Development of multilayer mirrors for the XUV Doppler telescope

Details Development of multilayer mirrors for the XUV Doppler telescope Development of multilayer mirrors for the XUV Doppler telescope

Jul 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997spie.3113..193n&link_type=abstract

Proc. SPIE Vol. 3113, p. 193-201, Grazing Incidence and Multilayer X-Ray Optical Systems, Richard B. Hoover; Arthur B. Walker; E

Physics

2

Scientific paper

We present the development status of the normal incidence XUV multilayer mirrors for XUV Doppler telescope, which observes coronal velocity fields of the whole sun. The telescope has two narrow band-pass multilayer mirrors tuned to slightly longer and shorter wavelengths around the Fe XIV line at 211.3 Angstrom. From the intensity difference of the images taken with these two bands, we can obtain Dopplergram of 1.8 MK plasma of the whole sun. It is required that the multilayer has high wavelength-resolution ((lambda) /(Delta) (lambda) approximately 30 per mirror), anti-reflection coating for intense He II 304 angstrom emission line and high d-spacing uniformity of approximately 1%.

Affiliated with

Also associated with

No associations

Rating

Development of multilayer mirrors for the XUV Doppler telescope 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 Development of multilayer mirrors for the XUV Doppler telescope, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Development of multilayer mirrors for the XUV Doppler telescope will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1417188