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相关论文: Redefining the limit dates for the Maunder Minimum

200 篇论文

The power spectral analyses of the Sun's surface equatorial rotation rate determined from the Mt. Wilson daily Doppler velocity measurements during the period 3 December 1985 to 5 March 2007 suggests the existence of 7.6 year, 2.8 year,…

太阳与恒星天体物理 · 物理学 2009-11-13 J. Javaraiah , R. K. Ulrich , L. Bertello , J. E. Boyden

Based on the planet-satellite dynamics, a new perspective on the birth and evolution of the Solar System was proposed in 2004. This new perspective has 1:2 Mean Motion Resonance (1:2 MMR, that is Ps/Pj = 2) implicit in itself . This paper…

天体物理学 · 物理学 2008-08-01 Bijay Kumar Sharma

A phenomenological model is presented for the quantitative description of individual solar cycles' features, such as onset, intensity, evolution, in terms of the number of M and X-class solar flares. The main elements of the model are the…

太阳与恒星天体物理 · 物理学 2020-08-14 Eleni Petrakou

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

We have measured the physical properties of polar coronal holes from the minimum activity phase of solar cycle 23 (1996-1997) to the present minimum of solar cycle 24 (2007-2009) using the UVCS instrument on SOHO. Observations in H I Lyman…

太阳与恒星天体物理 · 物理学 2010-05-19 M. P. Miralles , S. R. Cranmer , A. V. Panasyuk , M. Uzzo

We introduce a new method for predicting sunspot number (SSN) that, based on successful back projections, can predict features of the SSN several solar cycles in advance. The method applies Fourier analysis to the annual SILSO SSN record,…

太阳与恒星天体物理 · 物理学 2026-05-05 Ian Edmonds , Peter Killen

The study of young Sun-like stars is of fundamental importance to understand the magnetic activity and rotational evolution of the Sun. Space-borne photometry by the Kepler telescope provides unprecedented datasets to investigate these…

太阳与恒星天体物理 · 物理学 2019-06-12 A. F. Lanza , Y. Netto , A. S. Bonomo , H. Parviainen , A. Valio , S. Aigrain

After a prolonged and deep solar minimum at the end of Cycle 23, the current Solar Cycle 24 is one of the lowest cycles. These two periods of deep minimum and mini maximum are separated by a period of increasing solar activity. We study the…

太阳与恒星天体物理 · 物理学 2015-09-01 O. P. M. Aslam , Badruddin

If dark matter (DM) is unstable, in order to be present today, its lifetime needs to be longer than the age of the Universe, t_U ~ 4 10^{17} s. It is usually assumed that if DM decays it would do it with some strength through a radiative…

天体物理学 · 物理学 2009-06-23 Sergio Palomares-Ruiz

We present the results of study of a possible relationship between the space weather and terrestrial markets of agricultural products. It is shown that to implement the possible effect of space weather on the terrestrial harvests and…

大气与海洋物理 · 物理学 2015-06-12 Lev Pustilnik , Gregory Yom Din

We have proposed a model to obtain the length of the day and month at any geologic time. The day is found to increase by 0.002 sec/century since the seventeenth century. The lengthening of the day is attributed entirely to the increasing…

综合物理 · 物理学 2007-05-23 A. I. Arbab

The growth rate of solar activity in the early phase of a solar cycle has been known to be well correlated with the subsequent amplitude (solar maximum). It provides very useful information for a new solar cycle as its variation reflects…

太阳与恒星天体物理 · 物理学 2011-12-30 Z. L. Du , H. N. Wang

It is very important to forecast the future solar activity due to its effect on our planet and near space. Here, we employ the new version of the sunspot number index (version 2) to analyse the relationship between the solar maximum…

太阳与恒星天体物理 · 物理学 2016-09-08 V. M. S. Carrasco , J. M. Vaquero , M. C. Gallego

We present the first spectropolarimetric time-series analysis of the Maunder Minimum analog HD 166620, using 12 nights of data from CFHT/SPIRou and a single epoch from CFHT/ESPaDOnS. While individual Stokes $V$ profiles exhibit no…

太阳与恒星天体物理 · 物理学 2026-03-20 Federica Chiti , Jennifer L. van Saders , Oleg Kochukhov , Travis S. Metcalfe

The study of variations in solar activity is important for understanding the underlying mechanism of solar activity and for predicting the level of activity in view of the activity impact on space weather and global climate. Here we have…

太阳与恒星天体物理 · 物理学 2017-11-15 J. Javaraiah

We show here a component of the meridional circulation developing at medium-high latitudes (40-50 degrees) before the new solar cycle starts. Like the torsional oscillation of the zonal flows, this extra circulation seems to precede the…

太阳与恒星天体物理 · 物理学 2015-05-18 I. Gonzalez Hernandez , R. Howe , R. Komm , F. Hill

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

The MOdified Newtonian Dynamics (MOND) is an attempt to modify the gravitation theory to solve the Dark Matter problem. This phenomenology is very successful at the galactic level. The main effect produced by MOND in the Solar System is…

广义相对论与量子宇宙学 · 物理学 2014-05-14 A. Hees , W. M. Folkner , R. A. Jacobson , R. S. Park

Although systematic measurements of the solar polar magnetic field exist only from mid 1970s, other proxies can be used to infer the polar field at earlier times. The observational data indicate a strong correlation between the polar field…

天体物理学 · 物理学 2009-11-13 Jie Jiang , Piyali Chatterjee , Arnab Rai Choudhuri

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
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