Results 51 to 60 of about 93,758 (219)
The Astrophysical JournalAmong several dozen known repeating fast radio bursts, those precisely localized offer the best opportunities to explore their multiwavelength counterparts, which are key to uncovering their origins.
Zhen Yan +10 more
doaj +1 more source
Telescope array bursts, radio pulses and axion quark nuggets
European Physical Journal C: Particles and Fields, 2022 Telescope array (TA) experiment has recorded Abbasi et al. (Phys Lett A 381(32):2565–2572, https://doi.org/10.1016/j.physleta.2017.06.022 , 2017), Okuda (J Phys Conf Ser 1181:012067, https://doi.org/10.1088/1742-6596/1181/1/012067 , 2019) several short ...
Xunyu Liang, Ariel Zhitnitsky
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Observations of Low Frequency Solar Radio Bursts from the Rosse Solar-Terrestrial Observatory
, 2012 The Rosse Solar-Terrestrial Observatory (RSTO; www.rosseobservatory.ie) was established at Birr Castle, Co. Offaly, Ireland (53 05'38.9", 7 55'12.7") in 2010 to study solar radio bursts and the response of the Earth's ionosphere and geomagnetic field. To
A. Kontogeorgos +27 more
core +1 more source
ILLUMINATING THE DARKEST GAMMA-RAY BURSTS WITH RADIO OBSERVATIONS [PDF]
, 2013 We present X-ray, optical, near-infrared (IR), and radio observations of gamma-ray bursts (GRBs) 110709B and 111215A, as well as optical and near-IR observations of their host galaxies.
Berger, E. +23 more
core +2 more sources
Galactic and cosmological fast radio bursts as scaled-up solar radio bursts [PDF]
Monthly Notices of the Royal Astronomical Society, 2020 ABSTRACT Fast radio bursts (FRBs) are bright milliseconds radio transients with large dispersion measures. Recently, FRB 200428 was detected in temporal coincidence with a hard X-ray flare from the Galactic magnetar SGR 1935+2154, which supports that at least some FRBs are from magnetar activity.
F Y Wang, G Q Zhang, Z G Dai
openaire +2 more sources
A Review of Recent Solar Type III Imaging Spectroscopy
Frontiers in Astronomy and Space Sciences, 2020 Solar type III radio bursts are the most common impulsive radio signatures from the Sun, stimulated by electron beams traveling through the solar corona and solar wind.
Hamish A. S. Reid
doaj +1 more source
Verifying and reporting Fast Radio Bursts [PDF]
Monthly Notices of the Royal Astronomical Society, 2018 Fast Radio Bursts (FRBs) are a class of short-duration transients at radio wavelengths with inferred astrophysical origin. The prototypical FRB is a broadband signal that occurs over the extent of the receiver frequency range, is narrow in time, and is highly dispersed, following a v(-2) relation.
Griffin Foster +8 more
openaire +3 more sources
LOFAR observations of fine spectral structure dynamics in type IIIb radio bursts [PDF]
, 2018 Solar radio emission features a large number of fine structures demonstrating great variability in frequency and time. We present spatially resolved spectral radio observations of type IIIb bursts in the $30-80$ MHz range made by the Low Frequency Array (
Kontar, E. P. +2 more
core +2 more sources
The Astrophysical JournalWe present a comprehensive study of type III radio bursts and their association with solar flares of magnitude M1.0 and larger, as observed by four widely separated spacecraft (Parker Solar Probe, Solar Orbiter, STEREO-A, and Wind). Our main focus is the
Vratislav Krupar +10 more
doaj +1 more source
DLITE—An inexpensive, deployable interferometer for solar radio burst observations
Frontiers in Astronomy and Space Sciences, 2022 Solar radio bursts (SRBs) are brief periods of enhanced radio emission from the Sun. SRBs can provide unique insights into the plasma structure where emission occurs.
George Carson +5 more
doaj +1 more source