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相关论文: Multi-timescale Solar Cycles and the Possible Impl…

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The sunspot record since 1749 is made of three major cycles (9.98, 10.9 and 11.86 yr). The side frequencies are related to the spring tidal period of Jupiter and Saturn (9.93 yr) and to the tidal sidereal period of Jupiter (11.86 yr). A…

太阳与恒星天体物理 · 物理学 2012-03-20 Nicola Scafetta

The North-South asymmetry of solar activity has been recognized for different solar phenomena. Following Waldmeier, it is now assumed that solar activity dominates in the Northern solar hemisphere during the ascending part of the secular…

空间物理 · 物理学 2007-05-23 K. Georgieva , B. Kirov

Reliable prediction of the solar cycle is a formidable challenge, yet it is increasingly vital in our technology-dependent society as solar activity drives space weather. Various methods, including precursors, nonlinear curve fitting and…

太阳与恒星天体物理 · 物理学 2026-04-20 Bidya Binay Karak

The extension of the sunspot number series backward in time is of considerable interest for dynamo theory, solar, stellar, and climate research. We have used records of the Be-10 concentration in polar ice to reconstruct the average sunspot…

天体物理学 · 物理学 2009-11-10 Ilya G. Usoskin , Sami K. Solanki , Manfred Schuessler , Kalevi Mursula , Katja Alanko

The unexpected development of cycle 24 emphasizes the need for a better way to model future solar activity. In this article, we analyze the accumulation of spotless days during individual cycles from 1798-2010. The analysis shows that…

太阳与恒星天体物理 · 物理学 2011-04-27 M. Lindholm Nielsen , H. Kjeldsen

Because of the lack of reliable sunspot observation, the quality of sunspot number series is poor in the late 18th century, leading to the abnormally long solar cycle (1784--1799) before the Dalton minimum. Using the newly recovered solar…

太阳与恒星天体物理 · 物理学 2009-07-22 Ilya G. Usoskin , Kalevi Mursula , Rainer Arlt , Gennady A. Kovaltsov

Solar flares strongly affect the Sun's atmosphere as well as the Earth's environment. Quantifying the maximum possible energy of solar flares of the present-day Sun, if any, is thus a key question in heliophysics. The largest solar flares…

太阳与恒星天体物理 · 物理学 2015-06-12 G. Aulanier , P. Demoulin , C. J. Schrijver , M. Janvier , E. Pariat , B. Schmieder

Solar quasi-biennial oscillations with period range 0.6 to 4 years, are prominent in records of solar activity. Here we show that the 1.6 year quasi-biennial oscillation in solar activity has the exceptional feature of phase inversion…

太阳与恒星天体物理 · 物理学 2021-10-27 Ian R. Edmonds

We investigated the Korean records of naked-eye sunspot observations and found an implication of periodicity of about 200-year. Adding the Chinese records we showed that the historical naked-eye sunspot observations have the similar…

太阳与恒星天体物理 · 物理学 2019-12-25 Kim Chol-jun , Kim Jik-su

Guided by the working hypothesis that the Schwabe cycle of solar activity is synchronized by the 11.07 years alignment cycle of the tidally dominant planets Venus, Earth and Jupiter, we reconsider the phase diagrams of sediment accumulation…

太阳与恒星天体物理 · 物理学 2020-10-07 F. Stefani , J. Beer , A. Giesecke , T. Gloaguen , M. Seilmayer , R. Stepanov , T. Weier

We describe the peculiarity of two recurrent white light flares occurred on Sept. 06, 2017, in the super Active Region (SAR) NOAA 12673, with a time interval, between their peaks, of about 3 hours. These events of X2.2 and X9.3 GOES class…

太阳与恒星天体物理 · 物理学 2018-12-12 P. Romano , A. Elmhamdi , M. Falco , P. Costa , A. S. Kordi , H. A. Al-Trabulsy , R. M. Al-Shammari

Solar activity cycle varies in amplitude. The last Cycle 24 is the weakest in the past century. Sun's activity dominates Earth's space environment. The frequency and intensity of the Sun's activity are accordant with the solar cycle. Hence…

太阳与恒星天体物理 · 物理学 2022-02-16 Wei Guo , Jie Jiang , Jing-Xiu Wang

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

We propose a simple method for prediction of the 11-year solar cycle maximum that is based on two relations. One of them is well known Waldmeier's rule that binds the amplitude of a cycle and the length of its ascending phase. The second…

太阳与恒星天体物理 · 物理学 2022-08-03 Vladimir G. Ivanov

The dynamic activity of the Sun, governed by its cycle of sunspots -- strongly magnetized regions that are observed on its surface -- modulate our solar system space environment creating space weather. Severe space weather leads to…

太阳与恒星天体物理 · 物理学 2020-05-26 Aleix Espuña-Fontcuberta , Saikat Chatterjee , Dhrubaditya Mitra , Dibyendu Nandy

The idea of a planetary origin for the solar cycle dates back to the nineteenth century. Despite unsurmounted problems, it is still advocated by some. Stefani, Giesecke, and Weier (2019) thus recently proposed a scenario based on this idea.…

太阳与恒星天体物理 · 物理学 2022-08-31 Henri-Claude Nataf

We study and compare characteristics of sunspot group latitude distribution in two catalogs: the extended Greenwich (1874--2014) and Schwabe ones (1825--1867). We demonstrate that both datasets reveal similar links between latitude and…

太阳与恒星天体物理 · 物理学 2016-03-11 V. G. Ivanov , E. V. Miletsky

This work builds on a recently developed self-consistent synchronization model of the solar dynamo which attempts to explain Rieger-type periods, the Schwabe/Hale cycle and the Suess-de Vries and Gleissberg cycles in terms of resonances of…

太阳与恒星天体物理 · 物理学 2025-05-27 F. Stefani , G. M. Horstmann , G. Mamatsashvili , T. Weier

The combined Greenwich and Solar Optical Observing Network (SOON) sunspot group data during 1874-2013 are analyzed and studied the relatively long-term variations in the annual sums of the areas of sunspot groups in 0-10 deg, 10-20 deg, and…

太阳与恒星天体物理 · 物理学 2014-07-03 J. Javaraiah

Further development of the work of Obridko et al. [1] based on recent data confirms the assumption that the 25th cycle of solar activity is a medium-low cycle. Its height is expected to be $125.2\pm5.6$, and the expected date of the maximum…

太阳与恒星天体物理 · 物理学 2023-07-13 V. N. Obridko , D. D. Sokoloff , M. M. Katsova