
TL;DR
This paper investigates the contributions of global and local solar dynamos to small-scale magnetic flux, concluding that the global dynamo dominates at most scales except possibly below 10 km, based on analysis of Hinode data.
Contribution
It provides evidence that the global dynamo is the primary source of small-scale magnetic flux, challenging the idea of a significant local dynamo contribution at observable scales.
Findings
Nearly all small-scale flux is supplied by the global dynamo.
Local dynamo contribution is only possible below about 10 km scales.
Hinode data was used to determine the Sun's basal magnetic flux density.
Abstract
It is often claimed that there is not only one, but two different types of solar dynamos: the one that is responsible for the appearance of sunspots and the 11-yr cycle, frequently referred to as the "global dynamo", and a statistically time-invariant dynamo, generally referred to as the "local dynamo", which is supposed to be responsible for the ubiquitous magnetic structuring observed at small scales. Here we examine the relative contributions of these two qualitatively different dynamos to the small-scale magnetic flux, with the following conclusion: The local dynamo does not play a significant role at any of the spatially resolved scales, nearly all the small-scale flux, including the flux revealed by Hinode, is supplied by the global dynamo. This conclusion is reached by careful determination of the Sun's noise-corrected basal magnetic flux density while making use of a flux…
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