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相关论文: Predicting the solar maximum with the rising rate

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As photovoltaic power is expanding rapidly worldwide, it is imperative to assess its promise under future climate scenarios. While a great deal of research has been devoted to trends of mean solar radiation, less attention has been paid to…

大气与海洋物理 · 物理学 2020-11-13 Jun Yin , Annalisa Molini , Amilcare Porporato

The solar cycle and its associated magnetic activity are the main drivers behind changes in the interplanetary environment and the Earth's upper atmosphere (commonly referred to as space weather). These changes have a direct impact on the…

太阳与恒星天体物理 · 物理学 2013-04-12 Andrés Muñoz-Jaramillo , María Dasi-Espuig , Laura A. Balmaceda , Edward E. DeLuca

It is assumed that the solar cell efficiency of PV device is closely related to the solar irradiance, considered the solar parameter Global Solar Irradiance (G) and the meteorological parameters like daily data of Earth Skin Temperature…

应用统计 · 统计学 2012-06-08 Kashif Bin Zaheer , Waseem Ahmed Ansari , Syed Mohammad Murshid Raza

The 11-yr cycle of sunspots undergo amplitude modulation over longer timescales. As a part of this long-term modulation in solar activity, the decennial rhythm occasionally breaks, with quiescent phases with very few sunspots observed over…

太阳与恒星天体物理 · 物理学 2025-09-05 Chitradeep Saha , Sanghita Chandra , Dibyendu Nandy

We explore consequences for the solar dynamo of a newly-developed physical hypothesis describing a weak coupling of the orbital and rotational motions of extended bodies. The coupling is given by - c ((dL/dt) x omega sub alpha) x r, where…

太阳与恒星天体物理 · 物理学 2017-06-07 James H. Shirley

Solar cycle is modeled as a forced and damped harmonic oscillator and the amplitudes, frequencies, phases and decay factors of such a harmonic oscillator are estimated by non-linear fitting the equation of sinusoidal and transient parts to…

太阳与恒星天体物理 · 物理学 2022-04-12 K M Hiremath

A striking feature of the solar cycle is that at the beginning, sunspots appear around mid-latitudes, and over time the latitudes of emergences migrate towards the equator. The maximum level of activity varies from cycle to cycle. For…

太阳与恒星天体物理 · 物理学 2024-12-25 Akash Biswas

We analyze the occurrence frequency distributions of peak fluxes $P$, total fluxes $E$, and durations $T$ of solar flares over the last three solar cycles (during 1980--2010) from hard X-ray data of HXRBS/SMM, BATSE/CGRO, and RHESSI. From…

太阳与恒星天体物理 · 物理学 2012-01-13 Markus J. Aschwanden

We show that there is a previously unreported quad-annual variation in the ~13.5 day component of the aa index of geomagnetic activity. We derive a model based on the planetary tidal effect at the solar surface due to Mercury and Jupiter…

地球与行星天体物理 · 物理学 2014-01-14 I. R. Edmonds

The planetary hypothesis of the solar cycle is an old idea in which the gravitational influence of the planets has a non-negligible effect on the causes of the solar magnetic cycle. In this work we looked for a possible causal link in…

地球与行星天体物理 · 物理学 2012-07-24 Rodolfo Gustavo Cionco , Rosa Hilda Compagnucci

We examine the evolution of the zonal flow pattern in the upper solar convection zone during the current extended solar minimum, and compare it with that during the previous minimum. The results suggest that a configuration matching that at…

太阳与恒星天体物理 · 物理学 2015-09-24 R. Howe , J. Christensen-Dalsgaard , F. Hill , R. Komm , J. Schou , M. J. Thompson

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

The Sun's magnetic dynamo cycle features a distinct pattern: a propagating region of sunspot emergence appears around 30 degrees latitude and vanishes near the equator every 11 years. Moreover, longitudinal flows called "torsional…

Long-term evolution characteristics of the solar transition region have been unclear. In this study, daily images of the solar full disk derived from the observations by the Solar Dynamics Observatory/Atmospheric Imaging Assembly at 304 A…

太阳与恒星天体物理 · 物理学 2024-12-13 W. Q. Chen , K. J. Li , J. C. Xu

The Sun is the major source of heat and light in our solar system. The solar cycle is the 11-year cycle of solar activity that can be determined by the rise and fall in the numbers and surface area of sunspots. Solar activity is associated…

太阳与恒星天体物理 · 物理学 2018-05-01 Ryan Manuel D. Guido

We present observations of the extended solar cycle activity in white-light coronagraphs, and compare them with the more familiar features seen in the Fe XIV green-line corona. We show that the coronal activity zones seen in the emission…

太阳与恒星天体物理 · 物理学 2013-02-22 S. J. Tappin , R. C. Altrock

We present a hybrid forecasting strategy that combines numerical modeling, statistical forecasting, and machine learning methods to predict enhanced bursts of solar activity. These bursts, referred to here as space weather seasons, occur on…

太阳与恒星天体物理 · 物理学 2026-05-27 Juie Shetye , Mausumi Dikpati

We construct a new solar cycle phase clock which maps each of the last 18 solar cycles onto a single normalized epoch for the approximately 22 year Hale (magnetic polarity) cycle, using the Hilbert transform of daily sunspot numbers (SSN)…

太阳与恒星天体物理 · 物理学 2021-08-25 S. C. Chapman , S. W. McIntosh , R. J. Leamon , N. W. Watkins

The average tilt angle of sunspot groups emerging throughout the solar cycle determines the net magnetic flux crossing the equator, which is correlated with the strength of the subsequent cycle. I suggest that a deep-seated, non-local…

太阳与恒星天体物理 · 物理学 2015-10-28 Emre Işık

The data from solar neutrino experiments together with standard solar model predictions are used in order to derive the possible profile of the magnetic field inside the Sun, assuming the existence of a sizeable neutrino magnetic moment and…

天体物理学 · 物理学 2009-10-30 Joao Pulido