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Luminosity distribution of fast radio bursts from CHIME/FRB Catalog 1 by means of the updated Macquart relation
Fast radio bursts (FRBs) are extremely strong radio flares lasting several micro- to milliseconds and come from unidentified objects at cosmological...
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Magnetar spin-down glitch clearing the way for FRB-like bursts and a pulsed radio episode
Magnetars are a special subset of the isolated neutron star family, with X-ray and radio emission mainly powered by the decay of their immense...
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Fast radio bursts at the dawn of the 2020s
Since the discovery of the first fast radio burst (FRB) in 2007, and their confirmation as an abundant extragalactic population in 2013, the study of...
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Simulating Solar Radio Bursts Using Generative Adversarial Networks
Solar flares are one of the most extreme drivers of space weather in our solar system. The impulsive solar radio emission associated with a solar...
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Search for low-energy signals from fast radio bursts with the Borexino detector
The search for neutrino events in correlation with 42 most intense fast radio bursts (FRBs) has been performed using the Borexino dataset from...
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Cosmological model-independent constraints on the baryon fraction in the IGM from fast radio bursts and supernovae data
Fast Radio Bursts (FRBs) are millisecond-duration radio transients with an observed dispersion measure ( DM ) greater than the expected Milky Way...
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Repeating fast radio bursts: Coherent circular polarization by bunches
Fast radio bursts (FRBs) are millisecond-duration signals that are highly dispersed at distant galaxies. However, the physical origin of FRBs is...
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Exploring the Circular Polarisation of Low–Frequency Solar Radio Bursts with LOFAR
The Sun is an active star that often produces numerous bursts of electromagnetic radiation at radio wavelengths. Low frequency radio bursts have...
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The physics of fast radio bursts
In 2007, a very bright radio pulse was identified in the archival data of the Parkes Telescope in Australia, marking the beginning of a new research...
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Comparative Analysis of the Observational Properties of Fast Radio Bursts at the Frequencies of 111 and 1400 MHz
Abstract—A comparative analysis of the observational characteristics of fast radio bursts at the frequencies 111 and 1400 MHz is carried out. The...
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Coronal Signatures of Flare Generated Fast-Mode Wave at EUV and Radio Wavelengths
This paper presents a detailed study of the type II solar radio burst that occurred on 06 March 2014 using combined data analysis. It is a classical...
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Periodic-chaotic alternating regimes during a fast solar metric-radio pulsation event
In the magnetically dominated corona, loop-like structures are expected to undergo pulsating events which are highly structured in time and...
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An X-ray burst from a magnetar enlightening the mechanism of fast radio bursts
Fast radio bursts (FRBs) are millisecond radio pulses originating from powerful enigmatic sources at extragalactic distances. Neutron stars with...
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Analysis of Type II and Type III Radio Bursts Associated with SEPs from Non-Interacting/Interacting Radio-Loud CMEs
We analyze radio bursts observed in events with interacting/non-interacting CMEs that produced major SEPs (I p > 10 MeV) from April 1997 to December...
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Gamma-Ray Bursts
Gamma-ray bursts (GRBs) are short and intense bursts of ∼100 keV−1 MeV photons, usually followed by long-lasting decaying afterglow emission in a...
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Solar Radio Burst Prediction Based on a Multimodal Model
Solar radio bursts are intense radio radiation sources that occur during the energy-release process and represent a hot topic in solar-physics and...
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Near-Earth Interplanetary Coronal Mass Ejections and Their Association with DH Type II Radio Bursts During Solar Cycles 23 and 24
We analyse the characteristics of interplanetary coronal mass ejections (ICMEs) during Solar Cycles 23 and 24. The present analysis is primarily...
