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An extensive program for the calculation of galactic cosmic-ray propagation has been developed. This is a continuation of the work described in Strong & Youssefi (1995). The main motivation for developing this code is the prediction of…

天体物理学 · 物理学 2009-10-30 A. W. Strong , I. V. Moskalenko

Progress in astronomy comes from interpreting the signals encoded in the light received from distant objects: the distribution of light over the sky (images), over photon wavelength (spectrum), over polarization angle, and over time…

天体物理仪器与方法 · 物理学 2013-09-26 Simon Vaughan

We present a new model for the Galactic distribution of free electrons. It (a) describes the distribution of the free electrons responsible for pulsar dispersion measures and thus can be used for estimating the distances to pulsars; (b)…

天体物理学 · 物理学 2009-09-29 J. M. Cordes , T. J. W. Lazio

A brief survey of nuclide abundances in the solar-system and in cosmic rays and of the believed mechanisms of their synthesis is given. The role of spallation processes in nucleosynthesis is discussed. A short review of recent measurements,…

天体物理学 · 物理学 2007-05-23 Stepan G. Mashnik

As the Stars and Stellar Evolution (SSE) panel is fully aware, the next decade will see major advances in our understanding of these areas of research. To quote from their charge, these advances will occur in studies of the Sun as a star,…

Self-organized criticality describes a class of dynamical systems that maintain themselves in an attractor state with no intrinsic length or time scale. Fundamentally, this theoretical construct requires a mechanism for instability that may…

太阳与恒星天体物理 · 物理学 2022-02-02 Adina D. Feinstein , Darryl Z. Seligman , Maximilian N. Günther , Fred C. Adams

Determining the spatial distribution of Galactic cosmic rays (CRs) is fundamental to understand how these particles propagate in interstellar space and to infer their source spectra. The most sensitive method of studying this problem is…

高能天体物理现象 · 物理学 2025-09-26 Paolo Lipari , Silvia Vernetto

An extensive program for the calculation of galactic cosmic-ray propagation has been developed. Primary and secondary nucleons, primary and secondary electrons, secondary positrons and antiprotons are included. Fragmentation and energy…

天体物理学 · 物理学 2007-05-23 A. W. Strong , I. V. Moskalenko

The notions of self-organised criticality (SOC) and turbulence are traditionally considered to be applicable to disjoint classes of phenomena. Nevertheless, scale-free burst statistics is a feature shared by turbulent as well as…

等离子体物理 · 物理学 2009-11-13 Kristoffer Rypdal , Boris Kozelov , Svetlana Ratynskaia , Boris Klumov , Christina Knapek

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

Some years ago we proposed a new approach for the analysis of galaxy and cluster correlations based on the concepts and methods of modern statistical physics. This led to the surprising result that galaxy correlations are fractal and not…

天体物理学 · 物理学 2016-08-30 L. Pietronero , M. Montuori , F. Sylos Labini

This paper presents an analysis of the smoothness problem in cosmology by focussing on the ambiguities originated in the simplifying hypotheses aimed at observationally verifying if the large-scale distribution of galaxies is homogeneous,…

天体物理学 · 物理学 2015-06-24 Marcelo B. Ribeiro

The characterization of global energy storage and release in the coupled solar wind-magnetosphere system remains one of the fundamental problems of space physics.Recently, it has been realised that a new paradigm in physics, that of Self…

天体物理学 · 物理学 2021-04-28 Sandra Chapman , Nicholas Watkins

As the panel on Planetary Systems and Star Formation (PSF) is fully aware, the next decade will see major advances in our understanding of these areas of research. To quote from their charge, these advances will occur in studies of solar…

Precise analyses of the statistical and scaling properties of galaxy distribution are essential to elucidate the large-scale structure of the universe. Given the ongoing debate on its statistical features, the development of statistical…

天体物理学 · 物理学 2007-05-23 M. Bottaccio , M. Montuori , L. Pietronero

The structures formation of the Universe appears as if it were a classically self-similar random process at all astrophysical scales. An agreement is demonstrated for the present hypotheses of segregation with a size of astrophysical…

天体物理学 · 物理学 2008-11-26 G. Iovane , E. Laserra , F. S. Tortoriello

Although the paradigm of criticality is centred around spatial correlations and their anomalous scaling, not many studies of Self-Organised Criticality (SOC) focus on spatial correlations. Often, integrated observables, such as avalanche…

统计力学 · 物理学 2017-08-01 Gary Willis , Gunnar Pruessner

A formalism is presented that allows cosmological experiments to be tested for consistency, and allows a simple frequentist interpretation of the resulting significance levels. As an example of an application, this formalism is used to…

天体物理学 · 物理学 2009-10-07 Max Tegmark , Emory Bunn , Wayne Hu

We analyzed the soft X-ray light curves from the {\sl Geostationary Operational Environmental Satellites (GOES)} over the last 37 years (1975-2011) and measured with an automated flare detection algorithm over 300,000 solar flare events…

太阳与恒星天体物理 · 物理学 2012-07-18 Markus J. Aschwanden , Samuel L. Freeland

We search for outliers in extreme events of statistical size distributions of astrophysical data sets, motivated by the {\sl Dragon-King hypothesis} of Sornette (2009), which suggests that the most extreme events in a statistical…

太阳与恒星天体物理 · 物理学 2019-08-07 Markus J. Aschwanden