Showing 5,501 - 5,520 results of 18,314 for search 'significantly ((((((mean decrease) OR (largest decrease))) OR (teer decrease))) OR (a decrease))', query time: 0.41s Refine Results
  1. 5501

    Outcomes of Sc onϕ(η). by Siva Sankari (2827295)

    Published 2025
    “…This study finds that the velocity of the fluid decreases with magnetic constraint intensification and time retardation. however, heat transfer increases at higher radiation, and heat absorption/emission parameters but decreases with a higher Prandtl number, while an increased Schmidt number leads to decreased concentration profiles. …”
  2. 5502

    Outcomes of K on . by Siva Sankari (2827295)

    Published 2025
    “…This study finds that the velocity of the fluid decreases with magnetic constraint intensification and time retardation. however, heat transfer increases at higher radiation, and heat absorption/emission parameters but decreases with a higher Prandtl number, while an increased Schmidt number leads to decreased concentration profiles. …”
  3. 5503

    Outcomes of <i>Ω</i> on . by Siva Sankari (2827295)

    Published 2025
    “…This study finds that the velocity of the fluid decreases with magnetic constraint intensification and time retardation. however, heat transfer increases at higher radiation, and heat absorption/emission parameters but decreases with a higher Prandtl number, while an increased Schmidt number leads to decreased concentration profiles. …”
  4. 5504

    Outcomes of Pe on . by Siva Sankari (2827295)

    Published 2025
    “…This study finds that the velocity of the fluid decreases with magnetic constraint intensification and time retardation. however, heat transfer increases at higher radiation, and heat absorption/emission parameters but decreases with a higher Prandtl number, while an increased Schmidt number leads to decreased concentration profiles. …”
  5. 5505

    HAM and Numerical solution for . by Siva Sankari (2827295)

    Published 2025
    “…This study finds that the velocity of the fluid decreases with magnetic constraint intensification and time retardation. however, heat transfer increases at higher radiation, and heat absorption/emission parameters but decreases with a higher Prandtl number, while an increased Schmidt number leads to decreased concentration profiles. …”
  6. 5506

    Outcomes of K on by Siva Sankari (2827295)

    Published 2025
    “…This study finds that the velocity of the fluid decreases with magnetic constraint intensification and time retardation. however, heat transfer increases at higher radiation, and heat absorption/emission parameters but decreases with a higher Prandtl number, while an increased Schmidt number leads to decreased concentration profiles. …”
  7. 5507

    Outcomes of Nt on by Siva Sankari (2827295)

    Published 2025
    “…This study finds that the velocity of the fluid decreases with magnetic constraint intensification and time retardation. however, heat transfer increases at higher radiation, and heat absorption/emission parameters but decreases with a higher Prandtl number, while an increased Schmidt number leads to decreased concentration profiles. …”
  8. 5508

    Variations of Pr and Ec to ). by Siva Sankari (2827295)

    Published 2025
    “…This study finds that the velocity of the fluid decreases with magnetic constraint intensification and time retardation. however, heat transfer increases at higher radiation, and heat absorption/emission parameters but decreases with a higher Prandtl number, while an increased Schmidt number leads to decreased concentration profiles. …”
  9. 5509

    HAM and Numerical solution for . by Siva Sankari (2827295)

    Published 2025
    “…This study finds that the velocity of the fluid decreases with magnetic constraint intensification and time retardation. however, heat transfer increases at higher radiation, and heat absorption/emission parameters but decreases with a higher Prandtl number, while an increased Schmidt number leads to decreased concentration profiles. …”
  10. 5510

    HAM and Numerical solution for . by Siva Sankari (2827295)

    Published 2025
    “…This study finds that the velocity of the fluid decreases with magnetic constraint intensification and time retardation. however, heat transfer increases at higher radiation, and heat absorption/emission parameters but decreases with a higher Prandtl number, while an increased Schmidt number leads to decreased concentration profiles. …”
  11. 5511

    HAM and Numerical solution for . by Siva Sankari (2827295)

    Published 2025
    “…This study finds that the velocity of the fluid decreases with magnetic constraint intensification and time retardation. however, heat transfer increases at higher radiation, and heat absorption/emission parameters but decreases with a higher Prandtl number, while an increased Schmidt number leads to decreased concentration profiles. …”
  12. 5512

    Outcomes of Sb on . by Siva Sankari (2827295)

    Published 2025
    “…This study finds that the velocity of the fluid decreases with magnetic constraint intensification and time retardation. however, heat transfer increases at higher radiation, and heat absorption/emission parameters but decreases with a higher Prandtl number, while an increased Schmidt number leads to decreased concentration profiles. …”
  13. 5513

    Diagram of the flow model. by Siva Sankari (2827295)

    Published 2025
    “…This study finds that the velocity of the fluid decreases with magnetic constraint intensification and time retardation. however, heat transfer increases at higher radiation, and heat absorption/emission parameters but decreases with a higher Prandtl number, while an increased Schmidt number leads to decreased concentration profiles. …”
  14. 5514

    HAM and Numerical solution for . by Siva Sankari (2827295)

    Published 2025
    “…This study finds that the velocity of the fluid decreases with magnetic constraint intensification and time retardation. however, heat transfer increases at higher radiation, and heat absorption/emission parameters but decreases with a higher Prandtl number, while an increased Schmidt number leads to decreased concentration profiles. …”
  15. 5515

    Variations of Sb and Pe to -χ�(0). by Siva Sankari (2827295)

    Published 2025
    “…This study finds that the velocity of the fluid decreases with magnetic constraint intensification and time retardation. however, heat transfer increases at higher radiation, and heat absorption/emission parameters but decreases with a higher Prandtl number, while an increased Schmidt number leads to decreased concentration profiles. …”
  16. 5516

    Outcomes of λ on . by Siva Sankari (2827295)

    Published 2025
    “…This study finds that the velocity of the fluid decreases with magnetic constraint intensification and time retardation. however, heat transfer increases at higher radiation, and heat absorption/emission parameters but decreases with a higher Prandtl number, while an increased Schmidt number leads to decreased concentration profiles. …”
  17. 5517

    Outcomes of Pr on by Siva Sankari (2827295)

    Published 2025
    “…This study finds that the velocity of the fluid decreases with magnetic constraint intensification and time retardation. however, heat transfer increases at higher radiation, and heat absorption/emission parameters but decreases with a higher Prandtl number, while an increased Schmidt number leads to decreased concentration profiles. …”
  18. 5518

    Outcomes of Ec on by Siva Sankari (2827295)

    Published 2025
    “…This study finds that the velocity of the fluid decreases with magnetic constraint intensification and time retardation. however, heat transfer increases at higher radiation, and heat absorption/emission parameters but decreases with a higher Prandtl number, while an increased Schmidt number leads to decreased concentration profiles. …”
  19. 5519

    Histogram of the area factorψ. by Hong Zhang (25820)

    Published 2025
    “…The measured <i>I</i><sub>s</sub> decreases following a power-law trend as <i>β</i> and <i>D</i> increase, with weathering reducing the sensitivity of <i>I</i><sub>s</sub> to <i>β</i> but not significantly altering its sensitivity to <i>D</i>. …”
  20. 5520

    Raw dataset Fig. 6. by Hong Zhang (25820)

    Published 2025
    “…The measured <i>I</i><sub>s</sub> decreases following a power-law trend as <i>β</i> and <i>D</i> increase, with weathering reducing the sensitivity of <i>I</i><sub>s</sub> to <i>β</i> but not significantly altering its sensitivity to <i>D</i>. …”