000			03394nam a22004455i 4500
001			u374925
003			SIRSI
005			20160812084258.0
007			cr nn 008mamaa
008			120731s2011 gw | s |||| 0|eng d
020			_a9783642150289 _9978-3-642-15028-9
040			_cMX-MeUAM
050		4	_aQB4
082	0	4	_a520 _223
100	1		_aGlindemann, Andreas. _eauthor.
245	1	0	_aPrinciples of Stellar Interferometry _h[recurso electrónico] / _cby Andreas Glindemann.
264		1	_aBerlin, Heidelberg : _bSpringer Berlin Heidelberg : _bImprint: Springer, _c2011.
300			_aXVIII, 346 p. _bonline resource.
336			_atext _btxt _2rdacontent
337			_acomputer _bc _2rdamedia
338			_aonline resource _bcr _2rdacarrier
347			_atext file _bPDF _2rda
490	1		_aAstronomy and Astrophysics Library, _x0941-7834
505	0		_a1 Propagation of Light -- 2 Imaging Process – Propagation through Optical Systems -- 3 Atmospheric Turbulence -- 4 Instrumental Techniques -- 5 Observing through Atmospheric Turbulence -- 6 Modern Interferometers -- A Appendix -- References -- Index.
520			_aOver the last decade, stellar interferometry has developed from a specialist tool to a mainstream observing technique, attracting scientists whose research benefits from milliarcsecond angular resolution. Stellar interferometry has become part of the astronomer’s toolbox, complementing single-telescope observations by providing unique capabilities that will advance astronomical research. This carefully written book is intended to provide a solid understanding of the principles of stellar interferometry to students starting an astronomical research project in this field or to develop instruments and to astronomers using interferometry but who are not interferometrists per se. Illustrated by excellent drawings and calculated graphs the imaging process in stellar interferometers is explained starting from first principles on light propagation and diffraction wave propagation through turbulence is described in detail using Kolmogorov statistics the impact of turbulence on the imaging process is discussed both for single telescopes and for interferometers instrumental techniques like beam combination and array layout are described, and the requirements for delay lines are derived visibility measurements (modulus and phase) through turbulence are analyzed and limitations are quantified correction methods (fringe tracking and adaptive optics) are presented, discussing closed loop operation with a dual feed system. The book closes with examples of contemporary stellar interferometers and useful appendices on the Fourier transform and atmospheric transmission bands.
650		0	_aPhysics.
650	1	4	_aPhysics.
650	2	4	_aAstronomy, Observations and Techniques.
650	2	4	_aOptics, Optoelectronics, Plasmonics and Optical Devices.
650	2	4	_aOptics and Electrodynamics.
650	2	4	_aNumerical and Computational Physics.
710	2		_aSpringerLink (Online service)
773	0		_tSpringer eBooks
776	0	8	_iPrinted edition: _z9783642150272
830		0	_aAstronomy and Astrophysics Library, _x0941-7834
856	4	0	_zLibro electrónico _uhttp://148.231.10.114:2048/login?url=http://link.springer.com/book/10.1007/978-3-642-15028-9
596			_a19
942			_cLIBRO_ELEC
999			_c202805 _d202805