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Diffraction-Limited Imaging with Very Large Teelescopes. In: NATO ASI Series. Series C: Mathematical and Physical Sciences Vol. 274.
Language: English
Published by Dordrecht, Kluwer,, 1989
Seller: Buch & Cafe Antiquarius, Bonn, NRW, Germany
Association Member: GIAQ
Seller rating 5 out of 5 stars
First Edition
Gr.-8°, original hardcover. 1. ed. Numerous fig., XIV, 433 p. Shelfmark on spine, stamp on title, otherwise very fine copy. Sprache: Englisch Gewicht in Gramm: 0.
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Diffraction-Limited Imaging with Very Large Telescopes (Nato Science Series C:)
Seller: Ria Christie Collections, Uxbridge, United Kingdom
Seller rating 5 out of 5 stars
£ 137.84
£ 11.98 shipping
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Diffraction-Limited Imaging with Very Large Telescopes (Nato Science Series C:, 274)
Seller: Ria Christie Collections, Uxbridge, United Kingdom
Seller rating 5 out of 5 stars
£ 137.84
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Ships from United Kingdom to U.S.A.Quantity: Over 20 available
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Diffraction Limited Imaging With Very Large Telescopes
Seller: GreatBookPricesUK, Woodford Green, United Kingdom
Seller rating 5 out of 5 stars
£ 137.83
£ 15 shipping
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Condition: As New. Unread book in perfect condition.
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Condition: New.
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Planets Outside the Solar System: Theory and Observations (Nato Science Series C:, 532)
Seller: Phatpocket Limited, Waltham Abbey, HERTS, United Kingdom
Seller rating 5 out of 5 stars
Condition: Good. Pencil on inside page. Your purchase helps support Sri Lankan Children's Charity 'The Rainbow Centre'. Ex-library, so some stamps and wear, but in good overall condition. Our donations to The Rainbow Centre have helped provide an education and a safe haven to hundreds of children who live in appalling conditions.
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Diffraction-Limited Imaging with Very Large Telescopes
Language: English
Published by Springer Netherlands, 2011
ISBN 10: 9401075530 ISBN 13: 9789401075534
Condition: New.
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Diffraction-Limited Imaging with Very Large Telescopes
Language: English
Published by Springer Netherlands, 1989
ISBN 10: 0792301927 ISBN 13: 9780792301929
Gebunden. Condition: New.
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Diffraction Limited Imaging With Very Large Telescopes
Seller: GreatBookPricesUK, Woodford Green, United Kingdom
Seller rating 5 out of 5 stars
£ 152.32
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Ships from United Kingdom to U.S.A.Quantity: Over 20 available
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Condition: New. pp. 456.
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Condition: New. pp. 452.
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Planets Outside the Solar System: Theory and Observations
Language: English
Published by Springer Netherlands, 1999
ISBN 10: 0792357094 ISBN 13: 9780792357094
Condition: New.
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Planets Outside the Solar System: Theory and Observations
Language: English
Published by Springer Netherlands, 1999
ISBN 10: 0792357086 ISBN 13: 9780792357087
Gebunden. Condition: New.
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Diffraction-Limited Imaging with Very Large Telescopes
Language: English
Published by Springer Netherlands, 2011
ISBN 10: 9401075530 ISBN 13: 9789401075534
Taschenbuch. Condition: Neu. Druck auf Anfrage Neuware - Printed after ordering - A few years ago, a real break-through happened in observational astronomy: the un derstanding of the effect of atmospheric turbulence on the structure of stellar images, and of ways to overcome this dramatic degradation. This opened a route to diffraction-limited observations with large telescopes in the optical domain. Soon, the first applications of this new technique led to some outstanding astrophysical results, both at visible and infrared wavelengths. Yet, the potential of interferometric observations is not fully foreseeable as the first long-baseline arrays of large optical telescopes are being built or cOIIllnissioned right now. In this respect a comparison with the evolution of radio-astronomy is tempting. From a situation where, in spite of the construction of giant antennas, low angular resolution was prevailing, the introduction of long baseline and very long baseline interferometry and the rapid mastering of sophisticated image reconstruction techniques, have brought on a nearly routine basis high dynamic range images with milliarcseconds resolution. This, of course, has completely changed our views of the radio sky.
