Asosiy kontentga oʻtish
AkademScholar

Kashfiyot

Xizmatlar

Identifikatsiya

Ishlab chiquvchilar uchun

Ekotizim

Muassasalar

Bariloche Atomic Centre

Nom variantlari: Centro Atómico Bariloche

Davlat:
AR
ROR:
https://ror.org/05m802881
7
h-indeks
286
Iqtiboslar
90
Asarlar
139
Mualliflar
Vaqt boʻyicha

Vaqt boʻyicha tahlil

Iqtibos sharhi

Yillar boʻyicha nashrlar (ustun) va iqtiboslar (chiziq)

  • Nashrlar
  • Iqtiboslar
03581005010015020020172018201920202021202220232024202520262017: Nashrlar 3, Iqtiboslar 32018: Nashrlar 2, Iqtiboslar 12019: Nashrlar 6, Iqtiboslar 162020: Nashrlar 7, Iqtiboslar 92021: Nashrlar 9, Iqtiboslar 92022: Nashrlar 3, Iqtiboslar 312023: Nashrlar 10, Iqtiboslar 92024: Nashrlar 4, Iqtiboslar 422025: Nashrlar 7, Iqtiboslar 1132026: Nashrlar 3, Iqtiboslar 31

Iqtibos tarixi

05010015020020172018201920202021202220232024202520262017: Iqtiboslar 32018: Iqtiboslar 12019: Iqtiboslar 162020: Iqtiboslar 92021: Iqtiboslar 92022: Iqtiboslar 312023: Iqtiboslar 92024: Iqtiboslar 422025: Iqtiboslar 1132026: Iqtiboslar 31

Nashr tarixi

03581020172018201920202021202220232024202520262017: Nashrlar 32018: Nashrlar 22019: Nashrlar 62020: Nashrlar 72021: Nashrlar 92022: Nashrlar 32023: Nashrlar 102024: Nashrlar 42025: Nashrlar 72026: Nashrlar 3

h-indeks evolyutsiyasi

Yillar boʻyicha jamlangan h-indeks

03581020172018201920202021202220232024202520262017: h-indeks 32018: h-indeks 32019: h-indeks 32020: h-indeks 32021: h-indeks 42022: h-indeks 42023: h-indeks 52024: h-indeks 52025: h-indeks 62026: h-indeks 7

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. The joint evaluated fission and fusion nuclear data library, JEFF-3.320202 iqtibos
  6. A 3‐Year Sample of Almost 1,600 Elves Recorded Above South America by the Pierre Auger Cosmic‐Ray Observatory20202 iqtibos
  7. 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
  8. A Search for Photons with Energies Above 2 × 1017 eV Using Hybrid Data from the Low-Energy Extensions of the Pierre Auger Observatory20222 iqtibos
  9. Large-scale Cosmic-ray Anisotropies with 19 yr of Data from the Pierre Auger Observatory20241 iqtibos
  10. A composition-informed search for large-scale anisotropy with the Pierre Auger Observatory20251 iqtibos