Focal-plane arrays (FPAs) are widely used in radio astronomy. FPAs are arrays of receivers placed at the focus of the optical system in a radio-telescope. The optical system may be a reflector or a lens. Traditional radio-telescopes have only one receiver at the focus of the telescope, but radio-telescopes are now starting to be equipped with focal plane arrays, which are of three different types: multi-beam feed arrays, bolometer arrays, and the experimental phased-array feeds.
Multi-beam feed arrays consist of a small array of feed horns at the focus of a radio-telescope. Each feed horn is connected to a receiver to measure the received power and each horn and receiver pair is sensitive to radio waves from a slightly different direction in the sky. A feed array with n receivers will increase the survey speed of the telescope by a factor of n, making them very powerful survey instruments. Because radio wavelengths are large, the resulting feed arrays are amongst the largest radio-astronomy receivers ever built. Examples include the multi-beam arrays on the Parkes Observatory,[1][2] and the ALFA array at Arecibo Observatory,[3] both of which have been used for major pulsar and Hydrogen line studies, such as HIPASS.
Bolometer arraysedit
Bolometer arrays are arrays of bolometer receivers which measure the energy of incoming radio photons. They are typically used for astronomy at millimeter wavelengths. Examples include the SCUBA receiver on the James Clerk Maxwell Telescope and the LABOCA [4] instrument on the APEX telescope.
Phased array feedsedit
Phased Array Feeds are an experimental type of focal plane array using phased array technology in which antenna elements are closely spaced so that they do not act independently, but instead act as sensors of the electromagnetic field across the focal plane of the telescope. The outputs of the receivers are then coherently combined in a beamformer with appropriate weights to synthesise several discrete beams. They are currently being developed for the Apertif [5] upgrade to the Westerbork Synthesis Radio Telescope, and for the Australian Square Kilometre Array Pathfinder radio telescope.
Switched array feedsedit
A switchable array of feed antennas in the focal plane is referred to as a switchable FPA. With this configuration, it is possible to switch between a set of beams directed in different directions. This makes the system steerable in the switching sense, thus creating a multi-beam system. In a switched FPA, the distance between feeding elements are chosen following [6]
where F is the focal length of the optical system, D is the diameter of the optical system and λ is the wavelength.
Monopulse feedsedit
The angle to the observed target (e.g. a meteor in meteor studies) can be estimated using amplitude monopulse. In such a configuration, three signals are collected from four feed elements. These signals are the elevation difference signal, the azimuth difference signal and the sum signal.
^Cohen, R.J.; Caswell, J.L.; Brooks, K.; Burton, M.G.; Chrysostomou, A.; Cox, J.; Diamond, P.J.; Ellingsen, S.; Fuller, G.A.; Gray, M.D.; Green, J.A.; Hoare, M.G.; Masheder, M.R.W.; McClure-Griffiths, N.; Pestalozzi, M.; Phillips, C.; Thompson, M.; Voronkov, M.; Walsh, A.; Ward-Thompson, D.; Wong-McSweeney, D.; Yates, J.A. (15 August 2006). The Parkes methanol multibeam survey. IAU Symposium #237: Star Formation in a Turbulent ISM. Proceedings of the International Astronomical Union. Vol. 2, no. S237. Prague. p. 403. Bibcode:2007IAUS..237..403C. doi:10.1017/S1743921307001913. hdl:2299/1767.
^. Archived from the original on 2009-09-03. Retrieved 2010-11-21.
^. Archived from the original on 2010-11-10. Retrieved 2010-11-21.
^. Archived from the original on 2015-01-16. Retrieved 2010-11-21.
^Frid, Henrik (2016). "Closed-Form Relation Between the Scan Angle and Feed Position for Extended Hemispherical Lenses Based on Ray Tracing". IEEE Antennas and Wireless Propagation Letters. 15: 1963. Bibcode:2016IAWPL..15.1963F. doi:10.1109/LAWP.2016.2545858. S2CID 24384665.
