Study of Large-Scale Vapor Explosions in Interaction of Fusible Metals with Water

2001 ◽  
Vol 32 (7-8) ◽  
pp. 7
Author(s):  
G. A. Kapinos ◽  
Yu. P. Meleshko ◽  
V. I. Nalivaev ◽  
O. V. Remizov ◽  
S. R. Kharitonov
Keyword(s):  
1979 ◽  
Vol 101 (2) ◽  
pp. 280-287 ◽  
Author(s):  
R. E. Henry ◽  
H. K. Fauske

A spontaneous nucleation model is proposed for the mechanisms which lead to explosive boiling in the free contacting mode. The model considers that spontaneous nucleation cannot occur until the thermal boundary layer is sufficiently thick to support a critical size vapor cavity, and that significant bubble growth requires an established pressure gradient in the cold liquid. This results in a prediction that, for an interface temperature above the spontaneous nucleation limit, large cold liquid droplets will remain in film boiling due to coalescence of vapor nuclei, whereas smaller droplets will be captured by the hot liquid surface and rapidly vaporize, which agrees with the experimental observations. The model also predicts that explosions are eliminated by an elevated system pressure or a supercritical contact interface temperature, and this is also in agreement with experimental data.


JOM ◽  
2021 ◽  
Author(s):  
Arne Simons ◽  
Inge Bellemans ◽  
Tijl Crivits ◽  
Kim Verbeken

1984 ◽  
Vol 106 (4) ◽  
pp. 728-734 ◽  
Author(s):  
M. Bu¨rger ◽  
D. S. Kim ◽  
W. Schwalbe ◽  
H. Unger ◽  
H. Hohmann ◽  
...  

Large-scale vapor explosions are described by thermal detonation waves, proceeding through a fuel-coolant mixture. A two-phase flow model is used for modeling the processes inside a wave. One phase is formed by the drops of melt and the other by the coolant and the fragments. For the interfacial transfer relations between the phases new descriptions are presented, which extend earlier thermal detonation models. The fragmentation behavior can be calculated from two different models, one based on deformation breakup and Taylor instability and another describing fragmentation by stripping of capillary waves induced by shear flow instabilities. In addition to the time development of the fragmented mass, the models give also the actual sizes of the fragments. Results of the fragmentation models are compared with the experiments on hydrodynamic fragmentation of single drops of gallium in water flows. For vapor explosion experiments with tin-water and salt-water systems the detonation cases are determined using the wave stripping model.


2002 ◽  
Vol 39 (8) ◽  
pp. 854-864 ◽  
Author(s):  
Yu MARUYAMA ◽  
Kiyofumi MORIYAMA ◽  
Hideo NAKAMURA

2004 ◽  
Vol 47 (2) ◽  
pp. 268-276
Author(s):  
Jie LIU ◽  
Seiichi KOSHIZUKA ◽  
Yoshiaki OKA

1987 ◽  
Vol 95 (3) ◽  
pp. 225-240 ◽  
Author(s):  
M. D. Oh ◽  
M. L. Corradini

1999 ◽  
Vol 173 ◽  
pp. 243-248
Author(s):  
D. Kubáček ◽  
A. Galád ◽  
A. Pravda

AbstractUnusual short-period comet 29P/Schwassmann-Wachmann 1 inspired many observers to explain its unpredictable outbursts. In this paper large scale structures and features from the inner part of the coma in time periods around outbursts are studied. CCD images were taken at Whipple Observatory, Mt. Hopkins, in 1989 and at Astronomical Observatory, Modra, from 1995 to 1998. Photographic plates of the comet were taken at Harvard College Observatory, Oak Ridge, from 1974 to 1982. The latter were digitized at first to apply the same techniques of image processing for optimizing the visibility of features in the coma during outbursts. Outbursts and coma structures show various shapes.


1994 ◽  
Vol 144 ◽  
pp. 29-33
Author(s):  
P. Ambrož

AbstractThe large-scale coronal structures observed during the sporadically visible solar eclipses were compared with the numerically extrapolated field-line structures of coronal magnetic field. A characteristic relationship between the observed structures of coronal plasma and the magnetic field line configurations was determined. The long-term evolution of large scale coronal structures inferred from photospheric magnetic observations in the course of 11- and 22-year solar cycles is described.Some known parameters, such as the source surface radius, or coronal rotation rate are discussed and actually interpreted. A relation between the large-scale photospheric magnetic field evolution and the coronal structure rearrangement is demonstrated.


Sign in / Sign up

Export Citation Format

Share Document