Results 21 to 30 of about 95,397 (283)

MODELING OF DIFFERENTIAL ROTATION IN RAPIDLY ROTATING SOLAR-TYPE STARS [PDF]

open access: yesThe Astrophysical Journal, 2011
36 pages, 10 figures, accepted to ...
Hotta, Hideyuki, Yokoyama, Takaaki
openaire   +2 more sources

Influence of projection effects on the observed differential rotation rate in the UV corona

open access: yesJournal of Advanced Research, 2013
Following previous investigations by Giordano and Mancuso [1] and Mancuso and Giordano [2,3] on the differential rotation of the solar corona as obtained through the analysis of the intensity time series of the O VI 1032 Å spectral line observed by the ...
Salvatore Mancuso, Silvio Giordano
doaj   +1 more source

Solar cycle-related variation in solar differential rotation and meridional flow in solar cycle 24

open access: yesEarth, Planets and Space, 2020
We studied temporal variation of the differential rotation and poleward meridional circulation during solar cycle 24 using the magnetic element feature tracking technique.
Shinsuke Imada   +3 more
doaj   +1 more source

Exploring the Temporal Variation of the Solar Quadrupole Moment J 2

open access: yesThe Astrophysical Journal, 2023
Recently, Rozelot & Eren pointed out that the first solar gravitational moment ( J _2 ) might exhibit a temporal variation. The suggested explanation is through the temporal variation of the solar rotation with latitude.
Saliha Eren, Jean-Pierre Rozelot
doaj   +1 more source

Solar Oblateness and Differentially Rotating Polytropes [PDF]

open access: yesInternational Astronomical Union Colloquium, 1970
Dicke and Goldenberg (1967a) measured the solar oblateness to be σ= (5±0.7) × 10-5 and subsequently interpreted this measurement as evidence that the solar interior rotates with a period of 1.d8. With this interpretation, they then showed that the observed oblateness causes an 8% discrepancy in the Einstein prediction of the perihelion advance of ...
G. G. Fahlman   +2 more
openaire   +1 more source

Time-series Doppler images and surface differential rotation of the effectively-single rapidly-rotating K-giant KU Pegasi [PDF]

open access: yes, 2016
According to most stellar dynamo theories, differential rotation (DR) plays a crucial role for the generation of toroidal magnetic fields. Numerical models predict surface differential rotation to be anti-solar for rapidly-rotating giant stars, i.e ...
Carroll, T. A.   +8 more
core   +2 more sources

Periodic Change of Solar Differential Rotation [PDF]

open access: yesThe Astrophysical Journal, 2005
The periodic oscillation of the inhomogeneous rotation of the Sun is studied by use of the MHD dynamo theory. There exists a turbulent electromotive force that is driven by the vorticity of the flow (i.e., the γ dynamo). In addition, its counterpart exists in the vorticity equation, that is, the rotation is induced by an inhomogeneous magnetic field in
S.‐I. Itoh   +3 more
openaire   +1 more source

Rotating Turbulent Thermal Convection and Solar Differential Rotation

open access: yes, 2022
The expansion of the rotating fluid will change the vorticity and rotational speed of the expanding region. In turbulent thermal convection, this microscopic effect is preserved. Tracking the fluid micelles shows that the average vorticity varies with density, producing vorticity transport and angular momentum transport from the low-density area to the
Chen, Haibin, Wu, Rong
openaire   +2 more sources

Radial differential rotation of solar corona using radio emissions [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society: Letters, 2021
ABSTRACT The present work is an effort to investigate possible radial variations in the solar coronal rotation by analysing the solar radio emission data at 15 different frequencies (275–1755 MHz) for the period starting from 1994 July to 1999 May.
Singh, Vivek Kumar   +4 more
openaire   +2 more sources

2D dynamics of the radiative core of low mass stars

open access: yesEPJ Web of Conferences, 2017
Understanding the internal rotation of low mass stars all along their evolution is of primary interest when studying their rotational dynamics, internal mixing and magnetic field generation.
Hypolite Delphine   +2 more
doaj   +1 more source

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