Monitoring the Solar Temperature: Empirical Calibration of the Temperature Sensitivity of C i lambda 5380

Details Monitoring the Solar Temperature: Empirical Calibration of the Temperature Sensitivity of C i lambda 5380 Monitoring the Solar Temperature: Empirical Calibration of the Temperature Sensitivity of C i lambda 5380

Jan 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997apj...474..798g&link_type=abstract

Astrophysical Journal v.474, p.798

Astronomy and Astrophysics

Astronomy

20

Techniques: Spectroscopic, Sun: Fundamental Parameters

Scientific paper

We observed a set of six dwarf stars spanning a range in temperatures around the solar value, and from them we have determined empirically the temperature sensitivity of C I lambda 5380.32, a line that has been monitored in the solar flux spectrum for nearly two decades at Kitt Peak. When the C I line is compared to the adjacent Fe I lambda 5379.58 line, it should be possible to detect apparent temperature differences of a fraction of 1 K.

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