Name | Modified | Size | Downloads / Week |
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Parent folder | |||
build | 2014-04-10 | 495 Bytes | |
revolve_grid.f90 | 2014-04-09 | 10.3 kB | |
README | 2014-04-09 | 2.5 kB | |
Totals: 3 Items | 13.3 kB | 0 |
REVOLVE_GRID is a revision of Todd White's original "hotdog" utility for turning a 2-D grid and optional flow solution into a 3-space equivalent. For axisymmetric vehicles, even at angle of attack, an initial 2-space grid and flow solution can provide an effective start for 3-space cases once the resulting singular grid lines are removed (see RADIAL_INTERP in conjunction with CAPSULE_GRID procedures). The right (starboard) half of the body of revolution is produced with a 180-degree rotation. Input Coordinate System: X streamwise, Y up Output Coordinate System: X streamwise, Y positive to the right, Z up The input dataset[s] are rotated about OX by the indicated angle (normally 180 or perhaps 360 degrees) to produce the specified number of grid points uniformly spaced in the azimuthal direction. The input 2-space grid may or may not include Z = 0. Reading is attempted first as multiblock 3-D (X/Y/Z), then retried as 2-D if necessary. All file names and other control inputs are prompted for, along with the number of species densities, ns, from which any velocity component indices are deduced. Any input flow field file should normally contain state variables in the following order, with zero or more extra variables appended: species densities (ns of them), vx & vy (no vz), temperature[s], any extras However, this does not suit flow inputs to a radiation solver such as NEQAIR, which expects 4 temperatures followed by species number densities. Therefore, provision is made for NO velocity components, meaning all of the flow variables are simply replicated at each azimumthal station. The resulting output file MAY have one extra flow variable (3rd velocity component) with the y and z components adjusted appropriately at each angular station for axial symmetry. 11/09/2011 David Saunders Initial adaptation of Todd White's hotdog tool. 05/10/2012 " " Testing of the function file option had been overlooked, and there were indexing errors. Apologies to Jay Hyatt. 04/08/2014 " " Todd found that flow datasets for radiation calculations don't contain velocity components, so there's now an option to handle that. 04/09/204 " " Allow for Z = 0. or not (3-D or 2-D) in the input grid (automatically detected). Authors: Todd White/David Saunders, ERC, Inc./NASA Ames Research Center, CA