Variation of energy throughput with off-axis angle for the S056 X-ray telescope

Details Variation of energy throughput with off-axis angle for the S056 X-ray telescope Variation of energy throughput with off-axis angle for the S056 X-ray telescope

Apr 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977apopt..16..806f&link_type=abstract

Applied Optics, vol. 16, Apr. 1977, p. 806-808.

Astronomy and Astrophysics

Astronomy

Skylab Program, Solar Instruments, Spaceborne Telescopes, X Ray Telescopes, Fresnel Reflectors, Reflectance, Solar Observatories, Solar X-Rays, Spaceborne Astronomy, X Ray Spectra

Scientific paper

The S056 solar X-ray telescope, a paraboloidal-hyperboloidal Wolter type I instrument, was used in the Skylab solar observatory to photograph the sun in various soft X-ray wavelength bands. It is necessary to know how the energy throughput of the telescope varies as a function of off-axis angle at various wavelengths in order to compare the relative intensities of solar X-ray emission from various areas of the sun captured on the same photographic frame.

Affiliated with

Also associated with

No associations

Rating

Variation of energy throughput with off-axis angle for the S056 X-ray 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 Variation of energy throughput with off-axis angle for the S056 X-ray telescope, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Variation of energy throughput with off-axis angle for the S056 X-ray telescope will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1616829