Combined analysis of solar neutrino and solar irradiance data: further evidence for variability of the solar neutrino flux and its implications concerning the solar core

TL;DR

This study combines solar neutrino and irradiance data to find evidence of solar core variability and rotation, suggesting an inhomogeneous core with a possible inner dynamo and magnetic field.

Contribution

It provides new evidence linking neutrino flux variability to solar core rotation, indicating a potential inner tachocline and dynamo not previously established.

Findings

Evidence of 11.85 yr^-1 modulation in neutrino and irradiance data

Solar core likely inhomogeneous and rotating at 12.85 yr^-1

Possible existence of an inner tachocline and dynamo

Abstract

A search for any particular feature in any single solar neutrino dataset is unlikely to establish variability of the solar neutrino flux since the count rates are very low. It helps to combine datasets, and in this article we examine data from both the Homestake and GALLEX experiments. These show evidence of modulation with a frequency of 11.85 yr-1, which could be indicative of rotational modulation originating in the solar core. We find that precisely the same frequency is prominent in power spectrum analyses of the ACRIM irradiance data for both the Homestake and GALLEX time intervals. These results suggest that the solar core is inhomogeneous and rotates with sidereal frequency 12.85 yr-1. We find, by Monte Carlo calculations, that the probability that the neutrino data would by chance match the irradiance data in this way is only 2 parts in 10,000. This rotation rate is significantly lower than that of the inner radiative zone (13.97 yr-1) as recently inferred from analysis of Super-Kamiokande data, suggesting that there may be a second, inner tachocline separating the core from the radiative zone. This opens up the possibility that there may be an inner dynamo that could produce a strong internal magnetic field and a second solar cycle.