Zobrazeno 1 - 10
of 21 623
pro vyhledávání: '"Meridional circulation"'
We have carried out inversions of travel times as measured by Gizon et al. (2020) to infer the internal profile of the solar meridional circulation (MC). A linear inverse problem has been solved by the regularized least-squares method with a constrai
Externí odkaz:
http://arxiv.org/abs/2406.12077
Climate variability on centennial timescales has often been linked to internal variability of the Atlantic Meridional Overturning Circulation (AMOC). However, due to the scarceness of suitable paleoclimate proxies and long climate model simulations,
Externí odkaz:
http://arxiv.org/abs/2406.09919
Autor:
Luo, Hongyu1,2,3 (AUTHOR), Yu, Haipeng1,2 (AUTHOR) yuhp@lzb.ac.cn, Hu, Zeyong1,2 (AUTHOR), Zhou, Jie4 (AUTHOR), Zhang, Bofei1,2,3 (AUTHOR), Yang, Yaoxian5 (AUTHOR), Cheng, Shanling4 (AUTHOR), Gong, Yongqi4 (AUTHOR), Ren, Yu4 (AUTHOR)
Publikováno v:
Journal of Climate. Jul2024, Vol. 37 Issue 13, p3543-3561. 19p.
Autor:
Banik, Deepayan, Menou, Kristen
Time-dependent meridional circulation and differential rotation in radiative zones are central open issues in stellar evolution theory. We streamline this challenging problem using the downward control principle of atmospheric science, under a geostr
Externí odkaz:
http://arxiv.org/abs/2402.16988
Publikováno v:
AGU advances, 2023, Volume 4, Issue 6
Jupiter's atmosphere comprises several dynamical regimes: the equatorial eastward flows and surrounding retrograde jets; the midlatitudes, with the eddy-driven, alternating jet-streams and meridional circulation cells; and the jet-free turbulent pola
Externí odkaz:
http://arxiv.org/abs/2312.10651
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Akademický článek
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Autor:
Herczeg, Aleczander, Jackiewicz, Jason
Mapping the large-scale subsurface plasma flow profile within the Sun has been attempted using various methods for several decades. One such flow in particular is the meridional circulation, for which numerous studies have been published. However, su
Externí odkaz:
http://arxiv.org/abs/2308.11035
We study a Jupiter-mass planet formation for the first time in radiative magneto-hydrodynamics (MHD) simulations and compare it with pure hydrodynamical simulations, as well as to different isothermal configurations. We found that the meridional circ
Externí odkaz:
http://arxiv.org/abs/2305.07864
The most widely accepted model of the solar cycle is the flux transport dynamo model. This model evolved out of the traditional $\alpha \Omega$ dynamo model which was first developed at a time when the existence of the Sun's meridional circulation wa
Externí odkaz:
http://arxiv.org/abs/2302.09390