Zenith angle distribution of cosmic ray showers measured with the Yakutsk array

Иванов, А. А.

doi:10.22323/1.301.0550

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Ta 9-year Spectrum2

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2017

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(2 citation statements)

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“…We divided the SD data set into two, of higher declination (δ > 26 • ) and lower declination (δ < 26 • ) bands [19]. The lower-declination energy spectrum for δ < 26 • is in good agreement with the Auger data of the same declination band allowing an energy shift within the uncertainties quoted by the both experiments [20]. Note that the TA "hotspot" is not included in this region [21].…”

Section: Ta 9-year Spectrummentioning

confidence: 99%

See 1 more Smart Citation

Energy Spectrum of Ultra-High-Energy Cosmic Rays Measured by The Telescope Array

Tsunesada¹,

Abu‐Zayyad²,

Ivanov³

et al. 2017

Proceedings of 35th International Cosmic Ray Conference — PoS(ICRC2017)

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The Telescope Array (TA) is a hybrid cosmic ray detector using air fluorescence detectors (FDs) and an array of surface detectors (SDs) which covers 700 km 2 in Utah. The TA Low-energy Extension (TALE) also consists of FDs with larger elevation angles and an infill SD array with 400 m spacing, which extends the observable energy range down to 4 PeV. In this contribution we present the spectrum from the TA SD, which has the largest statistics, the FD monocular spectrum, the FD-SD hybrid spectrum, and the lower energy spectrum obtained by TALE. We discuss the declination dependence of the energy spectrum in the northern sky.

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Section: Ta 9-year Spectrummentioning

confidence: 99%

“…However we found different suppression energies in the two bands, 10 19.59±0.06 eV for δ < 26 • and 10 19.85±0.03 eV for δ > 26 • . This is a hint of spectrum anisotropy of cosmic rays in the northern and southern skies [19,22,23] PoS(ICRC2017)535 …”

Section: Ta 9-year Spectrummentioning

confidence: 99%