Solar EUV emission line profiles of SI II and SI III and their center to limb variations

Astronomy and Astrophysics – Astronomy

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

33

Apollo Telescope Mount, Far Ultraviolet Radiation, Line Shape, Silicon, Solar Limb, Solar Spectra, Atomic Spectra, Chromosphere, Optical Thickness, Plasma Spectra, Skylab Program, Spaceborne Astronomy, Spectral Line Width, Spectroheliographs

Scientific paper

Spectral-line profiles of Si II and Si III are presented which were observed both at solar center and near the quiet solar limb with the EUV spectrograph of ATM/Skylab. Absolute intensities and line profiles are derived from the photographic data. A brief discussion is given of their center-to-limb variations and of the optical thickness of the chromosphere in these lines. Nonthermal broadening velocities are found for the optically thin lines from their full width at half-maximum intensity (FWHM).

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

Solar EUV emission line profiles of SI II and SI III and their center to limb variations 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 Solar EUV emission line profiles of SI II and SI III and their center to limb variations, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Solar EUV emission line profiles of SI II and SI III and their center to limb variations will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1420036

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