A UV spectral Atlas of a prominence

Details A UV spectral Atlas of a prominence A UV spectral Atlas of a prominence

Aug 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ap%26ss.170..179e&link_type=abstract

(IAU, European Regional Astronomy Meeting, 11th, La Laguna, Spain, July 3-8, 1989) Astrophysics and Space Science (ISSN 0004-640

Astronomy and Astrophysics

Astronomy

Solar Prominences, Solar Spectra, Spaceborne Astronomy, Ultraviolet Spectra, Chromosphere, Emission Spectra, Solar Activity, Spacelab Payloads, Spectral Resolution

Scientific paper

The ultraviolet spectrum of a large prominence has been observed with the High Resolution Telescope and Spectrograph on Spacelab. The spectrum covers the wavelength range 1335-1670 A and shows numerous emission lines from gas at chromospheric and transition region temperatures. An Atlas of the prominence spectrum has been made showing absolute calibrated intensities on an accurate wavelength scale. The Atlas includes for comparison the corresponding UV-spectrum from an average quiet solar region.

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