Vn8.4 GA4.0 Release Candidate: RC6.0
This page documents the vn8.4 GA4.0 release candidate xkawa
. This job has been developed and run by Luke Abraham on MONSooN.
Suitability for Release
Tropospheric Chemistry | |
Stratospheric Chemistry | Users should note the low stratospheric NOy. |
Tropospheric Aerosol | Users should note the high aerosol optical depth in this configuration. |
Stratospheric Aerosol | Users should note the high stratospheric sea-salt mixing ratios. |
Key
Release candidate still under evaluation |
Release candidate not scientifically suitable to be released |
Release candidate is suitable for development jobs, and may be scientifically suitable to be released for some applications |
Release candidate scientifically suitable to be released |
Release candidate does not consider the required chemistry or aerosol processes |
UKCA code
For this release the relevant and specific UKCA code changes (when compared to the trunk) have been merged into a package branch on PUMA
For the results presented here, revision number 16065
was used. The latest revision is 16246, see below.
For details as to which branches and fixes were included, please see PUMA Trac ticket #632.
Changes since xkawa run
There have been two changes to this branch since job xkawa
was completed. These have been tested by comparing a 1-month run of xkawa
-identical job xkawg
and running cumf
on the 1st January dump, comparing with the equivalent job with these changes in, xkawf
. These changes do not affect the model evolution.
- Deallocation of
qsmr
: When porting this job to ARCHER the Cray cce Fortran compiler picked up that the variableqsmr
was deallocated too early. The IBM xlf Fortran compiler allows deallocated arrays still to be accessed, but the Cray compiler does not (correctly!). This bug was corrected at revision number r16244. - ARCHER specific changes: There were two changes to this congfiguration that were found by Karthee Sivalingam when he ported job
xjcim
to ARCHER, which he placed in the branch fcm:um_br/dev/karthee/vn8.4_xjcim_port_fixes. I have merged this into the package branch at r16246.
The cumf
summary is below. While it says "files DO NOT compare" this is not due to any changes in the data fields, which are identical (as expected).
$ /projects/um1/vn8.4/ibm/utils/cumf xkawf/xkawfa.da20000101_00 xkawg/xkawga.da20000101_00 COMPARE - SUMMARY MODE ----------------------- Number of fields in file 1 = 47392 Number of fields in file 2 = 47392 Number of fields compared = 47392 FIXED LENGTH HEADER: Number of differences = 3 INTEGER HEADER: Number of differences = 0 REAL HEADER: Number of differences = 0 LEVEL DEPENDENT CONSTANTS: Number of differences = 0 LOOKUP: Number of differences = 33715 DATA FIELDS: Number of fields with differences = 0 files DO NOT compare
Using this branch
Note: if you wish to use this branch to develop some extra code, please follow these guidelines:
- Make your own branch (in the usual way) at vn8.4.
fcm merge
in the UKCA package branchfcm:um_br/pkg/Config/vn8.4_UKCA
.fcm commit
this before you make your own changes.- In the UMUI, turn off the UKCA package branch, and use your own branch that you have just made.
- It is advisable to use a working copy initially while you are getting any developments working.
- For production runs it is best to
fcm commit
all developments from the working copy and run from the repository using this revision number.- This will make it easier to repeat simulations at a later date if needed.
- Remember to perform frequent commits, even if you are still using the working copy - this makes it easier to backtrack changes when necessary.
Do not checkout the package branch, make changes, and commit them. This will cause problems for other UKCA users.
Functionality
Base Model
The base atmosphere model used here is the GA4.0 configuration. More information on GA4.0 development can be found on Global Atmosphere 4.0/Global Land 4.0 documentation pages (password required). A GMD paper documenting this model is also available.
The configuration is based on the Met Office job anenj
(via MONSooN job xhmaj
) which is derived from amche
(the standard GA4.0 N96L85 interactive dust model) via
amche
(base GA4.0 job) owned by Dan Copsey
akwxo
(UKCA turned on) owned by Mohit Dalvi
aneni
owned by Colin Johnson
anenj
xhmaj
owned by Mohit Dalvi
xjcib
(HOx recycling added) owned by Luke Abraham
xjcie
(some reaction rates updated)
xjcih
(O3 now interactive with radiation scheme)
xjcim
(made TS2000 - see Initial conditions and forcing)
xjcin
xjlla
(UKCA Tutorials base job; some branch consolidation) owned by Luke Abraham
xkawa
(package branch used, containing various bugfixes and additions) owned by Luke Abraham
For more information on these jobs and the UKCA release cycle, please see the the developing releases page.
Scaling (MONSooN)
Each compute node of the MONSooN phase 2 system contains four 3.8 GHz IBM Power 7 processors, and there is 64GB of RAM per node. Due to memory restrictions, UKCA is unable to run on less than 3 nodes. As noted below, the EW domain decomposition needed to be a multiple of 12. All simulations used 2 OpenMP threads which will not reduce the number of cores per node used.
More information on MONSooN can be found on the collaboration twiki (registration required).
12EW Decomposition
Scaling tests have been done from 3 to 9 nodes of MONSooN using a decomposition of 12EW, with a series of 1-day runs, with the results presented below.
The speedup in the plot above is calculated by assuming a linear scaling from 3 nodes down to 1 node. 5 simulations were performed for each number of nodes, and the envelope is 2 standard deviations (assuming that the standard deviation of the extrapolated 1-node data-point is the mean of the standard deviations of all other points). From these tests the recommended decomposition is 12 EW x 16 NS (i.e. 6 nodes, or 192 cores). Running on 6 nodes means that the model will complete 1 model month in approximately 2 hours. Although 3 nodes would be slightly more efficient, each simulation would take nearly twice as long and would therefore fall outside the 3-hour queue limit, which is undesirable.
Above 9 nodes the model not run as this is a 12EWx32NS which falls over due to the halo size in the model with the error message
???????????????????????????????????????????????????????????????????????????????? ???!!!???!!!???!!!???!!!???!!!???!!! ERROR ???!!!???!!!???!!!???!!!???!!!???!!!? ? Error in routine: DECOMP_DB:DECOMPOSE ? Error Code: 5 ? Error Message: Too many processors in the North-South direction ( 32) to support the extended halo size ( 5). Try running with 28 processors. ? Error generated from processor: 0 ? This run generated 5 warnings ????????????????????????????????????????????????????????????????????????????????
24EW Decomposition
Scaling tests have been done from 3 to 21 nodes of MONSooN using a decomposition of 24EW, with a series of 1-day runs, with the results presented below.
