Tools of Radio Astronomy. 6th ed. 2013

種類:

電子ブック

責任表示:

by Thomas L. Wilson, Kristen Rohlfs, Susanne Hüttemeister

出版情報:

Berlin, Heidelberg : Springer Berlin Heidelberg : Imprint: Springer, 2013

著者名:

• Wilson, Thomas L.
• Rohlfs, Kristen.
• Hüttemeister, Susanne.
• SpringerLink (Online service)

シリーズ名:

Astronomy and Astrophysics Library ;

ISBN:

9783642399503 [3642399509]    

注記:

Radio Astronomical Fundamentals -- ElectromagneticWave Propagation Fundamentals -- Wave Polarization -- Signal Processing and Receivers: Theory -- Practical Receiver Systems -- Fundamentals of Antenna Theory -- Practical Aspects of Filled Aperture Antennas -- Single Dish Observational Methods -- Interferometers and Aperture Synthesis -- Emission Mechanisms of Continuous Radiation -- Some Examples of Thermal and Nonthermal Radio Sources -- Spectral Line Fundamentals -- Line Radiation from Atoms -- Radio Recombination Lines -- Overview of Molecular Basics -- Molecules in Interstellar Space -- Some Useful Vector Relations & Fourier Transforms -- The Van Vleck Clipping Correction: One Bit Quantization -- Conventional Derivation of Square Law Detector Response & Receiver Noise -- The Reciprocity Theorem -- Filled Aperture Antennas -- The Hankel Transform -- Lists of Calibration Radio Sources -- The Mutual Coherence Function and van Cittert-Zernike Theorem -- Bibliography -- Index.
This 6th edition of “Tools of Radio Astronomy”, the most used introductory text in radio astronomy, has been revised to reflect the current state of this important branch of astronomy. This includes the use of satellites, low radio frequencies, the millimeter/sub-mm universe, the Cosmic Microwave Background and the increased importance of mm/sub-mm dust emission. Several derivations and presentations of technical aspects of radio astronomy and receivers, such as receiver noise, the Hertz dipole and  beam forming have been updated, expanded, re-worked or complemented by alternative derivations. These reflect advances in technology. The wider bandwidths of the Jansky-VLA and long wave arrays such as LOFAR and mm/sub-mm arrays such as ALMA required an expansion of the discussion of interferometers and aperture synthesis. Developments in data reduction algorithms have been included. As a result of the large amount of data collected in the past 20 years, the discussion of solar system radio astronomy, dust emissio

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