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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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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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Proceedings of the NATO Advanced Study Institute, Cargese, Corsica, September 13-23, 1988"
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Diffraction-Limited Imaging with Very Large Telescopes (Nato Science Series C:)
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Zustand: Sehr gut. Auflage: 1989. 433 Seiten dieselbe ISBN-anderes Cover, Cover leicht berieben und kleine Lagerspuren am Buch, Inhalt einwandfrei und ungelesen 153362 Sprache: Englisch Gewicht in Gramm: 800 23,4 x 15,6 x 2,7 cm, Gebundene Ausgabe. Bestandsnummer des Verkäufers 160020
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Diffraction-Limited Imaging with Very Large Telescopes (NATO Science Series C: (closed))
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Hardcover. Zustand: Very Good. Kluwer Academic pictorial hardcover, 1988, clean/tight, ex- MIT Lincoln Laboratory Library copy with minimal markings (M.I.T. lab library stamp on fep, writing on copyright page, card pocket on rear paste-down, no other markings). We will add a custom fitted mylar cover, bubble wrap the book and ship it in a New BOX- Not a plastic bag like the zombie sellers."Diffraction-Limited Imaging with Very Large Telescopes" NATO ASI Series; Series C: Mathematical and Physical Sciences - Vol. 274 (as pictured). Bestandsnummer des Verkäufers TEC1142
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Diffraction-Limited Imaging with Very Large Telescopes
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Diffraction-Limited Imaging with Very Large Telescopes (Nato Science Series C:, 274)
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Diffraction-Limited Imaging with Very Large Telescopes
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Springer Netherlands, Springer Netherlands Jun 1989, 1989
ISBN 10: 0792301927
ISBN 13: 9780792301929
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Buch. Zustand: Neu. Neuware -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.Springer Verlag GmbH, Tiergartenstr. 17, 69121 Heidelberg 456 pp. Englisch. Bestandsnummer des Verkäufers 9780792301929
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Diffraction-Limited Imaging with Very Large Telescopes
Verlag:
Springer Netherlands Jun 1989, 1989
ISBN 10: 0792301927
ISBN 13: 9780792301929
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Anbieter: BuchWeltWeit Ludwig Meier e.K., Bergisch Gladbach, Deutschland
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Buch. Zustand: Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -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. 456 pp. Englisch. Bestandsnummer des Verkäufers 9780792301929
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Diffraction-Limited Imaging with Very Large Telescopes (Nato Science Series C:, 274)
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Diffraction-Limited Imaging with Very Large Telescopes
Verlag:
Springer Netherlands, Springer Netherlands, 1989
ISBN 10: 0792301927
ISBN 13: 9780792301929
Neu
Hardcover
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Buch. Zustand: 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. Bestandsnummer des Verkäufers 9780792301929
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Diffraction Limited Imaging With Very Large Telescopes
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Diffraction Limited Imaging With Very Large Telescopes
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