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Solar activity is studied using a cluster analysis of the time-fluctuations of the sunspot number. It is shown that in an Historic period the high activity components of the solar cycles exhibit strong clustering, whereas in a Modern period…

天体物理学 · 物理学 2010-11-02 A. Bershadskii

Solar active longitudes show a characteristic migration pattern in the Carrington coordinate system when they can be identified at all. By following this migration, the longitudinal activity distribution around the center of the band can be…

太阳与恒星天体物理 · 物理学 2014-01-09 N. Gyenge , T. Baranyi , A. Ludmány

Severity of warming predicted by climate models depends on their Transient Climate Response (TCR). Inter-model spread of TCR has persisted at ~100% of its mean for decades. Existing observational constraints of TCR are based on observed…

大气与海洋物理 · 物理学 2023-12-25 King-Fai Li , Ka-Kit Tung

The diagram of indices of coronal and chromospheric activity allowed us to reveal stars where solar-type activity appears and regular cycles are forming. Using new consideration of a relation between coronal activity and the rotation rate,…

太阳与恒星天体物理 · 物理学 2015-08-06 M. M. Katsova , N. I. Bondar' , M. A. Livshits

Longitudinal distributions of the photospheric magnetic field studied on the base of National Solar Observatory (Kitt Peak) data (1976 - 2003) displayed two opposite patterns during different parts of the 11-year solar cycle.…

天体物理学 · 物理学 2007-12-17 E. S. Vernova , M. I. Tyasto , D. G. Baranov

In this splinter session, ten speakers presented results on solar and stellar activity and how the two fields are connected. This was followed by a lively discussion and supplemented by short, one-minute highlight talks. The talks presented…

太阳与恒星天体物理 · 物理学 2014-08-14 H. M. Günther , K. Poppenhaeger , P. Testa , S. Borgniet , S. Brun , H. Cegla , C. Garraffo , A. Kowalski , A. Shapiro , E. Shkolnik , F. Spada , A. Vidotto

The relationship between cosmic ray intensity decreases and solar events is still an open field of space research. In this work a complete study of solar events occurred from January 2003 to December 2005, is considered. This three-years…

空间物理 · 物理学 2010-09-30 A. Papaioannou , P. Makrantoni , H. Mavromichalaki

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

Evaluating the magnitude of natural climate variations is important because it can greatly affect future climate policies. As an example, we examine the influence of changes in solar activity (solar wind in particular) on surface…

大气与海洋物理 · 物理学 2018-07-12 Kiminori Itoh , Shinya Matsuo , Hiroshi Serizawa , Kazuyoshi Yamashita , Takashi Amemiya

In solar cycles 23-24, solar activity noticeably decreased, and, as a result, solar wind parameters decreased. Based on the measurements of the OMNI base for the period 1976-2019, the time profiles of the main solar wind parameters and…

Solar activities have a great impact on modern high-tech systems, such as human aerospace, satellite communication and navigation, deep space exploration, and related scientific research. Therefore, studying the long - term evolution trend…

太阳与恒星天体物理 · 物理学 2024-02-21 Peixin Luo , Baolin Tan

The study of solar active longitudes has generated a great interest in the recent years. In this work we have used an unique continuous sunspot data series obtained from Kodaikanal observatory and revisited the problem. Analysis of the data…

太阳与恒星天体物理 · 物理学 2017-01-25 Sudip Mandal , Subhamoy Chatterjee , Dipankar Banerjee

Recently, Jenkins, et al. have reported the detection of correlations between fluctuations in nuclear decay rates and Earth-Sun distance, which suggest that nuclear decay rates can be affected by solar activity. In this paper, we report the…

天体物理学 · 物理学 2010-07-07 Jere H. Jenkins , Ephraim Fischbach

The Sun experienced a period of unprecedented activity during the 20th century, now called the Modern Maximum (MM). The decay of the MM after cycle 19 has changed the Sun, the heliosphere, and the planetary environments in many ways.…

太阳与恒星天体物理 · 物理学 2024-03-14 K. Mursula , A. A. Pevtsov , T. Asikainen , I. Tähtinen , A. R. Yeates

As the 21st century progresses, photovoltaic technology is becoming a major provider of the worlds electricity, while effects of global climate change unfold. This development begs the question: is climate change affecting the energy…

物理与社会 · 物理学 2019-08-20 Ian Marius Peters , Tonio Buonassisi

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

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

How the solar electromagnetic energy entering the Earth's atmosphere varied since pre-industrial times is an important consideration in the climate change debate. Detrimental to this debate, estimates of the change in total solar irradiance…

太阳与恒星天体物理 · 物理学 2021-02-19 K. L. Yeo , S. K. Solanki , N. A. Krivova , M. Rempel , L. S. Anusha , A. I. Shapiro , R. V. Tagirov , V. Witzke

We have analyzed the full set of SOHO/MDI f- and p-mode oscillation frequencies from 1996 to date in a search for evidence of solar radius evolution during the rising phase of the current activity cycle. Like Antia et al. (2000), we find…

天体物理学 · 物理学 2009-11-06 W. A. Dziembowski , P. R. Goode , J. Schou

The Sun's variability is controlled by the progression and interaction of the magnetized systems that form the 22-year magnetic activity cycle (the "Hale Cycle'') as they march from their origin at $\sim$55 degrees latitude to the equator,…

太阳与恒星天体物理 · 物理学 2021-12-07 Robert Leamon , Scott McIntosh , Alan Title