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Panoramic Radio Astronomy [PDF]

open access: yesProceedings of Panoramic Radio Astronomy: Wide-field 1-2 GHz research on galaxy evolution — PoS(PRA2009), 2010
In this contribution we give a brief overview of the Panoramic Radio Astronomy (PRA) conference held on 2-5 June 2009 in Groningen, the Netherlands. The conference was motivated by the on-going development of a large number of new radio telescopes and instruments which, within a few years, will bring a major improvement over current facilities ...
Paolo Serra, George Heald
openaire   +3 more sources

The future for radio astronomy [PDF]

open access: yesAstronomy & Geophysics, 2013
THE TRANSIENT UNIVERSE Rene P Breton and Tom Hassall argue that, while radio astronomy has always involved transient phenomena, exploration of this part of the electromagnetic spectrum has been falling behind because of the lack of data. But the advent of a new generation of radio telescopes such as LOFAR, could change that.
Breton, Rene   +2 more
openaire   +3 more sources

The impact of cognitive radio on radio astronomy [PDF]

open access: yesProceedings of RFI mitigation workshop — PoS(RFI2010), 2010
The introduction of new communication techniques requires an increase in the efficiency of spectrum usage. Cognitive radio is one of the new techniques that fosters spectrum efficiency by using unoccupied frequency spectrum for communications. However, cognitive radio will increase the transmission power density and cause an increasing level of Radio ...
Albert-Jan Boonstra   +2 more
openaire   +3 more sources

After the SKA - Radio Astronomy in 2049 [PDF]

open access: yes, 2012
The concept of a Square Kilometre Array was developed to ensure that progress in Radio Astronomy in the early 21st Century continued at the same impressive pace as was achieved during the first 50 years. The SKA telescope is designed to pave that road to
Harvey-Smith, Lisa
core   +1 more source

Antenna Design and Implementation for the Future Space Ultra-Long Wavelength Radio Telescope [PDF]

open access: yes, 2018
In radio astronomy, the Ultra-Long Wavelengths (ULW) regime of longer than 10 m (frequencies below 30 MHz), remains the last virtually unexplored window of the celestial electromagnetic spectrum.
Aminaei, Amin   +6 more
core   +4 more sources

Frequencies for Radio Astronomy [PDF]

open access: yesNature, 1970
At present the scope of research in radio astronomy is limited by the allocation of frequencies, some of which have to be shared with other radio services. When the International Telecommunications Union reconsiders all frequency allocations next year, astronomers are hoping for an improvement.
openaire   +3 more sources

Radio physics and radio astronomy

open access: yes, 2017
Purpose: Review of investigations of cosmic sources radioemission scintillations due to interplanetary plasma irregularities made at the Institute of Radio Astronomy of the National Academy of Sciences of Ukraine, from the first observations in the mid-70s until now.
Kalinichenko, M, M   +13 more
openaire   +5 more sources

Meter- to Millimeter Emission from Cool Stellar Systems : Latest Results, Synergies Across the Spectrum, and Outlook for the Next Decade [PDF]

open access: yes, 2018
Splinter session summary, to appear in the proceedings of the 20th Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun (ed. S. J. Wolk)Radio observations of cool stellar systems provide unique information on their magnetic fields, high-energy ...
Berger, Edo   +14 more
core   +2 more sources

Radio Astronomical Polarimetry and the Lorentz Group [PDF]

open access: yes, 1999
In radio astronomy the polarimetric properties of radiation are often modified during propagation and reception. Effects such as Faraday rotation, receiver cross-talk, and differential amplification act to change the state of polarized radiation.
Barakat R.   +9 more
core   +3 more sources

Extragalactic Radio Continuum Surveys and the Transformation of Radio Astronomy

open access: yes, 2017
Next-generation radio surveys are about to transform radio astronomy by discovering and studying tens of millions of previously unknown radio sources.
A Aniyan   +109 more
core   +1 more source

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