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Publicado por Springer, 2002
ISBN 10: 1852334290ISBN 13: 9781852334291
Librería: Books Puddle, New York, NY, Estados Unidos de America
Libro
Condición: New. pp. 296.
Publicado por Springer, 2002
ISBN 10: 1852334290ISBN 13: 9781852334291
Librería: Majestic Books, Hounslow, Reino Unido
Libro
Condición: New. pp. 296 Illus.
Publicado por Springer, 2012
ISBN 10: 1447110870ISBN 13: 9781447110873
Librería: booksXpress, Bayonne, NJ, Estados Unidos de America
Libro
Soft Cover. Condición: new.
Publicado por Springer, 2000
ISBN 10: 0792363817ISBN 13: 9780792363811
Librería: Books From California, Simi Valley, CA, Estados Unidos de America
Libro
hardcover. Condición: Very Good.
Publicado por Springer, 2002
ISBN 10: 1852334290ISBN 13: 9781852334291
Librería: Romtrade Corp., STERLING HEIGHTS, MI, Estados Unidos de America
Libro
Condición: New. Brand New Original US Edition.We Ship to PO BOX Address also. EXPEDITED shipping option also available for faster delivery.This item may ship from the US or other locations in India depending on your location and availability.
Publicado por Springer, 2002
ISBN 10: 1852334290ISBN 13: 9781852334291
Librería: SMASS Sellers, IRVING, TX, Estados Unidos de America
Libro
Condición: New. Brand New Original US Edition. Customer service! Satisfaction Guaranteed. This item may ship from the US or our Overseas warehouse depending on your location and stock availability. We Ship to PO BOX Location also.
Publicado por Springer, 2002
ISBN 10: 1852334290ISBN 13: 9781852334291
Librería: BennettBooksLtd, North Las Vegas, NV, Estados Unidos de America
Libro
Condición: New. New. In shrink wrap. Looks like an interesting title! 1.2.
Publicado por Springer, 2002
ISBN 10: 1852334290ISBN 13: 9781852334291
Librería: booksXpress, Bayonne, NJ, Estados Unidos de America
Libro
Hardcover. Condición: new.
Publicado por Springer, 2002
ISBN 10: 1852334290ISBN 13: 9781852334291
Librería: Books Unplugged, Amherst, NY, Estados Unidos de America
Libro
Condición: Good. Buy with confidence! Book is in good condition with minor wear to the pages, binding, and minor marks within.
Publicado por Springer, 2002
ISBN 10: 1852334290ISBN 13: 9781852334291
Librería: GF Books, Inc., Hawthorne, CA, Estados Unidos de America
Libro
Condición: New. Book is in NEW condition.
Publicado por Springer, 2002
ISBN 10: 1852334290ISBN 13: 9781852334291
Librería: GF Books, Inc., Hawthorne, CA, Estados Unidos de America
Libro
Condición: Fine. Book is in Used-LikeNew condition. Pages and cover are clean and intact. Used items may not include supplementary materials such as CDs or access codes. May show signs of minor shelf wear.
Publicado por Springer, 2002
ISBN 10: 1852334290ISBN 13: 9781852334291
Librería: Book Deals, Tucson, AZ, Estados Unidos de America
Libro
Condición: New. New! This book is in the same immaculate condition as when it was published.
Publicado por Springer, 2012
ISBN 10: 1447110870ISBN 13: 9781447110873
Librería: Lucky's Textbooks, Dallas, TX, Estados Unidos de America
Libro
Condición: New.
Publicado por Springer, 2002
ISBN 10: 1852334290ISBN 13: 9781852334291
Librería: Lucky's Textbooks, Dallas, TX, Estados Unidos de America
Libro
Condición: New.
Publicado por Springer, 2002
ISBN 10: 1852334290ISBN 13: 9781852334291
Librería: Ria Christie Collections, Uxbridge, Reino Unido
Libro Impresión bajo demanda
Condición: New. PRINT ON DEMAND Book; New; Fast Shipping from the UK. No. book.
