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Foundation ::
Thermal Tools ::
VIEW
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VIEW
Radiation View Factor Program
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SOURCE CODE AVAILABLE
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The calculation of the radiation exchange between two gray, diffuse surfaces by the usual engineering method presents difficulties since it requires a full and precise description of both surfaces. Often the major difficulty in calculating the heat transfer rests with the accurate determination of the surface conditions. For multi-surface enclosure problems, or for radiation between surfaces whose mutual views are obstructed, the evaluation of the view factor is a major effort. For many situations, as in spacecraft or space structures, solar receivers, or industrial furnaces, estimates using graphical and numerical techniques are not adequate. Furthermore, in structures for which the changing position of the sun leads to different surfaces becoming radiantly important at different times, accurate determination of the viewfactor for all surfaces is particularly important.
The family of computer codes, VIEW, has been created to accomplish this task. VIEW is an interactive program that determines the viewfactors, graphically displays surfaces, and evaluates the solar irradiation of an assemblage of surfaces.
VIEWC and VIEWH
VIEWC and VIEWH compute the view factors between surfaces. These views may be obstructed either by other surfaces or by themselves. The view factors are generally computed by means of the contour integration technique originally developed by Mittalas and Stevenson. When there is the possibility that the radiation between any two surfaces is obstructed, their view factor is calculated either by means of a double area integral technique or by contour integration applied to surface sub-elements (VIEWC) or by a pixel projection method (VIEWH). Structures are defined to VIEWC/VIEWH in terms of a collection of flat surfaces, each of which has three or four edges (i.e. a triangle or a quadrilateral). VIEWC can also compute view factors for 2-D surfaces. There are several ways to enter the data for VIEWC/VIEWH. One way is compatible with the usual finite element surface definitions, allowing the use of finite element mesh generation programs to create input for VIEWC/VIEWH. The VIEWCI program eliminates excess common nodes in free form data input, thus reducing the amount of storage required.
VIEWI
VIEWI is an interactive graphics program for generating the surface information needed for VIEWC. The surfaces may be generated singly or in groups and the user may manipulate them in a variety of different ways to create the structure desired. VIEWI may also be used to generate finite element 2-D meshes. VIEWCM combines the output from two different VIEWI sessions in order to make a composite body. VIEWG provides interactive graphical display of the surfaces generated by VIEWI, with full hidden line removal and storage of the picture for high-speed processing (e.g. rapid rotation or perspective viewing of the structure).
VIEWO
VIEWO computes the solar radiation falling on an orbiting structure and the solar radiation which is reflected from the Earth. Input is the same as VIEWC/VIEWH, with additional data on the position of the structure with respect to the sun and earth. VIEWO runs in either batch or interactive mode and computes the solar load as a function of orbital position. Output from VIEWO includes: solar view factor, earth's longwave view factor, reflected solar view factor, and total solar load.
VIEWS
VIEWS computes specular reflections from surfaces and can be used in conjunction with VIEWO to track the progress of the Sun's rays as they reflect throughout the assemblage of surfaces.
VIEW carries the NASA case number LAR-14217. It was originally released as part of the COSMIC collection.
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