January 01, 1970
focal, plane, array, radio, astronomy, focal, plane, arrays, fpas, widely, used, radio, astronomy, fpas, arrays, receivers, placed, focus, optical, system, radio, telescope, optical, system, reflector, lens, traditional, radio, telescopes, have, only, receiver. Focal plane arrays FPAs are widely used in radio astronomy FPAs are arrays of receivers placed at the focus of the optical system in a radio telescope The optical system may be a reflector or a lens Traditional radio telescopes have only one receiver at the focus of the telescope but radio telescopes are now starting to be equipped with focal plane arrays which are of three different types multi beam feed arrays bolometer arrays and the experimental phased array feeds Contents 1 Multi beam feed arrays 2 Bolometer arrays 3 Phased array feeds 4 Switched array feeds 5 Monopulse feeds 6 See also 7 ReferencesMulti beam feed arrays editMulti beam feed arrays consist of a small array of feed horns at the focus of a radio telescope Each feed horn is connected to a receiver to measure the received power and each horn and receiver pair is sensitive to radio waves from a slightly different direction in the sky A feed array with n receivers will increase the survey speed of the telescope by a factor of n making them very powerful survey instruments Because radio wavelengths are large the resulting feed arrays are amongst the largest radio astronomy receivers ever built Examples include the multi beam arrays on the Parkes Observatory 1 2 and the ALFA array at Arecibo Observatory 3 both of which have been used for major pulsar and Hydrogen line studies such as HIPASS Bolometer arrays editBolometer arrays are arrays of bolometer receivers which measure the energy of incoming radio photons They are typically used for astronomy at millimeter wavelengths Examples include the SCUBA receiver on the James Clerk Maxwell Telescope and the LABOCA 4 instrument on the APEX telescope Phased array feeds editPhased Array Feeds are an experimental type of focal plane array using phased array technology in which antenna elements are closely spaced so that they do not act independently but instead act as sensors of the electromagnetic field across the focal plane of the telescope The outputs of the receivers are then coherently combined in a beamformer with appropriate weights to synthesise several discrete beams They are currently being developed for the Apertif 5 upgrade to the Westerbork Synthesis Radio Telescope and for the Australian Square Kilometre Array Pathfinder radio telescope Switched array feeds editA switchable array of feed antennas in the focal plane is referred to as a switchable FPA With this configuration it is possible to switch between a set of beams directed in different directions This makes the system steerable in the switching sense thus creating a multi beam system In a switched FPA the distance between feeding elements are chosen following 6 D d F l D displaystyle Delta d F lambda D nbsp where F is the focal length of the optical system D is the diameter of the optical system and l is the wavelength Monopulse feeds editThe angle to the observed target e g a meteor in meteor studies can be estimated using amplitude monopulse In such a configuration three signals are collected from four feed elements These signals are the elevation difference signal the azimuth difference signal and the sum signal See also editStaring arrayReferences edit Parkes 21 cm Multibeam Project Cohen R J Caswell J L Brooks K Burton M G Chrysostomou A Cox J Diamond P J Ellingsen S Fuller G A Gray M D Green J A Hoare M G Masheder M R W McClure Griffiths N Pestalozzi M Phillips C Thompson M Voronkov M Walsh A Ward Thompson D Wong McSweeney D Yates J A 15 August 2006 The Parkes methanol multibeam survey IAU Symposium 237 Star Formation in a Turbulent ISM Proceedings of the International Astronomical Union Vol 2 no S237 Prague p 403 Bibcode 2007IAUS 237 403C doi 10 1017 S1743921307001913 hdl 2299 1767 ALFA Archived from the original on 2009 09 03 Retrieved 2010 11 21 LABOCA Archived from the original on 2010 11 10 Retrieved 2010 11 21 Apertif Archived from the original on 2015 01 16 Retrieved 2010 11 21 Frid Henrik 2016 Closed Form Relation Between the Scan Angle and Feed Position for Extended Hemispherical Lenses Based on Ray Tracing IEEE Antennas and Wireless Propagation Letters 15 1963 Bibcode 2016IAWPL 15 1963F doi 10 1109 LAWP 2016 2545858 S2CID 24384665 Retrieved from https en wikipedia org w index php title Focal plane array radio astronomy amp oldid 1219843629, wikipedia, wiki, book, books, library,
