The Coronal Diagnostic Spectrometer for the Solar and Heliospheric Observatory

Details The Coronal Diagnostic Spectrometer for the Solar and Heliospheric Observatory The Coronal Diagnostic Spectrometer for the Solar and Heliospheric Observatory

Dec 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995soph..162..233h&link_type=abstract

Solar Physics, Volume 162, Issue 1-2, pp. 233-290

Physics

474

Solar Atmosphere, Extreme Uv Spectroscopy

Scientific paper

The Coronal Diagnostic Spectrometer is designed to probe the solar atmosphere through the detection of spectral emission lines in the extreme ultraviolet wavelength range 150 800 Å. By observing the intensities of selected lines and line profiles, we may derive temperature, density, flow and abundance information for the plasmas in the solar atmosphere. Spatial and temporal resolutions of down to a few arcseconds and seconds, respectively, allow such studies to be made within the fine-scale structure of the solar corona. Futhermore, coverage of large wavelength bands provides the capability for simultaneously observing the properties of plasmas across the wide temperature ranges of the solar atmosphere.

Affiliated with

Also associated with

No associations

Rating

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.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1564785