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AkademScholar

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Identifikatsiya

Ishlab chiquvchilar uchun

Ekotizim

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Fluminense Federal University

Nom variantlari: Universidade Federal Fluminense · UFF

Davlat:
BR
ROR:
https://ror.org/02rjhbb08
7
h-indeks
343
Iqtiboslar
116
Asarlar
225
Mualliflar
Vaqt boʻyicha

Vaqt boʻyicha tahlil

Iqtibos sharhi

Yillar boʻyicha nashrlar (ustun) va iqtiboslar (chiziq)

  • Nashrlar
  • Iqtiboslar
05101520025507510020172018201920202021202220232024202520262017: Nashrlar 8, Iqtiboslar 82018: Nashrlar 12, Iqtiboslar 202019: Nashrlar 9, Iqtiboslar 152020: Nashrlar 14, Iqtiboslar 162021: Nashrlar 9, Iqtiboslar 142022: Nashrlar 6, Iqtiboslar 332023: Nashrlar 6, Iqtiboslar 222024: Nashrlar 3, Iqtiboslar 612025: Nashrlar 2, Iqtiboslar 972026: Nashrlar 1, Iqtiboslar 30

Iqtibos tarixi

025507510020172018201920202021202220232024202520262017: Iqtiboslar 82018: Iqtiboslar 202019: Iqtiboslar 152020: Iqtiboslar 162021: Iqtiboslar 142022: Iqtiboslar 332023: Iqtiboslar 222024: Iqtiboslar 612025: Iqtiboslar 972026: Iqtiboslar 30

Nashr tarixi

0510152020172018201920202021202220232024202520262017: Nashrlar 82018: Nashrlar 122019: Nashrlar 92020: Nashrlar 142021: Nashrlar 92022: Nashrlar 62023: Nashrlar 62024: Nashrlar 32025: Nashrlar 22026: Nashrlar 1

h-indeks evolyutsiyasi

Yillar boʻyicha jamlangan h-indeks

03581020172018201920202021202220232024202520262017: h-indeks 32018: h-indeks 42019: h-indeks 42020: h-indeks 42021: 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. Comprehensive analysis of high-lying states in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mmultiscripts><mml:mi mathvariant="normal">O</mml:mi><mml:mprescripts/><mml:none/><mml:mn>18</mml:mn></mml:mmultiscripts></mml:math> populated with <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>,</mml:mo><mml:mi>p</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math> and <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mo>(</mml:mo><mml:mmultiscripts><mml:mi mathvariant="normal">O</mml:mi><mml:mprescripts/><mml:none/><mml:mn>18</mml:mn></mml:mmultiscripts><mml:mo>,</mml:mo><mml:mmultiscripts><mml:mi mathvariant="normal">O</mml:mi><mml:mprescripts/><mml:none/><mml:mn>16</mml:mn></mml:mmultiscripts><mml:mo>)</mml:mo></mml:mrow></mml:math> reactions20174 iqtibos
  3. 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
  4. Two-neutron transfer analysis of the<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mmultiscripts><mml:mi mathvariant="normal">O</mml:mi><mml:mprescripts/><mml:none/><mml:mn>16</mml:mn></mml:mmultiscripts><mml:mo>(</mml:mo><mml:mmultiscripts><mml:mi mathvariant="normal">O</mml:mi><mml:mprescripts/><mml:none/><mml:mn>18</mml:mn></mml:mmultiscripts><mml:mo>,</mml:mo><mml:mmultiscripts><mml:mi mathvariant="normal">O</mml:mi><mml:mprescripts/><mml:none/><mml:mn>16</mml:mn></mml:mmultiscripts><mml:mo>)</mml:mo><mml:mmultiscripts><mml:mi mathvariant="normal">O</mml:mi><mml:mprescripts/><mml:none/><mml:mn>18</mml:mn></mml:mmultiscripts></mml:mrow></mml:math>reaction20163 iqtibos
  5. 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
  6. A 3‐Year Sample of Almost 1,600 Elves Recorded Above South America by the Pierre Auger Cosmic‐Ray Observatory20202 iqtibos
  7. A Search for Photons with Energies Above 2 × 1017 eV Using Hybrid Data from the Low-Energy Extensions of the Pierre Auger Observatory20222 iqtibos
  8. Analysis of proton and neutron pair breakings: High-spin structures of 124–127 Te isotopes20151 iqtibos
  9. Microscopically derived potential energy surfaces from mostly structural considerations20161 iqtibos
  10. Stability of BEC Systems in Nonlinear Optical Lattices20100 iqtibos