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相关论文: Self-Organized Criticality in Stellar Flares

200 篇论文

We investigate the large-scale distribution of galaxy clusters taken from several X-ray catalogs. Different statistics of clustering like the conditional correlation function (CCF) and the minimal spanning tree (MST) as well as void…

天体物理学 · 物理学 2008-05-16 A. V. Tikhonov , A. I. Kopylov , S. Gottlober , G. Yepes

We review a series of recent results on global dynamic properties of radially symmetric self-gravitating compressible Euler flows, which naturally arise in the mathematical description of stars. We focus on the role of scaling invariances…

偏微分方程分析 · 数学 2023-06-06 Mahir Hadzic

It has been recently found that a number of systems displaying crackling noise also show a remarkable behavior regarding the temporal occurrence of successive events versus their size: a scaling law for the probability distributions of…

统计力学 · 物理学 2009-11-13 Alvaro Corral

(abridged) We study the hypothesis that observed X-ray/extreme ultraviolet emission from coronae of magnetically active stars is entirely (or to a large part) due to the superposition of flares, using an analytic approach to determine the…

天体物理学 · 物理学 2009-11-10 K. Arzner , M. Guedel

An improved version of the Olami-Feder-Christensen model has been introduced to consider avalanche size differences. Our model well demonstrates the power-law behavior and finite size scaling of avalanche size distribution in any range of…

统计力学 · 物理学 2015-05-20 Gui-Qing Zhang , Ugur Tirnakli , Lin Wang , Tian-Lun Chen

Solar-like oscillations have been observed by Kepler and CoRoT in many solar-type stars, thereby providing a way to probe the stars using asteroseismology. We provide the mode linewidths and mode heights of the oscillations of various stars…

The observed amplitude of the rotational photometric modulation of a star with spots should depend on the inclination of its rotational axis relative to our line of sight. Therefore, the distribution of observed rotational amplitudes of a…

地球与行星天体物理 · 物理学 2015-06-23 Tsevi Mazeh , Hagai B. Perets , Amy McQuillan , Eyal S. Goldstein

We report on the results of our simultaneous observations of three large stellar flares with soft X-rays (SXRs) and an H$\mathrm{\alpha}$ emission line from two binary systems of RS CVn type. The energies released in the X-ray and…

高能天体物理现象 · 物理学 2023-07-06 Hiroki Kawai , Yohko Tsuboi , Wataru B. Iwakiri , Yoshitomo Maeda , Satoru Katsuda , Ryo Sasaki , Junya Kohara , MAXI TEAM

Solar-like oscillations have been observed by {{\it Kepler}} and CoRoT in several solar-type stars. We study the variations of stellar p-mode linewidth as a function of effective temperature. Time series of 9 months of Kepler data have been…

We have studied the damage spreading (defined in the text) in the 'sandpile' model of self organised criticality. We have studied the variations of the critical time (defined in the text) and the total no of sites damaged at critical time…

凝聚态物理 · 物理学 2007-05-23 Ajanta Bhowal

Statistical analyses of finite sample distributions usually assume that fluctuations are self-averaging, i.e. that they are statistically similar in different regions of the given sample volume. By using the scale-length method, we test…

宇宙学与河外天体物理 · 物理学 2010-11-02 Francesco Sylos Labini , Nikolay L. Vasilyev , Yurij V. Baryshev

We describe analytical and numerical collisional evolution calculations for the size distribution of icy bodies in the Kuiper Belt. For a wide range of bulk properties, initial masses, and orbital parameters, our results yield power-law…

天体物理学 · 物理学 2009-11-10 Scott J. Kenyon , Benjamin C. Bromley

Atmospheric flows exhibit selfsimilar fluctuations on all scales(space-time) ranging from climate(kilometers/years) to turbulence(millimeters/seconds) manifested as fractal geometry to the global cloud cover pattern concomitant with inverse…

chao-dyn · 物理学 2007-05-23 A. Mary Selvam

We conducted high dispersion spectroscopic observations of 50 superflare stars with Subaru/HDS. These 50 stars were selected from the solar-type superflare stars that we had discovered from the Kepler data. More than half (34 stars) of…

太阳与恒星天体物理 · 物理学 2015-06-09 Yuta Notsu , Satoshi Honda , Hiroyuki Maehara , Shota Notsu , Takuya Shibayama , Daisaku Nogami , Kazunari Shibata

We extend a generic class of systems which have previously been shown to spontaneously develop scaling (power law) distributions of their elementary degrees of freedom. While the previous systems were linear and exploded exponentially for…

adap-org · 物理学 2009-10-28 S. Solomon , M. Levy

In an effort to examine the relationship between flare flux and corresponding CME mass, we temporally and spatially correlate all X-ray flares and CMEs in the LASCO and GOES archives from 1996 to 2006. We cross-reference 6,733 CMEs having…

太阳与恒星天体物理 · 物理学 2015-05-20 Alicia N. Aarnio , Keivan G. Stassun , W. Jeffrey Hughes , Sarah L. McGregor

The Kepler mission has led to the serendipitous discovery of a significant number of `super flares' - white light flares with energies between 10^33 erg and 10^36 erg - on solar-type stars. It has been speculated that these could be `freak'…

太阳与恒星天体物理 · 物理学 2014-09-05 R. Wichmann , B. Fuhrmeister , U. Wolter , E. Nagel

We perform an experimental study of the time behavior of the $\alpha$-wave events occuring in human electroencephalographic signals. We find that the fraction of the time spent in an $\alpha$-burst of time size $\tau$ exhibits a scaling…

生物物理 · 物理学 2009-10-31 Y. Georgelin , L. Poupard , R. Sartene , J. C. Wallet

Power laws in nature are considered to be signatures of complexity. The theory of self-organized criticality (SOC) was proposed to explain their origins. A longstanding principle of SOC is the \emph{separation of timescales} axiom. It…

神经元与认知 · 定量生物学 2019-07-03 Anirban Das , Anna Levina

We develop a statistical analytical model that predicts the occurrence frequency distributions and parameter correlations of avalanches in nonlinear dissipative systems in the state of a slowly-driven self-organized criticality (SOC)…

太阳与恒星天体物理 · 物理学 2015-06-03 Markus J. Aschwanden