Quiet sun observations of the AL I autoionization lines lambda 1932 and lambda 1936

Details Quiet sun observations of the AL I autoionization lines lambda 1932 and lambda 1936 Quiet sun observations of the AL I autoionization lines lambda 1932 and lambda 1936

Feb 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982soph...76..109c&link_type=abstract

Solar Physics, vol. 76, Feb. 1982, p. 109-116. Research supported by the Norges Almenvitenskapelige Forskningsrad;

Astronomy and Astrophysics

Astronomy

2

Aluminum, Autoionization, Solar Atmosphere, Solar Spectra, Spectral Line Width, Thermodynamic Equilibrium, Calcium, Magnesium, Metal Ions, Solar Limb, Ultraviolet Astronomy

Scientific paper

Quiet sun observations obtained during a rocket flight of the Al I autoionization lines 1932 A and 1936 A at solar pointings ranging from mu = 0.73 out to the visible limb. Absolute intensities are estimated to be accurate to about + or - 20%. These lines weaken progressively with decreasing mu but never go into emission before finally disappearing with the continuum just beyond the visible solar limb. The observations are then compared with LTE line profiles computed through the quiet sun atmosphere of Vernazza et al. (1976). Several areas of disagreement between the synthetic and observed profiles are discussed.

Affiliated with

Also associated with

No associations

Rating

Quiet sun observations of the AL I autoionization lines lambda 1932 and lambda 1936 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 Quiet sun observations of the AL I autoionization lines lambda 1932 and lambda 1936, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Quiet sun observations of the AL I autoionization lines lambda 1932 and lambda 1936 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1648577