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Solar activity is a process driven by many independent but interconnected phenomena. Although the 11-year cycle is the result of operation of the dynamo mechanism, the cause of longer secular variations is not clear. In search of such a…

太阳与恒星天体物理 · 物理学 2025-11-07 M. M. Katsova , V. N. Obridko , D. D. Sokoloff , N. V. Emelianov

Thermal tides can torque the atmosphere of hot Jupiters into asynchronous rotation, while these planets are usually assumed to be locked into spin-orbit synchronization with their host star. In this work, our goal is to characterize the…

地球与行星天体物理 · 物理学 2018-06-06 Pierre Auclair-Desrotour , Jérémy Leconte

We analyzed the sunspot-group daily data that were reported by Greenwich Photoheliogrphic Results (GPR) during the period 1874-1976 and Debrecen Photoheliographic Data (DPD) during the period 1977-2017. We determined the equatorial rotation…

太阳与恒星天体物理 · 物理学 2020-12-04 J. Javaraiah

Variations of the sunspot number are important indicators of the solar activity cycles. The sunspot formation is a result of a dynamo process inside the Sun, which is far from being understood. We use simple dynamical models of the dynamo…

天体物理学 · 物理学 2009-02-11 I. N. Kitiashvili , A. G. Kosovichev

We present an analysis of planetary moves, encoded in DE406 ephemerides. We show resonance cycles between most planets in Solar System, of differing quality. The most precise resonance - between Earth and Venus, which not only stabilizes…

综合物理 · 物理学 2014-02-27 P. A. Semi

In recent years solar oscillations have been studied in great detail, both observationally and theoretically; so, perhaps, the Sun currently is the best understood pulsating star. The observational studies include long, almost uninterrupted…

太阳与恒星天体物理 · 物理学 2010-02-01 A. G. Kosovichev

It has recently been claimed that there is significant coherence between the spectral peaks of the global temperature series over the last 160 years and those of the speed of the solar center of mass at periods of 10-10.5, 20-21, 30 and…

地球与行星天体物理 · 物理学 2014-04-24 Sverre Holm

Context. The relation between solar surface rotation and sunspot activity still remains open. Sunspot activity has dramatically reduced in solar cycle 24 and several solar activity indices and flux measurements experienced unprecedentedly…

太阳与恒星天体物理 · 物理学 2015-02-18 L. Zhang , K. Mursula , I. Usoskin

In this thesis, various studies are performed leading to better understanding of the 11-year solar cycle and its theoretical modeling with the flux transport dynamo model. Although this is primarily a theoretical thesis, there is a part…

太阳与恒星天体物理 · 物理学 2018-04-26 Gopal Hazra

Measurements of maximum magnetic flux, minimum intensity, and size are presented for 12 967 sunspot umbrae detected on the NASA/NSO spectromagnetograms between 1993 and 2004 to study umbral structure and strength during the solar cycle. The…

太阳与恒星天体物理 · 物理学 2011-04-07 T. A. Schad , M. J. Penn

Moons tidally interact with their host planets and stars. A close moon is quickly synchronised by the planet, or becomes captured in a higher spin-orbit resonance. However, the planet requires much more time to significantly alter its…

地球与行星天体物理 · 物理学 2025-09-15 Valeri V. Makarov , Michael Efroimsky

Star-planet interactions play, among other things, a crucial role in planetary orbital configurations by circularizing orbits, aligning the star and planet spin and synchronizing stellar rotation with orbital motions. This is especially…

Solar magnetic activity is expressed via variations of sunspots and active regions varying on different timescales. The most accepted is an 11-year period supposedly induced by the electromagnetic solar dynamo mechanism. There are also some…

太阳与恒星天体物理 · 物理学 2023-01-19 Valentina V. Zharkova , Irina Vasilieva , Simon Shepherd , Elena Popova

The latitudinal location of the sunspot zones in each hemisphere is determined by calculating the centroid position of sunspot areas for each solar rotation from May 1874 to June 2011. When these centroid positions are plotted and analyzed…

太阳与恒星天体物理 · 物理学 2015-05-30 D. H. Hathaway

Generation and diffusion of the magnetic field on the Sun is a key mechanism responsible for solar activity on all spatial and temporal scales - from the solar cycle down to the evolution of small-scale magnetic elements in the quiet Sun.…

太阳与恒星天体物理 · 物理学 2011-12-14 V. I. Abramenko , V. B. Yurchyshyn , P. R. Goode

While obviously having a common root, solar and planetary dynamo theory have taken increasingly divergent routes in the last two or three decades, and there are probably few experts now who can claim to be equally versed in both.…

太阳与恒星天体物理 · 物理学 2014-11-18 K. Petrovay

The sunspot activity is the end result of the cyclic destruction and regeneration of magnetic fields by the dynamo action. We propose a new method to analyze the daily sunspot areas data recorded since 1874. By computing the power spectral…

太阳与恒星天体物理 · 物理学 2015-05-20 Ilidio Lopes , Hugo G. Silva

Although sunspots have been systematically observed on the Sun's surface over the last four centuries, their magnetic properties have been revealed and documented only since the early 1900s. Sunspots typically appear in pairs of opposite…

太阳与恒星天体物理 · 物理学 2019-09-25 Soumitra Hazra , Dibyendu Nandy

The Solar Cycle is reviewed. The 11-year cycle of solar activity is characterized by the rise and fall in the numbers and surface area of sunspots. A number of other solar activity indicators also vary in association with the sunspots…

太阳与恒星天体物理 · 物理学 2015-10-01 David H. Hathaway

We applied the method of continuous wavelet-transform to high-quality time-frequency analysis to the sets of observations of relative sunspot numbers. Wavelet analysis of these data reveals the following pattern: at the same time there are…

太阳与恒星天体物理 · 物理学 2015-12-15 A. A. Borisov , E. A. Bruevich , V. V. Bruevich , I. K. Rozgacheva , E. V. Shimanovskaya
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