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相关论文: Internal-cycle variation of solar differential rot…

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On the base of the solar magnetic field measurements obtained in Stanford in 1976--2003 the properties of the cyclic evolution of the large-scale magnetic field are investigated. Some regularities are found in longitudinal and latitudinal…

天体物理学 · 物理学 2007-05-23 R. N. Ikhsanov , V. G. Ivanov

The annual temperature cycle of the earth closely follows the annual cycle of solar flux. At temperate latitudes, both driving and response cycles are well described by a strong annual sinusoidal component and a non-vanishing semiannual…

大气与海洋物理 · 物理学 2020-11-13 Yunxiang Song , Kyle B. Lawlor , Thomas A. Witten

Rotation is a significant characteristic of the Sun and other stars, and it plays an important role in understanding their dynamo actions and magnetic activities. In this study, the rotation of the solar chromospheric activity is…

太阳与恒星天体物理 · 物理学 2020-10-22 Jing-Chen Xu , Peng-Xin Gao , Xiang-Jun Shi

The Sun's global inertial modes are very sensitive to the solar differential rotation and to properties of the deep solar convection zone which are currently poorly constrained. These properties include the superadiabatic temperature…

太阳与恒星天体物理 · 物理学 2024-12-25 Laurent Gizon , Yuto Bekki , Aaron C. Birch , Robert H. Cameron , Damien Fournier , Jordan Philidet , B. Lekshmi , Zhi-Chao Liang

We present the multifractal study of the intermittency of the magnetic field turbulence in the fast and slow solar wind beyond the ecliptic plane during two solar minima (1997-1998, 2007-2008) and solar maximum (1999-2001). More precisely,…

空间物理 · 物理学 2019-05-23 Anna Wawrzaszek , Marius Echim , Roberto Bruno

It is suggested that the solar variability is due to the perturbed nature of the solar core and this variability is provided by the variability of the solar neutrino flux from the solar neutrino detectors i.e., Homestake, Superkamiokande,…

天体物理学 · 物理学 2007-05-23 Probhas Raychaudhuri

A new model has been proposed for magnetic field determination at different distances from the Sun during different solar cycle phases. The model depends on the observed large-scale non-polar photospheric magnetic fields and that measured…

太阳与恒星天体物理 · 物理学 2018-08-08 Irina A. Bilenko

Variations of the weak magnetic fields of the photosphere with periods of the order of the solar magnetic cycle were investigated. Synoptic maps of the photospheric magnetic field produced by NSO Kitt Peak for the period from 1978 to 2016…

太阳与恒星天体物理 · 物理学 2023-07-18 E. S. Vernova , M. I. Tyasto , D. G. Baranov

Helioseismology shows that the regions occupied by convection and differential rotation inside the sun almost coincide. This supports the leading theoretical concept for the origin of differential rotation as a result of interaction between…

太阳与恒星天体物理 · 物理学 2011-10-12 L. L. Kitchatinov

Whereas a variation of the solar luminosity, L, will inevitably cause a similar change of the total solar irradiance, S, the opposite is not true. In fact, the bulk of the days to months variations of S can be explained entirely in terms of…

天体物理学 · 物理学 2007-05-23 Sabatino Sofia , Linghuai H. Li

Using data from the Global Oscillation Network Group (GONG) covering the period from 1995 to 1998, we study the change with solar activity in solar f-mode frequencies. The results are compared with similar changes detected from the…

天体物理学 · 物理学 2015-06-24 H. M. Antia , Sarbani Basu , J. Pintar , B. Pohl

We argue that a variety of solar data suggest that the activity-cycle timescale variability of the total irradiance, is produced by structural adjustments of the solar interior. Assuming these adjustments are induced by variations of…

天体物理学 · 物理学 2009-10-31 L. H. Li , S. Sofia

Recent precise observations of solar global parameters are used to calibrate an upgraded solar model which takes into account magnetic fields in the solar interior. Historical data about sunspot numbers (from 1500 to the present) and solar…

天体物理学 · 物理学 2015-06-24 Sabatino Sofia , Linghuai H. Li

It has recently been discovered that the time phases (time-varying delays) of the irregular periodicities observed in the Sunspot series, consisting of the approximate 27-day latitude-averaged plasma rotation and approximate 11-yr magnetic…

太阳与恒星天体物理 · 物理学 2026-02-24 William A. Gardner , Antonio Napolitano

While it has been relatively easy to determine solar-cycle related changes in solar dynamics, determining changes in structure in the deeper layers of the Sun has proved to be difficult. By using helioseismic data obtained over two solar…

太阳与恒星天体物理 · 物理学 2021-08-25 Sarbani Basu

The Sun shrinks during solar maximum and regrows during solar minimum by a few kilometers. Here, we observe, for the first time, that the solar radius variation shows planetary relationship. This suggests that some remote planetary links…

综合物理 · 物理学 2022-02-10 Konstantin Zioutas , Marios Maroudas , Alexander Kosovichev

The solar magnetic activity consists of two periodic components: the main cycle with a period of 11 yr and a shorter cycle with a period of ~2 yrs. The origin of this second periodicity is still not well understood. We use almost 15 yrs of…

太阳与恒星天体物理 · 物理学 2015-06-11 R. Simoniello , K. Jain , S. C. Tripathy , S. Turck-Chieze , W. Finsterle , M. Roth

Asteroseismology has undergone a profound transformation as a scientific field following the CoRoT and Kepler space missions. The latter is now yielding the first measurements of latitudinal differential rotation obtained directly from…

太阳与恒星天体物理 · 物理学 2019-03-27 M. Bazot , O. Benomar , J. Christensen-Dalsgaard , L. Gizon , S. Hanasoge , M. Nielsen , P. Petit , K. R. Sreenivasan

The Sun and solar-type stars exhibit irregular cyclic variations in their magnetic activity over long time scales. To understand this irregularity, we employed the flux transport dynamo models to investigate the behavior of one solar mass…

太阳与恒星天体物理 · 物理学 2024-12-25 Vindya Vashishth

Recent advances in helioseismology, numerical simulations and mean-field theory of solar differential rotation have shown that the meridional circulation pattern may consist of two or more cells in each hemisphere of the convection zone.…

太阳与恒星天体物理 · 物理学 2018-02-28 V. V. Pipin , A. G. Kosovichev