The Narrabri Stellar Intensity Interferometer (NSII) was the first astronomical instrument to measure the diameters of a large number of stars at visible wavelengths. It was designed by (amongst others) Robert Hanbury Brown, who received the Hughes Medal in 1971 for this work. It was built by University of Sydney School of Physics and was located near the town of Narrabri in north-central New South Wales, Australia. Many of the components were constructed in the UK. The design was based on an earlier optical intensity interferometer built by Hanbury Brown and Richard Q. Twiss at Jodrell Bank in the UK. Whilst the original device had a maximum baseline of 10m, the NSII device consisted of a large circular track that allowed the detectors to be separated from 10 to 188m. The NSII operated fr
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| - Narrabri Stellar Intensity Interferometer (en)
- 納拉布里恆星強度干涉儀 (zh)
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| - 納拉布里恆星強度干涉儀 (NSII)是第一個測量大量恆星在可見光波長直徑的天文儀器。他是由(還有其他人)設計的,他因這項工作在1971年獲得。它是由雪梨大學物理學院建造,座落於澳州新南威爾斯中心偏北的納拉布里。它的設計是基於較早期由Hanbury Brown和在英國建造的光學。NSII從1963年工作至1974年,曾用來測量32顆恆星的角直徑。 (zh)
- The Narrabri Stellar Intensity Interferometer (NSII) was the first astronomical instrument to measure the diameters of a large number of stars at visible wavelengths. It was designed by (amongst others) Robert Hanbury Brown, who received the Hughes Medal in 1971 for this work. It was built by University of Sydney School of Physics and was located near the town of Narrabri in north-central New South Wales, Australia. Many of the components were constructed in the UK. The design was based on an earlier optical intensity interferometer built by Hanbury Brown and Richard Q. Twiss at Jodrell Bank in the UK. Whilst the original device had a maximum baseline of 10m, the NSII device consisted of a large circular track that allowed the detectors to be separated from 10 to 188m. The NSII operated fr (en)
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| - The Narrabri Stellar Intensity Interferometer (NSII) was the first astronomical instrument to measure the diameters of a large number of stars at visible wavelengths. It was designed by (amongst others) Robert Hanbury Brown, who received the Hughes Medal in 1971 for this work. It was built by University of Sydney School of Physics and was located near the town of Narrabri in north-central New South Wales, Australia. Many of the components were constructed in the UK. The design was based on an earlier optical intensity interferometer built by Hanbury Brown and Richard Q. Twiss at Jodrell Bank in the UK. Whilst the original device had a maximum baseline of 10m, the NSII device consisted of a large circular track that allowed the detectors to be separated from 10 to 188m. The NSII operated from 1963 until 1974, and was used to measure the angular diameters of 32 stars. (en)
- 納拉布里恆星強度干涉儀 (NSII)是第一個測量大量恆星在可見光波長直徑的天文儀器。他是由(還有其他人)設計的,他因這項工作在1971年獲得。它是由雪梨大學物理學院建造,座落於澳州新南威爾斯中心偏北的納拉布里。它的設計是基於較早期由Hanbury Brown和在英國建造的光學。NSII從1963年工作至1974年,曾用來測量32顆恆星的角直徑。 (zh)
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