The speedup in the plot above is calculated by assuming a linear scaling from 3 nodes down to 1 node. 5 simulations were performed for each number of nodes, and the envelope is 2 standard deviations (assuming that the standard deviation of the extrapolated 1-node data-point is the mean of the standard deviations of all other points). Note the change in y scales when compared to the above plot for 12EW decomposition.
12EW verses 24EW decomposition
In the plots above, the extrapolated 1-node value is calculated from the 12EW or 24EW 3-node value. In reality, these are actually slightly different. If the 1-node value is calculated as a mean of the 12EW and 24EW values (with the standard deviation calculated accordingly) we can then see that using a 12EW decomposition is more advantageous over the 24EW decomposition (shadings are 2 standard deviations).
Therefore the decomposition that should be used is 12 EW x 16 NS.
Chemistry
This job uses the CheST chemistry scheme - an amalgamation of the Stratospheric Chemistry scheme and the Tropospheric Chemistry with Isoprene scheme. The Fast-JX interactive photolysis scheme is used.
For more information on these schemes, please see
- Evaluation of the new UKCA climate-composition model – Part 1: The stratosphere
- Evaluation of the new UKCA climate-composition model – Part 2: The Troposphere
- Implementation of the Fast-JX Photolysis scheme (v6.4) into the UKCA component of the MetUM chemistry-climate model (v7.3)
Aerosols
This job uses an extension to the GLOMAP-mode aerosol scheme which extends it into the stratosphere, although it is also suitable for tropospheric work.
For information on GLOMAP-mode, please see
- Description and evaluation of GLOMAP-mode: a modal global aerosol microphysics model for the UKCA composition-climate model
- Impact of the modal aerosol scheme GLOMAP-mode on aerosol forcing in the Hadley Centre Global Environmental Model
- Aerosol microphysics simulations of the Mt. Pinatubo eruption with the UKCA composition-climate model
Pressure-level output for tracers and chemical diagnostics
All STASH items available in section 34 have an equivalent in section 35. Currently only O3 and the flux through the CH4+OH reaction have been set-up, but other fields can be output by copying these examples.
Note: the Heaviside function s35i173 also need to put output so that these fields can be processed correctly to remove points which should contain missing data. In the lower levels of the model the pressures will be low (especially over high orography) and these points need to be masked off. Valid points are where this function is equal to 1.
RCP Scenario Code
The RCP scenario branch, committed to the trunk at vn8.6, has equivalent functionality available in this job (UKCA lower boundary conditions only - further changes are required to have these affect the GHGs).
To use this functionality a hand-edit is required - see e.g. /home/ukca/hand_edits/VN8.4/UKCA_RCP6.0.ed
Pre-compiled builds
This job makes use of pre-compiled builds, as can be seen in the FCM panel. This decreases the time required for the compilation step.
Note that the reconfiguration executable (qxreconf
) has also been pre-compiled (this can be seen in the Compile and run options for the Atmosphere and Reconfiguration panel). This was required to allow the pre-compiled builds to work. If you want/need to change either the reconfiguration executable or the use of pre-compiled builds, you will need to change the settings in both the FCM and compilation options panels. Do not turn on compilation of the reconfiguration executable unless you change its location.
cumf
tests (MONSooN)
A handy test of a model is to know whether it bit-compares when re-running, and what restrictions (if any) there are on this. To do this, the cumf
utility is used, which is found at /projects/um1/vn8.4/ibm/utils/cumf
. There are 4 types of tests that should be run, a NRUN-NRUN test, a NRUN-CRUN test, a CRUN-CRUN test, and a change of dump frequency test.
All tests were run without STASH, climate meaning, or the UKCA evaluation suite hand-edit (~mdalvi/umui_jobs/hand_edits/vn8.4/add_ukca_eval1_diags_l85.ed
), as all of these can affect the dump by placing temporary fields in it. The model was run for 2 days, either with daily or 2-day dumping, and for the NRUN-CRUN test, the first step was for 1 day followed by a new job step for the 2nd day. Reconfiguration was only run once, at the start of the 1st test, and after that point the same .astart
file was used by all jobs.
NRUN-NRUN tests (MONSooN)
For this test the model is run twice. The 2-day dumps are then compared. For this test it makes no difference if you compare the dumps produced using daily-dumping or 2-day dumping, as both pass this test (when compared to the equivalent dump produced using the same dumping frequency).
COMPARE - SUMMARY MODE ----------------------- Number of fields in file 1 = 14272 Number of fields in file 2 = 14272 Number of fields compared = 14272 FIXED LENGTH HEADER: Number of differences = 3 INTEGER HEADER: Number of differences = 0 REAL HEADER: Number of differences = 0 LEVEL DEPENDENT CONSTANTS: Number of differences = 0 LOOKUP: Number of differences = 0 DATA FIELDS: Number of fields with differences = 0 files compare, ignoring Fixed Length Header
NRUN-CRUN tests (MONSooN)
For this test the 2nd day dump of a daily dumping run (which has been run in a single jobstep) is compared with the 2nd day dump of a run where this was produced on a CRUN step (i.e. where the 1st day dump was produced on the NRUN step). In this case, the dumps DO NOT compare.
COMPARE - SUMMARY MODE ----------------------- Number of fields in file 1 = 14272 Number of fields in file 2 = 14272 Number of fields compared = 14272 FIXED LENGTH HEADER: Number of differences = 4 INTEGER HEADER: Number of differences = 0 REAL HEADER: Number of differences = 3 LEVEL DEPENDENT CONSTANTS: Number of differences = 0 LOOKUP: Number of differences = 0 DATA FIELDS: Number of fields with differences = 12221 Field 1 : Stash Code 2 : U COMPNT OF WIND AFTER TIMESTEP : Number of differences = 27840 ... ... Field 14076 : Stash Code 38405 : DRY PARTICLE DIAMETER AITKEN-INS : Number of differences = 67 files DO NOT compare
This is not unexpected for UKCA, as there are many variables which are initialised at the start of a run, but not saved to a dump to be re-initialised correctly. This is a feature which will need to be addressed in the future.
It should be noted that this does not invalidate a run, or prevent you from re-running to fill-in data gaps. You should, however, ensure that you maintain the original job-step length. On MONSooN is it recommended that maintain a 1-month jobstep length, with the standard climate dumping frequency of 10-days.
CRUN-CRUN tests (MONSooN)
For this test the model is run a second time as NRUN-CRUN jobsteps. The 2-day dump from the 1st CRUN test is then compared with this newly generated 2-day dump from the 2nd CRUN. This test bit-compares.
