Asosiy kontentga oʻtish
AkademScholar
Muassasalar

Polytechnic University of Milan

Nom variantlari: Politecnico di Milano · École Polytechnique de Milan

Davlat:
IT
ROR:
https://ror.org/01nffqt88
8
h-indeks
693
Iqtiboslar
283
Asarlar
371
Mualliflar
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Vaqt boʻyicha tahlil

Iqtibos sharhi

Yillar boʻyicha nashrlar (ustun) va iqtiboslar (chiziq)

  • Nashrlar
  • Iqtiboslar
01325385005010015020020172018201920202021202220232024202520262017: Nashrlar 10, Iqtiboslar 102018: Nashrlar 24, Iqtiboslar 142019: Nashrlar 21, Iqtiboslar 202020: Nashrlar 17, Iqtiboslar 302021: Nashrlar 20, Iqtiboslar 342022: Nashrlar 16, Iqtiboslar 432023: Nashrlar 23, Iqtiboslar 962024: Nashrlar 9, Iqtiboslar 1232025: Nashrlar 32, Iqtiboslar 1572026: Nashrlar 19, Iqtiboslar 86

Iqtibos tarixi

05010015020020172018201920202021202220232024202520262017: Iqtiboslar 102018: Iqtiboslar 142019: Iqtiboslar 202020: Iqtiboslar 302021: Iqtiboslar 342022: Iqtiboslar 432023: Iqtiboslar 962024: Iqtiboslar 1232025: Iqtiboslar 1572026: Iqtiboslar 86

Nashr tarixi

01325385020172018201920202021202220232024202520262017: Nashrlar 102018: Nashrlar 242019: Nashrlar 212020: Nashrlar 172021: Nashrlar 202022: Nashrlar 162023: Nashrlar 232024: Nashrlar 92025: Nashrlar 322026: Nashrlar 19

h-indeks evolyutsiyasi

Yillar boʻyicha jamlangan h-indeks

03581020172018201920202021202220232024202520262017: h-indeks 42018: h-indeks 42019: h-indeks 52020: h-indeks 52021: h-indeks 52022: h-indeks 62023: h-indeks 72024: h-indeks 72025: h-indeks 72026: h-indeks 8

Eng koʻp iqtibos qilingan asarlar

  1. Rapid quasi-periodic oscillations in the relativistic jet of BL Lacertae20227 iqtibos
  2. Data-driven estimation of the invisible energy of cosmic ray showers with the Pierre Auger Observatory20195 iqtibos
  3. The optical behaviour of BL Lacertae at its maximum brightness levels: a blend of geometry and energetics20233 iqtibos
  4. 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
  5. 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
  6. 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
  7. A 3‐Year Sample of Almost 1,600 Elves Recorded Above South America by the Pierre Auger Cosmic‐Ray Observatory20202 iqtibos
  8. 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
  9. A Search for Photons with Energies Above 2 × 1017 eV Using Hybrid Data from the Low-Energy Extensions of the Pierre Auger Observatory20222 iqtibos
  10. Measurement of the Inelastic Proton-Proton Cross-Section at $\sqrt{s} \geq 40$ TeV Using the Hybrid Data of the Pierre Auger Observatory20251 iqtibos