Collection and Primitives Radiation
Transcript of Collection and Primitives Radiation
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Chapter 68: Collection and Primitives Radiation
68 Collection and Primitives
Radiation
Summary 1242
Introduction 1243
Modeling Details 1243
Solution Highlights 1243
Results 1250
Modeling Tips 1251
Input File(s) 1252
Video 1252
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Summary
Title Chapter 68: Collection and Primitives Radiation
Features: Enclosure Radiation
Primitive modeling
Small facet, Collection (Super Element), and Primitive radiation
Geometry & Boundary
Conditions
Material properties K = 0.001 W/m/oC, Emissivity, = 1.0, Absorptivity, = 1.0
Analysis characteristics Solution 400 / RC Network solver. Steady and transient thermal analysis.
Element type 4-node shell element CQUAD4
FE results
Space T = -273.15 oCRadiation insulated
upper side
Radiation insulated
Inner side
Normal Flux
1000 W/m2
Inner Side
Plate: 1.5 m x 1.5 m x 1 mm
Sphere: 1 m dia, t = 1 mm
Distance from Sphere center
to plate = 1 m
Small Facets
(1113 sec)
Collection (Super Element)
(6 sec)
Primitives
(3 sec)
104.8
Temperatures
104.6 104.3
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Introduction
This problem demonstrates three enclosure radiation loads of SOL 400 RC Network Solver: Small Facets, Collection(Super Element), and Primitives. Three methods will be used to solve the same model - small facet method, super
element method and primitive method. You can compare the speed and accuracy among the three methods.
Modeling DetailsThis model consists of a hemi-sphere and a plate. They are all primitive surfaces. The hemi-sphere and plate radiate
to each other, the other sides are radiation insulated. A heat flux 1000 W/ m is applied to the inner side of the hemi-sphere. A black coating is applied on the surface of both hemi-sphere and plate. An extremely low conductivity
material and extremely thin 2-D shell property are used to show the pour radiation effect.
Figure 68-1 Model Geometry and Materials
Solution HighlightsEnclosure Radiation has three options: Small Facets, Collection (Super Element), and Primitives. The small facets
method is the traditional way of FEM modelers to calculate radiation view factors. The collection and primitives are
the unique methods for speeding up radiation calculation in RC Network Solver. All the facets in the application region
will be treated as one radiation node. This makes the radiation analysis much faster and more efficient. The primitive
method also utilizes true geometric shapes for radiation analysis. A special algorithm is developed to match the
radiation results back to the finer conduction mesh. More details on collection and primitives can be referenced in
MSC Sinda for Patran user's guide.
RC Network Solver uses VIEWEX entry to simulate the enclosure radiation loads. RADC entry is used to represent the
MLI or Coating materials. These two entries are introduced in Chapter 66: Satellite in Orbit. The SET3 and RADCOL
cards are used to represent the collection (Super Element). The SET3 and PRIMx cards are used to represent the
primitives.
CHBDYE 9346 8735 1 2 2
CHBDYE 9347 8736 1 2 2
Space T = -273.15 oCRadiation insulated
upper side
12x12 mesh
Radiation insulated
Inner side
Normal Flux
1000 W/m2
Inner Side
Plate: 1.5 m x 1.5 m x 1 mm
Sphere: 1 m dia, t = 1 mm
Distance from Sphere center
to plate = 1 m
AxB mesh = 1x1
K= 0.001 W/m/oCCp = 1 J/Kg/oC
= 1 Kg/m3
Emissivity = 1
Absorptivity = 1
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$!
SET3 2 ELEM 9043 9044 9045 9046 9047 9048+
+ 9049 9050 9051 9052 9053 9054 9055 9056+...
$! Radiation Collection
RADCOL 3 2 2 2
...
CHBDYE 9746 930 1 3 2
CHBDYE 9747 931 1 3 2
$!
SET3 4 ELEM 9348 9349 9350 9351 9352 9353+
+ 9354 9355 9356 9357 9358 9359 9360 9361+...
$! Primitive Shape
$!----------------------------------------------------------------------------!$
PRIM1 2 3 2 3
-0.75 -0.75 1. 0.75 -0.75 1.
-0.75 0.75 1. 1 1
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Specifies a collection of boundary elements to be used as a single face in the radiation calculation. This will decrease
computation time at the small cost of accuracy. Computational savings and accuracy are dependent on the coarseness
of the collection versus the constituents. View factors of the collection are redistributed across the elements for
calculation of the radiative energy transfer.
Format
Example
Remarks
1. This entry is for RC Network solver only.
2. IVIEWF/IVIEWB will default to 0 if left blank. This would indicate that the corresponding front and/or back do
participate in the radiation.
3. IF an IVIEWF is specified, there must also be a RADMIDF for surface material properties. If an IVIEWB is
specified there must also be a RADMIDB for surface material properties.
