The spectrum of Fe XVII in the solar corona

Details The spectrum of Fe XVII in the solar corona The spectrum of Fe XVII in the solar corona

Jun 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976mnras.175..489h&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 175, June 1976, p. 489-499.

Astronomy and Astrophysics

Astronomy

42

Iron, Metal Ions, Rocket-Borne Instruments, Solar Corona, Solar X-Rays, X Ray Spectra, Astronomical Spectroscopy, Bragg Angle, Electron Transitions, Line Spectra, Skylark Rocket Vehicle

Scientific paper

The wavelengths and intensities of n = 3-2 and n = 4-2 transitions in Fe XVII are reduced from meaurements of the X-ray spectra of three coronal active regions. The observations were made using Bragg X-ray spectrometers operated on two Skylark rocket vehicles. New wavelength measurements are given with an uncertainty of + or - 0.003 A. Relative intensities are compared with calculated values. Agreement is generally good, except for some of the 2p(6)-2p(5)3s lines. A feature near 11.0 A in the measured spectra is tentatively identified with a blend of two previously unknown inner-shell transitions.

Affiliated with

Also associated with

No associations

Rating

The spectrum of Fe XVII in the solar corona 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 The spectrum of Fe XVII in the solar corona, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The spectrum of Fe XVII in the solar corona will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1784655