Search
Search Results
-
Fast Radio Bursts
The era of fast radio bursts (FRBs) was open in 2007, when a very bright radio pulse of unknown origin was discovered occasionally in the archival...
-
Fast Radio Bursts
The era of fast radio bursts (FRBs) was open in 2007, when a very bright radio pulse of unknown origin was discovered occasionally in the archival...
-
Detection of ultra-fast radio bursts from FRB 20121102A
Fast radio bursts (FRBs) are extragalactic transient flashes of radio waves with typical durations of milliseconds. FRBs have been shown, however, to...
-
The discovery and significance of fast radio bursts
In 2007 we were part of a team that discovered the so-called “Lorimer Burst”, the first example of a new class of objects now known as fast radio...
-
A link between repeating and non-repeating fast radio bursts through their energy distributions
Fast radio bursts (FRBs) are extremely energetic, millisecond-duration radio flashes that reach Earth from extragalactic distances. Broadly speaking,...
-
Stimulated decay of collapsing axion stars and fast radio bursts
The radiation mechanism of fast radio bursts (FRBs) has been extensively studied but still remains elusive. In the search for dark matter candidates,...
-
Cosmology with fast radio bursts in the era of SKA
We present a forecast of the cosmological parameter estimation using fast radio bursts (FRBs) from the upcoming Square Kilometre Array (SKA),...
-
On the Problems of Detecting Fast Radio Bursts with the LPA LPI
AbstractWe present a verification of fast radio bursts (FRBs) previously published by V.A. Fedorova and A.E. Rodin. These FRBs were found in the...
-
Repeating fast radio bursts produced by a strange star interacting with its planet in an eccentric orbit
FRB 180916 is an important repeating fast radio burst (FRB) source. Interestingly, the activity of FRB 180916 shows a well-regulated behavior, with a...
-
Magnetic Properties of Source Regions of CMEs and DH Type II Radio Bursts
The Sun is a dynamic star that exhibits various phenomena, including solar flares, coronal mass ejections (CMEs), and Type II radio bursts. CMEs are...
-
Comparison Between Radio Loud and Radio Quiet Fast CMEs: A Reason for Radio Quietness
It is well known that fast CMEs are mostly associated with magnetohydrodynamic (MHD) shocks in the solar corona, forming type-II radio bursts....
-
-
A Catalog of Metric Type II Radio Bursts Detected by RSTN During Solar Cycle 24
In this study, we compile a catalog of metric type II radio bursts using the Radio Solar Telescope Network (RSTN) to study the occurrence,...
-
-
Observations of the Fast Radio Burst FRB 20220912A with the LPA LPI and Fast Radio Telescopes
AbstractThis paper presents the result of the search for pulses from the fast radio burst FRB 20220912A with the LPA LPI antenna at a frequency of...
-
Properties of Type-II Radio Bursts in Relation to Magnetic Complexity of the Solar Active Regions
Type-II radio bursts are believed to occur as a result of the shock driven by flares or coronal mass ejections (CMEs). While the shock waves are...
-
Forecasting constraints on the baryon mass fraction in the IGM from fast radio bursts and type Ia supernovae
Fast Radio Bursts (FRBs) are millisecond transient radio events with a high energy. By identifying the origin of the burst, it is possible to measure...
-
Burst timescales and luminosities as links between young pulsars and fast radio bursts
Fast radio bursts (FRBs) are extragalactic radio flashes of unknown physical origin. Their high luminosities and short durations require extreme...
-
The observed impact of galaxy halo gas on fast radio bursts
Galaxies and groups of galaxies exist in dark-matter haloes filled with diffuse gas. The diffuse gas represents up to 80% of the mass in baryonic...
