Language:
English
繁體中文
Help
回圖書館首頁
手機版館藏查詢
Login
Back
Switch To:
Labeled
|
MARC Mode
|
ISBD
Hydrodynamic Simulations of Ejecta P...
~
Karkhanis, Varad Abhimanyu.
Linked to FindBook
Google Book
Amazon
博客來
Hydrodynamic Simulations of Ejecta Production From Shocked Metallic Surfaces.
Record Type:
Electronic resources : Monograph/item
Title/Author:
Hydrodynamic Simulations of Ejecta Production From Shocked Metallic Surfaces./
Author:
Karkhanis, Varad Abhimanyu.
Published:
Ann Arbor : ProQuest Dissertations & Theses, : 2017,
Description:
108 p.
Notes:
Source: Dissertation Abstracts International, Volume: 79-01(E), Section: B.
Contained By:
Dissertation Abstracts International79-01B(E).
Subject:
Mechanical engineering. -
Online resource:
http://pqdd.sinica.edu.tw/twdaoapp/servlet/advanced?query=10607383
ISBN:
9780355132878
Hydrodynamic Simulations of Ejecta Production From Shocked Metallic Surfaces.
Karkhanis, Varad Abhimanyu.
Hydrodynamic Simulations of Ejecta Production From Shocked Metallic Surfaces.
- Ann Arbor : ProQuest Dissertations & Theses, 2017 - 108 p.
Source: Dissertation Abstracts International, Volume: 79-01(E), Section: B.
Thesis (Ph.D.)--The University of North Carolina at Charlotte, 2017.
The phenomenon of mass ejection into vacuum from a shocked metallic free surfaces can have a deleterious effect on the implosion phase of the Inertial Confinement Fusion (ICF) process. Often, the ejecta take the form of a cloud of particles that are the result of microjetting sourced from imperfections on the metallic free surface. Significant progress has been achieved in the understanding of ejecta dynamics by treating the process as a limiting case of the baroclinically-driven Richtmyer-Meshkov Instability (RMI). This conceptual picture is complicated by several practical considerations including breakup of spikes due to surface tension and yield strength of the metal. Thus, the problem involves a wide range of physical phenomena, occurring often under extreme conditions of material behavior.
ISBN: 9780355132878Subjects--Topical Terms:
649730
Mechanical engineering.
Hydrodynamic Simulations of Ejecta Production From Shocked Metallic Surfaces.
LDR
:02984nmm a2200325 4500
001
2160449
005
20180727091502.5
008
190424s2017 ||||||||||||||||| ||eng d
020
$a
9780355132878
035
$a
(MiAaPQ)AAI10607383
035
$a
(MiAaPQ)uncc:11488
035
$a
AAI10607383
040
$a
MiAaPQ
$c
MiAaPQ
100
1
$a
Karkhanis, Varad Abhimanyu.
$3
3348369
245
1 0
$a
Hydrodynamic Simulations of Ejecta Production From Shocked Metallic Surfaces.
260
1
$a
Ann Arbor :
$b
ProQuest Dissertations & Theses,
$c
2017
300
$a
108 p.
500
$a
Source: Dissertation Abstracts International, Volume: 79-01(E), Section: B.
500
$a
Adviser: Praveen Ramaprabhu.
502
$a
Thesis (Ph.D.)--The University of North Carolina at Charlotte, 2017.
520
$a
The phenomenon of mass ejection into vacuum from a shocked metallic free surfaces can have a deleterious effect on the implosion phase of the Inertial Confinement Fusion (ICF) process. Often, the ejecta take the form of a cloud of particles that are the result of microjetting sourced from imperfections on the metallic free surface. Significant progress has been achieved in the understanding of ejecta dynamics by treating the process as a limiting case of the baroclinically-driven Richtmyer-Meshkov Instability (RMI). This conceptual picture is complicated by several practical considerations including breakup of spikes due to surface tension and yield strength of the metal. Thus, the problem involves a wide range of physical phenomena, occurring often under extreme conditions of material behavior.
520
$a
We describe an approach in which continuum simulations using ideal gases can be used to capture key aspects of ejecta growth associated with the RMI. The approach exploits the analogy between the Rankine-Hugoniot jump conditions for ideal gases and the linear relationship between the shock velocity and particle velocity governing shocked metals. Such simulations with Upsilon-law fluids have been successful in accurately predicting the velocity and mass of ejecta for different shapes, and in excellent agreement with experiments. We use the astrophysical FLASH code, developed at the University of Chicago to model this problem. Based on insights from our simulations, we suggest a modified expression for ejecta velocities that is valid for large initial perturbation amplitudes. The expression for velocities is extended to ejecta originating from cavities with any arbitrary shape. The simulations are also used to validate a recently proposed source model for ejecta that predicts the ejected mass per unit area for sinusoidal and non-standard shapes. Such simulations and theoretical models play an important role in the design of target experiment campaigns.
590
$a
School code: 0694.
650
4
$a
Mechanical engineering.
$3
649730
650
4
$a
Aerospace engineering.
$3
1002622
650
4
$a
Mechanics.
$3
525881
690
$a
0548
690
$a
0538
690
$a
0346
710
2
$a
The University of North Carolina at Charlotte.
$b
Mechanical Engineering.
$3
1286885
773
0
$t
Dissertation Abstracts International
$g
79-01B(E).
790
$a
0694
791
$a
Ph.D.
792
$a
2017
793
$a
English
856
4 0
$u
http://pqdd.sinica.edu.tw/twdaoapp/servlet/advanced?query=10607383
based on 0 review(s)
Location:
ALL
電子資源
Year:
Volume Number:
Items
1 records • Pages 1 •
1
Inventory Number
Location Name
Item Class
Material type
Call number
Usage Class
Loan Status
No. of reservations
Opac note
Attachments
W9359996
電子資源
11.線上閱覽_V
電子書
EB
一般使用(Normal)
On shelf
0
1 records • Pages 1 •
1
Multimedia
Reviews
Add a review
and share your thoughts with other readers
Export
pickup library
Processing
...
Change password
Login