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AkademScholar

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Ekotizim

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University of Naples Federico II

Nom variantlari: Universitat de Nàpols Frederic II · Università degli Studi di Napoli Federico II · Universität Neapel Federico II · Université de Naples - Frédéric-II

Davlat:
IT
ROR:
https://ror.org/05290cv24
15
h-indeks
1,473
Iqtiboslar
418
Asarlar
589
Mualliflar
Vaqt boʻyicha

Vaqt boʻyicha tahlil

Iqtibos sharhi

Yillar boʻyicha nashrlar (ustun) va iqtiboslar (chiziq)

  • Nashrlar
  • Iqtiboslar
013253850012525037550020172018201920202021202220232024202520262017: Nashrlar 24, Iqtiboslar 62018: Nashrlar 17, Iqtiboslar 272019: Nashrlar 23, Iqtiboslar 282020: Nashrlar 26, Iqtiboslar 322021: Nashrlar 36, Iqtiboslar 722022: Nashrlar 19, Iqtiboslar 892023: Nashrlar 25, Iqtiboslar 1652024: Nashrlar 32, Iqtiboslar 2672025: Nashrlar 45, Iqtiboslar 3722026: Nashrlar 23, Iqtiboslar 293

Iqtibos tarixi

012525037550020172018201920202021202220232024202520262017: Iqtiboslar 62018: Iqtiboslar 272019: Iqtiboslar 282020: Iqtiboslar 322021: Iqtiboslar 722022: Iqtiboslar 892023: Iqtiboslar 1652024: Iqtiboslar 2672025: Iqtiboslar 3722026: Iqtiboslar 293

Nashr tarixi

01325385020172018201920202021202220232024202520262017: Nashrlar 242018: Nashrlar 172019: Nashrlar 232020: Nashrlar 262021: Nashrlar 362022: Nashrlar 192023: Nashrlar 252024: Nashrlar 322025: Nashrlar 452026: Nashrlar 23

h-indeks evolyutsiyasi

Yillar boʻyicha jamlangan h-indeks

0510152020172018201920202021202220232024202520262017: h-indeks 52018: h-indeks 52019: h-indeks 52020: h-indeks 52021: h-indeks 62022: h-indeks 72023: h-indeks 92024: h-indeks 102025: h-indeks 132026: h-indeks 15

Eng koʻp iqtibos qilingan asarlar

  1. Decay of excited nuclei produced in<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mmultiscripts><mml:mi mathvariant="normal">Kr</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>78</mml:mn><mml:mo>,</mml:mo><mml:mn>82</mml:mn></mml:mrow></mml:mmultiscripts></mml:math><mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mo>+</mml:mo></mml:mrow></mml:math><mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mmultiscripts><mml:mi mathvariant="normal">Ca</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>40</mml:mn></mml:mrow></mml:mmultiscripts></mml:math>reactions at 5.5 MeV/nucleon201113 iqtibos
  2. Data-driven estimation of the invisible energy of cosmic ray showers with the Pierre Auger Observatory20195 iqtibos
  3. Decay of excited nuclei produced in the<sup>78,82</sup>Kr+<sup>40</sup>Ca reactions at 5.5 MeV/nucleon20114 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. The persistent shadow of the supermassive black hole of M8720253 iqtibos
  6. 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
  7. 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
  8. A 3‐Year Sample of Almost 1,600 Elves Recorded Above South America by the Pierre Auger Cosmic‐Ray Observatory20202 iqtibos
  9. 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
  10. Gravitational wave astronomy with TianQin20252 iqtibos