This paper presents an analysis of the shortcomingsof dipoles in space-based low frequency radio astronomy. It is atthese frequencies that it is expected to uncover more informationabout the beginning of the universe, the Dark Ages. At thismoment there is a 5 m tripole setup, part of the Netherlands-China Low Frequency Explorer (NCLE) on Earth-Moon-L2 HaloOrbit. However, the dipole is limited in term of bandwidth,size and impedance. To further increase the sensitivity, moreadvanced structures are needed which can be packed in thesame volume. This paper will present multiple solutions to theproblem in the form of inflatable antennas and the usage of shapememory alloys which are both viable options. A future solutionis a combination of both f...
This paper presents a brief overview of the state of the art for the design of an ultra low frequenc...
At frequencies below about 30 MHz, radio astronomy becomes increasingly difficult from the Earth's s...
This paper presents a brief overview of the state of the art for the design of an ultra low frequenc...
This paper presents an analysis of the shortcomingsof dipoles in space-based low frequency radio ast...
The Orbiting Low Frequency Antennas for Radio Astronomy (OLFAR) project is investigating an orbiting...
The past two decades have witnessed a renewed interest in low frequency radio astronomy, with a part...
Purpose: Theoretical and experimental studies of the active antenna – an element of the low-frequenc...
Low-frequency radio astronomy is limited by severe ionospheric distortions below 50 MHz and complete...
The moon is a unique location in our solar system and provides important information regarding the e...
The non transparency and severe propagation effects of the terrestrial ionosphere make it impossible...
New interesting astronomical science drivers for very low frequency radio astronomy have emerged, ra...
OLFAR, Orbiting Low Frequency Antennas for Radio Astronomy, will be a space mission to observe the u...
The Jet Propulsion Laboratory (JPL) is developing concepts and technologies for low frequency radio ...
This paper presents a brief overview of the state of the art for the design of an ultra low frequenc...
At frequencies below about 30 MHz, radio astronomy becomes increasingly difficult from the Earth's s...
This paper presents a brief overview of the state of the art for the design of an ultra low frequenc...
This paper presents an analysis of the shortcomingsof dipoles in space-based low frequency radio ast...
The Orbiting Low Frequency Antennas for Radio Astronomy (OLFAR) project is investigating an orbiting...
The past two decades have witnessed a renewed interest in low frequency radio astronomy, with a part...
Purpose: Theoretical and experimental studies of the active antenna – an element of the low-frequenc...
Low-frequency radio astronomy is limited by severe ionospheric distortions below 50 MHz and complete...
The moon is a unique location in our solar system and provides important information regarding the e...
The non transparency and severe propagation effects of the terrestrial ionosphere make it impossible...
New interesting astronomical science drivers for very low frequency radio astronomy have emerged, ra...
OLFAR, Orbiting Low Frequency Antennas for Radio Astronomy, will be a space mission to observe the u...
The Jet Propulsion Laboratory (JPL) is developing concepts and technologies for low frequency radio ...
This paper presents a brief overview of the state of the art for the design of an ultra low frequenc...
At frequencies below about 30 MHz, radio astronomy becomes increasingly difficult from the Earth's s...
This paper presents a brief overview of the state of the art for the design of an ultra low frequenc...