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• W2043452962 abstract "The distribution of magnetic fluxes found in the solar magnetic carpet, the photospheric magnetic field of the quiet-Sun, is investigated. A total of 27 500 concentrations are studied with fluxes ranging between a few times 1017 and a few times 1020 Mx. A histogram of the fluxes shows that there are more small fluxes and more large fluxes than anticipated by an exponential distribution. However, there are significantly fewer large and small fluxes than a power-law distribution fitted to the middle of the range. Thus, the fluxes are not distributed in the form of either an exponential or a power-law distribution, as previously suggested. Instead, the Weibull distribution, which involves both a power law and an exponential, is found to provide both a statistically good fit to the data and a physically reasonable prediction for the total absolute flux density. The best-fitting Weibull distribution has a Kolmogorov–Smirnov D statistic of approximately 0.07 – well below the 5 per cent significance level and the Weibull distribution predicts the observed total absolute flux densities to within better than 92 per cent." @default.
• W2043452962 created "2016-06-24" @default.
• W2043452962 creator A5084851547 @default.
• W2043452962 date "2002-09-01" @default.
• W2043452962 modified "2023-09-24" @default.
• W2043452962 title "Nature of the magnetic carpet – I. Distribution of magnetic fluxes" @default.
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• W2043452962 doi "https://doi.org/10.1046/j.1365-8711.2002.05618.x" @default.
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