High-efficiency 'superchromatic' polarimetry optics for use in optical astronomical spectrographs

Computer Science – Performance

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

30

Astronomical Polarimetry, Astronomical Spectroscopy, Spectrographs, Astronomical Observatories, Beam Splitters, Charge Coupled Devices, Performance Prediction, Telescopes

Scientific paper

A design for an optical spectropolarimeter consisting of a Pancharatnam half-wave plate and a modified Glan-Taylor polarizing beam splitter retrofitted to an existing astronomical spectrograph is described. The wave plate has a retardance of 180 +/-2 deg over the entire design wavelength range from 3200 A to 1.1 micron. The calcite polarizing beam splitter has a beam separation of one beam diameter, and a low length-to-width ratio of 1.035, making efficient use of the limited space available in most spectrographs. Cassegrain CCD spectrographs on the Mount Locke 2.7-m and Mount Palomar 5-in telescopes have been retrofitted with spectropolarimeters of the type described. The combination of these 'superachromatic' polarimeter parts with the high-efficiency CCD detectors now used in these and many other astronomical spectrographs should lead to a great expansion of spectropolarimetry in many branches of astronomical research.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

High-efficiency 'superchromatic' polarimetry optics for use in optical astronomical spectrographs does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with High-efficiency 'superchromatic' polarimetry optics for use in optical astronomical spectrographs, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and High-efficiency 'superchromatic' polarimetry optics for use in optical astronomical spectrographs will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1541961

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.