Add to ORKGThe ALFA mission is a proposed astronomical observatory in space to make high resolution radio images at frequencies below the ionospheric cutoff ( ∼ 20 MHz). This multi-satellite interferometric array will image solar as well as non-solar phenomena in the frequency range 0.03- 30 MHz. In this paper, we provide an overview of the ALFA mission, with particular emphasis on solar studies to be undertaken
Context. The Sun is an active source of radio emission which is often associated with ener...
The Solar Imaging Radio Array (SIRA) is a mission to perform aperture synthesis imaging of low frequ...
© 2015, Springer Science+Business Media Dordrecht. The Atacama Large Millimeter/submillimeter Array ...
Restricted Access. Radio Astronomy at Long Wavelengths, Geophysical Monograph Series, Vol. 119, Eds....
Restricted Access.The frequency range below a few tens of MHz is unexplored with high angular resolu...
Low frequency imaging radio arrays such as MWA, LWA and LOFAR have been recently commissioned, and s...
At frequencies below about 30 MHz, radio astronomy becomes increasingly difficult from the Earth's s...
The Low Frequency Array (LOFAR) will be a radio astronomy interferometric array operating in the app...
OLFAR, Orbiting Low Frequency Antennas for Radio Astronomy, will be a space mission to observe the u...
The Low Frequency Array (LOFAR) will be a radio astronomy interferometric array operating in the app...
Restricted Access.At sufficiently low frequencies, no ground-based radio array will be able to produ...
The frequency band below 30 MHz is one of the last unexplored bands in radio astronomy. This band is...
New interesting astronomical science drivers for very low frequency radio astronomy have emerged, ra...
New interesting astronomical science drivers for very low frequency radio astronomy have emerged, ra...
c.j.m.verhoeventudelft.nl Abstract—Recently new and interesting science drivers have emerged for ver...
Context. The Sun is an active source of radio emission which is often associated with ener...
The Solar Imaging Radio Array (SIRA) is a mission to perform aperture synthesis imaging of low frequ...
© 2015, Springer Science+Business Media Dordrecht. The Atacama Large Millimeter/submillimeter Array ...
Restricted Access. Radio Astronomy at Long Wavelengths, Geophysical Monograph Series, Vol. 119, Eds....
Restricted Access.The frequency range below a few tens of MHz is unexplored with high angular resolu...
Low frequency imaging radio arrays such as MWA, LWA and LOFAR have been recently commissioned, and s...
At frequencies below about 30 MHz, radio astronomy becomes increasingly difficult from the Earth's s...
The Low Frequency Array (LOFAR) will be a radio astronomy interferometric array operating in the app...
OLFAR, Orbiting Low Frequency Antennas for Radio Astronomy, will be a space mission to observe the u...
The Low Frequency Array (LOFAR) will be a radio astronomy interferometric array operating in the app...
Restricted Access.At sufficiently low frequencies, no ground-based radio array will be able to produ...
The frequency band below 30 MHz is one of the last unexplored bands in radio astronomy. This band is...
New interesting astronomical science drivers for very low frequency radio astronomy have emerged, ra...
New interesting astronomical science drivers for very low frequency radio astronomy have emerged, ra...
c.j.m.verhoeventudelft.nl Abstract—Recently new and interesting science drivers have emerged for ver...
Context. The Sun is an active source of radio emission which is often associated with ener...
The Solar Imaging Radio Array (SIRA) is a mission to perform aperture synthesis imaging of low frequ...
© 2015, Springer Science+Business Media Dordrecht. The Atacama Large Millimeter/submillimeter Array ...