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相关论文: Phase lags of solar hemispheric cycles

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The solar northern and southern hemispheres exhibit differences between the intensities and time profiles of the activity cycles. The time variation of these properties has been studied in a previous article on the data of Cycles 12-23. The…

太阳与恒星天体物理 · 物理学 2016-07-29 Judit Muraközy

A long-term variation is detected in the north-south differences of the solar activity, the phase difference of hemispheric cycles alternates by four Schwabe cycles. This variability is demonstrated by two different methods. It can be the…

太阳与恒星天体物理 · 物理学 2014-01-10 J. Muraközy , A. Ludmány

Research results from solar-dynamo models show the northern and southern hemispheres may evolve separately throughout the solar cycle. The observed phase lag between the hemispheres provides information regarding the strength of hemispheric…

太阳与恒星天体物理 · 物理学 2015-05-18 A. A. Norton , J. C. Gallagher

Numerical simulations that reproduce solar-like magnetic cycles can be used to generate long-term statistics. The variations in N-S hemispheric cycle synchronicity and amplitude produced in simulations has not been widely compared to…

太阳与恒星天体物理 · 物理学 2014-11-27 Aimee A. Norton , Paul Charbonneau , Dario Passos

We investigate the phase difference of the sunspot cycles in the two hemispheres and compare it with the latitudinal sunspot distribution. If the north-south phase difference exhibits a long-term tendency, it should not be regarded as a…

太阳与恒星天体物理 · 物理学 2015-05-20 N. V. Zolotova , D. I. Ponyavin , R. Arlt , I. Tuominen

Observations of the sun suggest that solar activities systematically create north-south hemispheric asymmetries. For instance, the hemisphere in which the sunspot activity is more active tends to switch after the early half of each solar…

太阳与恒星天体物理 · 物理学 2017-04-12 D. Syukuya , K. Kusano

The solar cycle onset at mid-latitudes, the slow down of the sunspot drift toward the equator, the tail-like attachment and the overlap of successive cycles at the time of activity minimum are delicate issues in $\alpha\Omega$ dynamo wave…

太阳与恒星天体物理 · 物理学 2016-09-07 R. Simoniello , S. C. Tripathy , K. Jain , F. Hill

North-south (N-S) asymmetry of solar activity is a known statistical phenomenon but its significance is difficult to prove or theoretically explain. Here we consider each solar hemisphere as a separate dynamical system connected with the…

太阳与恒星天体物理 · 物理学 2017-04-06 D. M. Volobuev , N. G. Makarenko

The appearance of dark sunspots over the solar photosphere is not considered to be symmetric between the northern and southern hemispheres. Among the different conclusions obtained by several authors, we can point out that the North-South…

太阳与恒星天体物理 · 物理学 2023-07-19 Leonardo F. G. Batista , Thiago M. Santiago , Paulo C. F. da Silva Filho , Cleo V. Silva , Daniel B. de Freitas

The peculiar behaviour of the solar cycle 23 and its prolonged minima has been one of the most studied problems over the last few years. In the present paper, we study the asymmetries in active region magnetic flux in the northern and…

太阳与恒星天体物理 · 物理学 2015-02-03 Juie Shetye , Durgesh Tripathi , Mausumi Dikpati

We study the asymmetric distribution of weak photospheric magnetic field values in the two hemispheres separately using synoptic maps from SDO/HMI, SOLIS/VSM and WSO during solar cycles 21-24. We calculate the weak-field asymmetry (shift)…

太阳与恒星天体物理 · 物理学 2019-10-09 Tibebu Getachew , Ilpo Virtanen , Kalevi Mursula

Solar and heliospheric parameters can depict notable differences between the northern and southern hemisphere. Although hemispheric asymmetries of some heliospheric parameters vary systematically with Hale cycle, this is not common for…

太阳与恒星天体物理 · 物理学 2023-06-21 Kalevi Mursula

The daily sunspot numbers of the whole disk as well as the northern and southern hemispheres from January 1, 1945 to December 31, 2010 are used to investigate the temporal variation of the rotational cycle length through the continuous…

太阳与恒星天体物理 · 物理学 2015-06-03 J. -L. Xie , X. -J. Shi , J. -C. Xu

The evolution of the solar activity comprises, apart from the well-known 11-year cycle, various temporal scales ranging from months up to the secondary cycles known as mid-term oscillations. Its nature deserves a physical explanation. In…

太阳与恒星天体物理 · 物理学 2020-08-04 D. D. Sokoloff , A. S. Shibalova , V. N. Obridko , V. V. Pipin

We create a continuous series of daily and monthly hemispheric sunspot numbers (HSNs) from 1874 to 2020, which will be continuously expanded in the future with the HSNs provided by SILSO. Based on the available daily measurements of…

太阳与恒星天体物理 · 物理学 2023-01-06 Astrid M. Veronig , Shantanu Jain , Tatiana Podladchikova , Werner Poetzi , Frederic Clette

Hemispheric irregularities of solar magnetic activity is a well-observed phenomenon -- the origin of which has been studied through numerical simulations and data-analysis techniques. In this work we explore possible causes generating…

太阳与恒星天体物理 · 物理学 2019-12-18 Prantika Bhowmik

We investigate spatio-temporal evolution of high-degree acoustic mode frequencies of the Sun and the surface magnetic activity, over the course of multiple solar cycles, to improve our understanding of the connection between the solar…

太阳与恒星天体物理 · 物理学 2023-12-20 Mackenzie A. Baird , Sushanta C. Tripathy , Kiran Jain

The data of sunspot numbers, sunspot areas and solar flare index during cycle 23 are analyzed to investigate the intermediate-term periodicities. Power spectral analysis has been performed separately for the data of the whole disk, northern…

太阳与恒星天体物理 · 物理学 2009-11-16 Bhuwan Joshi , P. Pant , P. K. Manoharan

In this paper, we have made a statistical analysis of solar H$\alpha$ flares that occurred during the period 1996 to 2005 to investigate their spatial distribution with respect to northern and southern hemispheres of the Sun. The analysis…

天体物理学 · 物理学 2007-08-16 Bhuwan Joshi , P. Pant , P. K. Manoharan , Kavita Pandey

It is well accepted that the solar cycle originates from a magnetohydrodynamics dynamo deep inside the Sun. Many dynamo models have long been proposed based on a lot of observational constraints. In this paper, using 342 NSO/Kitt Peak solar…

天体物理学 · 物理学 2009-06-23 W. B. Song
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