Stark effect at the SI I series limit

Details Stark effect at the SI I series limit Stark effect at the SI I series limit

Sep 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apj...240..702j&link_type=abstract

Astrophysical Journal, Part 1, vol. 240, Sept. 1, 1980, p. 702-708.

Other

6

Atomic Spectra, Silicon, Solar Spectra, Stark Effect, Sunspots, Energy Levels, Line Spectra, Magnetohydrodynamic Waves, Red Shift

Scientific paper

Small redshifts and weakenings of high n lines in members of the Si series observed over a sunspot are interpreted as due to the Stark effect. Other origins, including Doppler motions, appear to be excluded. The spectra were obtained with high spatial resolution using the NRL high-resolution telescope and spectrograph. The origin of the Stark effect is not yet certain. An interpretation in terms of a quasi-static quadratic effect would require rather high perturber densities. An alternative interpretation would be a motional Stark effect, arising perhaps through the presence of magnetohydrodynamic waves.

Affiliated with

Also associated with

No associations

Rating

Stark effect at the SI I series limit 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 Stark effect at the SI I series limit, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Stark effect at the SI I series limit will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-904333