IOP Publishing, Journal of Physics: Conference Series, (271), p. 012015, 2011
DOI: 10.1088/1742-6596/271/1/012015
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We examine the differences between ring-diagram mode frequency estimates from samples of Global Oscillation Network Group [GONG], Michelson Doppler Imager [MDI] and Helioseismic and Magnetic Imager [HMI] data, and find that different instruments and analysis pipelines do result in small systematic differences which may not be uniform across the solar disk.