Temporal characteristics of shock-heated air radiation
- 作者: Bykova N.G.1, Kozlov P.V.1, Zabelinsky I.E.1, Gerasimov G.Y.1, Levashov V.Y.1
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隶属关系:
- Lomonosov Moscow State University
- 期: 卷 44, 编号 8 (2025)
- 页面: 18-25
- 栏目: Combustion, explosion and shock waves
- URL: https://ter-arkhiv.ru/0207-401X/article/view/688995
- DOI: https://doi.org/10.31857/S0207401X25080021
- ID: 688995
如何引用文章
详细
The paper presents the results of measuring the time spectrograms of shock-heated air radiation obtained on the STS-M and DDST-M shock tubes of the Institute of Mechanics (Moscow State University) using an integral method that records the time evolution of radiation passing through the measuring section of the shock tubes in narrow spectral ranges specially selected using monochromators. The measurements were performed for atomic lines and molecular bands in the wavelength range from vacuum ultraviolet to infrared radiation at an initial pressure before the shock wave of 0.25 Torr and shock wave velocities from 7.8 to 11.0 km/s. The obtained results are compared with the experimental data of other authors.
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作者简介
N. Bykova
Lomonosov Moscow State University
编辑信件的主要联系方式.
Email: vyl69@mail.ru
Institute of Mechanics
俄罗斯联邦, MoscowP. Kozlov
Lomonosov Moscow State University
Email: vyl69@mail.ru
Institute of Mechanics
俄罗斯联邦, MoscowI. Zabelinsky
Lomonosov Moscow State University
Email: vyl69@mail.ru
Institute of Mechanics
俄罗斯联邦, MoscowG. Gerasimov
Lomonosov Moscow State University
Email: vyl69@mail.ru
Institute of Mechanics
俄罗斯联邦, MoscowV. Levashov
Lomonosov Moscow State University
Email: vyl69@mail.ru
Institute of Mechanics
俄罗斯联邦, Moscow参考
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