Astronomy and Astrophysics – Astronomy
Scientific paper
May 1976
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976rspta.281..359t&link_type=abstract
(Royal Society, Discussion on the Physics of the Solar Atmosphere, London, England, Jan. 14, 15, 1975.) Royal Society (London),
Astronomy and Astrophysics
Astronomy
Far Ultraviolet Radiation, Skylab Program, Solar Prominences, Solar Spectra, Spectroheliographs, Ultraviolet Spectra, Astronomical Spectroscopy, Hydrogen Ions, Solar Corona, Solar Limb, Spaceborne Astronomy, Stellar Mass Ejection
Scientific paper
Five major eruptions were observed to produce spectacular phenomena above the limb during Skylab. All are seen best in He II at 304 A. The event of January 17, 1974 was the only one that was observed in high transition and coronal lines. This eruption had at least five major parts; their forms were entirely different spatially, and they maximized at different temperatures. The observations began not less than 20 min after the main eruptive phase and extended for 1 h. The greatest detail was present in He II at 304 A; this included groups of long curved rays 2 arcsec in diameter at the instrumental resolution. Many parts of the He II feature changed intensity but not position. Therefore, it is difficult to distinguish mass motion from spatially changing excitation.
No associations
LandOfFree
Eruptive prominences recorded by the X u.v. spectroheliograph on 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 Eruptive prominences recorded by the X u.v. spectroheliograph on SKYLAB, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Eruptive prominences recorded by the X u.v. spectroheliograph on SKYLAB will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1797959