Publicado por Springer, 2012
ISBN 10: 1447110870ISBN 13: 9781447110873
Librería: Ria Christie Collections, Uxbridge, Reino Unido
Libro Impresión bajo demanda
Condición: New. PRINT ON DEMAND Book; New; Fast Shipping from the UK. No. book.
Publicado por Springer London Ltd, 2012
ISBN 10: 1447110870ISBN 13: 9781447110873
Librería: THE SAINT BOOKSTORE, Southport, Reino Unido
Libro Impresión bajo demanda
Paperback / softback. Condición: New. This item is printed on demand. New copy - Usually dispatched within 5-9 working days.
Publicado por Springer London, 2012
ISBN 10: 1447110870ISBN 13: 9781447110873
Librería: moluna, Greven, Alemania
Libro Impresión bajo demanda
Condición: New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. Fusion bonding is one of the three methods available for joining composite and dissimilar materials. While the other two, mechanical fastening and adhesion bonding, have been the subject of wide coverage both in textbooks and monographs, fusion bonding is c.
Publicado por Springer London, 2002
ISBN 10: 1852334290ISBN 13: 9781852334291
Librería: moluna, Greven, Alemania
Libro Impresión bajo demanda
Gebunden. Condición: New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. Fusion bonding is one of the three methods available for joining composite and dissimilar materials. While the other two, mechanical fastening and adhesion bonding, have been the subject of wide coverage both in textbooks and monographs, fusion bonding is c.
Publicado por Springer, 2000
ISBN 10: 0792363817ISBN 13: 9780792363811
Librería: booksXpress, Bayonne, NJ, Estados Unidos de America
Libro
Hardcover. Condición: new.
Publicado por Springer, 2010
ISBN 10: 9048154928ISBN 13: 9789048154920
Librería: booksXpress, Bayonne, NJ, Estados Unidos de America
Libro
Soft Cover. Condición: new.
Publicado por Springer, 2010
ISBN 10: 9048154928ISBN 13: 9789048154920
Librería: Lucky's Textbooks, Dallas, TX, Estados Unidos de America
Libro
Condición: New.
Publicado por Springer, 2000
ISBN 10: 0792363817ISBN 13: 9780792363811
Librería: Lucky's Textbooks, Dallas, TX, Estados Unidos de America
Libro
Condición: New.
Publicado por Springer Netherlands Mai 2000, 2000
ISBN 10: 0792363817ISBN 13: 9780792363811
Librería: BuchWeltWeit Ludwig Meier e.K., Bergisch Gladbach, Alemania
Libro Impresión bajo demanda
Buch. Condición: Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -Adaptive optics allows the theoretical limit of angular resolution to be achieved from a large telescope, despite the presence of turbulence. Thus an eight meter class telescope, such as one of the four in the Very Large Telescope operated by ESO in Chile, will in future be routinely capable of an angular resolution of almost 0.01 arcsec, compared tot he present resolution of about 0.5 arcsec for conventional imaging in good condition. All the world's major telescopes either have adaptive optics or are in the process of building AO systems. It turns out that a reasonable fraction of the sky can be observed using adaptive optics, with moderately good imaging quality, provided imaging in done in the near IR. To move out of the near IR, with its relatively poor angular resolution, astronomers need a laser guide star. There is a layer of Na atoms at approximately 90 km altitude that can be excited by a laser to produce such a source, or Rayleigh scattering can be employed lower in the atmosphere. But the production and use of laser guide stars is not trivial, and the key issues determining their successful implementation are discussed here, including the physics of the Na atom, the cone effect, tilt determination, sky coverage, and numerous potential astronomical applications. 368 pp. Englisch.
