{"action":"created","issue":{"url":"https://api.github.com/repos/StrikeNP/trac_test/issues/322","repository_url":"https://api.github.com/repos/StrikeNP/trac_test","labels_url":"https://api.github.com/repos/StrikeNP/trac_test/issues/322/labels{/name}","comments_url":"https://api.github.com/repos/StrikeNP/trac_test/issues/322/comments","events_url":"https://api.github.com/repos/StrikeNP/trac_test/issues/322/events","html_url":"https://github.com/StrikeNP/trac_test/issues/322","id":332174332,"node_id":"MDU6SXNzdWUzMzIxNzQzMzI=","number":322,"title":"Output microphysics correlations to setup.txt file (Trac #322)","user":{"login":"StrikeNP","id":2577059,"node_id":"MDQ6VXNlcjI1NzcwNTk=","avatar_url":"https://avatars0.githubusercontent.com/u/2577059?v=4","gravatar_id":"","url":"https://api.github.com/users/StrikeNP","html_url":"https://github.com/StrikeNP","followers_url":"https://api.github.com/users/StrikeNP/followers","following_url":"https://api.github.com/users/StrikeNP/following{/other_user}","gists_url":"https://api.github.com/users/StrikeNP/gists{/gist_id}","starred_url":"https://api.github.com/users/StrikeNP/starred{/owner}{/repo}","subscriptions_url":"https://api.github.com/users/StrikeNP/subscriptions","organizations_url":"https://api.github.com/users/StrikeNP/orgs","repos_url":"https://api.github.com/users/StrikeNP/repos","events_url":"https://api.github.com/users/StrikeNP/events{/privacy}","received_events_url":"https://api.github.com/users/StrikeNP/received_events","type":"User","site_admin":false},"labels":[{"id":963997231,"node_id":"MDU6TGFiZWw5NjM5OTcyMzE=","url":"https://api.github.com/repos/StrikeNP/trac_test/labels/Migrated%20from%20Trac","name":"Migrated from Trac","color":"FFFFFF","default":false},{"id":963997516,"node_id":"MDU6TGFiZWw5NjM5OTc1MTY=","url":"https://api.github.com/repos/StrikeNP/trac_test/labels/clubb_src","name":"clubb_src","color":"FFFFFF","default":false},{"id":963997501,"node_id":"MDU6TGFiZWw5NjM5OTc1MDE=","url":"https://api.github.com/repos/StrikeNP/trac_test/labels/dschanen@uwm.edu","name":"dschanen@uwm.edu","color":"FFFFFF","default":false},{"id":963997043,"node_id":"MDU6TGFiZWw5NjM5OTcwNDM=","url":"https://api.github.com/repos/StrikeNP/trac_test/labels/enhancement","name":"enhancement","color":"a2eeef","default":true}],"state":"open","locked":false,"assignee":null,"assignees":[],"milestone":{"url":"https://api.github.com/repos/StrikeNP/trac_test/milestones/4","html_url":"https://github.com/StrikeNP/trac_test/milestone/4","labels_url":"https://api.github.com/repos/StrikeNP/trac_test/milestones/4/labels","id":3423155,"node_id":"MDk6TWlsZXN0b25lMzQyMzE1NQ==","number":4,"title":"3. Refactor CLUBB","description":null,"creator":{"login":"StrikeNP","id":2577059,"node_id":"MDQ6VXNlcjI1NzcwNTk=","avatar_url":"https://avatars0.githubusercontent.com/u/2577059?v=4","gravatar_id":"","url":"https://api.github.com/users/StrikeNP","html_url":"https://github.com/StrikeNP","followers_url":"https://api.github.com/users/StrikeNP/followers","following_url":"https://api.github.com/users/StrikeNP/following{/other_user}","gists_url":"https://api.github.com/users/StrikeNP/gists{/gist_id}","starred_url":"https://api.github.com/users/StrikeNP/starred{/owner}{/repo}","subscriptions_url":"https://api.github.com/users/StrikeNP/subscriptions","organizations_url":"https://api.github.com/users/StrikeNP/orgs","repos_url":"https://api.github.com/users/StrikeNP/repos","events_url":"https://api.github.com/users/StrikeNP/events{/privacy}","received_events_url":"https://api.github.com/users/StrikeNP/received_events","type":"User","site_admin":false},"open_issues":99,"closed_issues":45,"state":"open","created_at":"2018-06-13T20:01:14Z","updated_at":"2018-06-14T17:10:56Z","due_on":null,"closed_at":null},"comments":9,"created_at":"2018-06-13T21:39:37Z","updated_at":"2018-06-14T17:11:20Z","closed_at":null,"author_association":"OWNER","body":"**Introduction**\n\nWhen we use the upscaled KK_microphysics or Latin hypercube sampling, we need to specify certain horizontal correlations (rrp2_on_rrainm2_cloud, corr_sNc_LL_below, etc.)  These are listed in module parameters_microphys.\n\nOf course, if we predict these parameters at some point, then we won't need to write out these outputs.\n\n**Technical spec**\n\nOutput all variables in namelist microphysics_setting to the text file (xxx_setup.txt) that Ryan created in ticket #150?\n\n**Tests**\n\n1.  run_bindiff_all.bash should detect no differences between the new and old code.\n\n2.  When you run a case, all the correlations should appear with the correct values in the setup.txt file. \n\n3.  CLUBB and setup.txt should behave appropriately whether the Khairoutdinov-Kogan microphysics is used, the Morrison microphysics is used, or no microphysics is used.