東華大學圖書館 |

語系: 繁體中文

說明(常見問題)

回圖書館首頁

手機版館藏查詢

登入

回首頁

切換: 標籤 | MARC模式 | ISBD

General theory of light propagation ...

McKechnie, T. Stewart.

FindBook

Google Book

Amazon

博客來

General theory of light propagation and imaging through the atmosphere

紀錄類型:	書目-電子資源 : Monograph/item
正題名/作者:	General theory of light propagation and imaging through the atmosphere/ by T. Stewart McKechnie.
作者:	McKechnie, T. Stewart.
出版者:	Cham :Springer International Publishing : : 2016.,
面頁冊數:	xxix, 624 p. :ill. (some col.), digital ;24 cm.
內容註:	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.
Contained By:	Springer eBooks
標題:	Meteorological optics. -
電子資源:	http://dx.doi.org/10.1007/978-3-319-18209-4
ISBN:	9783319182094$q(electronic bk.)

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

General theory of light propagation and imaging through the atmosphere[electronic resource] /by T. Stewart McKechnie. - Cham :Springer International Publishing :2016. - xxix, 624 p. :ill. (some col.), digital ;24 cm. - Springer series in optical sciences,v.1960342-4111 ;. - Springer series in optical sciences ;164..

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.

This book lays out a new, general theory of light propagation and imaging through Earth's turbulent atmosphere. Current theory is based on the – now widely doubted – assumption of Kolmogorov turbulence. The new theory is based on a generalized atmosphere, the turbulence characteristics of which can be established, as needed, from readily measurable properties of point-object, or star, images. The pessimistic resolution predictions of Kolmogorov theory led to lax optical tolerance prescriptions for large ground-based astronomical telescopes which were widely adhered to in the 1970s and 1980s. Around 1990, however, it became clear that much better resolution was actually possible, and Kolmogorov tolerance prescriptions were promptly abandoned. Most large telescopes built before 1990 have had their optics upgraded (e.g., the UKIRT instrument) and now achieve, without adaptive optics (AO), almost an order of magnitude better resolution than before. As well as providing a more comprehensive and precise understanding of imaging through the atmosphere with large telescopes (both with and without AO), the new general theory also finds applications in the areas of laser communications and high-energy laser beam propagation.

ISBN: 9783319182094$q(electronic bk.)

Standard No.: 10.1007/978-3-319-18209-4doiSubjects--Topical Terms:

1017024
Meteorological optics.

LC Class. No.: QC976.S3

Dewey Class. No.: 551.565

General theory of light propagation and imaging through the atmosphere
LDR:03231nmm a2200337 a 4500 001 2028687
003 DE-He213
005 20160715085849.0
006 m d
007 cr nn 008maaau
008 160908s2016 gw s 0 eng d
020 $a 9783319182094$q(electronic bk.)
020 $a 9783319182087$q(paper)
024 7 $a 10.1007/978-3-319-18209-4 $2 doi
035 $a 978-3-319-18209-4
040 $a GP $c GP
041 0 $a eng
050 4 $a QC976.S3
072 7 $a PHJ $2 bicssc
072 7 $a PHK $2 bicssc
072 7 $a SCI021000 $2 bisacsh
082 0 4 $a 551.565 $2 23
090 $a QC976.S3 $b M154 2016
100 1 $a McKechnie, T. Stewart. $3 2179245
245 1 0 $a General theory of light propagation and imaging through the atmosphere $h [electronic resource] / $c by T. Stewart McKechnie.
260 $a Cham : $b Springer International Publishing : $b Imprint: Springer, $c 2016.
300 $a xxix, 624 p. : $b ill. (some col.), digital ; $c 24 cm.
490 1 $a Springer series in optical sciences, $x 0342-4111 ; $v v.196
505 0 $a 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.
520 $a This book lays out a new, general theory of light propagation and imaging through Earth's turbulent atmosphere. Current theory is based on the – now widely doubted – assumption of Kolmogorov turbulence. The new theory is based on a generalized atmosphere, the turbulence characteristics of which can be established, as needed, from readily measurable properties of point-object, or star, images. The pessimistic resolution predictions of Kolmogorov theory led to lax optical tolerance prescriptions for large ground-based astronomical telescopes which were widely adhered to in the 1970s and 1980s. Around 1990, however, it became clear that much better resolution was actually possible, and Kolmogorov tolerance prescriptions were promptly abandoned. Most large telescopes built before 1990 have had their optics upgraded (e.g., the UKIRT instrument) and now achieve, without adaptive optics (AO), almost an order of magnitude better resolution than before. As well as providing a more comprehensive and precise understanding of imaging through the atmosphere with large telescopes (both with and without AO), the new general theory also finds applications in the areas of laser communications and high-energy laser beam propagation.
650 0 $a Meteorological optics. $3 1017024
650 0 $a Light $x Scattering. $3 603682
650 1 4 $a Physics. $3 516296
650 2 4 $a Optics and Electrodynamics. $3 1066865
650 2 4 $a Measurement Science and Instrumentation. $3 1066390
650 2 4 $a Astronomy, Observations and Techniques. $3 1066822
650 2 4 $a Atmospheric Sciences. $3 1019179
650 2 4 $a Mathematical Methods in Physics. $3 890898
710 2 $a SpringerLink (Online service) $3 836513
773 0 $t Springer eBooks
830 0 $a Springer series in optical sciences ; $v 164. $3 1568151
856 4 0 $u http://dx.doi.org/10.1007/978-3-319-18209-4
950 $a Physics and Astronomy (Springer-11651)