COMPARE - SUMMARY MODE ----------------------- Number of fields in file 1 = 14272 Number of fields in file 2 = 14272 Number of fields compared = 14272 FIXED LENGTH HEADER: Number of differences = 3 INTEGER HEADER: Number of differences = 0 REAL HEADER: Number of differences = 0 LEVEL DEPENDENT CONSTANTS: Number of differences = 0 LOOKUP: Number of differences = 0 DATA FIELDS: Number of fields with differences = 0 files compare, ignoring Fixed Length Header
This means that it is possible to re-run a UKCA job-step, and assuming that the dump frequency is the same (and that they started from the same dump), then the results will be reproducible.
change of dump frequency test (MONSooN)
In this test a 2-day long run is performed with daily dumping (in a single job-step), and then a 2-day run is performed with 2-day dumping. In this case, these dumps DO NOT bit-compare.
COMPARE - SUMMARY MODE ----------------------- Number of fields in file 1 = 14272 Number of fields in file 2 = 14272 Number of fields compared = 14272 FIXED LENGTH HEADER: Number of differences = 3 INTEGER HEADER: Number of differences = 0 REAL HEADER: Number of differences = 3 LEVEL DEPENDENT CONSTANTS: Number of differences = 0 LOOKUP: Number of differences = 0 DATA FIELDS: Number of fields with differences = 12221 Field 1 : Stash Code 2 : U COMPNT OF WIND AFTER TIMESTEP : Number of differences = 27840 ... ... Field 14076 : Stash Code 38405 : DRY PARTICLE DIAMETER AITKEN-INS : Number of differences = 68 files DO NOT compare
This may also be to do with the way certain fields are initialised in UKCA. You should therefore try to maintain the 10-day dumping frequency. If this is done, and the job-steps are consistently a month long, then a repeated run of this configuration will be bit-reproducible, as the CRUN-CRUN test was passed.
This should be compared to the equivalent test performed on ARCHER, which passed.
Initial conditions and forcing
xkawa
was initialised from the final dump ofxjcin
(dated 2015-12-01), then re-dated usingchange_dump_date
to 1999-12-01.- See
/projects/ukca/inputs/initial/vn84GA4_UKCA.19991201_00.txt
- See
- SSTs and sea-ice use daily values from the Reynolds dataset, produced by meaning over the transient values from 1995-01-01 to 2005-01-01 using
cdo ydaymean
.- See
/projects/ukca/inputs/ancil/surf/reynolds.qrclim.sst.avg2000.txt
for SSTs. - See
/projects/ukca/inputs/ancil/surf/reynolds.qrclim.seaice.avg2000.txt
for the sea-ice. - Note: there was a minor error with these files, in that the time is set to midnight and not noon. However, this is unlikely to cause any major problems.
- See
- Time-slice conditions for the year 2000 (actual date 2000-12-01), known as TS2000, were used using the RCP scenario conditions for GHGs and WMO2011 values for ODSs.
- These are the forcings specified for the CCMI transient REF-C1/2 simulations
- These values are set in the Spec of trace gases section of the UMUI
- Note that CFC-114 is only used in UKCA and not in the radiation scheme (as the spectral file does not consider CFC-114). This is done with the hand-edit
~ukca/hand_edits/VN8.4/CFC-114_not_in_Rad.ed
.
- Note that CFC-114 is only used in UKCA and not in the radiation scheme (as the spectral file does not consider CFC-114). This is done with the hand-edit
- These were calculated using the
scenario
function on PUMA:
$ /home/ukca/bin/scenario 2000/12/01 USER USER-SUPPLIED SCENARIO SELECTED. PLEASE INPUT FILENAME /home/ukca/tools/scenario/RCP6_MIDYR_CONC_WMO2011_CCMI.DAT ----------------------------------------------- | 2000/12/01 USER SCENARIO: | ----------------------------------------------- | CFCl3 = 1.23542E-09 CFC11/F11 | | CF2Cl2 = 2.26638E-09 CFC12/F12 | | CF2ClCFCl2 = 5.29666E-10 CFC113/F113 | | CF2ClCF2Cl = 9.73663E-11 CFC114/F114 | | CF2ClCF3 = 4.25934E-11 CFC115/F115 | | CCl4 = 5.19557E-10 | | MeCCl3 = 1.95889E-10 CH3CCl3 | | CHF2Cl = 4.31321E-10 HCFC22 | | MeCFCl2 = 5.35084E-11 HCFC141b | | MeCF2Cl = 4.24961E-11 HCFC142b | | CF2ClBr = 2.34011E-11 H1211 | | CF2Br2 = 2.74854E-13 H1202 | | CF3Br = 1.46645E-11 H1301 | | CF2BrCF2Br = 4.48740E-12 H2402 | | MeCl = 9.58777E-10 CH3Cl | | MeBr = 2.80100E-11 CH3Br | | CH2Br2 = 1.80186E-11 | | N2O = 4.80116E-07 | | CH4 = 9.67017E-07 | | CF3CHF2 = 6.18271E-12 HFC125 | | CH2FCF3 = 5.43855E-11 HFC134a | | H2 = 3.45280E-08 | | N2 = 7.54682E-01 | | CO2 = 5.61246E-04 | ----------------------------------------------- UM/UKCA LBC MMRs for: 2000/12/01, using the USER scenario VALUES FOR USE IN THE UMUI (ZERO VALUES CAN BE TREATED AS "Excluded"): CH4 = 9.670E-07 N2O = 4.801E-07 CFC11 = 1.235E-09 CFC12 = 2.266E-09 CFC113 = 5.297E-10 HCFC22 = 4.313E-10 HFC125 = 6.183E-12 HFC134a = 5.439E-11 CO2 = 5.61246E-04 VALUES FOR USE IN THE UKCA HAND-EDIT: MeBrMMR=2.80100E-11, MeClMMR=9.58777E-10, CH2Br2MMR=1.80186E-11, H2MMR=3.45280E-08, N2MMR=0.75468 , CFC114MMR=9.73663E-11, CFC115MMR=4.25934E-11, CCl4MMR=5.19557E-10, MeCCl3MMR=1.95889E-10, HCFC141bMMR=5.35084E-11, HCFC142bMMR=4.24961E-11, H1211MMR=2.34011E-11, H1202MMR=2.74854E-13, H1301MMR=1.46645E-11, H2402MMR=4.48740E-12,
- AR5 emissions are used for the CheST chemistry, with MeOH emissions coming from the MEGAN model.
ARCHER port: xkawe
This job has been ported to ARCHER as job xkawe
, which included the updates to the FCM branch to revision number r16246, as stated above. More information about ARCHER can be found at www.archer.ac.uk.
