Fizika Goreniya i Vzryva
RUS  ENG    JOURNALS   PEOPLE   ORGANISATIONS   CONFERENCES   SEMINARS   VIDEO LIBRARY   PACKAGE AMSBIB  
General information
Latest issue
Archive

Search papers
Search references

RSS
Latest issue
Current issues
Archive issues
What is RSS



Fizika Goreniya i Vzryva:
Year:
Volume:
Issue:
Page:
Find






Personal entry:
Login:
Password:
Save password
Enter
Forgotten password?
Register


Fizika Goreniya i Vzryva, 2020, Volume 56, Issue 4, Pages 5–13
DOI: https://doi.org/10.15372/FGV20200401
(Mi fgv690)
 

This article is cited in 4 scientific papers (total in 4 papers)

Radiative fraction and flame length of propane jet diffusion flames in a crossflow

J.-W. Wangab, J. Fanga, J.-F. Guanb, L.-Y. Zhaoa, S.-B. Lina, H. R. Shaha, Y.-M. Zhanga, J.-H. Suna

a University of Science and Technology of China, 230026, Hefei, Anhui, China
b Tsinghua University, 230601, Hefei, Anhui, China
Full-text PDF (494 kB) Citations (4)
Abstract: Many industrial combustion devices rely on jet flame combustion in the crossflow to achieve mixing and reaction. Previous research offers a limited predictive capability regarding the coupling effects of the crossflow and jet flow on the flame radiative fraction. In this work, a new theoretical equation is derived to relate the radiative fraction to the fuel flow rate and the crossflow velocity. The experimental results show that the flame length increases as the crossflow velocity increases for all considered flames. The results of this work suggest that the stretching factor is 0.08 s. The radiative fraction is almost independent of the nozzle diameter in the case of a low crossflow velocity. The crossflow has the strongest effect on the radiative fraction for a smaller nozzle diameter. This is because of the effect of the crossflow and jet flow velocities on the soot residence time, which is proportional to the radiative fraction.
Keywords: crossflow, propane, radiative fraction, soot, turbulent diffusion flame.
Funding agency Grant number
National Natural Science Foundation of China 51636008
51576186
National Key Research and Development Program of China 2016YFC0801500
National Natural Science Foundation of China
Chinese Academy of Sciences QYZDB-SSW-JSC029
Fundamental Research Funds for the Central Universities of China WK2320000042
WK2320000036
Anhui Provincial Natural Science Foundation 1908085QE205
State Key Laboratory of Fire Science HZ2020-KF12
Received: 09.01.2020
Revised: 19.02.2020
English version:
Combustion, Explosion and Shock Waves, 2020, Volume 56, Issue 4, Pages 375–382
DOI: https://doi.org/10.1134/S0010508220040012
Bibliographic databases:
Document Type: Article
UDC: 536.46
Language: Russian
Citation: J.-W. Wang, J. Fang, J.-F. Guan, L.-Y. Zhao, S.-B. Lin, H. R. Shah, Y.-M. Zhang, J.-H. Sun, “Radiative fraction and flame length of propane jet diffusion flames in a crossflow”, Fizika Goreniya i Vzryva, 56:4 (2020), 5–13; Combustion, Explosion and Shock Waves, 56:4 (2020), 375–382
Citation in format AMSBIB
\Bibitem{WanFanGua20}
\by J.-W.~Wang, J.~Fang, J.-F.~Guan, L.-Y.~Zhao, S.-B.~Lin, H.~R.~Shah, Y.-M.~Zhang, J.-H.~Sun
\paper Radiative fraction and flame length of propane jet diffusion flames in a crossflow
\jour Fizika Goreniya i Vzryva
\yr 2020
\vol 56
\issue 4
\pages 5--13
\mathnet{http://mi.mathnet.ru/fgv690}
\crossref{https://doi.org/10.15372/FGV20200401}
\elib{https://elibrary.ru/item.asp?id=43152521}
\transl
\jour Combustion, Explosion and Shock Waves
\yr 2020
\vol 56
\issue 4
\pages 375--382
\crossref{https://doi.org/10.1134/S0010508220040012}
Linking options:
  • https://www.mathnet.ru/eng/fgv690
  • https://www.mathnet.ru/eng/fgv/v56/i4/p5
  • This publication is cited in the following 4 articles:
    Citing articles in Google Scholar: Russian citations, English citations
    Related articles in Google Scholar: Russian articles, English articles
    Fizika Goreniya i Vzryva Fizika Goreniya i Vzryva
    Statistics & downloads:
    Abstract page:24
    Full-text PDF :4
     
      Contact us:
     Terms of Use  Registration to the website  Logotypes © Steklov Mathematical Institute RAS, 2024