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AkademScholar

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Identifikatsiya

Ishlab chiquvchilar uchun

Ekotizim

Muassasalar

University of Catania

Nom variantlari: Università degli Studi di Catania · Universität Catania · Université de catane

Davlat:
IT
ROR:
https://ror.org/03a64bh57
8
h-indeks
644
Iqtiboslar
236
Asarlar
383
Mualliflar
Vaqt boʻyicha

Vaqt boʻyicha tahlil

Iqtibos sharhi

Yillar boʻyicha nashrlar (ustun) va iqtiboslar (chiziq)

  • Nashrlar
  • Iqtiboslar
0613192505010015020020172018201920202021202220232024202520262017: Nashrlar 10, Iqtiboslar 102018: Nashrlar 9, Iqtiboslar 392019: Nashrlar 7, Iqtiboslar 312020: Nashrlar 23, Iqtiboslar 242021: Nashrlar 16, Iqtiboslar 342022: Nashrlar 6, Iqtiboslar 502023: Nashrlar 10, Iqtiboslar 432024: Nashrlar 14, Iqtiboslar 842025: Nashrlar 24, Iqtiboslar 1372026: Nashrlar 10, Iqtiboslar 90

Iqtibos tarixi

05010015020020172018201920202021202220232024202520262017: Iqtiboslar 102018: Iqtiboslar 392019: Iqtiboslar 312020: Iqtiboslar 242021: Iqtiboslar 342022: Iqtiboslar 502023: Iqtiboslar 432024: Iqtiboslar 842025: Iqtiboslar 1372026: Iqtiboslar 90

Nashr tarixi

0613192520172018201920202021202220232024202520262017: Nashrlar 102018: Nashrlar 92019: Nashrlar 72020: Nashrlar 232021: Nashrlar 162022: Nashrlar 62023: Nashrlar 102024: Nashrlar 142025: Nashrlar 242026: Nashrlar 10

h-indeks evolyutsiyasi

Yillar boʻyicha jamlangan h-indeks

03581020172018201920202021202220232024202520262017: h-indeks 52018: h-indeks 52019: h-indeks 52020: h-indeks 52021: h-indeks 52022: h-indeks 52023: h-indeks 62024: h-indeks 62025: h-indeks 72026: h-indeks 8

Eng koʻp iqtibos qilingan asarlar

  1. Global and Regional IUCN Red List Assessments: 1620239 iqtibos
  2. Indirect determination of the astrophysical <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mi>S</mml:mi></mml:math> factor for the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mmultiscripts><mml:mi>Li</mml:mi><mml:mprescripts/><mml:none/><mml:mn>6</mml:mn></mml:mmultiscripts></mml:math>(<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mi>p</mml:mi><mml:mo>,</mml:mo><mml:mi>γ</mml:mi><mml:mo>)</mml:mo><mml:mmultiscripts><mml:mi>Be</mml:mi><mml:mprescripts/><mml:none/><mml:mn>7</mml:mn></mml:mmultiscripts></mml:mrow></mml:math> reaction using the asymptotic normalization coefficient method20218 iqtibos
  3. Global and Regional IUCN Red List Assessments: 1320228 iqtibos
  4. Global and Regional IUCN Red List Assessments: 1420227 iqtibos
  5. Astrophysical S-factor for the 3He(α,γ)7Be reaction via the asymptotic normalization coefficient (ANC) method20205 iqtibos
  6. The Relationship between Motivation and the Role of the Night of the Museums Event: Case Study in Oradea Municipality, Romania20235 iqtibos
  7. Data-driven estimation of the invisible energy of cosmic ray showers with the Pierre Auger Observatory20195 iqtibos
  8. 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
  9. Quasifission and fusion-fission processes in the reactions<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mmultiscripts><mml:mi>Kr</mml:mi><mml:mprescripts/><mml:none/><mml:mn>78</mml:mn></mml:mmultiscripts><mml:mo>+</mml:mo><mml:mmultiscripts><mml:mi>Ca</mml:mi><mml:mprescripts/><mml:none/><mml:mn>40</mml:mn></mml:mmultiscripts></mml:mrow></mml:math>and<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mmultiscripts><mml:mi>Kr</mml:mi><mml:mprescripts/><mml:none/><mml:mn>86</mml:mn></mml:mmultiscripts><mml:mo>+</mml:mo><mml:mmultiscripts><mml:mi>Ca</mml:mi><mml:mprescripts/><mml:none/><mml:mn>48</mml:mn></mml:mmultiscripts></mml:mrow></mml:math>at 10 MeV/nucleon bombarding energy20164 iqtibos
  10. 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