2.8 Inquiring about D.S. HREF="./Modulef.css" TITLE="Modulef CSS"> ALT="Modulef"> ALT="previous"> ALT="up"> ALT="next"> ALT="contents"> ALT="[BIG]"> ALT="[Normal]"> ALT="[small]"> Next: 2.9 Extrema of a D.S. B Up: 2 Manipulation of solutions Prev: 2.7 Computing the flux and temperature >Contents 2.8 Inquiring about D.S. Preprocessor IMAGXX lists the contents of an arbitrary D.S. Preprocessor INFOXX is used to obtain information on any object stored in D.S. B, NOPO, TAE, COOR, MAIL or GEOM. The modules called are respectively INFOBB, INFONO, INFOTA, INFOCO, INFOMA or INFONO (after conversion to NOPO). For other types of structures, only IMAGXX can be used, as the specific program has not yet been developed to this date. Regarding the processing of D.S. B, we have modules IMB, IMBND0 and PRINTB. The first two are called via IMAGXX depending on ND. The last is used to obtain a printout of the structure, including the variational unknowns, the number of degrees of freedom per node, as well as their mnemonics. SUBROUTINE PRINTB(M,NFB,NIB,NFTYNO,NITYNO,TSIFO,IND1,ITAB,IND2, + NFNDL1,NINDL1,IMPR) C +++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++ C AIM : PRINT A D.S. B C --- C +++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++ where M is the super array, NFB, NIB are the file number and level of D.S. B, NFTYNO, NITYNO are the file number and level of D.S. TYNO used here (it can be constructed by using module COTYNO), TSIFO is the array indicating clearly (4 times 4 characters) the names of the variational unknowns if they differ from those in arrays containing D.S. MAIL or TYNO, IND1 is set to 1 is we consider the array above, and 0 if not, ITAB is the title if desired, IND2 is set to 1 if we consider the array above, and 0 if not, NFNDL1, NINDL1 are the file number and level of structure NDL1, used if ND is zero, IMPR is the print parameter. ALT="Modulef"> ALT="previous"> ALT="up"> ALT="next"> ALT="contents"> ALT="[BIG]"> ALT="[Normal]"> ALT="[small]"> Next: 2.9 Extrema of a D.S. B Up: 2 Manipulation of solutions Prev: 2.7 Computing the flux and temperature >Contents
