the spectrum and of the radio source motion with imaging was conducted. Results. The study shows how the fundamental…
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