About: Argunov–Cassegrain telescope     Goto   Sponge   NotDistinct   Permalink

An Entity of Type : owl:Thing, within Data Space : dbpedia.demo.openlinksw.com associated with source document(s)
QRcode icon
http://dbpedia.demo.openlinksw.com/c/5U5rjVpDQH

The Argunov–Cassegrain telescope is a catadioptric telescope design first introduced in 1972 by P. P. Argunov. All optics are spherical, and the classical Cassegrain secondary mirror is replaced by a sub-aperture secondary corrector group consisting of three air-spaced elements, two lenses and a Mangin mirror (the element farthest from the primary mirror).

AttributesValues
rdfs:label
  • Argunov–Cassegrain telescope (en)
  • 阿古諾夫-卡塞格林望遠鏡 (zh)
rdfs:comment
  • The Argunov–Cassegrain telescope is a catadioptric telescope design first introduced in 1972 by P. P. Argunov. All optics are spherical, and the classical Cassegrain secondary mirror is replaced by a sub-aperture secondary corrector group consisting of three air-spaced elements, two lenses and a Mangin mirror (the element farthest from the primary mirror). (en)
  • 阿古諾夫-卡塞格林望遠鏡的設計是在1972年由P.P. 阿古諾夫首度介紹給世人的。他所有的光學元件都是球面鏡,並將傳統卡塞格林式的次鏡換成三個有空氣隙的透鏡元件。距離主鏡最遠的透鏡是曼京鏡,它的作用如同第二個鏡子的表面,在對向天空的一面有反射用的塗層。阿古諾夫的系統只使用球狀的表面,避免了的製造和測試。然而,獲得的好處似乎很少,因為這套系統實際上非常難以製做,它需要精確的自由區域球的曲率半徑以取代等效的非球面鏡。 (zh)
foaf:depiction
  • http://commons.wikimedia.org/wiki/Special:FilePath/Diagram_Reflector_ArgunovCassegrain.svg
dcterms:subject
Wikipage page ID
Wikipage revision ID
Link from a Wikipage to another Wikipage
Link from a Wikipage to an external page
sameAs
dbp:wikiPageUsesTemplate
thumbnail
has abstract
  • The Argunov–Cassegrain telescope is a catadioptric telescope design first introduced in 1972 by P. P. Argunov. All optics are spherical, and the classical Cassegrain secondary mirror is replaced by a sub-aperture secondary corrector group consisting of three air-spaced elements, two lenses and a Mangin mirror (the element farthest from the primary mirror). (en)
  • 阿古諾夫-卡塞格林望遠鏡的設計是在1972年由P.P. 阿古諾夫首度介紹給世人的。他所有的光學元件都是球面鏡,並將傳統卡塞格林式的次鏡換成三個有空氣隙的透鏡元件。距離主鏡最遠的透鏡是曼京鏡,它的作用如同第二個鏡子的表面,在對向天空的一面有反射用的塗層。阿古諾夫的系統只使用球狀的表面,避免了的製造和測試。然而,獲得的好處似乎很少,因為這套系統實際上非常難以製做,它需要精確的自由區域球的曲率半徑以取代等效的非球面鏡。 (zh)
gold:hypernym
prov:wasDerivedFrom
page length (characters) of wiki page
foaf:isPrimaryTopicOf
is Link from a Wikipage to another Wikipage of
is Wikipage redirect of
is Wikipage disambiguates of
is foaf:primaryTopic of
Faceted Search & Find service v1.17_git147 as of Sep 06 2024


Alternative Linked Data Documents: ODE     Content Formats:   [cxml] [csv]     RDF   [text] [turtle] [ld+json] [rdf+json] [rdf+xml]     ODATA   [atom+xml] [odata+json]     Microdata   [microdata+json] [html]    About   
This material is Open Knowledge   W3C Semantic Web Technology [RDF Data] Valid XHTML + RDFa
OpenLink Virtuoso version 08.03.3332 as of Dec 5 2024, on Linux (x86_64-generic-linux-glibc212), Single-Server Edition (378 GB total memory, 76 GB memory in use)
Data on this page belongs to its respective rights holders.
Virtuoso Faceted Browser Copyright © 2009-2025 OpenLink Software