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Found 3 entries in the Bibliography.
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Solar wind rotation rate and shear at coronal hole boundaries. Possible consequences for magnetic field inversions
Context. In situ measurements by several spacecraft have revealed that the solar wind is frequently perturbed by transient structures that have been interpreted as magnetic folds, jets, waves, and flux ropes that propagate rapidly away from the Sun over a large range of heliocentric distances. Parker Solar Probe (PSP), in particular, has detected very frequent rotations of the magnetic field vector at small heliocentric radial distances, accompanied by surprisingly large solar wind rotation rates. The physical origin of such ...
Pinto, R.~F.; Poirier, N.; Rouillard, A.~P.; Kouloumvakos, A.; Griton, L.; Fargette, N.; Kieokaew, R.; Lavraud, B.; Brun, A.~S.;
Published by: \aap Published on: sep
YEAR: 2021   DOI: 10.1051/0004-6361/202040180
Sun: corona; Sun: rotation; Solar wind; Astrophysics - Solar and Stellar Astrophysics
The Steady Global Corona and Solar Wind: A Three-dimensional MHD Simulation with Turbulence Transport and Heating
Usmanov, Arcadi; Matthaeus, William; Goldstein, Melvyn; Chhiber, Rohit;
Published by: \apj Published on: 09/2018
YEAR: 2018   DOI: 10.3847/1538-4357/aad687
Parker Data Used; magnetohydrodynamics: MHD; methods: numerical; Solar wind; Sun: corona; Sun: rotation; turbulence
3D ELECTRON DENSITY DISTRIBUTIONS IN THE SOLAR CORONA DURING SOLAR MINIMA: ASSESSMENT FOR MORE REALISTIC SOLAR WIND MODELING
Knowledge of the electron density distribution in the solar corona put constraints on the magnetic field configurations for coronal modeling and on initial conditions for solar wind modeling. We work with polarized SOHO/LASCO-C2 images from the last two recent minima of solar activity (1996-1997 and 2008-2010), devoid of coronal mass ejections. The goals are to derive the 4D electron density distributions in the corona by applying a newly developed time-dependent tomographic reconstruction method and to compare the result ...
de Patoul, Judith; Foullon, Claire; Riley, Pete;
Published by: The Astrophysical Journal Published on: 11/2015
YEAR: 2015   DOI: 10.1088/0004-637X/814/1/68
Astrophysics - Solar and Stellar Astrophysics; parker solar probe; Solar Probe Plus; Solar wind; Sun: corona; Sun: evolution; Sun: fundamental parameters; Sun: rotation