Ported Model
The development of this job is very similar to xkawa
as described in the base model section above, but branches off from job xjcim
like so:
xjcim
(made TS2000 - see Initial conditions and forcing) owned by Luke Abraham
xjnjb
(ARCHER port of xjcim
, with some bugfixes) owned by Karthee Sivalingam
xjqka
(UKCA Tutorials base job; some branch consolidation and use of pre-compiled builds) owned by Luke Abraham
xjrna
(direct copy of xjqka
) owned by ukca
UMUI user
xkawe
(code changes etc. as per xkawa
but with ARCHER bugfixes at r16246) owned by Luke Abraham
Scaling (ARCHER)
Each compute node contains two 2.7 GHz, 12-core Ivy Bridge processors, which can support 2 hardware threads, and there is 64GB of RAM per node. Due to memory restrictions, UKCA is unable to run on less than 6 nodes (meaning that the 4-node debug queue is not available). As noted below, the EW domain decomposition needed to be a multiple of 12. All simulations used 2 OpenMP threads (halving the number of cores available per node). Only 12EW decomposition was used, as the scaling tests on MONSooN showed that this was preferable over the 24EW decomposition.
Scaling tests have been done from 6 to 26 nodes of ARCHER with a series of 1-day runs, with the results presented below.
The speedup in the plot above is calculated by assuming a linear scaling from 6 nodes down to 1 node. 5 simulations were performed for each number of nodes, and the envelope is 2 standard deviations (assuming that the standard deviation of the extrapolated 1-node data-point is the mean of the standard deviations of all other points). From these tests the recommended decomposition is 12 EW x 12 NS (i.e. 12 nodes, or 144 cores), although any number of nodes from 6-12 should cost approximately the same amount of allocation units as there is linear scaling. Above 12 nodes the model will still run quicker, but as the scaling is no longer linear this will 'cost' more per model year. The model should not be run on more than 24 nodes, as the model will then become slower than if run in a 12EWx24NS decomposition.
Also note that the model run length has a much larger standard deviation ("jitter") on ARCHER than on MONSooN. Users should ensure that the requested run-time is at least 10% longer than the estimated run-time to ensure that the model does not exceed this limit due to this jitter.
cumf
tests (ARCHER)
As was done for MONSooN, cumf
tests were also done on ARCHER. The utility can be found at /work/n02/n02/hum/vn8.4/cce/utils/cumf
.
All tests were run without STASH, climate meaning, or the UKCA evaluation suite hand-edit (~mdalvi/umui_jobs/hand_edits/vn8.4/add_ukca_eval1_diags_l85.ed
), as all of these can affect the dump by placing temporary fields in it. The model was run for 2 days, either with daily or 2-day dumping, and for the NRUN-CRUN test, the first step was for 1 day followed by a new job step for the 2nd day. Reconfiguration was only run once, at the start of the 1st test, and after that point the same .astart
file was used by all jobs.
NRUN-NRUN tests (ARCHER)
For this test the model is run twice. The 2-day dumps are then compared. For this test it makes no difference if you compare the dumps produced using daily-dumping or 2-day dumping, as both pass this test (when compared to the equivalent dump produced using the same dumping frequency).
COMPARE - SUMMARY MODE ----------------------- Number of fields in file 1 = 14272 Number of fields in file 2 = 14272 Number of fields compared = 14272 FIXED LENGTH HEADER: Number of differences = 2 INTEGER HEADER: Number of differences = 0 REAL HEADER: Number of differences = 0 LEVEL DEPENDENT CONSTANTS: Number of differences = 0 LOOKUP: Number of differences = 0 DATA FIELDS: Number of fields with differences = 0 files compare, ignoring Fixed Length Header
NRUN-CRUN tests (ARCHER)
For this test the 2nd day dump of a daily dumping run (which has been run in a single jobstep) is compared with the 2nd day dump of a run where this was produced on a CRUN step (i.e. where the 1st day dump was produced on the NRUN step). In this case, the dumps DO NOT compare.
COMPARE - SUMMARY MODE ----------------------- Number of fields in file 1 = 14272 Number of fields in file 2 = 14272 Number of fields compared = 14272 FIXED LENGTH HEADER: Number of differences = 3 INTEGER HEADER: Number of differences = 0 REAL HEADER: Number of differences = 3 LEVEL DEPENDENT CONSTANTS: Number of differences = 0 LOOKUP: Number of differences = 0 DATA FIELDS: Number of fields with differences = 12221 Field 1 : Stash Code 2 : U COMPNT OF WIND AFTER TIMESTEP : Number of differences = 27840 ... ... Field 14076 : Stash Code 38405 : DRY PARTICLE DIAMETER AITKEN-INS : Number of differences = 69 files DO NOT compare
This is not unexpected for UKCA, as there are many variables which are initialised at the start of a run, but not saved to a dump to be re-initialised correctly. This is a feature which will need to be addressed in the future.
It should be noted that this does not invalidate a run, or prevent you from re-running to fill-in data gaps. You should, however, ensure that you maintain the original job-step length. On MONSooN is it recommended that maintain a 1-month jobstep length, with the standard climate dumping frequency of 10-days.
CRUN-CRUN tests (ARCHER)
For this test the model is run a second time as NRUN-CRUN jobsteps. The 2-day dump from the 1st CRUN test is then compared with this newly generated 2-day dump from the 2nd CRUN. This test bit-compares.
COMPARE - SUMMARY MODE ----------------------- Number of fields in file 1 = 14272 Number of fields in file 2 = 14272 Number of fields compared = 14272 FIXED LENGTH HEADER: Number of differences = 3 INTEGER HEADER: Number of differences = 0 REAL HEADER: Number of differences = 0 LEVEL DEPENDENT CONSTANTS: Number of differences = 0 LOOKUP: Number of differences = 0 DATA FIELDS: Number of fields with differences = 0 files compare, ignoring Fixed Length Header
This means that it is possible to re-run a UKCA job-step, and assuming that the dump frequency is the same (and that they started from the same dump), then the results will be reproducible.
change of dump frequency test (ARCHER)
In this test a 2-day long run is performed with daily dumping (in a single job-step), and then a 2-day run is performed with 2-day dumping. In this case, these dumps bit-compare.
COMPARE - SUMMARY MODE ----------------------- Number of fields in file 1 = 14272 Number of fields in file 2 = 14272 Number of fields compared = 14272 FIXED LENGTH HEADER: Number of differences = 3 INTEGER HEADER: Number of differences = 0 REAL HEADER: Number of differences = 0 LEVEL DEPENDENT CONSTANTS: Number of differences = 0 LOOKUP: Number of differences = 0 DATA FIELDS: Number of fields with differences = 0 files compare, ignoring Fixed Length Header
Compare this to MONSooN, where this test failed. This means that on ARCHER, if you need to change the dump frequency for some reason at some point during a run, the run will still bit-compare to a run where this was not done. However, you should still try to maintain the 10-day dumping frequency.
