The 1640.4 A H-alpha line of He II observed from SKYLAB

Details The 1640.4 A H-alpha line of He II observed from SKYLAB The 1640.4 A H-alpha line of He II observed from SKYLAB

Jul 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975apj...199l..67f&link_type=abstract

Astrophysical Journal, vol. 199, July 1, 1975, pt. 2, p. L67-L70. NASA-supported research.

Astronomy and Astrophysics

Astronomy

24

H Alpha Line, Helium Ions, Skylab Program, Solar Spectra, Luminous Intensity, Molecular Collisions, Radiative Recombination, Solar Corona, Spaceborne Astronomy, Spectroheliographs

Scientific paper

Profiles obtained from NRL Skylab solar spectra of the 1640.4 A feature identified as the H-alpha line of He II are discussed and compared with theoretical profiles derived assuming (1) collisional excitation and (2) radiative recombination as the dominant excitation mechanism. Relative intensities of this line as a function of altitude above and below the solar white-light limb are also given for a representative quiet sun region and for a polar coronal hole.

Affiliated with

Also associated with

No associations

Rating

The 1640.4 A H-alpha line of He II observed from SKYLAB 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 1640.4 A H-alpha line of He II observed from SKYLAB, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The 1640.4 A H-alpha line of He II observed from SKYLAB will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1755244