Comptes Rendus
no. 4
Ultra-high-energy cosmic rays / Rayons cosmiques de ultra-haute énergie
Cosmic rays from the knee to the ankle
[Rayons cosmiques du genou à la cheville]
Mario Edoardo Bertaina1 
1 Department of Physics, University of Torino, Via Pietro Giuria, 1, 10125 Torino, Italy
Comptes Rendus. Physique, Ultra-high-energy cosmic rays: From the ankle to the tip of the spectrum, Volume 15 (2014) no. 4, pp. 300-308.

La forme et la composition du spectre des primaires ainsi que les anisotropies à grande échelle dans la distribution d'arrivée des rayons cosmiques sont des éléments clés pour comprendre l'origine, l'accélération et la propagation du rayonnement galactique. En dehors des particularités spectrales bien connues que sont le genou et la cheville, la mesure du spectre en énergie révèle également, entre ces deux particularités, une déviation claire, bien que moins prononcée, par rapport à une loi de puissance unique : le spectre se durcit jusqu'à ∼2×1016 eV et tombe ensuite à partir de ∼1017 eV. La composition en masse, quant à elle, devient plus lourde après le genou, et ce jusqu'à ∼1017 eV, valeur à partir de laquelle elle chute rapidement. Un durcissement de la composante légère au-dessus de 1017 eV a aussi été mesuré. De premières indications d'anisotropies dans les mesures des directions d'arrivée depuis l'hémisphère sud ont été rapportées à ∼1015 eV.

The shape and composition of the primary spectrum as well as the large-scale anisotropy in the arrival direction of cosmic rays are key elements to understand the origin, acceleration and propagation of the Galactic radiation. Besides the well-known knee and ankle features, the measured energy spectrum exhibits also a less pronounced but still clear deviation from a single power law between the knee and the ankle, with a spectral hardening at ∼2×1016 eV and a steepening at ∼1017 eV. The average mass composition gets heavier after the knee till ∼1017 eV, where a bending of the heavy component is observed. An indication of a hardening of the light component just above 1017 eV has been measured as well. First indications of anisotropy of the arrival direction in the southern hemisphere have been reported at ∼1015 eV.

Publié le :
DOI : 10.1016/j.crhy.2014.03.001
Keywords: Cosmic rays, Energy spectrum, Mass composition, Anisotropy, Knee, Ankle
Mots-clés : Rayons cosmiques, Spectre en énergie, Composition en masse, Anisotropies, Genou, Cheville

Mario Edoardo Bertaina 1

1 Department of Physics, University of Torino, Via Pietro Giuria, 1, 10125 Torino, Italy 
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Mario Edoardo Bertaina. Cosmic rays from the knee to the ankle. Comptes Rendus. Physique, Ultra-high-energy cosmic rays: From the ankle to the tip of the spectrum, Volume 15 (2014) no. 4, pp. 300-308. doi : 10.1016/j.crhy.2014.03.001. https://comptes-rendus.academie-sciences.fr/physique/articles/10.1016/j.crhy.2014.03.001/

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