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Diffraction-Limited Imaging with Very Large Telescopes
Language: English
Published by Springer Netherlands, Springer Netherlands, 1989
ISBN 10: 0792301927 ISBN 13: 9780792301929
Buch. Condition: Neu. Druck auf Anfrage Neuware - Printed after ordering - A few years ago, a real break-through happened in observational astronomy: the un derstanding of the effect of atmospheric turbulence on the structure of stellar images, and of ways to overcome this dramatic degradation. This opened a route to diffraction-limited observations with large telescopes in the optical domain. Soon, the first applications of this new technique led to some outstanding astrophysical results, both at visible and infrared wavelengths. Yet, the potential of interferometric observations is not fully foreseeable as the first long-baseline arrays of large optical telescopes are being built or cOIIllnissioned right now. In this respect a comparison with the evolution of radio-astronomy is tempting. From a situation where, in spite of the construction of giant antennas, low angular resolution was prevailing, the introduction of long baseline and very long baseline interferometry and the rapid mastering of sophisticated image reconstruction techniques, have brought on a nearly routine basis high dynamic range images with milliarcseconds resolution. This, of course, has completely changed our views of the radio sky.
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Adaptive Optics for Astronomy: (Closed)) (Nato Science Series C:)
Seller: Ria Christie Collections, Uxbridge, United Kingdom
Seller rating 5 out of 5 stars
£ 189.04
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Planets Outside the Solar System: Theory and Observations (Nato Science Series C:, 532)
Seller: Ria Christie Collections, Uxbridge, United Kingdom
Seller rating 5 out of 5 stars
£ 189.04
£ 11.98 shipping
Ships from United Kingdom to U.S.A.Quantity: Over 20 available
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Adaptive Optics for Astronomy (Nato Science Series C:, 423)
Seller: Ria Christie Collections, Uxbridge, United Kingdom
Seller rating 5 out of 5 stars
£ 189.04
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Diffraction-Limited Imaging with Very Large Telescopes
Language: English
Published by Springer Netherlands, 2013
ISBN 10: 9401075530 ISBN 13: 9789401075534
Paperback. Condition: Brand New. 452 pages. 9.25x6.10x1.02 inches. In Stock.
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Taschenbuch. Condition: Neu. Planets Outside the Solar System: Theory and Observations | Jean-Marie Mariotti (u. a.) | Taschenbuch | Einband - flex.(Paperback) | Englisch | 1999 | Springer | EAN 9780792357094 | Verantwortliche Person für die EU: Springer Netherlands, Haberstr. 7, 69126 Heidelberg, buchhandel-buch[at]springer[dot]com | Anbieter: preigu.
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Taschenbuch. Condition: Neu. Adaptive Optics for Astronomy | D. M. Alloin (u. a.) | Taschenbuch | xviii | Englisch | 2010 | Springer | EAN 9789048143757 | Verantwortliche Person für die EU: Springer Verlag GmbH, Tiergartenstr. 17, 69121 Heidelberg, juergen[dot]hartmann[at]springer[dot]com | Anbieter: preigu.
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Planets Outside the Solar System
Language: English
Published by Kluwer Academic Publishers, 1999
ISBN 10: 0792357086 ISBN 13: 9780792357087
Seller: Kennys Bookshop and Art Galleries Ltd., Galway, GY, Ireland
Seller rating 5 out of 5 stars
Condition: New. Proceedings of the NATO Advanced Study Institute, held in Cargese, Corsica, France, May 5-15, 1998 Editor(s): Mariotti, Jean-Marie; Alloin, Danielle M. Series: NATO Science Series C. Num Pages: 421 pages, biography. BIC Classification: PGS; RBX. Category: (P) Professional & Vocational; (UP) Postgraduate, Research & Scholarly; (UU) Undergraduate. Dimension: 234 x 156 x 25. Weight in Grams: 802. . 1999. Hardback. . . . .
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Planets Outside the Solar System
Language: English
Published by Kluwer Academic Publishers, 1999
ISBN 10: 0792357094 ISBN 13: 9780792357094
Seller: Kennys Bookshop and Art Galleries Ltd., Galway, GY, Ireland
Seller rating 5 out of 5 stars
Condition: New. The observation and understanding of extra-solar planetary systems has become a topic that poses challenges to many fields of human knowledge. This book sets out a synthesis of the advances. It intends to help young students, researchers, engineers involved or about to become involved in quest for extra-solar planets. Editor(s): Mariotti, Jean-Marie; Alloin, Danielle M. Series: NATO Science Series C. Num Pages: 446 pages, index. BIC Classification: PGS; RBX. Category: (P) Professional & Vocational; (UP) Postgraduate, Research & Scholarly; (UU) Undergraduate. Dimension: 235 x 155. Weight in Grams: 688. . 1999. Paperback. . . . .
