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AkademScholar

Kashfiyot

Xizmatlar

Identifikatsiya

Ishlab chiquvchilar uchun

Ekotizim

Muassasalar

Colorado School of Mines

Nom variantlari: CSM

Davlat:
US
ROR:
https://ror.org/04raf6v53
6
h-indeks
276
Iqtiboslar
94
Asarlar
149
Mualliflar
Vaqt boʻyicha

Vaqt boʻyicha tahlil

Iqtibos sharhi

Yillar boʻyicha nashrlar (ustun) va iqtiboslar (chiziq)

  • Nashrlar
  • Iqtiboslar
05101520025507510020172018201920202021202220232024202520262017: Nashrlar 4, Iqtiboslar 12018: Nashrlar 4, Iqtiboslar 72019: Nashrlar 5, Iqtiboslar 72020: Nashrlar 6, Iqtiboslar 122021: Nashrlar 1, Iqtiboslar 232022: Nashrlar 5, Iqtiboslar 202023: Nashrlar 3, Iqtiboslar 262024: Nashrlar 5, Iqtiboslar 272025: Nashrlar 16, Iqtiboslar 592026: Nashrlar 4, Iqtiboslar 43

Iqtibos tarixi

025507510020172018201920202021202220232024202520262017: Iqtiboslar 12018: Iqtiboslar 72019: Iqtiboslar 72020: Iqtiboslar 122021: Iqtiboslar 232022: Iqtiboslar 202023: Iqtiboslar 262024: Iqtiboslar 272025: Iqtiboslar 592026: Iqtiboslar 43

Nashr tarixi

0510152020172018201920202021202220232024202520262017: Nashrlar 42018: Nashrlar 42019: Nashrlar 52020: Nashrlar 62021: Nashrlar 12022: Nashrlar 52023: Nashrlar 32024: Nashrlar 52025: Nashrlar 162026: Nashrlar 4

h-indeks evolyutsiyasi

Yillar boʻyicha jamlangan h-indeks

03581020172018201920202021202220232024202520262017: h-indeks 42018: h-indeks 42019: h-indeks 42020: h-indeks 42021: h-indeks 42022: h-indeks 52023: h-indeks 52024: h-indeks 52025: h-indeks 62026: h-indeks 6

Eng koʻp iqtibos qilingan asarlar

  1. Optimal Energy Scheduling of Load Demand with Two-Level Multi-objective Functions in Smart Electrical Grid20255 iqtibos
  2. 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
  3. 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
  4. 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
  5. 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
  6. Large-scale Cosmic-ray Anisotropies with 19 yr of Data from the Pierre Auger Observatory20241 iqtibos
  7. Measurement of the Inelastic Proton-Proton Cross-Section at $\sqrt{s} \geq 40$ TeV Using the Hybrid Data of the Pierre Auger Observatory20251 iqtibos
  8. Calibration and Performance of the Surface Scintillator Detector of the Pierre Auger Observatory20251 iqtibos
  9. Authors19750 iqtibos
  10. Neutron-transfer reaction studies with fission fragment radioactive ion beams near [sup 132]Sn20090 iqtibos