RADCOL Radiation Collective Entity
1 2 3 4 5 6 7 8 9 10
RADCOL RADCOLID 701 2 1.0
1 2 3 4 5 6 7 8 9 10
RADCOL 101 5 6 2 3 7
Field Contents Type Default
RADCOLID Radiation Collection identification number. I 0 Required
IVIEWF A VIEW entry identification number for the front face. I 0 0
IVIEWB A VIEW entry identification number for the back face. I 0 0
RADMIDF RADM identification number for the front face I 0 0
RADMIDB RADM identification number for the back face. I 0 0
SET3 idn ID of the element collection to be considered a super
element.
I 0
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Specifies the properties of geometric primitives to be used in radiation calculations in place of elements.
Format
PRIMx Thermal Geometric Primitives for RC Radiation
1 2 3 4 5 6 7 8 9 10
PRIM1 PRIMID IVIEWF IVIEWB RADMIDF RADMIDB SET3ID +
+ P1(1) P1(2) P1(3) P2(1) P@(2) P2(3) +
+ P3(1) P3(2) P3(3) A_mesh B_mesh
1 2 3 4 5 6 7 8 9 10
PRIM2 PRIMID IVIEWF IVIEWB RADMIDF RADMIDB SET3ID +
+ P1(1) P1(2) P1(3) P2(1) P@(2) P2(3) +
+ P3(1) P3(2) P3(3) P4(1) P4(2) P4(3) A_mesh B_mesh
1 2 3 4 5 6 7 8 9 10
PRIM3 PRIMID IVIEWF IVIEWB RADMIDF RADMIDB SET3ID +
+ P1(1) P1(2) P1(3) P2(1) P@(2) P2(3) +
+ P3(1) P3(2) P3(3) A_mesh B_mesh
1 2 3 4 5 6 7 8 9 10
PRIM4 PRIMID IVIEWF IVIEWB RADMIDF RADMIDB SET3ID +
+ P1(1) P1(2) P1(3) P2(1) P@(2) P2(3) +
+ P3(1) P3(2) P3(3) Diam1 Diam2 Angle1 Angle2
A_mesh B_mesh
1 2 3 4 5 6 7 8 9 10
PRIM5 PRIMID IVIEWF IVIEWB RADMIDF RADMIDB SET3ID +
+ P1(1) P1(2) P1(3) P2(1) P@(2) P2(3) +
+ P3(1) P3(2) P3(3) Diam1 Angle1 Angle2 A_mesh B_mesh
1 2 3 4 5 6 7 8 9 10
PRIM6 PRIMID IVIEWF IVIEWB RADMIDF RADMIDB SET3ID +
+ P1(1) P1(2) P1(3) P2(1) P@(2) P2(3) +
+ P3(1) P3(2) P3(3) Diam1 Diam2 Angle1 Angle2
A_mesh B_mesh
1 2 3 4 5 6 7 8 9 10
PRIM7 PRIMID IVIEWF IVIEWB RADMIDF RADMIDB SET3ID +
+ P1(1) P1(2) P1(3) P2(1) P@(2) P2(3) +
+ P3(1) P3(2) P3(3) Diam1 Angle1 Angle2 Trunc1 Trunc2
A_mesh B_mesh
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1 2 3 4 5 6 7 8 9 10
PRIM8 PRIMID IVIEWF IVIEWB RADMIDF RADMIDB SET3ID +
+ P1(1) P1(2) P1(3) P2(1) P@(2) P2(3) +
+ P3(1) P3(2) P3(3) Diam1 Angle1 Angle2 Trunc1 Trunc2
A_mesh B_mesh
Field Contents Type Default
PRIMID Primitive identification number; unique to all
other PRIMx
I 0 Required
SET3 ID ID of the element collection to which thisprimitive describes. This collection acts as the
elements that will exist in the thermal model,
but the collection will be absent from the
radiation model. Instead, the primitive will be
used to calculate radiation and be
redistributed back onto the elements. All
radiation properties for the primitive will be
applied to the element collection and must beconsistent across.
I > 0 Required
RADMID ID of the radiation material properties used to
describe this primitive for analysis.
Pi(a) The position of point i in the a axis as
described in the correlating picture. For
example, P2(2) denotes the y coordinate of
the second point. Position is always describedin global coordinates.
R Required
Diamx Diameter x of the primitive if applicable and
as described in the correlating picture.
R 0.0 Required
Anglex Angle x of the primitive if applicable and as
described in the correlating picture.
0 R 360.0 Required
Truncx Truncation x of the primitive if all are
pickable and as described in the correlatingpicture.
R 0 for PRIM8 Required
-0.5*Diam1 R 0.5*Diam1 for PRIM7
A-mesh Number of mesh spaces in parametric
direction-1 as described in the correlating
picture.
I 0 Required
B_mesh Number of mesh spaces in parametric
direction-2 as described in the correlatingpicture.
I 0 Required
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Remarks
1. This entry is for RC Network solver only.
2. SET3 should include all the elements which belong to this primitive. It will cause wrong results if only a partial
of the elements are included.