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Condition: New. pp. 360.
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Condition: New. pp. 448.
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Condition: New. pp. 446 Softcover reprint of the original 1st ed. 1999 edition.
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Taschenbuch. Condition: Neu. Druck auf Anfrage Neuware - Printed after ordering - For many astronomers, Adaptive Optics is something like a dream coming true. Sinee 1609 and the first observations of celestial bodies performed with the help of an optieal teleseope, astronomers have always fighted to improve the 'resolving power' of their instruments. For a long time, engineers have trimmed the optieal quality of the teleseopes, until they finally reaehed the barrier set by the atmospherie turbulence, a few seconds of are. At that point, the intrinsic quality of the site beeame a major issue to establish new observatories with modern telescopes, and astronomers started to desert the urban skies and to migrate toward mountains and deserts. This quest has been sueeessful and a few privileged sites, where the average natural 'seeing' is close to 0. 5', are now hosting clusters of giant telescopes of the 4 m and soon 10 m class. Yet, this atmospherie limit corresponds in the visible wavelength range to the diffraetion limit of a 20 em telescope only. The loss was severe: a faetor 20 in angular and several hundred in peak energy eoncentration, i. e. in deteetivity of resolution very faint objeets. In the beginning of the seventies, two doors half opened to provide a way out of this dead-end. First, the technique of speckle interferometry (and its various related developments) has allowed to restore the diffraetion limit of large telescopes at visible and infrared wavelengths (see, e. g.
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Taschenbuch. Condition: Neu. Druck auf Anfrage Neuware - Printed after ordering - The question of the existence of other worlds and other living beings has been present in the human quest for knowledge since as far as Epicurus. For centuries this question belonged to the fields of philosophy and theology. The theoretical problem of the formation of the Solar System, and hence of other planetary systems, was tackled only during the 18th century, while the first observational attempts for a detection started less than one hundred years ago. Direct observation of an extra-solar planetary system is an extraordinarily difficult problem: extra-solar planets are at huge distances, are incredibly faint and are overwhelmed by the bright light of their own stars. With virtually no observational insight to test their models, theoreticians have remained for decades in a difficult position to make substantial progress. Yet, the field of stellar formation has provided since the 1980s both the the oretical and observational evidences for the formation of discs at the stage of star birth and for debris materials orbiting the very young stellar systems. It was tempting to consider that these left-overs might indeed later agglomerate into planetary systems more or less similar to ours. Then came observational evidences for planets outside the Solar System.
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Adaptive Optics for Astronomy
Language: English
Published by Springer Netherlands, Springer Netherlands, 1994
ISBN 10: 0792327489 ISBN 13: 9780792327486
Buch. Condition: Neu. Druck auf Anfrage Neuware - Printed after ordering - For many astronomers, Adaptive Optics is something like a dream coming true. Sinee 1609 and the first observations of celestial bodies performed with the help of an optieal teleseope, astronomers have always fighted to improve the 'resolving power' of their instruments. For a long time, engineers have trimmed the optieal quality of the teleseopes, until they finally reaehed the barrier set by the atmospherie turbulence, a few seconds of are. At that point, the intrinsic quality of the site beeame a major issue to establish new observatories with modern telescopes, and astronomers started to desert the urban skies and to migrate toward mountains and deserts. This quest has been sueeessful and a few privileged sites, where the average natural 'seeing' is close to 0. 5', are now hosting clusters of giant telescopes of the 4 m and soon 10 m class. Yet, this atmospherie limit corresponds in the visible wavelength range to the diffraetion limit of a 20 em telescope only. The loss was severe: a faetor 20 in angular and several hundred in peak energy eoncentration, i. e. in deteetivity of resolution very faint objeets. In the beginning of the seventies, two doors half opened to provide a way out of this dead-end. First, the technique of speckle interferometry (and its various related developments) has allowed to restore the diffraetion limit of large telescopes at visible and infrared wavelengths (see, e. g.
