JPL Technical Report Server

Exo-atmospheric telescopes for Deep Space Optical Communications

Show simple item record

dc.contributor.author Hurd, William J.
dc.contributor.author Moe, Rud V.
dc.contributor.author Dennis, Michael L.
dc.contributor.author MacNeal, Bruce E.
dc.contributor.author Walker, Jon Z.
dc.contributor.author Ortiz, Gerardo G.
dc.contributor.author Eegholm, Bente
dc.contributor.author Fairbrother, debora A.
dc.contributor.author Cheng, Edward S.
dc.contributor.author Kasunic, Keith J.
dc.date.accessioned 2006-02-14T16:17:00Z
dc.date.available 2006-02-14T16:17:00Z
dc.date.issued 2006-03
dc.identifier.citation 2006 IEEE Aerospace Conference, Big Sky, MT, March 4-11, 2006 en
dc.identifier.uri http://hdl.handle.net/2014/38680
dc.description.abstract For deep space optical communications, optical telescopes located above the Earth's atmosphere would have significant performance advantages over telescopes mounted on the Earth's surface. Link outages due to cloud cover would be eliminated, atmospheric attenuation would be eliminated, and signal degradation due to stray light would be reduced. A study has been conducted to compare various exo-atmospheric platforms for the Earth end of the optical link. en
dc.description.sponsorship NASA en
dc.format.extent 972417 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US en
dc.publisher Pasadena, CA : Jet Propulsion Laboratory, National Aeronautics and Space Administration, 2005. en
dc.subject optical communications en
dc.subject orbiting optical terminal en
dc.title Exo-atmospheric telescopes for Deep Space Optical Communications en
dc.type Preprint en


Files in this item

This item appears in the following Collection(s)

Show simple item record

Search


Browse

My Account