Known Issues
Interactive Dry Deposition Scheme
Currently it is possible to request dry-deposition for a species in the ukca_chem_strattrop.F90
module (the first 1 in the last three columns of numbers) e.g.
! 30 DD:12,WD:12, chch_t( 30,'HCl ', 1,'TR ',' ', 1, 1, 0), &
but if values for the required species have not been set in ukca_aerod.F90
and ukca_surfddr.F90
then no dry deposition will in fact be calculated. Please see UKCA Chemistry and Aerosol Tutorial 7 (Adding dry deposition of chemical species) for details as to how to add new values.
Because of this, you should see warning messages such as this in the .leave file:
? Warning Message: Surface resistance values not set for HCl ? Warning Message: Surface resistance values not set for HOCl ? Warning Message: Surface resistance values not set for HBr ? Warning Message: Surface resistance values not set for HOBr ? Warning Message: Surface resistance values not set for DMSO ? Warning Message: Surface resistance values not set for Monoterp ? Warning Message: Surface resistance values not set for Sec_Org
Currently none of the above species (HCl, HOCl, HBr, HOBr, DMSO, Monoterp, or Sec_Org) are in fact dry deposited in this job configuration.
Low Stratospheric NOy
There is an issue with low stratospheric NOy in UKCA, as can be seen in the profiles of HNO3 above (calculated by meaning over the whole 10-year simulation.), and it is currently being investigated. For more information, see details from the NOy PEG.
High Stratospheric Sea-Salt Mixing Ratios
As Graham Mann notes below in the aerosol evaluation, there are high sea-salt mixing ratios in the stratosphere.
High Aerosol Optical Depth
As Jane Mulcahy notes below in the aerosol evaluation, this model configuration has high aerosol optical depth.
Reconfiguration Issues
Section 34, Item 163 (CLOUD DROPLET NO CONC^(-1/3) (m))
While field s34i163 does exist in the input dump, if reconfiguration is requested this will fail with an error unless an initial condition is supplied for this field. For more information see [1]. It is being investigated.
The file /projects/ukca/nlabra/ANCILS_N96L85/s34i163_Dec.anc
contains the field from the initial dump (/projects/ukca/inputs/initial/vn84GA4_UKCA.19991201_00
) and can be used in the Initialisation of user prognostics UMUI panel.
East-West Decomposition
On both MONSooN and ARCHER, the model is unable to run unless the East-West decomposition is a multiple of 12 (i.e. 12, 24 etc). This limits the possible domain decompositions, which must be multiples of 32 on MONSooN and 24 on ARCHER, to fit within the nodes efficiently.
MONSooN decomposition errors
On MONSooN, if running without multiple of 12 for the EW decomposition the job will exit with a floating point exception.
ARCHER decomposition errors
On ARCHER, if running without a multiple of 12 for the EW decomposition the job will often exit with a segmentation fault in the ukca_calc_tropopause
routine. This is the output when setting the ATP_ENABLED
environment variable to 1 (set in Script Inserts and Modifications):
Application 9844563 is crashing. ATP analysis proceeding... ATP Stack walkback for Rank 19 starting: _start@start.S:113 __libc_start_main@libc-start.c:226 flumemain_@flumeMain.f90:48 um_shell_@um_shell.f90:1865 u_model_@u_model.f90:2931 ukca_main1_@ukca_main1-ukca_main1.f90:4848 ukca_calc_tropopause$ukca_tropopause_@ukca_tropopause.f90:178 ATP Stack walkback for Rank 19 done Process died with signal 11: 'Segmentation fault' Forcing core dumps of ranks 19, 0
Failing NRUN-CRUN tests
See the explanation of this test for MONSooN or ARCHER. The UKCA code management group is aware of this.
It should be noted that on MONSooN this configuration also fails the change of dump frequency test, whereas this is passed on ARCHER.
Further Work Needed
Further work will need to be done to:
- Link the GLOMAP-mode aerosol to the heterogeneous reactions, especially for the stratospheric chemistry.
- Link the GLOMAP-mode aerosol to the Fast-JX interactive photolysis scheme.
- Extend the RCP scenario code to
atmos_physics1.F90
to all the values of CO2, CH4, N2O etc. seen by the radiation scheme to be updated in the same way as for the chemistry. - Tidy-up the AerChem chemistry extensions required for GLOMAP-mode, so that they match better those for the TropIsop/CheT scheme.
- Link to the JULES land-surface scheme to allow for interactive isoprene and monoterpene emissions.
Results (MONSooN)
MOOSE
All results from this run were saved to MOOSE, and can be found at moose:/crum/xkawa
. As well as the standard pp-output, monthly, seasonal, and annual supermeans were created and are also available in the ama.pp
directory.
Running the command moo ls -l moose:/crum/xkawa
gives
C colin.johnson 45.65 GBP 421803130880 2014-07-20 18:27:13 GMT moose:/crum/xkawa/ada.file C colin.johnson 3.09 GBP 28512510160 2014-07-24 15:56:40 GMT moose:/crum/xkawa/ama.pp C colin.johnson 20.50 GBP 189410089848 2014-07-25 11:20:50 GMT moose:/crum/xkawa/apa.pp C colin.johnson 24.85 GBP 229627024000 2014-07-25 11:22:33 GMT moose:/crum/xkawa/apb.pp C colin.johnson 20.95 GBP 193541722824 2014-07-20 20:25:13 GMT moose:/crum/xkawa/apm.pp C colin.johnson 6.93 GBP 63989055776 2014-07-20 18:31:17 GMT moose:/crum/xkawa/aps.pp C colin.johnson 1.73 GBP 16005498776 2014-07-20 18:32:26 GMT moose:/crum/xkawa/apy.pp
Further information on how to use MOOSE can be found on the collaboration twiki.
Note: If you take a copy of this job and run it, you must first manually make the MOOSE set to hold the data in the archive. This is done by
moo mkset --project-owner=project-YOUR_MONSooN_PROJECT -v moose:/crum/jobid
For instance, if you were in the UKCA project you would have --project-owner=project-ukca
. This can be done after the job has started running. The archiving intelligently knows which files need archiving through the use of files named archive_XXXXXX.do
. The files also control the deleting of files and dumps once they have been archived or are no longer needed. If, for some reason, the files cannot be archived (e.g. MOOSE is down or the set has not yet been made) then the files will not be deleted. They will continue being generated and existing on the /projects
disk until they can be archived.