\n\nAttachments:\n\n\nMigrated from http://carson.math.uwm.edu/trac/clubb/ticket/322\n```json\n{\n    \"status\": \"closed\", \n    \"changetime\": \"2010-09-15T21:45:21\", \n    \"description\": \"'''Introduction'''\\n\\nWhen we use the upscaled KK_microphysics or Latin hypercube sampling, we need to specify certain horizontal correlations (rrp2_on_rrainm2_cloud, corr_sNc_LL_below, etc.)  These are listed in module parameters_microphys.\\n\\nOf course, if we predict these parameters at some point, then we won't need to write out these outputs.\\n\\n'''Technical spec'''\\n\\nOutput all variables in namelist microphysics_setting to the text file (xxx_setup.txt) that Ryan created in ticket #150?\\n\\n'''Tests'''\\n\\n1.  run_bindiff_all.bash should detect no differences between the new and old code.\\n\\n2.  When you run a case, all the correlations should appear with the correct values in the setup.txt file. \\n\\n3.  CLUBB and setup.txt should behave appropriately whether the Khairoutdinov-Kogan microphysics is used, the Morrison microphysics is used, or no microphysics is used.\", \n    \"reporter\": \"vlarson@uwm.edu\", \n    \"cc\": \"vlarson@uwm.edu\", \n    \"resolution\": \"Verified by V. Larson\", \n    \"_ts\": \"1284587121000000\", \n    \"component\": \"clubb_src\", \n    \"summary\": \"Output microphysics correlations to setup.txt file\", \n    \"priority\": \"minor\", \n    \"keywords\": \"\", \n    \"time\": \"2010-04-11T21:44:54\", \n    \"milestone\": \"3. Refactor CLUBB\", \n    \"owner\": \"dschanen@uwm.edu\", \n    \"type\": \"enhancement\"\n}\n```\n"},"comment":{"url":"https://api.github.com/repos/StrikeNP/trac_test/issues/comments/397370144","html_url":"https://github.com/StrikeNP/trac_test/issues/322#issuecomment-397370144","issue_url":"https://api.github.com/repos/StrikeNP/trac_test/issues/322","id":397370144,"node_id":"MDEyOklzc3VlQ29tbWVudDM5NzM3MDE0NA==","user":{"login":"StrikeNP","id":2577059,"node_id":"MDQ6VXNlcjI1NzcwNTk=","avatar_url":"https://avatars0.githubusercontent.com/u/2577059?v=4","gravatar_id":"","url":"https://api.github.com/users/StrikeNP","html_url":"https://github.com/StrikeNP","followers_url":"https://api.github.com/users/StrikeNP/followers","following_url":"https://api.github.com/users/StrikeNP/following{/other_user}","gists_url":"https://api.github.com/users/StrikeNP/gists{/gist_id}","starred_url":"https://api.github.com/users/StrikeNP/starred{/owner}{/repo}","subscriptions_url":"https://api.github.com/users/StrikeNP/subscriptions","organizations_url":"https://api.github.com/users/StrikeNP/orgs","repos_url":"https://api.github.com/users/StrikeNP/repos","events_url":"https://api.github.com/users/StrikeNP/events{/privacy}","received_events_url":"https://api.github.com/users/StrikeNP/received_events","type":"User","site_admin":false},"created_at":"2018-06-14T17:11:20Z","updated_at":"2018-06-14T17:11:20Z","author_association":"OWNER","body":"**Trac update on 2010/06/08 at 19:47**\nvlarson@uwm.edu changed description from:\n\n> '''Introduction'''\n> \n> When we use the upscaled KK_microphysics or Latin hypercube sampling, we need to specify certain horizontal correlations (rrp2_on_rrainm2_cloud, corr_sNc_LL_below, etc.)  These are listed in module parameters_microphys.\n> \n> Of course, if we predict these parameters at some point, then we won't need to write out these outputs.\n> \n> '''Technical spec'''\n> \n> Output these to the text file (xxx_setup.txt) that Ryan created in ticket #150?\n> \n> '''Tests'''\n> \n> 1.  run_bindiff_all.bash should detect no differences between the new and old code.\n> \n> 2.  When you run a case, all the correlations should appear with the correct values in the setup.txt file. \n> \n> 3.  CLUBB and setup.txt should behave appropriately whether the Khairoutdinov-Kogan microphysics is used, the Morrison microphysics is used, or no microphysics is used.\n\nto:\n\n> '''Introduction'''\n> \n> When we use the upscaled KK_microphysics or Latin hypercube sampling, we need to specify certain horizontal correlations (rrp2_on_rrainm2_cloud, corr_sNc_LL_below, etc.)  These are listed in module parameters_microphys.\n> \n> Of course, if we predict these parameters at some point, then we won't need to write out these outputs.\n> \n> '''Technical spec'''\n> \n> Output all variables in namelist microphysics_setting to the text file (xxx_setup.txt) that Ryan created in ticket #150?\n> \n> '''Tests'''\n> \n> 1.  run_bindiff_all.bash should detect no differences between the new and old code.\n> \n> 2.  When you run a case, all the correlations should appear with the correct values in the setup.txt file. \n> \n> 3.  CLUBB and setup.txt should behave appropriately whether the Khairoutdinov-Kogan microphysics is used, the Morrison microphysics is used, or no microphysics is used.\n\n"}}
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