The MarkI helioseismic experiment.I. Measurements of the solar gravitational redshift (1976-2013)
Teodoro Roca Cort\'es, Pere L. Pall\'e

TL;DR
This paper reports 38 years of high-precision measurements of the solar gravitational redshift using the Mark-I helioseismic instrument, revealing variations correlated with solar activity and a slight discrepancy with theoretical predictions.
Contribution
It provides the longest continuous dataset of solar gravitational redshift measurements, demonstrating instrumental stability and revealing solar cycle-related variations.
Findings
Measured solar gravitational redshift of 600.4 ± 0.8 m/s
Detected amplitude variation of ±5 m/s correlated with solar activity
Found a 5% discrepancy with theoretical predictions, likely due to spectral line asymmetry
Abstract
The resonant scattering solar spectrophotometer 'Mark-I', designed and build at the University of Birmingham (UK) and located at the Observatorio del Teide (Spain), has been continuously in operation for the past 38 years. During this period of time, it has provided high precision measurements of the radial velocity of the Sun as a star, which has enabled the study of the small velocity fluctuations produced by the solar oscillations and the characterization of their spectrum. So far, it has been one of the pioneer experiments in the field of helioseismology and contributed to the development of that area. Moreover, because of its high sensitivity and long term instrumental stability, it also provides an accurate determination (to within a few parts in ) of the absolute daily velocity offset, which contains the so-called 'solar gravitational red-shift'. In the present paper,…
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