You should not need to do anything with the fieldsfiles until the whole simulation has been completed (in this case, the whole 10-years). When it does you will find that, while the climate mean files and dumps have been archived, the last files in the e.g. *.pa*
or *.pb*
streams etc will not have been. You will need to archive these manually by, e.g.
moo put -f -vv -c=umpp jobida.pzYYYYmmm moose:/crum/jobid/apz.pp/jobida.pzYYYYmmm.pp
Where the -c=umpp
converts the files from 64-bit fieldsfiles to 32-bit pp-files. Remember to put the .pp
at the end of the name of the file in the set on MOOSE.
Evaluation Suite Output
A set of standard results from a mean of the 10-year run, as well as from each of the 10 years can be found in the following documents.
These were generated from the UKCA Evaluation Suite available on the MONSooN post-processor.
Mean over the 10-year simulation
Results from individual years
- Xkawa_EvalChemAer_yr01.pdf
- Xkawa_EvalChemAer_yr02.pdf
- Xkawa_EvalChemAer_yr03.pdf
- Xkawa_EvalChemAer_yr04.pdf
- Xkawa_EvalChemAer_yr05.pdf
- Xkawa_EvalChemAer_yr06.pdf
- Xkawa_EvalChemAer_yr07.pdf
- Xkawa_EvalChemAer_yr08.pdf
- Xkawa_EvalChemAer_yr09.pdf
- Xkawa_EvalChemAer_yr10.pdf
Aerosol Evaluation
Graham Mann has kindly produced the following plots for GLOMAP-mode evaluation:
Graham commented that: "The only issue I'd say is that there seems to be a problem with an anomalously high sea-salt mixing ratio in the stratosphere in these runs."
Jane Mulcahy has calculated the aerosol optical depth from the GLOMAP-mode fields, and has provided the following plots:
Jane has commented: "In my opinion the AODs are looking quite high particularly in spring and summer over anthropogenic regions. This is symptomatic of problems we are also seeing in our latest GA6 based runs. Looking at the surface sulphate and SO2 evaluation in Grahams plots this also looks high over Europe. So it is possible that there is insufficient removal of SO2 (no gas phase plume scavenging as yet). (The) biomass burning is also looking low in JJA. (I) would also caution users about high AOD."
Lightning NOx
The average annual Lightning NOx emitted is 4.03285 Tg(N)/year over the whole 10-year simulation.
The lightning NOx emitted in each of the individual years of the run is:
- year 01 4.06726 Tg(N)/year
- year 02 4.01840 Tg(N)/year
- year 03 4.06754 Tg(N)/year
- year 04 4.08320 Tg(N)/year
- year 05 3.99700 Tg(N)/year
- year 06 3.96347 Tg(N)/year
- year 07 4.01116 Tg(N)/year
- year 08 4.03512 Tg(N)/year
- year 09 4.04277 Tg(N)/year
- year 10 4.04452 Tg(N)/year
STASH Table
Below is a listing of all the STASH requests that were output by the model.
The output was sent to three different usage profiles, corresponding to:
- UPA: These files contain daily output, and go to the
*.pa*.pp
files, held in theapa.pp
directory on MOOSE. - UPB: These files contain monthly out from UKCA that could not fit in the climate meaning stream due to space limitations. These go to the
*.pb*.pp
files, held in theapb.pp
directory on MOOSE. - UPMEAN: This is the climate meaning stream, and holds a large number of dynamical and UKCA related diagnostics. These go to the:
*.pm*.pp
files for monthly means, held in theapm.pp
directory on MOOSE.*.ps*.pp
files for seasonal means, held in theaps.pp
directory on MOOSE.*.py*.pp
files for annual means, held in theapy.pp
directory on MOOSE.- no decadal means were created during this run, but if they were, they would be
*.px*.pp
files, held in theapx.pp
directory on MOOSE.
Section | Item | Name | Time Profile | Domain Profile | Usage Profile |
0 | 4 | THETA AFTER TIMESTEP | TDMPMN | DALLTH | UPMEAN |
0 | 10 | SPECIFIC HUMIDITY AFTER TIMESTEP | TDMPMN | DALLTH | UPMEAN |
0 | 12 | QCF AFTER TIMESTEP | TDMPMN | DALLTH | UPMEAN |
0 | 23 | SNOW AMOUNT OVER LAND AFT TSTP KG/M | TDMPMN | DIAG | UPMEAN |
0 | 24 | SURFACE TEMPERATURE AFTER TIMESTEP | TDAYM | DIAG | UPA |
0 | 24 | SURFACE TEMPERATURE AFTER TIMESTEP | TDMPMN | DIAG | UPMEAN |
