Results 41 to 50 of about 513 (133)

FLOWS OF MAGNETIC FIELD IN THE SUN’S PHOTOSPHERE

Proceedings of the 25th All-Russia Conference on Solar and Solar-Terrestrial Physics, 2021
E.S. Vernova, M.I. Tyasto, D.G. Baranov
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On the differences between plage and quiet sun in the solar photosphere

The Astrophysical Journal, 1992
Time sequences of interleaved observations of the continuum intensity, longitudinal magnetic field, vertical velocity in the midphotosphere, and the line-center intensity in Ni I 6768 A were obtained in an active-region plage and the surrounding relatively field-free area near disk center. Spacetime Fourier filtering techniques are used to separate the
Alan M. Title, Kenneth P. Topka, Theodore D. Tarbell, Wolfgang Schmidt, Christiaan Balke, Goran Scharmer   +5 more
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Dynamics of Large-Scale Solar Flows. [PDF]

Space Sci Rev, 2023
Hotta H, Bekki Y, Gizon L, Noraz Q, Rast M.   +4 more
europepmc   +1 more source

The Sun's Photosphere [PDF]

Nature, 1877
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Turbulent convection as a significant hidden provider of magnetic helicity in solar eruptions. [PDF]

Sci Rep, 2023
Toriumi S, Hotta H, Kusano K.
europepmc   +1 more source

Measuring the magnetic fields in the chromospheres of low-mass stars. [PDF]

Nat Commun
Cang T, Petit P, Donati JF, Tian H, Fu J, Li H, Bellotti S, Hu X, Ma X, Lopez Ariste A, Xing K, Morin J, Lu H, Zong W.   +13 more
europepmc   +2 more sources

Diagnostics of photospheric jets of the quiet Sun atmosphere [PDF]

Kinematika i fizika nebesnyh tel (Online), 2019
M.I. Stodilka, A.V. Sukhorukov, A.I. Prysiazhnyi   +2 more
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Vortex Motions in the Solar Atmosphere: Definitions, Theory, Observations, and Modelling. [PDF]

Space Sci Rev, 2023
Tziotziou K, Scullion E, Shelyag S, Steiner O, Khomenko E, Tsiropoula G, Canivete Cuissa JR, Wedemeyer S, Kontogiannis I, Yadav N, Kitiashvili IN, Skirvin SJ, Dakanalis I, Kosovichev AG, Fedun V.   +14 more
europepmc   +1 more source

Modeling Sun photosphere granulation as a boiling process

In this paper I try to extract typical Sun photosphere granule sizes and then map it to the boiling process in the liquids using Reynolds number definition. So that if granules would be formed as some sort of plasma bubbles formation and flow, what would be the requirements of such "boiling" process ?
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Motions in the Sun at the Photospheric Level VIII. Solar Rotation and Photospheric Circulation [PDF]

Monthly Notices of the Royal Astronomical Society, 1959
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