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Jiří Blažek

Ism variantlari: J. Blazek

Soʻnggi maʼlum muassasa:
FZU ‒ Institute of Physics of the Academy of Sciences of the Czech Republic
ORCID:
0000-0002-5870-8947
4
h-indeks
0
i10-indeksi
91
Iqtiboslar
36
Asarlar
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Iqtibos sharhi

Yillar boʻyicha nashrlar (ustun) va iqtiboslar (chiziq)

  • Nashrlar
  • Iqtiboslar
035810025507510020172018201920202021202220232024202520262017: Nashrlar 4, Iqtiboslar 02018: Nashrlar 1, Iqtiboslar 02019: Nashrlar 1, Iqtiboslar 22020: Nashrlar 5, Iqtiboslar 32021: Nashrlar 7, Iqtiboslar 02022: Nashrlar 2, Iqtiboslar 22023: Nashrlar 9, Iqtiboslar 02024: Nashrlar 2, Iqtiboslar 272025: Nashrlar 3, Iqtiboslar 572026: Nashrlar 1, Iqtiboslar 0

Iqtibos tarixi

025507510020172018201920202021202220232024202520262017: Iqtiboslar 02018: Iqtiboslar 02019: Iqtiboslar 22020: Iqtiboslar 32021: Iqtiboslar 02022: Iqtiboslar 22023: Iqtiboslar 02024: Iqtiboslar 272025: Iqtiboslar 572026: Iqtiboslar 0

Nashr tarixi

03581020172018201920202021202220232024202520262017: Nashrlar 42018: Nashrlar 12019: Nashrlar 12020: Nashrlar 52021: Nashrlar 72022: Nashrlar 22023: Nashrlar 92024: Nashrlar 22025: Nashrlar 32026: Nashrlar 1

h-indeks evolyutsiyasi

Yillar boʻyicha jamlangan h-indeks

0134520172018201920202021202220232024202520262017: h-indeks 02018: h-indeks 02019: h-indeks 12020: h-indeks 22021: h-indeks 22022: h-indeks 22023: h-indeks 22024: h-indeks 32025: h-indeks 42026: h-indeks 4

Eng koʻp iqtibos qilingan asarlar

  1. 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 Learning20252 iqtibos
  2. A 3‐Year Sample of Almost 1,600 Elves Recorded Above South America by the Pierre Auger Cosmic‐Ray Observatory20201 iqtibos
  3. Search for photons above <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>18</mml:mn></mml:mrow></mml:msup></mml:mrow><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>eV</mml:mi></mml:math> by simultaneously measuring the atmospheric depth and the muon content of air showers at the Pierre Auger Observatory20240 iqtibos
  4. Constraints on metastable superheavy dark matter coupled to sterile neutrinos with the Pierre Auger Observatory20240 iqtibos
  5. Search for the Anomalous Events Detected by ANITA Using the Pierre Auger Observatory20250 iqtibos
  6. 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 Observatory20250 iqtibos
  7. Search for Ultra-high-energy Neutrons from Galactic Sources with the Pierre Auger Observatory20260 iqtibos
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