0 | 25 | BOUNDARY LAYER DEPTH AFTER TIMESTEP | TDMPMN | DIAG | UPMEAN |
0 | 28 | SURFACE ZONAL CURRENT AFTER TIMESTE | TDMPMN | DIAG | UPMEAN |
0 | 29 | SURFACE MERID CURRENT AFTER TIMESTE | TDMPMN | DIAG | UPMEAN |
0 | 31 | FRAC OF SEA ICE IN SEA AFTER TSTEP | TDMPMN | DIAG | UPMEAN |
0 | 32 | SEA ICE DEPTH (MEAN OVER ICE) | TDMPMN | DIAG | UPMEAN |
0 | 58 | SULPHUR DIOXIDE EMISSIONS | TDMPMN | DIAG | UPMEAN |
0 | 59 | DIMETHYL SULPHIDE EMISSIONS (ANCIL) | TDMPMN | DIAG | UPMEAN |
0 | 101 | SO2 MASS MIXING RATIO AFTER TSTEP | TDMPMN | DALLTH | UPMEAN |
0 | 102 | DIMETHYL SULPHIDE MIX RAT AFTER TS | TDMPMN | DALLTH | UPMEAN |
0 | 103 | SO4 AITKEN MODE AEROSOL AFTER TSTEP | TDMPMN | DALLTH | UPMEAN |
0 | 104 | SO4 ACCUM. MODE AEROSOL AFTER TSTEP | TDMPMN | DALLTH | UPMEAN |
0 | 105 | SO4 DISSOLVED AEROSOL AFTER TSTEP | TDMPMN | DALLTH | UPMEAN |
0 | 121 | 3D NATURAL SO2 EMISSIONS KG/M2/S | TDMPMN | DALLTH | UPMEAN |
0 | 126 | HIGH LEVEL SO2 EMISSIONS KG/M2/S | TDMPMN | DIAG | UPMEAN |
0 | 132 | DMS CONCENTRATION IN SEAWATER | TDMPMN | DIAG | UPMEAN |
0 | 211 | CCA WITH ANVIL AFTER TIMESTEP | TDMPMN | DALLTH | UPMEAN |
0 | 254 | QCL AFTER TIMESTEP | TDMPMN | DALLTH | UPMEAN |
0 | 266 | BULK CLOUD FRACTION IN EACH LAYER | TDMPMN | DALLTH | UPMEAN |
0 | 301 | NOx surf emissions | TDMPUKC3 | DIAG | UPMEAN |
0 | 302 | CH4 surf emissions | TDMPUKC3 | DIAG | UPMEAN |
0 | 303 | CO surf emissions | TDMPUKC3 | DIAG | UPMEAN |
0 | 309 | C5H8 surf emissions | TDMPUKC3 | DIAG | UPMEAN |
0 | 310 | BC fossil fuel surf emissions | TDMPUKC3 | DIAG | UPMEAN |
0 | 311 | BC biofuel surf emissions | TDMPUKC3 | DIAG | UPMEAN |
0 | 312 | OC fossil fuel surf emissions | TDMPUKC3 | DIAG | UPMEAN |
0 | 313 | OC biofuel surf emissions | TDMPUKC3 | DIAG | UPMEAN |
0 | 314 | Monoterpene surf emissions | TDMPUKC3 | DIAG | UPMEAN |
0 | 322 | BC BIOMASS 3D EMISSION | TDMPUKC3 | DALLTH | UPMEAN |
0 | 323 | OC BIOMASS 3D EMISSION | TDMPUKC3 | DALLTH | UPMEAN |
0 | 340 | NOX AIRCRAFT EMS IN KG/S/GRIDCELL | TDMPUKC3 | DALLTH | UPMEAN |
0 | 407 | PRESSURE AT RHO LEVELS AFTER TS | TDMPMN | DALLRH | UPMEAN |
0 | 408 | PRESSURE AT THETA LEVELS AFTER TS | TDMPMN | DALLTH | UPMEAN |
0 | 409 | SURFACE PRESSURE AFTER TIMESTEP | TDMPMN | DIAG | UPMEAN |
0 | 507 | OPEN SEA SURFACE TEMP AFTER TIMESTE | TDMPMN | DIAG | UPMEAN |
0 | 509 | SEA ICE ALBEDO AFTER TS | TDMPMN | DIAG | UPMEAN |
1 | 201 | NET DOWN SURFACE SW FLUX: SW TS ONL | TDMPMN | DIAG | UPMEAN |
1 | 203 | NET DN SW RAD FLUX:OPEN SEA:SEA MEA | TDMPMN | DIAG | UPMEAN |
1 | 207 | INCOMING SW RAD FLUX (TOA): ALL TSS | TDMPMN | DIAG | UPMEAN |
1 | 208 | OUTGOING SW RAD FLUX (TOA) | TDMPMN | DIAG | UPMEAN |
1 | 209 | CLEAR-SKY (II) UPWARD SW FLUX (TOA) | TDMPMN | DIAG | UPMEAN |
1 | 210 | CLEAR-SKY (II) DOWN SURFACE SW FLUX | TDMPMN | DIAG | UPMEAN |
1 | 211 | CLEAR-SKY (II) UP SURFACE SW FLUX | TDMPMN | DIAG | UPMEAN |
1 | 221 | LAYER CLD LIQ RE * LAYER CLD WEIGHT | TDMPMN | DALLTHCL | UPMEAN |
1 | 223 | LAYER CLOUD WEIGHT FOR MICROPHYSICS | TDMPMN | DALLTHCL | UPMEAN |
1 | 225 | CONV CLOUD LIQ RE * CONV CLD WEIGHT | TDMPMN | DALLTHCL | UPMEAN |
1 | 226 | CONV CLOUD WEIGHT FOR MICROPHYSICS | TDMPMN | DALLTHCL | UPMEAN |
1 | 235 | TOTAL DOWNWARD SURFACE SW FLUX | TDMPMN | DIAG | UPMEAN |
1 | 241 | DROPLET NUMBER CONC * LYR CLOUD WGT | TDMPMN | DALLTHCL | UPMEAN |
1 | 242 | LAYER CLOUD LWC * LAYER CLOUD WEIGH | TDMPMN | DALLTHCL | UPMEAN |
1 | 280 | COLUMN-INTEGRATED Nd * SAMP. WEIGHT | TDMPMN | DIAG | UPMEAN |
1 | 281 | SAMP. WEIGHT FOR COL. INT. Nd | TDMPMN | DIAG | UPMEAN |
1 | 282 | 2-D CLOUD-TOP CDNC x WEIGHT (cm-3) | TDMPMN | DIAG | UPMEAN |
1 | 283 | WEIGHT FOR 2-D CLOUD-TOP CDNC | TDMPMN | DIAG | UPMEAN |
2 | 201 | NET DOWN SURFACE LW RAD FLUX | TDMPMN | DIAG | UPMEAN |
2 | 203 | NET DN LW RAD FLUX:OPEN SEA:SEA MEA | TDMPMN | DIAG | UPMEAN |
2 | 204 | TOTAL CLOUD AMOUNT IN LW RADIATION | TDMPMN | DIAG | UPMEAN |
2 | 205 | OUTGOING LW RAD FLUX (TOA) | TDMPMN | DIAG | UPMEAN |
2 | 206 | CLEAR-SKY (II) UPWARD LW FLUX (TOA) | TDMPMN | DIAG | UPMEAN |
