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Adiabatic Spectrum of Radio Emission of Plasma Clouds, Emitted by the Sun During Solar Flares, and Inhomogeneities of the Spectrum of Radio Emission of Clouds
AbstractIt is known that so-called solar flares systematically occur in the area of sunspots. They are accompanied by radiation in almost all...
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Detection of long-lasting aurora-like radio emission above a sunspot
Auroral radio emissions in planetary magnetospheres typically feature highly polarized, intense radio bursts, usually attributed to electron...
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Stellar Wind and the Efficiency of Plasma Radio Emission from Exoplanets
AbstractWe present the results of our study of the influence of stellar activity on the efficiency of the plasma radio emission generation mechanism...
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An emission-state-switching radio transient with a 54-minute period
Long-period radio transients are an emerging class of extreme astrophysical events of which only three are known. These objects emit highly...
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Adiabatic Radio Emission Spectrum of the Sun’s Coronal Holes
AbstractCoronal holes on the Sun have been observed at individual frequencies for quite a long time in the wavelength range from radio to X-rays....
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Linear to circular conversion in the polarized radio emission of a magnetar
Radio emission from magnetars provides a unique probe of the relativistic, magnetized plasma within the near-field environment of these...
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Detection of Radio Emission from the Geminga-Like Gamma-Ray Pulsar J1836+5925
AbstractThe detection of radio emission from the gamma-ray pulsar J1836+5925 is reported. Rare events of radio emission from this object have been...
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Radio Emission Spectrum of Supernova Remnant G74.9+1.2
AbstractMeasurements of the flux densities of the supernova remnant (SNR) G74.9+1.2 (CTB 87) at frequencies of 4840 and 8450 MHz were carried out...
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Limits on dark matter annihilation from the shape of radio emission in M31
Well-motivated models of dark matter often result in a population of electrons and positrons within galaxies produced through dark matter...
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Strong and weak pulsar radio emission due to thunderstorms and raindrops of particles in the magnetosphere
Pulsars radiate radio signals when they rotate. However, some old pulsars often stop radiating for some periods. The underlying mechanism remains...
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Exploring diffuse radio emission in galaxy clusters and groups with uGMRT and SKA
Diffuse radio emission has been detected in a considerable number of galaxy clusters and groups, revealing the presence of pervasive cosmic magnetic...
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On the High-Frequency Spectrum of Radio Emission from Extensive Air Showers in a Kinetic Model
AbstractRadio emission of the electron excess of the extensive air shower (EAS) charge is calculated in the kinetic model, where in contrast to the...
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The Development of a Theory for Radio Emission
The discovery of the synchrotron radiation mechanism as the explanation of galactic and extragalactic sources of radio emission marked a major... -
Radio Emission Variability of Supernova Remnants and a Possible Explanation of the Phenomenon
AbstractThe flux densities and current spectra of plerions and combined supernova remnants (SNRs): 3C58, 3C144, G11.2–0.3, G21.5–0.9, and 3C396 are...
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Modeling of thermal and non-thermal radio emission from HH80-81 jet
Protostellar jets are one of the primary signposts of star formation. A handful of protostellar objects exhibit radio emission from ionized jets, of...
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Radio Emission of Extensive Air Showers in the Kinetic Model
AbstractThe radio emission of the electron excess of the extensive air shower (EAS) charge is calculated in the kinetic model of the cascade...
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Resonant Interaction of Energetic Electrons with Radio Emission in the Magnetospheres of Exoplanets
We analyze the resonant interaction of energetic electrons with radio emission in the magnetospheres of exoplanets using the planet Tau Bootis b as...
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Radio Variability and Broad-Band Spectra of Infrared Galaxies with and without OH Megamaser Emission
Abstract —We study the radio variability of galaxies with and without sources of hydroxyl (OH) megamaser radiation based on the continuum radio...
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State Primary Standard of the Power Spectral Density Unit of Noise Radio Emission in the Frequency Range from 0.002 to 178.3 GHz Get 21-2021
In 2021, the State primary standard of the power spectral density unit of noise radio emission in the frequency range of 0.002 to 178.3 GHz GET...