JPL Technical Report Server

An optical vortex coronagraph

Show simple item record

dc.contributor.author Palacios, David M.
dc.date.accessioned 2005-09-30T17:26:28Z
dc.date.available 2005-09-30T17:26:28Z
dc.date.issued 2005-07
dc.identifier.citation SPIE Optics and Photonics Annual Meeting, San Diego, CA, July 31, 2005 en
dc.identifier.clearanceno 05-1974
dc.identifier.uri http://hdl.handle.net/2014/37606
dc.description.abstract In this manuscript, I will discuss the aberration sensitivity of an optical vortex coronagraph and the key advantages it may hold over other coronagraph architectures. I will also provide numerical simulations demonstrating high contrast imaging in the presence of low-order static aberrations. en
dc.description.sponsorship NASA en
dc.format.extent 202312 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 coronagraphs en
dc.subject planet detection en
dc.subject optical vortices en
dc.title An optical vortex coronagraph 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