Little is known about the radio astronomical universe at frequencies below 10 MHz because such radiation does not penetrate the ionosphere. A cubesat-based telescope for the 1--10 MHz band could be rapidly and economically deployed in low earth orbit. We consider possible transient and steady sources, and application to study of the ionosphere itself.Comment: 5 pp., 1 fi
The frequency band below 30 MHz is one of the last unexplored bands in radio astronomy. This band is...
Radio waves provide a useful diagnostic tool to investigate the properties of the ionosphere because...
The epoch of formation of the first luminous structures (stars and galaxies) called the Comic Dawn, ...
The frequency band below 30 MHz is one of the last unexplored bands in radio astronomy. This band is...
Opening the last frequency window for radio astronomy in the sub - 30 MHz region includes a few chal...
Opening the last frequency window for radio astronomy in the sub - 30 MHz region includes a few chal...
OLFAR, Orbiting Low Frequency Antennas for Radio Astronomy, will be a space mission to observe the u...
The Lunar Surface Electromagnetics Explorer 'LuSEE Night' is a low frequency radio astronomy experim...
\u3cp\u3eOpening the last frequency window for radio astronomy in the sub - 30 MHz region includes a...
This paper introduces the first results of observations with the Ultra-Long-Wavelength (ULW) -- Low ...
Opening the last frequency window for radio astronomy in the sub - 30 MHz region includes a few chal...
Opening the last frequency window for radio astronomy in the sub - 30 MHz region includes a few chal...
\u3cp\u3eThe past two decades have witnessed a renewed interest in low frequency radio astronomy, wi...
New interesting astronomical science drivers for very low frequency radio astronomy have emerged, ra...
The epoch of formation of the first luminous structures (stars and galaxies) called the Comic Dawn, ...
The frequency band below 30 MHz is one of the last unexplored bands in radio astronomy. This band is...
Radio waves provide a useful diagnostic tool to investigate the properties of the ionosphere because...
The epoch of formation of the first luminous structures (stars and galaxies) called the Comic Dawn, ...
The frequency band below 30 MHz is one of the last unexplored bands in radio astronomy. This band is...
Opening the last frequency window for radio astronomy in the sub - 30 MHz region includes a few chal...
Opening the last frequency window for radio astronomy in the sub - 30 MHz region includes a few chal...
OLFAR, Orbiting Low Frequency Antennas for Radio Astronomy, will be a space mission to observe the u...
The Lunar Surface Electromagnetics Explorer 'LuSEE Night' is a low frequency radio astronomy experim...
\u3cp\u3eOpening the last frequency window for radio astronomy in the sub - 30 MHz region includes a...
This paper introduces the first results of observations with the Ultra-Long-Wavelength (ULW) -- Low ...
Opening the last frequency window for radio astronomy in the sub - 30 MHz region includes a few chal...
Opening the last frequency window for radio astronomy in the sub - 30 MHz region includes a few chal...
\u3cp\u3eThe past two decades have witnessed a renewed interest in low frequency radio astronomy, wi...
New interesting astronomical science drivers for very low frequency radio astronomy have emerged, ra...
The epoch of formation of the first luminous structures (stars and galaxies) called the Comic Dawn, ...
The frequency band below 30 MHz is one of the last unexplored bands in radio astronomy. This band is...
Radio waves provide a useful diagnostic tool to investigate the properties of the ionosphere because...
The epoch of formation of the first luminous structures (stars and galaxies) called the Comic Dawn, ...