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19912026
most citedPlanck 2015 results. XIII. Cosmological parameters

10.6k citations

Showing 2015 · astro-ph.SRShow all

13 papers · 2 filters

astro-ph.SR2015★ 3 cited

A new model for heating of Solar North Polar Coronal Hole

E. Devlen, D. Zengin Çamurdan, M. Yardımcı +1

This paper presents a new model of North Polar Coronal Hole (NPCH) to study dissipation/propagation of MHD waves. We investigate the effects of the isotropic viscosity and heat con…

astro-ph.SR2015★ 20 cited

The dynamics of Wolf numbers based on nonlinear dynamo with magnetic helicity: comparisons with observations

Ya. Kleeorin, N. Safiullin, N. Kleeorin +3

We investigate the dynamics of solar activity using a nonlinear one-dimensional dynamo model and a phenomenological equation for the evolution of Wolf numbers. This system of equat…

astro-ph.SR2015★ 21 cited

The detailed chemical composition of the terrestrial planet host Kepler-10

F. Liu, D. Yong, M. Asplund +7

Chemical abundance studies of the Sun and solar twins have demonstrated that the solar composition of refractory elements is depleted when compared to volatile elements, which coul…

astro-ph.SR2015★ 30 cited

Magnetic flux concentrations from turbulent stratified convection

P. J. Käpylä, A. Brandenburg, N. Kleeorin +2

(abridged) Context: The mechanisms that cause the formation of sunspots are still unclear. Aims: We study the self-organisation of initially uniform sub-equipartition magnetic fiel…

astro-ph.SR2015★ 98 cited

Multiple dynamo modes as a mechanism for long-term solar activity variations

Maarit J. Käpylä, Petri J. Käpylä, Nigul Olspert +4

Solar magnetic activity shows both smooth secular changes, such as the Grand Modern Maximum, and quite abrupt drops that are denoted as Grand Minima. Direct numerical simulations (…

astro-ph.SR2015★ 300 cited

Gaia FGK Benchmark Stars: Effective temperatures and surface gravities

U. Heiter, P. Jofré, B. Gustafsson +3

Large Galactic stellar surveys and new generations of stellar atmosphere models and spectral line formation computations need to be subjected to careful calibration and validation…