EUV Full-Sun Imaged Spectral Atlas Using the SOHO Coronal Diagnostic Spectrometer
Abstract
The Coronal Diagnostic Spectrometer (CDS) aboard the Solar and Heliospheric Observatory (SOHO) carries out a regular program of measuring the full-disk irradiance using the Normal Incidence Spectrograph (NIS). The full-disk solar spectrum is returned in the wavelength bands 308-379 Å and 513-633 Å, with a spectral resolution between 0.3 and 0.6 Å. A recent modification to the CDS on-board software allows simultaneous moderate resolution monochromatic images to be made of the stronger lines in these wavelength ranges. We report on observations made 23 April 1998, 21 May 1998, and 22 June 1998. A total of 69 monochromatic full-Sun images are extracted from the spectral line data. For the first time, spectrally resolved images of the full Sun in He ii 303.8 Å and Si xi 303.3 Å are presented and compared. Velocity maps of the Sun in singly ionized helium are presented. Correlations of intensity to velocity over a wide range of transition region and coronal temperatures are shown. Lines from He i to Fe xiv show statistical red shifts of 1-7 km s−1 between active regions and quiet Sun areas. Velocity maps of Mg ix and x are presented, showing strong upflow and downflow regions associated with active regions, but not correlated with the brightest emission. Changes in line width are also presented in He i, with discussion of similar features in other lines of comparable temperature. Corrections which need to be applied to CDS/NIS data to extract meaningful velocities and line widths are presented and discussed. The identifications of the lines in the CDS spectrum are examined. The spatial and spectral variation of the background component of the CDS spectrum is examined.
- Publication:
-
Solar Physics
- Pub Date:
- July 2000
- DOI:
- 10.1023/A:1005203001242
- Bibcode:
- 2000SoPh..195...45T
- Keywords:
-
- Line Width;
- Background Component;
- Monochromatic Image;
- Heliospheric Observatory;
- Coronal Temperature