Publicado por Springer Netherlands Dez 2010, 2010
ISBN 10: 9048154928ISBN 13: 9789048154920
Librería: BuchWeltWeit Ludwig Meier e.K., Bergisch Gladbach, Alemania
Libro Impresión bajo demanda
Taschenbuch. Condición: Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -Adaptive optics allows the theoretical limit of angular resolution to be achieved from a large telescope, despite the presence of turbulence. Thus an eight meter class telescope, such as one of the four in the Very Large Telescope operated by ESO in Chile, will in future be routinely capable of an angular resolution of almost 0.01 arcsec, compared tot he present resolution of about 0.5 arcsec for conventional imaging in good condition. All the world's major telescopes either have adaptive optics or are in the process of building AO systems. It turns out that a reasonable fraction of the sky can be observed using adaptive optics, with moderately good imaging quality, provided imaging in done in the near IR. To move out of the near IR, with its relatively poor angular resolution, astronomers need a laser guide star. There is a layer of Na atoms at approximately 90 km altitude that can be excited by a laser to produce such a source, or Rayleigh scattering can be employed lower in the atmosphere. But the production and use of laser guide stars is not trivial, and the key issues determining their successful implementation are discussed here, including the physics of the Na atom, the cone effect, tilt determination, sky coverage, and numerous potential astronomical applications. 368 pp. Englisch.
Publicado por Springer, 2010
ISBN 10: 9048154928ISBN 13: 9789048154920
Librería: Ria Christie Collections, Uxbridge, Reino Unido
Libro Impresión bajo demanda
Condición: New. PRINT ON DEMAND Book; New; Fast Shipping from the UK. No. book.
Publicado por Springer, 2000
ISBN 10: 0792363817ISBN 13: 9780792363811
Librería: Ria Christie Collections, Uxbridge, Reino Unido
Libro Impresión bajo demanda
Condición: New. PRINT ON DEMAND Book; New; Fast Shipping from the UK. No. book.
Publicado por Springer, 2002
ISBN 10: 1852334290ISBN 13: 9781852334291
Librería: Mispah books, Redhill, SURRE, Reino Unido
Libro
Hardcover. Condición: Like New. Like New. book.
Publicado por Springer Netherlands, 2010
ISBN 10: 9048154928ISBN 13: 9789048154920
Librería: AHA-BUCH GmbH, Einbeck, Alemania
Libro
Taschenbuch. Condición: Neu. Druck auf Anfrage Neuware - Printed after ordering - Adaptive optics allows the theoretical limit of angular resolution to be achieved from a large telescope, despite the presence of turbulence. Thus an eight meter class telescope, such as one of the four in the Very Large Telescope operated by ESO in Chile, will in future be routinely capable of an angular resolution of almost 0.01 arcsec, compared tot he present resolution of about 0.5 arcsec for conventional imaging in good condition. All the world's major telescopes either have adaptive optics or are in the process of building AO systems. It turns out that a reasonable fraction of the sky can be observed using adaptive optics, with moderately good imaging quality, provided imaging in done in the near IR. To move out of the near IR, with its relatively poor angular resolution, astronomers need a laser guide star. There is a layer of Na atoms at approximately 90 km altitude that can be excited by a laser to produce such a source, or Rayleigh scattering can be employed lower in the atmosphere. But the production and use of laser guide stars is not trivial, and the key issues determining their successful implementation are discussed here, including the physics of the Na atom, the cone effect, tilt determination, sky coverage, and numerous potential astronomical applications.
Publicado por Springer Netherlands, 2000
ISBN 10: 0792363817ISBN 13: 9780792363811
Librería: AHA-BUCH GmbH, Einbeck, Alemania
Libro
Buch. Condición: Neu. Druck auf Anfrage Neuware - Printed after ordering - Adaptive optics allows the theoretical limit of angular resolution to be achieved from a large telescope, despite the presence of turbulence. Thus an eight meter class telescope, such as one of the four in the Very Large Telescope operated by ESO in Chile, will in future be routinely capable of an angular resolution of almost 0.01 arcsec, compared tot he present resolution of about 0.5 arcsec for conventional imaging in good condition. All the world's major telescopes either have adaptive optics or are in the process of building AO systems. It turns out that a reasonable fraction of the sky can be observed using adaptive optics, with moderately good imaging quality, provided imaging in done in the near IR. To move out of the near IR, with its relatively poor angular resolution, astronomers need a laser guide star. There is a layer of Na atoms at approximately 90 km altitude that can be excited by a laser to produce such a source, or Rayleigh scattering can be employed lower in the atmosphere. But the production and use of laser guide stars is not trivial, and the key issues determining their successful implementation are discussed here, including the physics of the Na atom, the cone effect, tilt determination, sky coverage, and numerous potential astronomical applications.