Computer Science
Scientific paper
Nov 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992esasp.348...17h&link_type=abstract
In ESA, Proceedings of the First SOHO Workshop: Coronal Streamers, Coronal Loops, and Coronal and Solar Wind Composition p 17-19
Computer Science
5
Extreme Ultraviolet Radiation, Line Spectra, Soho Mission, Solar Atmosphere, Solar Corona, Spectral Emission, Ultraviolet Spectrometers, European Space Programs, Nasa Space Programs, Plasma Acceleration, Plasma Diagnostics, Remote Sensing, Satellite-Borne Instruments, Solar Wind
Scientific paper
The Coronal Diagnostic Spectrometer (CDS) is designed to probe the solar atmosphere through the analysis of spectral emission lines in the extreme ultraviolet wavelength range 150 to 800 A. By observing the absolute and relative intensities of selected lines and line profiles, the temperature, density, flow, and abundance information for the plasmas in the solar atmosphere are derived. Simultaneous coverage of large wavelength bands combined with spatial and temporal resolutions of a few arc seconds and down to 1 second will provide a unique tool for pursuing the goals of SOHO (Solar and Heliospheric Observatory).
Harrison Richard A.
Sawyer Eric C.
No associations
LandOfFree
The coronal diagnostic spectrometer for the Solar and Heliospheric Observatory 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 coronal diagnostic spectrometer for the Solar and Heliospheric Observatory, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The coronal diagnostic spectrometer for the Solar and Heliospheric Observatory will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1552140