3. PRIMID should be unique across all primitives (PRIMx) in the model.
4. About the primitives:
PRIM1: Rectangle
PRIM2: Quad
PRIM3: Triangle
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PRIM7: Sphere
PRIM8: Parabolic
Results
Figure 68-2 Temperature contour of Model for Case 1 (Steady State)
Small Facets
(1113 sec)
Collection (Super Element)
(6 sec)
Primitives
(3 sec)
104.8
Temperatures
104.6 104.3
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The following form illustrates the Thermica execute times and temperature results. (Windows XP v2002 SP3, Dell
Precision | M65 laptop, Intel Core(TM) 2 CPU, [email protected], 997MHz, 3.25GB of RAM).
Modeling TipsAs you can see, the temperature results are about the same, but the collection and primitives methods are much faster
then the traditional small facets method. Because of the feature of the re-match algorithm, no obstructions between the
two collections or primitives are allowed; otherwise we may lose some accuracy.
The parabolic primitive has not been supported yet in SimXpert, but MD Nastran/RC Network Solver supports that.
In MSC Sinda for Patran, you can put multiple primitives inside one application region, the translator will
automatically separate them to be multiple single- primitive loads, but SimXpert does not support this feature, one
single primitive is required for one primitive load.
You can preview the AB mesh of the primitive (Figure 68-3). These AB mesh is used to form the radiation model in
Thermica or other external radiation codes. The AB mesh does not have to be congruent with the conduction mesh.
Figure 68-3 AB mesh preview in SimXpert
Table 1-1 Speed and Result Comparison among the Three Methods (Ray count: 500,000)
Radiation Executing Time (s) Temperature Result (C)
Small facets method 1113 -79.74 to 104.8
Collection method 6 -79.67 to 104.6
Primitives method 3 -79.53 to 104.3
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Input File(s)
VideoClick on the image or caption below to view a streaming video of this problem; it lasts approximately 30 minutes and
explains how the steps are performed.
Figure 68-4 Video of the Above Steps
Files DescriptionQT16_hemi_sph_sf.dat MD Nastran SOL400/RC Network Solver thermal input file
QT33_hemi_sph_se.dat MD Nastran SOL400/RC Network Solver thermal input file
QT32_hemi_sph_pr.dat MD Nastran SOL400/RC Network Solver thermal input file
Space T = -273.15 oCRadiation insulated
upper side
Radiation insulated
Inner side
Normal Flux
1000 W/m2
Inner Side
Plate: 1.5 m x 1.5 m x 1 mm
Sphere: 1 m dia, t = 1 mm
Distance from Sphere center
to plate = 1 m
http://www.mscsoftware.com/training_videos/mdug/ch068/2010/ch068.swfhttp://www.mscsoftware.com/doc/nastran/mdug/input_files/ch068/QT16_hemi_sph_sf.dathttp://www.mscsoftware.com/doc/nastran/mdug/input_files/ch068/QT33_hemi_sph_se.dathttp://www.mscsoftware.com/doc/nastran/mdug/input_files/ch068/QT32_hemi_sph_pr.dathttp://www.mscsoftware.com/training_videos/mdug/ch068/2010/ch068.swfhttp://www.mscsoftware.com/training_videos/mdug/ch068/2010/ch068.swfhttp://www.mscsoftware.com/training_videos/mdug/ch068/2010/ch068.swfhttp://www.mscsoftware.com/training_videos/mdug/ch068/2010/ch068.swfhttp://www.mscsoftware.com/training_videos/mdug/ch068/2010/ch068.swfhttp://www.mscsoftware.com/training_videos/mdug/ch068/2010/ch068.swfhttp://www.mscsoftware.com/training_videos/mdug/ch068/2010/ch068.swfhttp://www.mscsoftware.com/training_videos/mdug/ch068/2010/ch068.swfhttp://www.mscsoftware.com/training_videos/mdug/ch068/2010/ch068.swfhttp://www.mscsoftware.com/training_videos/mdug/ch068/2010/ch068.swfhttp://www.mscsoftware.com/training_videos/mdug/ch068/2010/ch068.swfhttp://www.mscsoftware.com/training_videos/mdug/ch068/2010/ch068.swfhttp://www.mscsoftware.com/training_videos/mdug/ch068/2010/ch068.swfhttp://www.mscsoftware.com/training_videos/mdug/ch068/2010/ch068.swfhttp://www.mscsoftware.com/training_videos/mdug/ch068/2010/ch068.swfhttp://www.mscsoftware.com/training_videos/mdug/ch068/2010/ch068.swfhttp://www.mscsoftware.com/training_videos/mdug/ch068/2010/ch068.swfhttp://www.mscsoftware.com/doc/nastran/mdug/input_files/ch068/QT32_hemi_sph_pr.dathttp://www.mscsoftware.com/doc/nastran/mdug/input_files/ch068/QT33_hemi_sph_se.dathttp://www.mscsoftware.com/doc/nastran/mdug/input_files/ch068/QT16_hemi_sph_sf.dat