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相关论文: The Chemical Composition of Cosmic Rays

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Recent results on the composition of cosmic rays in the energy region from about 10^14 to 10^18 eV are reviewed.

高能天体物理现象 · 物理学 2015-06-12 Joerg R. Hoerandel

Cosmic rays are relativistic particles that come to the Earth from outer space. Despite a great effort made in both experimental and theoretical research, their origin is still unknown. One of the main keys to understand their nature is the…

高能天体物理现象 · 物理学 2022-12-23 A. D. Supanitsky

The most recent experimental results on the cosmic ray composition and energy spectrum above 1 TeV are reviewed and discussed. All data agree on the presence of the so-called ``knee'' at an energy E(knee) = 3-4 PeV; the knee is seen in all…

天体物理学 · 物理学 2009-10-31 A. Castellina

Our knowledge of the mass composition of cosmic rays is deficient at all energies above 10^17. Here systematic differences between different measurements are discussed and, in particular, it is argued that there is no compelling evidence to…

天体物理学 · 物理学 2009-11-10 A. A. Watson

It is shown that our knowledge of the mass composition of cosmic rays is deficient at all energies above 10^17 eV. Systematic differences between different measurements are discussed and, in particular, it is argued that there is no…

天体物理学 · 物理学 2007-05-23 A. A. Watson

We briefly review the status of cosmic ray studies between $10^{14}$ eV and the highest observed energies, namely a few times $10^{20}$ eV. Because of the rather low incident fluxes in this energy range, the studies mostly rely on ground…

天体物理学 · 物理学 2009-10-31 Murat Boratav , Alan A. Watson

Investigations of the origin of cosmic rays are presented. Different methods are discussed: studies of cosmic gamma rays of energy from 30 MeV to about 10^15 eV (since photons point to their places of origin), studies of the mass…

天体物理学 · 物理学 2016-08-30 Jacek Szabelski

The energies of cosmic rays, fully ionized charged nuclei, extend over a wide range up to 10^20 eV. A particularly interesting energy region spans from 10^14 to 10^18 eV, where the all-particle energy spectrum exhibits two interesting…

天体物理学 · 物理学 2016-08-31 Joerg R. Hoerandel

Cosmic rays around the knee are generally believed to be of galactic origin. Observations on their energy spectrum and chemical composition are important for understanding the acceleration and propagation of these cosmic rays. In addition,…

高能天体物理现象 · 物理学 2017-03-01 Donghwa Kang

The small change in the spectral slope of the overall intensity of cosmic rays near 1 PeV may be associated with the endpoint energy of supernova shock acceleration. A crucial test of this connection and other ideas of the origin of the…

天体物理学 · 物理学 2011-05-23 S. P. Swordy , D. B. Kieda

This review summarizes recent developments in the understanding of high-energy cosmic rays. It focuses on galactic and presumably extragalactic particles in the energy range from the knee (10^15 eV) up to the highest energies observed…

高能天体物理现象 · 物理学 2009-10-06 J. Bluemer , R. Engel , J. R. Hoerandel

The present experimental status concerning the composition of cosmic rays in the PeV region is reviewed. The results are compared to predictions of contemporary models for the acceleration and propagation of galactic cosmic rays.

天体物理学 · 物理学 2009-11-10 Joerg R Hoerandel

Results from the KASCADE air shower experiment investigating the origin of cosmic rays in the energy region from 10^13 to 10^17 eV are presented. Attention is drawn on the investigation of interactions in the atmosphere and the energy…

天体物理学 · 物理学 2019-08-21 J. R. Hoerandel

Using the concept developed in earlier papers, that the cosmic rays originate in three different main sites, a) the normal supernova explosions into the interstellar medium, b) the supernova explosions into a stellar wind, and c) powerful…

天体物理学 · 物理学 2007-05-23 T. Stanev , P. L. Biermann , T. K. Gaisser

Arrival directions of extensive air showers by using world data are considered. It is found that the shower distribution in zenith angle at the energies E>10^{19} eV and E>4x10^{19} eV differs from each other. By our estimations, the shower…

天体物理学 · 物理学 2016-02-09 A. A. Mikhailov

Cosmic rays represent one of the most important energy transformation processes of the universe. They bring information about the surrounding universe, our galaxy, and very probably also the extragalactic space, at least at the highest…

高能天体物理现象 · 物理学 2022-02-24 G. Di Sciascio

The observation of a small change in spectral slope, or 'knee' in the fluxes of cosmic rays near energies 10^15 eV has caused much speculation since its discovery over 40 years ago. The origin of this feature remains unknown. A small…

Interpretation of the energy spectrum and arrival distribution of cosmic rays is complicated by lack of knowledge of the nature of the primaries. We review claims for the mass composition above 1017 eV where it can be determined only…

天体物理学 · 物理学 2007-05-23 M. T. Dova , A. A. Watson , A. G. Mariazzi

Cosmic rays are the highest energy particles found in nature. Measurements of the mass composition of cosmic rays between 10^{17} eV and 10^{18} eV are essential to understand whether this energy range is dominated by Galactic or…

高能天体物理现象 · 物理学 2016-05-03 S. Buitink , A. Corstanje , H. Falcke , J. R. Hörandel , T. Huege , A. Nelles , J. P. Rachen , L. Rossetto , P . Schellart , O. Scholten , S. ter Veen , S. Thoudam , T. N. G. Trinh , J. Anderson , A. Asgekar , I. M. Avruch , M. E. Bell , M. J. Bentum , G. Bernardi , P. Best , A. Bonafede , F. Breitling , J. W. Broderick , W. N. Brouw , M. Brüggen , H. R. Butcher , D. Carbone , B. Ciardi , J. E. Conway , F. de Gasperin , E. de Geus , A. Deller , R. -J. Dettmar , G. van Diepen , S. Duscha , J. Eislöffel , D. Engels , J. E. Enriquez , R. A. Fallows , R. Fender , C. Ferrari , W. Frieswijk , M. A. Garrett , J. M. Griessmeier , A. W. Gunst , M. P. van Haarlem , T. E. Hassall , G. Heald , J. W. T. Hessels , M. Hoeft , A. Horneffer , M. Iacobelli , H. Intema , E. Juette , A. Karastergiou , V. I. Kondratiev , M. Kramer , M. Kuniyoshi , G. Kuper , J. van Leeuwen , G. M. Loose , P. Maat , G. Mann , S. Markoff , R. McFadden , D. McKay-Bukowski , J. P. McKean , M. Mevius , D. D. Mulcahy , H. Munk , M. J. Norden , E. Orru , H. Paas , M. Pandey-Pommier , V. N. Pandey , M. Pietka , R. Pizzo , A. G. Polatidis , W. Reich , H. J. A. Röttgering , A. M. M. Scaife , D. J. Schwarz , M. Serylak , J. Sluman , O. Smirnov , B. W. Stappers , M. Steinmetz , A. Stewart , J. Swinbank , M. Tagger , Y. Tang , C. Tasse , M. C. Toribio , R. Vermeulen , C. Vocks , C. Vogt , R. J. van Weeren , R. A. M. J. Wijers , S. J. Wijnholds , M. W. Wise , O. Wucknitz , S. Yatawatta , P. Zarka , J. A. Zensus

A spectrum of cosmic rays within energy range 10^15 - 3x10^17 eV was derived from the data of the small Cherenkov setup, which is a part of the Yakutsk complex EAS array. In this, work a new series of observation is covered. These…

高能天体物理现象 · 物理学 2015-06-03 S. P. Knurenko , A. Sabourov
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