Shock Waves 1992
DOI: 10.1007/978-3-642-77648-9_45
|View full text |Cite
|
Sign up to set email alerts
|

Rayleigh-Taylor instability generated by rarefaction waves: Comparison with Richtmyer-Meshkov instability

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
1

Citation Types

0
1
0

Year Published

2010
2010
2013
2013

Publication Types

Select...
3

Relationship

0
3

Authors

Journals

citations
Cited by 3 publications
(1 citation statement)
references
References 5 publications
0
1
0
Order By: Relevance
“…In this problem, the flame length is the most crucial parameter defining the fuel consumption rate. Moreover, most of the existing R-M instability analysis is restricted to the shock refractions, while it is well known that expansion waves also produce an interface deformation similar to that of shocks [11]. Therefore, in this work we investigate the rates of interface increase following shock or expansion wave refractions in both types of refractions (fast/slow and slow/fast).…”
Section: Introductionmentioning
confidence: 99%
“…In this problem, the flame length is the most crucial parameter defining the fuel consumption rate. Moreover, most of the existing R-M instability analysis is restricted to the shock refractions, while it is well known that expansion waves also produce an interface deformation similar to that of shocks [11]. Therefore, in this work we investigate the rates of interface increase following shock or expansion wave refractions in both types of refractions (fast/slow and slow/fast).…”
Section: Introductionmentioning
confidence: 99%