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Pierre Kaufmann Radio Observatory

Coordinates: 23°11′07″S 46°33′30″W / 23.1852°S 46.5583°W / -23.1852; -46.5583
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Pierre Kauffman Radio Observatory
Alternative namesROI Edit this on Wikidata
Named afterPierre Kaufmann Edit this on Wikidata
Organization
LocationAtibaia, São Paulo, Brazil
Coordinates23°11′07″S 46°33′30″W / 23.1852°S 46.5583°W / -23.1852; -46.5583
Altitude819 m (2,687 ft) Edit this at Wikidata
Established1970 Edit this on Wikidata
Websitewww.cea.inpe.br/roi/ Edit this at Wikidata
Telescopes
  • Itapetinga Radio Telescope
  • Solar Patrol Equipment
  • Solar Radio Polarimeter Edit this on Wikidata
Pierre Kaufmann Radio Observatory is located in Brazil
Pierre Kaufmann Radio Observatory
Location of Pierre Kaufmann Radio Observatory
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Pierre Kauffman Radio Observatory (Portuguese: Rádio Observatório Pierre Kauffman - ROPK), formerly known as the Itapetinga Radio Observatory[1] (Portuguese: Rádio Observatório de Itapetinga - ROI), is a radio observatory located in the municipality of Atibaia in the state of São Paulo in Brazil. It is located approximately 7.5 km (4.7 mi) south of Atibaia and 40 km (25 mi) north of São Paulo. ROI was founded in 1970 by Universidade Presbiteriana Mackenzie (UPM).[2] Control of the facility was passed to the National Institute for Space Research (INPE) in 1982.[2] Today it is managed jointly by INPE, UPM, University do Vale do Paraíba (Univap), Universidade de São Paulo (USP), and Universidade Federal de Itajubá (UNIFEI).[3] In addition to the telescopes, the observatory has living quarters for visiting scientists. ROI is located inside a small radio quiet zone.[4] It was renamed in 2016 after Pierre Kauffman.

Telescopes

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  • A 13.7 m (45 ft) dish antenna was completed in 1974. It is housed in a radome which was replaced in 1990. It observes in bands from 18 GHz to 26 GHz and 40 GHz to 50 GHz simultaneously.[5] It is used for both astronomical and solar observations.[6][7]
  • The Solar Patrol Equipment (Portuguese: Equipamento de Patrulhamento Solar - SPUA) is an array of 1.5 m (4.9 ft) dish antennas on a common mount. It monitors the intensity and linear polarization of radio waves from the Sun at 12 GHz.[5]
  • The Solar Radio Polarimeter (Portuguese: Rádio Polarímetro Solar - RaPoSo) is a 1.5 m (4.9 ft) antenna with two low-noise receivers centered at 7 GHz. It monitors the intensity and circular polarization of radio waves from the Sun.[8] It was originally located at UPM's defunct Umuarama Radio Observatory near Campos do Jordão and is the oldest telescope at ROI.[9][10]

See also

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References

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  1. ^ "Rádio Observatório Pierre Kaufmann é reinaugurado em Atibaia". www.mackenzie.br (in Spanish). Retrieved 2023-11-18.
  2. ^ a b "Radiobservatório do Itapetinga - ROI/INPE". Radiobservatório do Itapetinga. Retrieved 2012-08-02.
  3. ^ "Comissão de Usuários". Radiobservatório do Itapetinga. Retrieved 2012-08-02.
  4. ^ "Zona de Silêncio". Radiobservatório do Itapetinga. Retrieved 2012-08-02.
  5. ^ a b "Instrumentos". Radiobservatório do Itapetinga. Retrieved 2012-08-02.
  6. ^ Giménez de Castro, C. G.; Raulin, J.-P.; Mandrini, C. H.; Kaufmann, P.; Magun, A. (January 2001). "Multi-resolution wavelet analysis of high time resolution millimeter wavelength observations of solar bursts". Astronomy and Astrophysics. 366: 317–325. Bibcode:2001A&A...366..317G. doi:10.1051/0004-6361:20000088. hdl:11336/22477.
  7. ^ Tateyama, C. E.; Strauss, F. M. (May 1992). "Centaurus a at 22 and 43 GHz". Monthly Notices of the Royal Astronomical Society. 256: 8–12. Bibcode:1992MNRAS.256....8T. doi:10.1093/mnras/256.1.8.
  8. ^ "Rádio Polarímetro Solar (RaPoSo) - Brasil". Radiobservatório do Itapetinga. Retrieved 2012-08-02.
  9. ^ Kaufmann, Pierre (February 1968). "Solar Physics at Mackenzie University, São, Paulo, Brazil". Solar Physics. 3 (2): 360–363. Bibcode:1968SoPh....3..360K. doi:10.1007/BF00155173. S2CID 120001508.
  10. ^ Kaufmann, Pierre (June 1971). "The New Itapetinga Radio Observatory, from Mackenzie University, São Paulo, Brasil". Solar Physics. 18 (2): 336–339. Bibcode:1971SoPh...18..336K. doi:10.1007/BF00145948. S2CID 122294683.