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Identifikatsiya

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Ekotizim

Mualliflar

A. Almela

Soʻnggi maʼlum muassasa:
National Technological University
ORCID:
0000-0003-1233-2670
6
h-indeks
1
i10-indeksi
97
Iqtiboslar
30
Asarlar
Vaqt boʻyicha

Vaqt boʻyicha tahlil

Iqtibos sharhi

Yillar boʻyicha nashrlar (ustun) va iqtiboslar (chiziq)

  • Nashrlar
  • Iqtiboslar
03581001325385020172018201920202021202220232024202520262017: Nashrlar 2, Iqtiboslar 02018: Nashrlar 1, Iqtiboslar 02019: Nashrlar 1, Iqtiboslar 72020: Nashrlar 2, Iqtiboslar 22021: Nashrlar 3, Iqtiboslar 02022: Nashrlar 1, Iqtiboslar 182023: Nashrlar 2, Iqtiboslar 22024: Nashrlar 4, Iqtiboslar 182025: Nashrlar 8, Iqtiboslar 362026: Nashrlar 1, Iqtiboslar 14

Iqtibos tarixi

01325385020172018201920202021202220232024202520262017: Iqtiboslar 02018: Iqtiboslar 02019: Iqtiboslar 72020: Iqtiboslar 22021: Iqtiboslar 02022: Iqtiboslar 182023: Iqtiboslar 22024: Iqtiboslar 182025: Iqtiboslar 362026: Iqtiboslar 14

Nashr tarixi

03581020172018201920202021202220232024202520262017: Nashrlar 22018: Nashrlar 12019: Nashrlar 12020: Nashrlar 22021: Nashrlar 32022: Nashrlar 12023: Nashrlar 22024: Nashrlar 42025: Nashrlar 82026: Nashrlar 1

h-indeks evolyutsiyasi

Yillar boʻyicha jamlangan h-indeks

03581020172018201920202021202220232024202520262017: h-indeks 02018: h-indeks 02019: h-indeks 22020: h-indeks 22021: h-indeks 22022: h-indeks 32023: h-indeks 32024: h-indeks 42025: h-indeks 62026: h-indeks 6

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. Large-scale Cosmic-ray Anisotropies with 19 yr of Data from the Pierre Auger Observatory20241 iqtibos
  8. Measurement of the Inelastic Proton-Proton Cross-Section at $\sqrt{s} \geq 40$ TeV Using the Hybrid Data of the Pierre Auger Observatory20251 iqtibos
  9. AugerPrime: Status and first results20251 iqtibos
  10. Search for photons above <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>18</mml:mn></mml:mrow></mml:msup></mml:mrow><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>eV</mml:mi></mml:math> by simultaneously measuring the atmospheric depth and the muon content of air showers at the Pierre Auger Observatory20240 iqtibos

Hammualliflar

Yana 15 ta asar katta kollaboratsiyada (50 dan ortiq muallif) — hammualliflar roʻyxatiga kiritilmagan

Skelet yozuvlar: 15 — katta kollaboratsiyada (50 dan ortiq muallif), hammualliflar roʻyxatiga kiritilmagan

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