Showing 1–20 of 41 results
/ Date/ Name
Feb 7, 2011The solar magnetic field since 1700: I. Characteristics of sunspot group emergence and reconstruction of the butterfly diagramSep 16, 2022Three-dimensional non-kinematic simulation of post-emergence evolution of bipolar magnetic regions and Babcock-Leighton dynamo of the SunMar 8, 2022Theory of solar oscillations in the inertial frequency range: Linear modes of the convection zoneApr 22, 2021A journey of exploration to the polar regions of a star: probing the solar poles and the heliosphere from high helio-latitudeAug 22, 2013Three-dimensional simulations of near-surface convection in main-sequence stars - I. Overall structureOct 18, 2024Low-latitude magnetic flux emergence on rapidly rotating solar-type starsDec 30, 2022Exploring the Solar Poles: The Last Great Frontier of the SunMar 25, 2013Helioseismology of sunspots: how sensitive are travel times to the Wilson depression and to the subsurface magnetic field?May 4, 2020The Sun is less active than other solar-like starsOct 28, 2020Vortex Flow Properties in Simulations of Solar Plage Region: Evidence for their role in chromospheric heatingSep 5, 2016Inflows towards active regions and the modulation of the solar cycle: a parameter studyMay 18, 2015Three-dimensional simulations of near-surface convection in main-sequence stars. III. The structure of small-scale magnetic flux concentrationsMay 18, 2015Three-dimensional simulations of near-surface convection in main-sequence stars. IV. Effect of small-scale magnetic flux concentrations on centre-to-limb variation and spectral linesJun 19, 2025Coriolis force acting on near-surface horizontal flows during simulations of flux emergence produces a tilt angle consistent with Joy's law on the SunMay 27, 2024The mean solar butterfly diagram and poloidal field generation rate at the surface of the SunNov 27, 2024Combined Surface Flux Transport and Helioseismic Far-side Active Region Model (FARM)Nov 8, 2024The rush to the poles and the role of magnetic buoyancy in the solar dynamoDec 26, 2025Simulations of facular magnetic fields on cool stars I: Main sequence stars with solar metallicityJun 10, 2020Average motion of emerging solar active region polarities II: Joy's lawMar 27, 2024The Sun's differential rotation is controlled by high-latitude baroclinically unstable inertial modes