Model help:FallVelocity: Difference between revisions

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==Model parameters==
==Model parameters==
= First tab header =
= Input Files and Directories =
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!Parameter!!Description!!Unit
!Parameter!!Description!!Unit
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|width="20%"|<span class="remove_this_tag">First parameter</span>
|width="20%"|Input directory
|width="60%"|<span class="remove_this_tag">Description parameter</span>
|width="60%"|path to input files
|width="20%"|<span class="remove_this_tag">[Units]</span>
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|Site prefix
|Site prefix for Input/Output files
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|Case prefix
|Case prefix for Input/Output files
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= Run Parameters =
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!Parameter!!Description!!Unit
!Parameter!!Description!!Unit
|-valign="top"
|-valign="top"
|width="20%"|<span class="remove_this_tag">First parameter</span>
|width="20%"|kinematic viscosity of water (ν)
|width="60%"|<span class="remove_this_tag">Description parameter</span>
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|width="20%"|<span class="remove_this_tag">[Units]</span>
|width="20%"| m<sup>2</sup> / s
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|Submerged specific gravity of sediment (R)
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| -
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|Grain size (D)
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| mm
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|Acceleration due to gravity (g)
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| -
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= About =
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!Parameter!!Description!!Unit
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|width="20%"|Model name
|width="60%"|name of the model
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|Author name
|name of the model author
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Revision as of 10:48, 6 May 2011

The CSDMS Help System

FallVelocity

This model is used to calculate Particle fall velocity.

Model introduction

This model calculate fall velocity for spheres. Uses formulation of Dietrich (1982).

Model parameters

Parameter Description Unit
Input directory path to input files
Site prefix Site prefix for Input/Output files
Case prefix Case prefix for Input/Output files
Parameter Description Unit
kinematic viscosity of water (ν) m2 / s
Submerged specific gravity of sediment (R) -
Grain size (D) mm
Acceleration due to gravity (g) -
Parameter Description Unit
Model name name of the model -
Author name name of the model author -

Uses ports

This will be something that the CSDMS facility will add

Provides ports

This will be something that the CSDMS facility will add

Main equations

[math]\displaystyle{ Re_{p} = {\frac{\sqrt { R g D } D}{\nu}} }[/math] (1)
[math]\displaystyle{ R_{f} = {\frac{v_{s}}{\sqrt { R g D }}} }[/math] (2)
[math]\displaystyle{ R_{f} = exp \left ( -b_{1} + b_{2} ln \left ( Re_{p} \right ) - b_{3} \left ( ln \left ( Re_{p} \right ) \right ) ^2 - b_{4} \left ( ln \left ( Re_{p} \right ) \right ) ^3 + b_{5} \left ( ln \left ( Re_{p} \right ) \right ) ^4 \right ) }[/math] (3)

Notes

This formulation is only valid for Reynold’s numbers less than or equal to 2.5·106. If Rep is greater than this upper limit, the function will alert the user, and exit the program.


Examples

An example run with input parameters, BLD files, as well as a figure / movie of the output

Follow the next steps to include images / movies of simulations:

See also: Help:Images or Help:Movies

Developer(s)

Gary Parker

References

Dietrich, E. W., 1982, Settling velocity of natural particles, Water Resources Research, 18 (6), 1626-1982.

Links