!> @file user_spectra.f90 !------------------------------------------------------------------------------! ! This file is part of the PALM model system. ! ! PALM is free software: you can redistribute it and/or modify it under the ! terms of the GNU General Public License as published by the Free Software ! Foundation, either version 3 of the License, or (at your option) any later ! version. ! ! PALM is distributed in the hope that it will be useful, but WITHOUT ANY ! WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR ! A PARTICULAR PURPOSE. See the GNU General Public License for more details. ! ! You should have received a copy of the GNU General Public License along with ! PALM. If not, see . ! ! Copyright 1997-2019 Leibniz Universitaet Hannover !------------------------------------------------------------------------------! ! ! Current revisions: ! ----------------- ! ! ! Former revisions: ! ----------------- ! $Id: user_spectra.f90 3655 2019-01-07 16:51:22Z eckhard $ ! Renamed output variables ! ! 3049 2018-05-29 13:52:36Z Giersch ! Error messages revised ! ! 3045 2018-05-28 07:55:41Z Giersch ! Corrected "Former revisions" section ! ! 2696 2017-12-14 17:12:51Z kanani ! Change in file header (GPL part) ! ! 2101 2017-01-05 16:42:31Z suehring ! ! 2000 2016-08-20 18:09:15Z knoop ! Forced header and separation lines into 80 columns ! ! 1960 2016-07-12 16:34:24Z suehring ! Consider additional spectra for passive scalar ! ! 1833 2016-04-07 14:23:03Z raasch ! spectrum renamed spectra_mod ! ! 1682 2015-10-07 23:56:08Z knoop ! Code annotations made doxygen readable ! ! 1320 2014-03-20 08:40:49Z raasch ! kind-parameters added to all INTEGER and REAL declaration statements, ! kinds are defined in new module kinds, ! old module precision_kind is removed, ! revision history before 2012 removed, ! comment fields (!:) to be used for variable explanations added to ! all variable declaration statements ! ! 1036 2012-10-22 13:43:42Z raasch ! code put under GPL (PALM 3.9) ! ! 211 2008-11-11 04:46:24Z raasch ! Former file user_interface.f90 split into one file per subroutine ! ! Description: ! ------------ !> Calculation of user-defined spectra. !> See section 3.5.4 on how to define, calculate, and output user defined !> quantities. !------------------------------------------------------------------------------! SUBROUTINE user_spectra( mode, m, pr ) USE arrays_3d USE control_parameters USE indices USE kinds USE spectra_mod USE statistics USE user IMPLICIT NONE CHARACTER (LEN=*) :: mode INTEGER(iwp) :: i !< INTEGER(iwp) :: j !< INTEGER(iwp) :: k !< INTEGER(iwp) :: m !< INTEGER(iwp) :: pr !< ! !-- Sample on how to calculate spectra of user-defined quantities. !-- Each quantity is identified by the corresponding user profile index !-- "pr_palm+#" where "#" is an integer starting from 1. These !-- user-profile-numbers must also be assigned to the respective strings !-- given by data_output_pr_user in routine user_check_data_output_pr. IF ( mode == 'preprocess' ) THEN SELECT CASE ( TRIM( data_output_sp(m) ) ) CASE ( 'u', 'v', 'w', 'theta', 'q', 's' ) !-- Not allowed here since these are the standard quantities used in !-- preprocess_spectra. ! CASE ( 'u*v*' ) ! pr = pr_palm+1 ! d(nzb+1:nzt,nys:nyn,nxl:nxr) = ustvst(nzb+1:nzt,nys:nyn,nxl:nxr) CASE DEFAULT message_string = 'Spectra of ' // & TRIM( data_output_sp(m) ) // ' can not be calculated' CALL message( 'user_spectra', 'UI0010', 0, 1, 0, 6, 0 ) END SELECT ELSEIF ( mode == 'data_output' ) THEN SELECT CASE ( TRIM( data_output_sp(m) ) ) CASE ( 'u', 'v', 'w', 'theta', 'q', 's' ) !-- Not allowed here since these are the standard quantities used in !-- data_output_spectra. ! CASE ( 'u*v*' ) ! pr = 6 CASE DEFAULT message_string = 'Spectra of ' // & TRIM( data_output_sp(m) ) // ' are not defined' CALL message( 'user_spectra', 'UI0011', 0, 0, 0, 6, 0 ) END SELECT ENDIF END SUBROUTINE user_spectra