research_highlights
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nocite=2015ApJ...805..133J | nocite=2015ApJ...805..133J | ||
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+ | In this paper we took our travel-time measurements from earlier work and tried to infer the deep, large-scale flows inside the Sun. To get some sense of our results using GONG ground-based data, we compared our results to those obtained from space-based data in {[2013ApJ...774L..29Z]}. | ||
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+ | We find some similarities between each group, notably a very unexpected shallow equatorward flow only 10% into the Sun. Such a feature had been expected to lie around 30% into the Sun. While the Stanford group finds some evidence of again a northward flow deeper down, our results do not indicate such a structure within the uncertainties. | ||
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+ | While the similarities are encouraging, | ||
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==== Deep Meridional Flow Measurements from GONG Data ==== | ==== Deep Meridional Flow Measurements from GONG Data ==== | ||
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+ | nocite=2014ApJ...784..145K | ||
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+ | This paper showed travel-time measurements of about 650 days of GONG data. Signatures of meridional flow in the deep convection zone are present, and preliminary evidence of a change of sign, indicating an equatorward flow for some large travel distances as seen in other recent work, is found. This is the first time this has been seen in GONG data. We only find reasonable results after correcting for center-to-limb systematics as in the {[2012ApJ...749L...5Z]} work, whereby we subtract off east-west measurements from the north-south ones (see figure on right). | ||
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+ | While that paper used space-based SDO/HMI observations, | ||
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+ | ==== References ==== | ||
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+ | <bibtex bibliography> | ||
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+ | </ | ||
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research_highlights.1721067916.txt.gz · Last modified: 2024/07/15 18:25 by jasonj