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AkademScholar

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Identifikatsiya

Ishlab chiquvchilar uchun

Ekotizim

Muassasalar

Institute of Nuclear Physics, Polish Academy of Sciences

Nom variantlari: Henryk Niewodniczański Institute of Nuclear Physics · Instytut Fizyki Jądrowej im. Henryka Niewodniczańskiego

Davlat:
PL
ROR:
https://ror.org/01n78t774
10
h-indeks
699
Iqtiboslar
398
Asarlar
539
Mualliflar
Vaqt boʻyicha

Vaqt boʻyicha tahlil

Iqtibos sharhi

Yillar boʻyicha nashrlar (ustun) va iqtiboslar (chiziq)

  • Nashrlar
  • Iqtiboslar
01325385005010015020020172018201920202021202220232024202520262017: Nashrlar 12, Iqtiboslar 72018: Nashrlar 14, Iqtiboslar 122019: Nashrlar 15, Iqtiboslar 212020: Nashrlar 19, Iqtiboslar 202021: Nashrlar 30, Iqtiboslar 312022: Nashrlar 13, Iqtiboslar 742023: Nashrlar 15, Iqtiboslar 482024: Nashrlar 15, Iqtiboslar 912025: Nashrlar 25, Iqtiboslar 1262026: Nashrlar 12, Iqtiboslar 67

Iqtibos tarixi

05010015020020172018201920202021202220232024202520262017: Iqtiboslar 72018: Iqtiboslar 122019: Iqtiboslar 212020: Iqtiboslar 202021: Iqtiboslar 312022: Iqtiboslar 742023: Iqtiboslar 482024: Iqtiboslar 912025: Iqtiboslar 1262026: Iqtiboslar 67

Nashr tarixi

01325385020172018201920202021202220232024202520262017: Nashrlar 122018: Nashrlar 142019: Nashrlar 152020: Nashrlar 192021: Nashrlar 302022: Nashrlar 132023: Nashrlar 152024: Nashrlar 152025: Nashrlar 252026: Nashrlar 12

h-indeks evolyutsiyasi

Yillar boʻyicha jamlangan h-indeks

03581020172018201920202021202220232024202520262017: h-indeks 52018: h-indeks 62019: h-indeks 62020: h-indeks 62021: h-indeks 62022: h-indeks 62023: h-indeks 72024: h-indeks 82025: h-indeks 92026: h-indeks 10

Eng koʻp iqtibos qilingan asarlar

  1. Charged-particle multiplicity and angular distributions in proton-emulsion interactions at 800 GeV19876 iqtibos
  2. Effects of t- and α-transfer on the spectroscopic information from the reaction20135 iqtibos
  3. Data-driven estimation of the invisible energy of cosmic ray showers with the Pierre Auger Observatory20195 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. A 3‐Year Sample of Almost 1,600 Elves Recorded Above South America by the Pierre Auger Cosmic‐Ray Observatory20202 iqtibos
  6. Applications of nanodosimetry in particle therapy planning and beyond20212 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. Physics Performance Report for PANDA: Strong Interaction Studies with Antiprotons20091 iqtibos
  9. Selenium Supplementation of Amaranth Sprouts Influences Betacyanin Content and Improves Anti-Inflammatory Properties via NFκB in Murine RAW 264.7 Macrophages20151 iqtibos
  10. Complex analysis of scattering 1p-shell nuclei in the framework of coupled channel method20161 iqtibos