Helium 10830 Å measurements of the Sun
Abstract
Measurements of the Sun in the near-infrared He I 10830 Å absorption line were performed using the echelle spectrograph with a dispersion of 6.71 mÅ per pixel at the Vacuum Tower Telescope (German Solar Telescopes, Teide Observatory, Izaña, Tenerife, Spain) on May 26, 1993. These measurements were compared with full-disc soft X-ray images of the Sun (Japanese solar satellite Yohkoh), full-disc solar images in Hα (Big Bear Solar Observatory), full-disc solar images in the He I 10830 Å line (National Solar Observatory, Kitt Peak) and with full-disc microwave solar maps at 37 GHz (Metsähovi Radio Research Station). In the He 10830 Å line the Sun displays a limb darkening similar to that in the visible part of the spectrum. Active regions and Hα filaments show a strong absorption in the He 10830 Å line, whereas the absorption is weak in coronal holes.
- Publication:
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Solar Physics
- Pub Date:
- January 1996
- DOI:
- Bibcode:
- 1996SoPh..163...79B
- Keywords:
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- Microwave;
- Absorption Line;
- Coronal Hole;
- Visible Part;
- Solar Observatory