Computer Science
Scientific paper
Nov 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992esasp.348..297m&link_type=abstract
In ESA, Proceedings of the First SOHO Workshop: Coronal Streamers, Coronal Loops, and Coronal and Solar Wind Composition p 297-3
Computer Science
2
Emission Spectra, Extreme Ultraviolet Radiation, Plasma Composition, Solar Corona, Solar Radiation, Abundance, Composition (Property), Line Spectra, Skylab Program, Soho Mission, Spectrum Analysis
Scientific paper
A study of the determination of element abundances in the quiet regions of the solar transition zone and corona is made. Early work with EUV spectral lines is reviewed together with subsequent analyses of Skylab observations. The intention of this study is to question some of the assumptions which have been made in these analyses and to look critically at the accuracy of past and present atomic data. The overall aim is to assess what further work is required to adapt these methods for use as diagnostic techniques with the SOHO (Solar and Heliospheric Observatory) instruments, in particular CDS (Coronal Diagnostic Spectrometer) and SUMER (Solar Ultraviolet Measurement of Emitted Radiation). Mention is also made of the importance of studying the coronal forbidden lines in the visible and infrared wavelength regions.
No associations
LandOfFree
Abundance determination in the quiet corona 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 Abundance determination in the quiet corona, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Abundance determination in the quiet corona will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1552353