program main !*****************************************************************************80 ! !! MAIN is the main program for DIVISION. ! ! Discussion: ! ! DIVISION demonstrates that division should be done to full precision. ! ! Especially when carrying out division, but also in other arithmetic ! operations, it is important that constants be specified as double ! precision values, by using the "D" identifier in the exponent field. ! ! Licensing: ! ! This code is distributed under the GNU LGPL license. ! ! Modified: ! ! 12 September 2005 ! ! Author: ! ! John Burkardt ! implicit none real ( kind = 8 ) a(4,4) real ( kind = 8 ) b(4,4) integer ( kind = 4 ) i call timestamp ( ) write ( *, '(a)' ) ' ' write ( *, '(a)' ) 'DIVISION:' write ( *, '(a)' ) ' FORTRAN90 version.' write ( *, '(a)' ) ' ' write ( *, '(a)' ) ' Demonstrate 16 ways to compute 1/3, expecting' write ( *, '(a)' ) ' a double precision real result.' write ( *, '(a)' ) ' ' write ( *, '(a)' ) ' The results, stored as a table, are:' write ( *, '(a)' ) ' ' write ( *, '(a)' ) & ' 1 / 3 1 / 3.0 1 / 3.0E+00 1 / 3.0D+00' write ( *, '(a)' ) & ' 1.0 / 3 1.0 / 3.0 1.0 / 3.0E+00 1.0 / 3.0D+00' write ( *, '(a)' ) & ' 1.0E+00 / 3 1.0E+00 / 3.0 1.0E+00 / 3.0E+00 1.0E+00 / 3.0D+00' write ( *, '(a)' ) & ' 1.0D+00 / 3 1.0D+00 / 3.0 1.0E+00 / 3.0E+00 1.0D+00 / 3.0D+00' a(1,1) = 1 / 3 a(1,2) = 1 / 3.0 a(1,3) = 1 / 3.0E+00 a(1,4) = 1 / 3.0D+00 a(2,1) = 1.0 / 3 a(2,2) = 1.0 / 3.0 a(2,3) = 1.0 / 3.0E+00 a(2,4) = 1.0 / 3.0D+00 a(3,1) = 1.0E+00 / 3 a(3,2) = 1.0E+00 / 3.0 a(3,3) = 1.0E+00 / 3.0E+00 a(3,4) = 1.0E+00 / 3.0D+00 a(4,1) = 1.0D+00 / 3 a(4,2) = 1.0D+00 / 3.0 a(4,3) = 1.0D+00 / 3.0E+00 a(4,4) = 1.0D+00 / 3.0D+00 write ( *, '(a)' ) ' ' write ( *, '(a)' ) ' The matrix of results:' write ( *, '(a)' ) ' ' do i = 1, 4 write ( *, '(4g20.14)' ) a(i,1:4) end do write ( *, '(a)' ) ' ' write ( *, '(a)' ) ' Defects might be more obvious if we multiply' write ( *, '(a)' ) ' by 3:' write ( *, '(a)' ) ' ' write ( *, '(a)' ) ' B = 3 * A:' write ( *, '(a)' ) ' ' b(1:4,1:4) = 3 * a(1:4,1:4) do i = 1, 4 write ( *, '(4g20.14)' ) b(i,1:4) end do write ( *, '(a)' ) ' ' write ( *, '(a)' ) ' B = 3.0 * A:' write ( *, '(a)' ) ' ' b(1:4,1:4) = 3.0 * a(1:4,1:4) do i = 1, 4 write ( *, '(4g20.14)' ) b(i,1:4) end do write ( *, '(a)' ) ' ' write ( *, '(a)' ) ' B = 3.0E+00 * A:' write ( *, '(a)' ) ' ' b(1:4,1:4) = 3.0E+00 * a(1:4,1:4) do i = 1, 4 write ( *, '(4g20.14)' ) b(i,1:4) end do write ( *, '(a)' ) ' ' write ( *, '(a)' ) ' B = 3.0D+00 * A:' write ( *, '(a)' ) ' ' b(1:4,1:4) = 3.0D+00 * a(1:4,1:4) do i = 1, 4 write ( *, '(4g20.14)' ) b(i,1:4) end do write ( *, '(a)' ) ' ' write ( *, '(a)' ) 'DIVISION:' write ( *, '(a)' ) ' Normal end of execution.' write ( *, '(a)' ) ' ' call timestamp ( ) stop end subroutine timestamp ( ) !*****************************************************************************80 ! !! TIMESTAMP prints the current YMDHMS date as a time stamp. ! ! Example: ! ! May 31 2001 9:45:54.872 AM ! ! Licensing: ! ! This code is distributed under the GNU LGPL license. ! ! Modified: ! ! 26 February 2005 ! ! Author: ! ! John Burkardt ! ! Parameters: ! ! None ! implicit none character ( len = 8 ) ampm integer d integer h integer m integer mm character ( len = 9 ), parameter, dimension(12) :: month = (/ & 'January ', 'February ', 'March ', 'April ', & 'May ', 'June ', 'July ', 'August ', & 'September', 'October ', 'November ', 'December ' /) integer n integer s integer values(8) integer y call date_and_time ( values = values ) y = values(1) m = values(2) d = values(3) h = values(5) n = values(6) s = values(7) mm = values(8) if ( h < 12 ) then ampm = 'AM' else if ( h == 12 ) then if ( n == 0 .and. s == 0 ) then ampm = 'Noon' else ampm = 'PM' end if else h = h - 12 if ( h < 12 ) then ampm = 'PM' else if ( h == 12 ) then if ( n == 0 .and. s == 0 ) then ampm = 'Midnight' else ampm = 'AM' end if end if end if write ( *, '(a,1x,i2,1x,i4,2x,i2,a1,i2.2,a1,i2.2,a1,i3.3,1x,a)' ) & trim ( month(m) ), d, y, h, ':', n, ':', s, '.', mm, trim ( ampm ) return end