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Unless otherwise noted, the content of this course material is licensed
under a Creative Commons BY 3.0 License.
http://creativecommons.org/licenses/by/3.0/
Copyright © 2009, August E. Evrard.
You assume all responsibility for use and potential liability associated with any use of the material. Material contains copyrighted content,
used in accordance with U.S. law. Copyright holders of content included in this material should contact open.michigan@umich.edu with
any questions, corrections, or clarifications regarding the use of content. The Regents of the University of Michigan do not license the use
of third party content posted to this site unless such a license is specifically granted in connection with particular content. Users of content
are responsible for their compliance with applicable law. Mention of specific products in this material solely represents the opinion of the
speaker and does not represent an endorsement by the University of Michigan. For more information about how to cite these materials
visit http://open.umich.edu/education/about/terms-of-use
Any medical information in this material is intended to inform and educate and is not a tool for self-diagnosis or a replacement for medical
evaluation, advice, diagnosis or treatment by a healthcare professional. You should speak to your physician or make an appointment to
be seen if you have questions or concerns about this information or your medical condition. Viewer discretion is advised: Material may
contain medical images that may be disturbing to some viewers.
Lesson Outline
• ideal fluid dynamics
• volume flux
• continuity equation
Source: V.van Gogh, Starry Night
I can describe the concept of ideal fluid
I can determine the volume flux in flowing fluid
I can solve the problem of continuity equation in flowing fluid
An ideal fluid is defined by the following set of characteristics. The
flow of the fluid must be
• steady
The velocity at any point in the flow does not change in time.
• incompressible
The density does not change with pressure.
• non-viscous
There are no sources of internal friction that could remove
energy from the flow.
• irrotational
An element (small piece) of the flow traces out a straight
path aligned with the fluid velocity, not a helical pattern
around it.
Ideal fluids
Ideal fluid flow is a simple, but
useful approximation to actual
fluid motion.
Arrows here represent the flow
velocity in a cross-sectional
cutout of the pipe.
The velocity is constant across the
area, there is no rotation, and no
drag (viscosity) near the edges of
the pipe.
STREAMLINE GEOMETRY
Small drag in streamlined position
Large drag in unstreamlined position
Both Images CC: BY-SA BoH (wimimedia commons) http://creativecommons.org/licenses/by-sa/3.0/
Turbulent flow: `vortex shedding’ around an obstacle
Steady (also called laminar) flow to the left of an island becomes
unsteady (or turbulent ) after passing by it. The grey scale image above
shows clouds in the atmosphere. Patches of the flow behind the obstacle
are spun up to create a series of vortices that alternately roll off, or ‘shed’,
from the top and bottom of the tube. The behavior downstream of the
tube is one of many examples of non-ideal fluid flow.
Island (from above)
ideal
fluid
flows
in
Source: NASA
Volume flux (Volume flow Rate)
Q = V/t
Q = Volume flux of fluid (m3/s)
V = Volume of flowing fluid (m3)
t = times taken by flowing fluid (s)
For a fluid of density r flowing through a pipe of cross-sectional
area A at speed v, the amount of mass Dm passing through a joint in
the pipe in a time interval Dt is given by
For regions of flow in which there are no sources or sinks of fluid,
the requirement that mass is neither created nor destroyed implies
that the product rAv is the same at all parts of the flow
Since an incompressible fluid has the same density at all points in the
flow (r=constant), then two locations (1 and 2) of a pipe with
different cross-sectional area will have the same volume flux.
Dm = r A v Dt
A1 v1 = A2 v2
r1 A1 v1 = r2 A2 v2
Conservation of mass for incompressible fluids

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Ideal fluid, volume flux and continuity equation

  • 1. Unless otherwise noted, the content of this course material is licensed under a Creative Commons BY 3.0 License. http://creativecommons.org/licenses/by/3.0/ Copyright © 2009, August E. Evrard. You assume all responsibility for use and potential liability associated with any use of the material. Material contains copyrighted content, used in accordance with U.S. law. Copyright holders of content included in this material should contact open.michigan@umich.edu with any questions, corrections, or clarifications regarding the use of content. The Regents of the University of Michigan do not license the use of third party content posted to this site unless such a license is specifically granted in connection with particular content. Users of content are responsible for their compliance with applicable law. Mention of specific products in this material solely represents the opinion of the speaker and does not represent an endorsement by the University of Michigan. For more information about how to cite these materials visit http://open.umich.edu/education/about/terms-of-use Any medical information in this material is intended to inform and educate and is not a tool for self-diagnosis or a replacement for medical evaluation, advice, diagnosis or treatment by a healthcare professional. You should speak to your physician or make an appointment to be seen if you have questions or concerns about this information or your medical condition. Viewer discretion is advised: Material may contain medical images that may be disturbing to some viewers.
  • 2. Lesson Outline • ideal fluid dynamics • volume flux • continuity equation Source: V.van Gogh, Starry Night
  • 3. I can describe the concept of ideal fluid I can determine the volume flux in flowing fluid I can solve the problem of continuity equation in flowing fluid
  • 4. An ideal fluid is defined by the following set of characteristics. The flow of the fluid must be • steady The velocity at any point in the flow does not change in time. • incompressible The density does not change with pressure. • non-viscous There are no sources of internal friction that could remove energy from the flow. • irrotational An element (small piece) of the flow traces out a straight path aligned with the fluid velocity, not a helical pattern around it. Ideal fluids
  • 5. Ideal fluid flow is a simple, but useful approximation to actual fluid motion. Arrows here represent the flow velocity in a cross-sectional cutout of the pipe. The velocity is constant across the area, there is no rotation, and no drag (viscosity) near the edges of the pipe.
  • 7. Small drag in streamlined position Large drag in unstreamlined position Both Images CC: BY-SA BoH (wimimedia commons) http://creativecommons.org/licenses/by-sa/3.0/
  • 8. Turbulent flow: `vortex shedding’ around an obstacle Steady (also called laminar) flow to the left of an island becomes unsteady (or turbulent ) after passing by it. The grey scale image above shows clouds in the atmosphere. Patches of the flow behind the obstacle are spun up to create a series of vortices that alternately roll off, or ‘shed’, from the top and bottom of the tube. The behavior downstream of the tube is one of many examples of non-ideal fluid flow. Island (from above) ideal fluid flows in Source: NASA
  • 9. Volume flux (Volume flow Rate) Q = V/t Q = Volume flux of fluid (m3/s) V = Volume of flowing fluid (m3) t = times taken by flowing fluid (s)
  • 10.
  • 11. For a fluid of density r flowing through a pipe of cross-sectional area A at speed v, the amount of mass Dm passing through a joint in the pipe in a time interval Dt is given by For regions of flow in which there are no sources or sinks of fluid, the requirement that mass is neither created nor destroyed implies that the product rAv is the same at all parts of the flow Since an incompressible fluid has the same density at all points in the flow (r=constant), then two locations (1 and 2) of a pipe with different cross-sectional area will have the same volume flux. Dm = r A v Dt A1 v1 = A2 v2 r1 A1 v1 = r2 A2 v2 Conservation of mass for incompressible fluids