Physics
Scientific paper
Sep 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008espm...12.2.20v&link_type=abstract
"12th European Solar Physics Meeting, Freiburg, Germany, held September, 8-12, 2008. Online at http://espm.kis.uni-freiburg.de/,
Physics
Scientific paper
The hydrogen lines are the most prominent lines in solar prominence spectra. Observations with the SUMER spectrometer on board SoHO showed that there are weak emission lines in the blue wings of the Lyman series which affect their profiles. We identified them as D I and He II lines in the Lyman alpha profile and He II lines in the upper Lyman series wings. The He II lines are identified as Balmer lines of He II. We attempt to characterize these lines in the blue wings of the Lyman series and consequently to provide supplementary He II information for further He I-He II non-LTE modelling.
Ajabshirizadeh Ali
Ebadi H.
Vial Jean-Claude
No associations
LandOfFree
The HeII (and DI) Lines in the Lyman Series of Solar Prominences 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 HeII (and DI) Lines in the Lyman Series of Solar Prominences, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The HeII (and DI) Lines in the Lyman Series of Solar Prominences will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1795703