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The X2.2-class solar flare of February 15, 2011, produced a powerful `sunquake' event, representing a seismic response to the flare impact. The impulsively excited seismic waves formed a compact wavepacket traveling through the solar…

Solar and Stellar Astrophysics · Physics 2011-02-22 A. G. Kosovichev

An overview is given on results from direct and indirect measurements of galactic cosmic rays. Their implications on the contemporary understanding of the origin of cosmic rays and the knee in their energy spectrum are discussed.

Astrophysics · Physics 2009-11-10 Joerg R. Hoerandel

Three pairs of possibly correlated ultra-high energy cosmic ray events were reported by Hayashida et al (1996). Here we calculate the propagation of the corresponding particles through both the intergalactic and galactic magnetic fields.…

Astrophysics · Physics 2010-11-30 Gustavo A. Medina Tanco

Cosmic rays are known to cause biological effects directly and through ionizing radiation produced by their secondaries. These effects have been detected in airline crews and other specific cases where members of the population are exposed…

Space Physics · Physics 2015-05-18 A. C. Overholt , A. L. Melott , D. Atri

A density disturbance in a system of gravitating mass, induced by a moving selected body gives rise to a dynamical screening of Newtonian potential of this body. When applied to the solar planetary system it means that as a result of the…

Astrophysics · Physics 2007-05-23 A. G. Bashkirov , A. V. Vityazev , G. V. Pechernikova

We present the results of a numerical simulation of propagation of cosmic rays with energy above $10^{15}$ eV in a complex magnetic field, made in general of a large scale component and a turbulent component. Several configurations are…

Astrophysics · Physics 2009-11-13 Daniel De Marco , Pasquale Blasi , Todor Stanev

The physics of Ultra High Energy Cosmic Rays will be reviewed, discussing the latest experimental results and theoretical models aiming at explaining the observations in terms of spectra, mass composition and possible sources. It will be…

High Energy Astrophysical Phenomena · Physics 2019-06-12 Roberto Aloisio

One of the most striking astrophysical phenomena today is the existence of cosmic ray particles with energies in excess of 10^20 eV. While their presence has been confirmed by a number of experiments, it is not clear where and how these…

High Energy Physics - Experiment · Physics 2009-11-11 Stefan Westerhoff

We study the nonlinear growth of kinetic gyroresonance instability of cosmic rays (CRs) induced by large scale compressible turbulence. This feedback of cosmic rays on turbulence was shown to induce an important scattering mechanism in…

High Energy Astrophysical Phenomena · Physics 2011-03-28 Huirong Yan , A. Lazarian

We consider the modification of extragalactic cosmic ray spectrum caused by cosmic ray interactions with infrared background photons which are present in the extragalactic space together with relic photons. It is assumed that cosmic ray…

Astrophysics · Physics 2008-11-26 E. V. Bugaev , P. A. Klimai

Cosmic rays are an important factor of space weather determining radiation conditions near the Earth and it seems to be essential to clarify radiation conditions near extrasolar planets too. Last year a terrestrial planet candidate was…

Solar and Stellar Astrophysics · Physics 2017-09-12 Alexei Struminsky , Andrei Sadovski , Anatoly Belov

High-speed solar wind streams (HSSs) interact with the preceding ambient solar wind to form Stream Interaction Regions (SIRs), which are a primary source of recurrent geomagnetic storms. However, HSSs may also encounter and subsequently…

Solar and Stellar Astrophysics · Physics 2024-02-14 Stephan G. Heinemann , Chaitanya Sishtla , Simon Good , Maxime Grandin , Jens Pomoell

The variation in the intensity of cosmic rays at small angular scales is attributed to the interstellar turbulence in the vicinity of the Solar system. We show that {a turbulent origin of the small-scale structures implies that} the…

High Energy Astrophysical Phenomena · Physics 2018-12-12 Rahul Kumar , Noemie Globus , David Eichler , Martin Pohl

The interaction of magnetic turbulence and relativistic particles is a important process for understanding particles propagation and acceleration in many astrophysical environments. Large-scale turbulence can be generated in the…

Cosmology and Nongalactic Astrophysics · Physics 2012-01-04 Gianfranco Brunetti

Cosmic rays physics is currently being studied with rather sophisticated detectors running in a variety of experimental conditions and atmospheric depths around the world. In this paper we describe the reasons why cosmic ray physics…

Astrophysics · Physics 2010-11-11 O. Saavedra , L. Jones

High-redshift primordial galaxies have recently been found with evolved stellar populations and complex star-formation histories reaching back to 250 Myr after the Big Bang. Their intense bursts of star-formation appear to be interspersed…

Astrophysics of Galaxies · Physics 2022-12-14 Ellis R. Owen

Research in cosmic rays is now nearly a century old, but most of the fundamental questions in this field remain unanswered, on the other hand the perspectives of future studies in the next decade are very bright. New detectors will provide…

Astrophysics · Physics 2009-11-07 Paolo Lipari

Multidimensional modification of gravity with a smaller mass scale of the gravitational interaction is considered. Stable by assumption dark matter particles could decay via interactions with virtual black holes. The decay rates of such…

High Energy Physics - Phenomenology · Physics 2023-12-12 E. V. Arbuzova , A. D. Dolgov , A. A. Nikitenko

Frequencies of volcanic eruptions in the past 270 years are compared with variations of solar activity and summary curve of principal components of the solar background magnetic field (SBMF).Frequency analysis with Morlet wavelet reveals…

Solar and Stellar Astrophysics · Physics 2022-08-10 I. Vasilieva , V. Zharkova

The maximum cosmic ray energy achievable by acceleration by a relativistic blast wave is derived. It is shown that forward shocks from long GRB in the interstellar medium are powerful enough to produce the Galactic cosmic-ray component up…

High Energy Astrophysical Phenomena · Physics 2015-05-27 David Eichler , Martin Pohl