Results 21 to 30 of about 1,109,066 (343)
Auto Recognition of Solar Radio Bursts Using the C-DCGAN Method
Frontiers in Physics, 2021 Solar radio bursts can be used to study the properties of solar activities and the underlying coronal conditions on the basis of the present understanding of their emission mechanisms. With the construction of observational instruments, around the world,
Weidan Zhang +7 more
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THE CRITICAL FREQUENCY OF THE IONOSPHERIC F2-LAYER AS OBTAINED FROM IONOSONDE DATA AND OBSERVATIONS OF SOLAR RADIO BURSTS [PDF]
Radio Physics and Radio Astronomy, 2022 Subject and Purpose. Studying the time variations shown by the critical frequencies of the ionospheric F2 layer through comparative analysis of ionosonde data and observations of type III solar radio bursts. Methods and Methodology.
L. O. Stanislavsky +4 more
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A new measurement of the Hubble constant using Fast Radio Bursts [PDF]
, 2021 Fast radio bursts (FRBs) are very short and bright transients visible over extragalactic distances. The radio pulse undergoes dispersion caused by free electrons along the line of sight, most of which are associated with the large-scale structure (LSS ...
S. Hagstotz, R. Reischke, R. Lilow
semanticscholar +1 more source
Odessa Astronomical Publications, 2020 . This paper presents the results of a comparative analysis of the relationship between solar cosmic rays (SCR), coronal mass ejections (CME), and coronal shock waves (CSW) with the parameters of solar continual type IV radio bursts, as well as with the ...
E. A. Isaeva
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The Host Galaxies and Progenitors of Fast Radio Bursts Localized with the Australian Square Kilometre Array Pathfinder [PDF]
2020 XXXIIIrd General Assembly and Scientific Symposium of the International Union of Radio Science, 2020 The Australian SKA Pathfinder (ASKAP) telescope has started to localize fast radio bursts (FRBs) to arcsecond accuracy from the detection of a single pulse, allowing their host galaxies to be reliably identified.
S. Bhandari
semanticscholar +1 more source
Fast Radio Bursts from Reconnection in a Magnetar Magnetosphere [PDF]
Astrophysical Journal, 2020 The nearly 100% linear polarization has been reported for a few fast radio bursts (FRBs). This finding places severe limits on the emission mechanism.
Y. Lyubarsky
semanticscholar +1 more source
The z-DM distribution of fast radio bursts [PDF]
, 2021 We develop a sophisticated model of FRB observations, accounting for the intrinsic cosmological gas distribution and host galaxy contributions, and give the most detailed account yet of observational biases due to burst width, dispersion measure, and the
C. James +5 more
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Solar Radio Burst Detection Based on the MobileViT-SSDLite Lightweight Model
The Astrophysical Journal Supplement Series, 2023 Real-time detection of solar radio bursts is crucial in solar physics research and space weather forecasting. However, current research on the automatic detection of solar radio bursts is limited to identifying the presence or absence of solar radio ...
Hailan He +4 more
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High time resolution and polarization properties of ASKAP-localized fast radio bursts [PDF]
, 2020 Combining high time and frequency resolution full-polarisation spectra of Fast Radio Bursts (FRBs) with knowledge of their host galaxy properties provides an opportunity to study both the emission mechanism generating them and the impact of their ...
C. Day +12 more
semanticscholar +1 more source
Radio Physics and Radio Astronomy, 2014 Features of sporadic decameter solar radio emission associated with some active regions according to observations made with radio telescope UTR-2 on August 1, 2014 are considered.
A. V. Antonov +7 more
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