Shock Wave Dynamics and Its Effects on Planetary Atmospheres
A special issue of Atmosphere (ISSN 2073-4433). This special issue belongs to the section "Planetary Atmospheres".
Deadline for manuscript submissions: closed (15 February 2020) | Viewed by 5826
Special Issue Editor
2. The Institute for Earth and Space Exploration, Western University, London, ON N6A 3K7, Canada
Interests: space physics; meteor science; infrasound; impact cratering; small bodies in the solar system
Special Issues, Collections and Topics in MDPI journals
Special Issue Information
Dear Colleagues,
Shock waves result from a sudden energy release and propagate rapidly though the medium at velocities initially much higher than the local speed of sound. While the concept of shock wave generation and propagation in an atmospheric gas has been investigated for a long time in the context of military applications (e.g., chemical and nuclear explosions), the shockwave phenomena resulting from other sources have received somewhat less scientific attention. The study of shock waves and their effect on planetary atmospheres is of great relevance to many disciplines in the scientific community, such as atmospheric physics, space exploration, and planetary defence. For example, the shock waves generated by large meteoroids could have profound effects on not only the surrounding atmosphere, but also on the surface. In addition to studying shock waves in the Earth’s atmosphere, there is great interest in shock wave phenomena in other atmosphere-bearing worlds, such as Mars, Venus and Titan, especially in the context of future space missions. An additional utility is the meteoroid impact threat assessment for future colonies on Mars.
This Special Issue is focused on shock waves and their effects on planetary atmospheres, including shock wave generation, propagation and attenuation, as well as source localization and characterization. Observational, experimental and theoretical studies are welcome.
We invite researchers to contribute original research articles as well as review articles on the topic of shock wave phenomena in planetary atmospheres including but not limited to the following subtopics:
- Generation, propagation, and attenuation of shock waves resulting from natural and anthropogenic sources (e.g., meteoroids, lightning, solar storms and re-entry vehicles)
- Propagation and attenuation of weak shock (i.e., infrasound)
- The effects of ducting and atmospheric stratification, and wind on the propagation and attenuation of shock
- Source detection (direct and indirect methods), localization and characterization
- Physico-chemical effects on the local atmosphere
- Shock waves in extra-terrestrial atmospheres (e.g., Mars, Venus, Titan, Jupiter)
Dr. Elizabeth A. Silber
Guest Editor
Manuscript Submission Information
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Keywords
- Shock wave
- Propagation
- Attenuation
- Continuum flow
- Rarefied flow
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