IS THE SPECTRAL TYPE OF THE SUN CONSTANT?
The spectral type of the whole Sun was monitored from 1988 August 25 through 1990 October 2. No changes as large as half a spectral subdivision were detected. The spectral type remained at G2V.
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Veröffentlicht in: | Publications of the Astronomical Society of the Pacific 1991-07, Vol.103 (665), p.642-644 |
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Format: | Artikel |
Sprache: | eng |
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Online-Zugang: | Volltext |
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Zusammenfassung: | The spectral type of the whole Sun was monitored from 1988 August 25 through 1990 October 2. No changes as large as half a spectral subdivision were detected. The spectral type remained at G2V. |
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ISSN: | 0004-6280 1538-3873 |
DOI: | 10.1086/132864 |