Starspots

KG Strassmeier - The Astronomy and Astrophysics Review, 2009 - Springer
Starspots are created by local magnetic fields on the surfaces of stars, just as sunspots.
Their fields are strong enough to suppress the overturning convective motion and thus block …

Magnetic structure of sunspots

JM Borrero, K Ichimoto - Living Reviews in Solar Physics, 2011 - Springer
In this review we give an overview about the current state-of-knowledge of the magnetic field
in sunspots from an observational point of view. We start by offering a brief description of …

Universal computation by multiparticle quantum walk

AM Childs, D Gosset, Z Webb - Science, 2013 - science.org
A quantum walk is a time-homogeneous quantum-mechanical process on a graph defined
by analogy to classical random walk. The quantum walker is a particle that moves from a …

[图书][B] Stellar magnetism

L Mestel - 2012 - books.google.com
Ongoing studies in mathematical depth, and inferences fromhelioseismological'observations
of the internal solar rotation have shown up the limitations in our knowledge of the solar …

Magnetic activity of F stars observed by Kepler

S Mathur, RA García, J Ballot, T Ceillier… - Astronomy & …, 2014 - aanda.org
Context. The study of stellar activity is important because it can provide new constraints for
dynamo models when combined with surface rotation rates and the depth of the convection …

Electric currents in flare ribbons: observations and three-dimensional standard model

M Janvier, G Aulanier, V Bommier… - The Astrophysical …, 2014 - iopscience.iop.org
We present for the first time the evolution of the photospheric electric currents during an
eruptive X-class flare, accurately predicted by the standard three-dimensional (3D) flare …

The Sun's supergranulation

M Rieutord, F Rincon - Living Reviews in Solar Physics, 2010 - Springer
The Sun's supergranulation refers to a physical pattern covering the surface of the quiet Sun
with a typical horizontal scale of approximately 30,000 km and a lifetime of around 1.8 d. Its …

Local helioseismology: three-dimensional imaging of the solar interior

L Gizon, AC Birch, HC Spruit - Annual Review of Astronomy and …, 2010 - annualreviews.org
The Sun supports a rich spectrum of internal waves that are continuously excited by
turbulent convection. The Global Oscillation Network Group (GONG) network and the …

Numerical sunspot models: robustness of photospheric velocity and magnetic field structure

M Rempel - The Astrophysical Journal, 2012 - iopscience.iop.org
ABSTRACT MHD simulations of sunspots have successfully reproduced many aspects of
sunspot fine structure as a consequence of magneto-convection in inclined magnetic field …

Achievements of Hinode in the first eleven years

Hinode Review Team, K Al-Janabi… - Publications of the …, 2019 - academic.oup.com
Hinode is Japan's third solar mission following Hinotori (1981–1982) and Yohkoh (1991–
2001): it was launched on 2006 September 22 and is in operation currently. Hinode carries …