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General theory of light propagation and imaging through the atmosphere / T. Stewart McKechnie.

Por: Colaborador(es): Tipo de material: TextoTextoSeries Springer Series in Optical Sciences ; 196Editor: Cham : Springer International Publishing : Springer, 2016Edición: 1st ed. 2016Descripción: xxix, 624 páginas : 190 ilustraciones, 13 ilustraciones en colorTipo de contenido:
  • texto
Tipo de medio:
  • computadora
Tipo de portador:
  • recurso en línea
ISBN:
  • 9783319182094
Formatos físicos adicionales: Edición impresa:: Sin títuloClasificación LoC:
  • QC350-467
Recursos en línea:
Contenidos:
Introduction -- Terms, Definitions and Theoretical foundations -- Diffraction -- Wave propagation after scattering by a thin atmospheric layer -- Wave propagation over extended atmospheric paths -- Properties of point-object im ages formed by telescopes -- Properties of point-object im ages formed by telescopes -- Average intensity envelopes of unresolved star images -- Core and halo structure in star images formed by large telescopes -- Statistical properties of stellar speckle patterns -- Star image appear ance for small and large average turbulence structure sizes -- Approximate intensity envelopes for star images formed by telescopes with/without AO -- Telescope optical tolerances and telescope resolution -- Laboratory simulation of im ages formed by large telescopes -- Laser beam propagation and atmospheric path characterization.- Atmospheric isoplanatic angle: Image stabilization and AO image correction.
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Springer eBooks

Introduction -- Terms, Definitions and Theoretical foundations -- Diffraction -- Wave propagation after scattering by a thin atmospheric layer -- Wave propagation over extended atmospheric paths -- Properties of point-object im ages formed by telescopes -- Properties of point-object im ages formed by telescopes -- Average intensity envelopes of unresolved star images -- Core and halo structure in star images formed by large telescopes -- Statistical properties of stellar speckle patterns -- Star image appear ance for small and large average turbulence structure sizes -- Approximate intensity envelopes for star images formed by telescopes with/without AO -- Telescope optical tolerances and telescope resolution -- Laboratory simulation of im ages formed by large telescopes -- Laser beam propagation and atmospheric path characterization.- Atmospheric isoplanatic angle: Image stabilization and AO image correction.

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