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AkademScholar

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Identifikatsiya

Ishlab chiquvchilar uchun

Ekotizim

Muassasalar

State University of Campinas (UNICAMP)

Nom variantlari: Universidade Estadual de Campinas (UNICAMP) · UNICAMP · Universidade Estadual de Campinas · University of Campinas

Davlat:
BR
ROR:
https://ror.org/04wffgt70
12
h-indeks
979
Iqtiboslar
365
Asarlar
439
Mualliflar
Vaqt boʻyicha

Vaqt boʻyicha tahlil

Iqtibos sharhi

Yillar boʻyicha nashrlar (ustun) va iqtiboslar (chiziq)

  • Nashrlar
  • Iqtiboslar
01325385006312518825020172018201920202021202220232024202520262017: Nashrlar 12, Iqtiboslar 162018: Nashrlar 19, Iqtiboslar 162019: Nashrlar 19, Iqtiboslar 302020: Nashrlar 31, Iqtiboslar 442021: Nashrlar 21, Iqtiboslar 732022: Nashrlar 11, Iqtiboslar 952023: Nashrlar 23, Iqtiboslar 742024: Nashrlar 37, Iqtiboslar 1782025: Nashrlar 49, Iqtiboslar 2222026: Nashrlar 23, Iqtiboslar 127

Iqtibos tarixi

06312518825020172018201920202021202220232024202520262017: Iqtiboslar 162018: Iqtiboslar 162019: Iqtiboslar 302020: Iqtiboslar 442021: Iqtiboslar 732022: Iqtiboslar 952023: Iqtiboslar 742024: Iqtiboslar 1782025: Iqtiboslar 2222026: Iqtiboslar 127

Nashr tarixi

01325385020172018201920202021202220232024202520262017: Nashrlar 122018: Nashrlar 192019: Nashrlar 192020: Nashrlar 312021: Nashrlar 212022: Nashrlar 112023: Nashrlar 232024: Nashrlar 372025: Nashrlar 492026: Nashrlar 23

h-indeks evolyutsiyasi

Yillar boʻyicha jamlangan h-indeks

0510152020172018201920202021202220232024202520262017: h-indeks 42018: h-indeks 52019: h-indeks 52020: h-indeks 62021: h-indeks 82022: h-indeks 82023: h-indeks 92024: h-indeks 102025: h-indeks 122026: h-indeks 12

Eng koʻp iqtibos qilingan asarlar

  1. Data-driven estimation of the invisible energy of cosmic ray showers with the Pierre Auger Observatory20195 iqtibos
  2. Observation of a high-energy cosmic-ray family caused by a Centauro-type nuclear interaction in the joint emulsion chamber experiment at the Pamirs19874 iqtibos
  3. 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
  4. 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
  5. Three-Particle Coincidence of the Long Range Pseudorapidity Correlation in High Energy Nucleus-Nucleus Collisions20103 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. Observation of very high energy cosmic-ray families in emulsion chambers at high mountain altitudes (I)19923 iqtibos
  8. A 3‐Year Sample of Almost 1,600 Elves Recorded Above South America by the Pierre Auger Cosmic‐Ray Observatory20202 iqtibos
  9. <scp>IAPT</scp> chromosome data 3320202 iqtibos
  10. 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