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相关论文: Correlation study of some solar activity indices i…

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A stable cyclicity of correlation coefficients Kcorr for some solar activity indices versus F10,7 was found after monthly averages values analysis. These indices are: Wolf numbers, 10,7 cm radio flux F10,7, 0,1-0,8 nm background, the total…

太阳与恒星天体物理 · 物理学 2015-09-29 E. A. Bruevich , G. V. Yakunina

The monthly average values of the main solar activity indices such as Wolf numbers (W), 10,7 cm radio flux (F10,7), 0,1-0,8 nm background, total solar irradiance and Mg II UV-index (280 nm core to wing ratio) were studied for 23 activity…

太阳与恒星天体物理 · 物理学 2011-03-01 E. A. Bruevich , G. V. Yakunina

The analysis of long-term variations of several solar activity indices (AI) since in last 40 years has been performed. We studied the AI which characterize the fluxes from different areas in solar atmosphere. Our consideration of mutual…

太阳与恒星天体物理 · 物理学 2019-01-01 E. A. Bruevich , V. V. Bruevich

In the present paper a systematic study is carried out to validate the similarity or degree of relationship between daily terrestrial cosmic rays intensity and three characteristics of about evolution of solar corona, like a number of…

太阳与恒星天体物理 · 物理学 2019-06-05 D. Sierra-Porta

The analysis of the observations of solar activity indexes SSN (NOAA Sunspot Numbers), the radio flux at a wavelength of 10.7 cm (F10.7) and the solar constant (TSI) during the cycles 22 - 24 is presented. We found a decrease of the…

太阳与恒星天体物理 · 物理学 2015-10-08 E. A. Bruevich , G. V. Yakunina

The solar F10.7 index is has been a reliable and sensitive activity index since 1947. As with other indices, it has been showing unusual behavior in the Cycle 23/24 minimum. The origins of the solar microwave flux lie in a variety of…

太阳与恒星天体物理 · 物理学 2010-03-24 Leif Svalgaard , Hugh S. Hudson

The large (X-ray class > M1) and very large (X-ray class >X1) flares (according to the observations of GOES-15 and Preliminary data from Current Catalog of Flare Events) in solar activity cycle 24 were analyzed. The monthly average values…

太阳与恒星天体物理 · 物理学 2018-03-21 E. A. Bruevich , T. V. Kazachevskaya , G. V. Yakunina

The analysis of the effect of the hysteresis, which manifests itself in an ambiguous relationship of radiation from the photosphere, chromosphere and corona on the rise and decline phases of the solar and stellar activity cycles have done.…

太阳与恒星天体物理 · 物理学 2016-07-29 E. A. Bruevich , G. V. Yakunina , T. V. Kazachevskaya , V. V. Katyushina , A. A. Nusinov

The present paper reviews results derived from statistical studies on solar activity indices. The prolonged minimum phase of cycle 23 raised the question of peculiarities inherent in cycle 23. The most important solar activity index is the…

太阳与恒星天体物理 · 物理学 2010-02-03 M. Temmer

To better understand the influence of the activity cycle on the solar atmosphere, we report the time variation of the radius observed at 37 GHz ($\lambda$=8.1 mm) obtained by the Mets\"ahovi Radio Observatory (MRO) through Solar Cycles 22…

太阳与恒星天体物理 · 物理学 2019-12-17 Caius L. Selhorst , Juha Kallunki , C. G. Giménez de Castro , Adriana Valio , Joaquim E. R. Costa

Results of analysis of long time variations of solar activities based on monthly Wolf number series (1749-2011 years) are represented. Shown the presence of stable oscillations in autocorrelation function for the Wolf numbers series with a…

太阳与恒星天体物理 · 物理学 2012-02-09 V. M. Zhuravlev , S. V. Letunovskiy

(Abridged) We perform a detailed study of the main optical activity indicators (Ca II H & K, Balmer lines, Na I D$_{\rm 1}$ D$_{\rm 2}$, and He I D$_{\rm 3}$) measured for the Sun using the data provided by the HARPS-N solar-telescope feed…

Previous studies on the impact and influence of solar activity on terrestrial weather has yielded contradictory results in literature. Present study presents, on a global scale, the correlation between surface air temperature and two solar…

地球与行星天体物理 · 物理学 2023-05-30 S. T. Ogunjo , A. B. Rabiu

Aims. In this paper, we investigate the temporal evolution and north-south (N-S) asymmetry in the occurrence of solar flares during cycle 21, 22, and 23, and compare the results with traditional solar activity indices. Methods. The flare…

太阳与恒星天体物理 · 物理学 2017-05-08 Bhuwan Joshi , R. Bhattacharyya , K. K. Pandey , Upendra Kushwaha , Yong-Jae Moon

Variations of total solar irradiance (TSI), magnetic field, Ca II K-flux, faculae and plage areas due to the number and the type of sunspots/sunspot groups (SGs) are well established by using Solar Irradiance Platform and ground based data…

太阳与恒星天体物理 · 物理学 2016-09-02 Umit Deniz Goker , Jagdev Singh , Ferhat Nutku , Muthu Priyal

We study the shape of sunspot cycles using the Wolf sunspot numbers and group sunspot numbers of solar cycles 1-23. We determine the most typical "model" cycles and the most asymmetric cycles, and test the validity of the two Waldmeier…

太阳与恒星天体物理 · 物理学 2018-12-12 Jouni Takalo , Kalevi Mursula

The solar activity in the current, that is, the 24-th, sunspot cycle is analyzed. Cyclic variations in the sunspot number (SSN) and radiation fluxes in various spectral ranges have been estimated in comparison with the general level of the…

太阳与恒星天体物理 · 物理学 2018-05-01 E. A. Bruevich , V. V. Bruevich , G. V. Yakunina

We consider the statistical relationship between the growth rate of activity in the early phase of a solar cycle with its subsequent amplitude on the basis of four datasets of global activity indices (Wolf sunspot number, group sunspot…

天体物理学 · 物理学 2008-06-18 R. Cameron M. Schüssler

The paper shows the recurrence and cross recurrence plots of three time series, concerning data of the solar activity. The data are the sunspot number and the values of solar radio flux at 10.7 cm and of solar total irradiance, which are…

科普物理 · 物理学 2008-04-14 Amelia Sparavigna

The relationships between solar flare parameters (total importance, time duration, flare index, and flux) and sunspot activity (Rz) as well as those between geomagnetic activity (aa index) and the flare parameters can be well described by…

太阳与恒星天体物理 · 物理学 2015-06-03 Z. L. Du , H. N. Wang
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