Polarimetry of extreme ultraviolet lines in solar astronomy

Details Polarimetry of extreme ultraviolet lines in solar astronomy Polarimetry of extreme ultraviolet lines in solar astronomy

Aug 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991opten..30.1161f&link_type=abstract

Optical Engineering (ISSN 0091-3286), vol. 30, Aug. 1991, p. 1161-1168.

Physics

6

Extreme Ultraviolet Radiation, Far Ultraviolet Radiation, Line Spectra, Polarimetry, Solar Atmosphere, Solar Corona, Layers, Linear Polarization, Lyman Alpha Radiation, Mirrors, Thin Films

Scientific paper

Ways are suggested in which recent advancements in the fabrication of ultrasmooth, low scatter flow-polished mirror substrates and high-quality multilayer and interference film coatings can be used to create novel optical instruments for observing linear-polarization effects in the outer solar atmosphere. Attention is given to the observational parameters of all-reflective FUV/EUV imaging polarimeters; such a coronagraph/polarimeter, operating at Ly-alpha, could yield the first measurements of coronal vector magnetic fields.

Affiliated with

Also associated with

No associations

Rating

Polarimetry of extreme ultraviolet lines in solar astronomy 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 Polarimetry of extreme ultraviolet lines in solar astronomy, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Polarimetry of extreme ultraviolet lines in solar astronomy will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1306621