|Author||Stalin, C. S. ♦ Trivedi, C. ♦ Sinha, K. ♦ Sanwal, B. B.|
|Source||Aryabhatta Research Institute of Observational Sciences (ARIES)|
|Subject Domain (in DDC)||Natural sciences & mathematics ♦ Physics|
|Subject Keyword||Sun ♦ Atmosphere – sun ♦ Abundances – atomic data|
|Abstract||Solar IR spectra have been utilized to derive log gf value for atomic lines due to 17 chemical elements. From a recent publication in Astronomy and Astrophysics Supplement, we selected unblended solar lines in the infrared J and H bands, in the wavelength ranges 1.00 – 1.34 µm and 1.49 – 1.80 µm respectively. The observed central line depths were based on FTS atlas published at Liege and Kitt Peak National Observatory. The observed central line depths were fitted with the corresponding quantities in the calculated spectrum obtained using computer codes and a reliable solar model atmosphere. This provide us with a set of relative log gf values which we present here. Significant differences are noticed between the derived log gf values and those available in literature.|
|Part of series||basi25-353|
|Education Level||UG and PG|
|Learning Resource Type||Article|
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