@Article{Muņoz-JaramilloSWALTNPCCYWBDM:2015:MuSt,
author = "Muņoz-Jaramillo, Andr{\'e}s and Senkpeil, Ryan R. and
Windmueller, John C. and Amouzou, Ernest C. and Longcope, Dana W.
and Tlatov, Andrey G. and Nagovitsyn, Yury A. and Pevtsov, Alexei
A. and Chapman, Gary A. and Cookson, Angela M. and Yeates, Anthony
R. and Watson, Fraser T. and Balmaceda, Laura Antonia and DeLuca,
Edward E. and Martens, Petrus C. H.",
affiliation = "{Montana State University} and {Purdue University} and {Montana
State University} and {Montana State University} and {Montana
State University} and {Kislovodsk Mountain Astronomical Station of
the Pulkovo Observatory} and {Pulkovo Astronomical Observatory}
and {National Solar Observatory} and {California State University
Northridge} and {California State University Northridge} and
{Durham University} and {National Solar Observatory} and
{Instituto Nacional de Pesquisas Espaciais (INPE)} and
{Harvard-Smithsonian Center for Astrophysics} and {Georgia State
University}",
title = "Small-scale and global dynamos and the area and flux distributions
of active regions, sunspot groups, and sunspots: a multi-database
study",
journal = "The Astrophysical Journal",
year = "2015",
volume = "800",
number = "1",
keywords = "Sun: activity, Sun: magnetic fields, Sun: photosphere, sunspots.",
abstract = "In this work, we take advantage of 11 different sunspot group,
sunspot, and active region databases to characterize the area and
flux distributions of photospheric magnetic structures. We find
that, when taken separately, different databases are better fitted
by different distributions (as has been reported previously in the
literature). However, we find that all our databases can be
reconciled by the simple application of a proportionality
constant, and that, in reality, different databases are sampling
different parts of a composite distribution. This composite
distribution is made up by linear combination of Weibull and
log-normal distributionswhere a pure Weibull (log-normal)
characterizes the distribution of structures with fluxes below
(above) 1021Mx (1022Mx). Additionally, we demonstrate that the
Weibull distribution shows the expected linear behavior of a
power-law distribution (when extended to smaller fluxes), making
our results compatible with the results of Parnell et al. We
propose that this is evidence of two separate mechanisms giving
rise to visible structures on the photosphere: one directly
connected to the global component of the dynamo (and the
generation of bipolar active regions), and the other with the
small-scale component of the dynamo (and the fragmentation of
magnetic structures due to their interaction with turbulent
convection).",
doi = "10.1088/0004-637X/800/1/48",
url = "http://dx.doi.org/10.1088/0004-637X/800/1/48",
issn = "0004-637X",
language = "en",
targetfile = "Munoz_small.pdf",
urlaccessdate = "27 abr. 2024"
}