Temporal characteristics of shock-heated air radiation
- Авторлар: Bykova N.G.1, Kozlov P.V.1, Zabelinsky I.E.1, Gerasimov G.Y.1, Levashov V.Y.1
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Мекемелер:
- Lomonosov Moscow State University
- Шығарылым: Том 44, № 8 (2025)
- Беттер: 18-25
- Бөлім: Combustion, explosion and shock waves
- URL: https://consilium.orscience.ru/0207-401X/article/view/688995
- DOI: https://doi.org/10.31857/S0207401X25080021
- ID: 688995
Дәйексөз келтіру
Аннотация
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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Авторлар туралы
N. Bykova
Lomonosov Moscow State University
Хат алмасуға жауапты Автор.
Email: vyl69@mail.ru
Institute of Mechanics
Ресей, MoscowP. Kozlov
Lomonosov Moscow State University
Email: vyl69@mail.ru
Institute of Mechanics
Ресей, MoscowI. Zabelinsky
Lomonosov Moscow State University
Email: vyl69@mail.ru
Institute of Mechanics
Ресей, MoscowG. Gerasimov
Lomonosov Moscow State University
Email: vyl69@mail.ru
Institute of Mechanics
Ресей, MoscowV. Levashov
Lomonosov Moscow State University
Email: vyl69@mail.ru
Institute of Mechanics
Ресей, MoscowӘдебиет тізімі
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