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AkademScholar

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National Institute for Nuclear Physics, Gran Sasso National Laboratories

Nom variantlari: Istituto Nazionale di Fisica Nucleare, Laboratori Nazionali del Gran Sasso · Gran Sasso National Laboratories · Gran Sasso National Laboratory · INFN Gran Sasso National Laboratories · INFN Laboratori Nazionali del Gran Sasso · INFN-LNGS · LNGS · Laboratori Nazionali del Gran Sasso

Davlat:
IT
ROR:
https://ror.org/02s8k0k61
10
h-indeks
534
Iqtiboslar
100
Asarlar
144
Mualliflar
Vaqt boʻyicha

Vaqt boʻyicha tahlil

Iqtibos sharhi

Yillar boʻyicha nashrlar (ustun) va iqtiboslar (chiziq)

  • Nashrlar
  • Iqtiboslar
0510152005010015020020172018201920202021202220232024202520262017: Nashrlar 11, Iqtiboslar 12018: Nashrlar 4, Iqtiboslar 82019: Nashrlar 9, Iqtiboslar 272020: Nashrlar 13, Iqtiboslar 212021: Nashrlar 7, Iqtiboslar 142022: Nashrlar 9, Iqtiboslar 492023: Nashrlar 6, Iqtiboslar 462024: Nashrlar 7, Iqtiboslar 802025: Nashrlar 8, Iqtiboslar 1592026: Nashrlar 5, Iqtiboslar 107

Iqtibos tarixi

05010015020020172018201920202021202220232024202520262017: Iqtiboslar 12018: Iqtiboslar 82019: Iqtiboslar 272020: Iqtiboslar 212021: Iqtiboslar 142022: Iqtiboslar 492023: Iqtiboslar 462024: Iqtiboslar 802025: Iqtiboslar 1592026: Iqtiboslar 107

Nashr tarixi

0510152020172018201920202021202220232024202520262017: Nashrlar 112018: Nashrlar 42019: Nashrlar 92020: Nashrlar 132021: Nashrlar 72022: Nashrlar 92023: Nashrlar 62024: Nashrlar 72025: Nashrlar 82026: Nashrlar 5

h-indeks evolyutsiyasi

Yillar boʻyicha jamlangan h-indeks

03581020172018201920202021202220232024202520262017: h-indeks 22018: h-indeks 32019: h-indeks 32020: h-indeks 42021: h-indeks 42022: h-indeks 52023: h-indeks 62024: h-indeks 72025: h-indeks 92026: h-indeks 10

Eng koʻp iqtibos qilingan asarlar

  1. Data-driven estimation of the invisible energy of cosmic ray showers with the Pierre Auger Observatory20195 iqtibos
  2. Testing hadronic-model predictions of depth of maximum of air-shower profiles and ground-particle signals using hybrid data of the Pierre Auger Observatory20243 iqtibos
  3. Inference of the Mass Composition of Cosmic Rays with Energies from <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:msup><mml:mn>10</mml:mn><mml:mn>18.5</mml:mn></mml:msup></mml:math> to <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:msup><mml:mrow><mml:mn>10</mml:mn></mml:mrow><mml:mrow><mml:mn>20</mml:mn></mml:mrow></mml:msup><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>eV</mml:mi></mml:mrow></mml:math> Using the Pierre Auger Observatory and Deep Learning20253 iqtibos
  4. Measurement of the depth of maximum of air-shower profiles with energies between <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:msup><mml:mn>10</mml:mn><mml:mn>18.5</mml:mn></mml:msup></mml:math> and <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:msup><mml:mn>10</mml:mn><mml:mn>20</mml:mn></mml:msup><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>eV</mml:mi></mml:math> using the surface detector of the Pierre Auger Observatory and deep learning20253 iqtibos
  5. A 3‐Year Sample of Almost 1,600 Elves Recorded Above South America by the Pierre Auger Cosmic‐Ray Observatory20202 iqtibos
  6. Energy Spectrum of Ultrahigh-Energy Cosmic Rays across Declinations <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"> <mml:mo>−</mml:mo> <mml:mn>9</mml:mn> <mml:mn>0</mml:mn> <mml:mi>°</mml:mi> </mml:math> to <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"> <mml:mo>+</mml:mo> <mml:mn>44.8</mml:mn> <mml:mi>°</mml:mi> </mml:math> as Measured at the Pierre Auger Observatory20252 iqtibos
  7. A Search for Photons with Energies Above 2 × 1017 eV Using Hybrid Data from the Low-Energy Extensions of the Pierre Auger Observatory20222 iqtibos
  8. Large-scale Cosmic-ray Anisotropies with 19 yr of Data from the Pierre Auger Observatory20241 iqtibos
  9. Nitrogen gas spillage in a confined space located in the Gran Sasso Underground Nuclear Physics Laboratory: an outstanding oxygen deficiency hazard case study20130 iqtibos
  10. Searches for Anisotropies in the Arrival Directions of the Highest Energy Cosmic Rays Detected by the Pierre Auger Observatory20150 iqtibos