'Radio astronomy' diaporamas de présentation

Note on Posted Slides

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An Introduction to Radio Astronomy Marcus Leech VE3MDL

An Introduction to Radio Astronomy Marcus Leech VE3MDL. Image appears courtesy NRAO/AUI. What is Radio Astronomy?. Astronomy at wavelengths from a few mm to tens of meters Visible light has wavelengths in the region of 500nm, that is, 5.0x10 -7 meters

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Science enabled by NRAO facilities into the next decade

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Eddington, Ryle and Hoyle

Eddington, Ryle and Hoyle. Jasper Wall. How a major 20th Century discovery was lost in noise and confusion. What were the great surprise discoveries of the 20th century?. Richard Ellis, arXiv:0701024:. Cosmic expansion (Slipher and Hubble 1917-1925)

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Lunatic fringe: probing the dark ages from the dark side of the Moon

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An Introduction to the ITU

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Budapest University of Technology and Economy Research Seminar October 2006

Budapest University of Technology and Economy Research Seminar October 2006. Standardisation and Interoperability of the Technology and equipment for BPL Systems. Key Points of Talk. Current Developments of BPL in the World Technical Restrictions and Limitations

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Low Frequency, Wide-Field Astronomy with PAPER: Precision Array to Probe the Epoch of Reionization

Low Frequency, Wide-Field Astronomy with PAPER: Precision Array to Probe the Epoch of Reionization. Nicole Gugliucci Graduate Student, UVa /NRAO Advisor: Rich Bradley. Collaborators: D. Backer, A. Parsons, J. Manley, G. Foster, M . Wright, D. Werthimer , CASPER group (UCB),

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Radio Astronomy Timeline

Radio Astronomy Timeline. By Winter Sie-Hilland and Kevin Mogk. Image courtesy of NRAO/AUI. Major Discoveries. 1951 the 21 cm line for neutral Hydrogen is first observed ( National Radio Astronomy Observatory . 2011.) 1941 First radio map of the sky by Grote Gerber ( MITTON 20057 p289)

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Observing the Solar System Chapter 14.1 [p. 538]

Observing the Solar System Chapter 14.1 [p. 538]. Early Ideas of the Solar System. The Greeks thought that they were inside a rotating dome they called the celestial sphere. The Greeks also thought that the universe was perfect and unchangeable.

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Analysis of Adaptive Array Algorithm Performance for Satellite Interference Cancellation in Radio Astronomy

Analysis of Adaptive Array Algorithm Performance for Satellite Interference Cancellation in Radio Astronomy. Lisha Li, Brian D. Jeffs, Andrew Poulsen, and Karl Warnick Brigham Young University XXVII URSI General Assembly 2002 . Summary.

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ITU-R Standardization Activities

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WRC 2007 Results October 22 ~ November 16, 2007 Geneva, Switzerland

WRC 2007 Results October 22 ~ November 16, 2007 Geneva, Switzerland. Masatoshi OHISHI RAFCAP meeting 2008. WRC-07 Agenda Item 1.17.

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Scientific Opportunities

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Observational techniques meeting #14

Observational techniques meeting #14. Cosmic microwave background: history + basic instrumentation CMB: recent developments MM/ SubMM instrumentation: SCUBA -> ALMA Sunyaev-Zeldovich effect; detection; implications Light echoes IFU spectrographs Neutrino detectors TEV telescopes

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Radio Astronomy in Mexico

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IUCAF

IUCAF. Scientific Committee on Frequency Allocations for Radio Astronomy and Space Science formerly known as the I nter- U nion C ommission on the A llocation of F requencies for Space Research and Radio Astronomy. The brief of IUCAF. To study and coordinate

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Closing Plenary Meeting report for IG THz Group

Closing Plenary Meeting report for IG THz Group. Meeting was called to order at 1:30pm and finished at 5.30 pm. Meeting minutes of the July meeting were updated and approved Five presentations have been made:

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BACKGROUND

The Pulsar Search Collaboratory Your discovery is here! Sue Ann Heatherly, PI National Radio Astronomy Observatory, Green Bank, WV. The Pulsar Search Collaboratory (PSC) project is a partnership between the National Radio Astronomy Observatory in Green Bank, WV, West Virginia University.

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