2 | 207 | DOWNWARD LW RAD FLUX: SURFACE | TDMPMN | DIAG | UPMEAN |
2 | 208 | CLEAR-SKY (II) DOWN SURFACE LW FLUX | TDMPMN | DIAG | UPMEAN |
2 | 251 | AITKEN MODE (SOLUBLE) STRATO AOD | TDAYM | DIAGAOT | UPA |
2 | 251 | AITKEN MODE (SOLUBLE) STRATO AOD | TDMPMN | DIAGAOT | UPMEAN |
2 | 252 | ACCUM MODE (SOLUBLE) STRATO AOD | TDAYM | DIAGAOT | UPA |
2 | 252 | ACCUM MODE (SOLUBLE) STRATO AOD | TDMPMN | DIAGAOT | UPMEAN |
2 | 253 | COARSE MODE (SOLUBLE) STRATO AOD | TDAYM | DIAGAOT | UPA |
2 | 253 | COARSE MODE (SOLUBLE) STRATO AOD | TDMPMN | DIAGAOT | UPMEAN |
2 | 254 | AITKEN MODE (INSOL) STRATO AOD | TDAYM | DIAGAOT | UPA |
2 | 254 | AITKEN MODE (INSOL) STRATO AOD | TDMPMN | DIAGAOT | UPMEAN |
2 | 255 | ACCUM MODE (INSOL) STRATO AOD | TDAYM | DIAGAOT | UPA |
2 | 255 | ACCUM MODE (INSOL) STRATO AOD | TDMPMN | DIAGAOT | UPMEAN |
2 | 256 | COARSE MODE (INSOL) STRATO AOD | TDAYM | DIAGAOT | UPA |
2 | 256 | COARSE MODE (INSOL) STRATO AOD | TDMPMN | DIAGAOT | UPMEAN |
2 | 284 | SULPHATE OPTICAL DEPTH IN RADIATION | TDMPMN | DIAGAOT | UPMEAN |
2 | 285 | MINERAL DUST OPTICAL DEPTH IN RADN. | TDMPMN | DIAGAOT | UPMEAN |
2 | 298 | TOTAL OPTICAL DEPTH IN RADIATION | TDMPMN | DIAGAOT | UPMEAN |
2 | 300 | AITKEN MODE (SOLUBLE) OPTICAL DEPTH | TDAYM | DIAGAOT | UPA |
2 | 300 | AITKEN MODE (SOLUBLE) OPTICAL DEPTH | TDMPMN | DIAGAOT | UPMEAN |
2 | 301 | ACCUM MODE (SOLUBLE) OPTICAL DEPTH | TDAYM | DIAGAOT | UPA |
2 | 301 | ACCUM MODE (SOLUBLE) OPTICAL DEPTH | TDMPMN | DIAGAOT | UPMEAN |
2 | 302 | COARSE MODE (SOLUBLE) OPTICAL DEPTH | TDAYM | DIAGAOT | UPA |
2 | 302 | COARSE MODE (SOLUBLE) OPTICAL DEPTH | TDMPMN | DIAGAOT | UPMEAN |
2 | 303 | AITKEN MODE (INSOL) OPTICAL DEPTH | TDAYM | DIAGAOT | UPA |
2 | 303 | AITKEN MODE (INSOL) OPTICAL DEPTH | TDMPMN | DIAGAOT | UPMEAN |
2 | 304 | ACCUM MODE (INSOL) OPTICAL DEPTH | TDAYM | DIAGAOT | UPA |
2 | 304 | ACCUM MODE (INSOL) OPTICAL DEPTH | TDMPMN | DIAGAOT | UPMEAN |
2 | 305 | COARSE MODE (INSOL) OPTICAL DEPTH | TDAYM | DIAGAOT | UPA |
2 | 305 | COARSE MODE (INSOL) OPTICAL DEPTH | TDMPMN | DIAGAOT | UPMEAN |
2 | 422 | DUST OPTICAL DEPTH FROM PROGNOSTIC | TDMPMN | DIAGAOT | UPMEAN |
3 | 217 | SURFACE SENSIBLE HEAT FLUX W/M | TDMPMN | DIAG | UPMEAN |
3 | 223 | SURFACE TOTAL MOISTURE FLUX KG/M2/ | TDMPMN | DIAG | UPMEAN |
3 | 224 | WIND MIX EN'GY FL TO SEA:SEA MN W/M | TDMPMN | DIAG | UPMEAN |
3 | 225 | 10 METRE WIND U-COMP B GRID | TDMPMN | DIAG | UPMEAN |
3 | 226 | 10 METRE WIND V-COMP B GRID | TDMPMN | DIAG | UPMEAN |
3 | 232 | EVAP FROM OPEN SEA: SEA MEAN KG/M2/ | TDMPMN | DIAG | UPMEAN |
3 | 234 | SURFACE LATENT HEAT FLUX W/M | TDMPMN | DIAG | UPMEAN |
3 | 237 | SPECIFIC HUMIDITY AT 1.5M | TDMPMN | DIAG | UPMEAN |
3 | 245 | RELATIVE HUMIDITY AT 1.5M | TDMPMN | DIAG | UPMEAN |
3 | 261 | GROSS PRIMARY PRODUCTIVITY KG C/M2/ | TDMPMN | DIAG | UPMEAN |
3 | 262 | NET PRIMARY PRODUCTIVITY KG C/M2/S | TDMPMN | DIAG | UPMEAN |
3 | 263 | PLANT RESPIRATION KG/M2/S | TDMPMN | DIAG | UPMEAN |
3 | 291 | NET PRIMARY PRODUCTIVITY ON PFTS | TDMPMN | DPFTS | UPMEAN |
3 | 293 | SOIL RESPIRATION KG C/M2/ | TDMPMN | DIAG | UPMEAN |
3 | 304 | TURBULENT MIXING HT AFTER B.LAYER m | TDMPMN | DIAG | UPMEAN |
3 | 305 | STABLE BL INDICATOR | TDMPMN | DIAG | UPMEAN |
3 | 307 | WELL_MIXED BL INDICATOR | TDMPMN | DIAG | UPMEAN |
3 | 310 | CUMULUS-CAPPED BL INDICATOR | TDMPMN | DIAG | UPMEAN |
3 | 332 | TOA OUTGOING LW RAD AFTER B.LAYER | TDMPMN | DIAG | UPMEAN |
3 | 392 | X-COMP OF MEAN SEA SURF STRESS N/M2 | TDMPMN | DIAG | UPMEAN |
3 | 394 | Y-COMP OF MEAN SEA SURF STRESS N/M2 | TDMPMN | DIAG | UPMEAN |
4 | 203 | LARGE SCALE RAINFALL RATE KG/M2/ | TDMPMN | DIAG | UPMEAN |
4 | 204 | LARGE SCALE SNOWFALL RATE KG/M2/ | TDMPMN | DIAG | UPMEAN |
4 | 216 | SO2 SCAVENGED BY LS PPN KG/M2/S | TDMPMN | DIAG | UPMEAN |
4 | 219 | SO4 DIS SCAVNGD BY LS PPN KG/M2/S | TDMPMN | DIAG | UPMEAN |
5 | 205 | CONVECTIVE RAINFALL RATE KG/M2/ | TDMPMN | DIAG | UPMEAN |
5 | 206 | CONVECTIVE SNOWFALL RATE KG/M2/ | TDMPMN | DIAG | UPMEAN |
5 | 214 | TOTAL RAINFALL RATE: LS+CONV KG/M2/ | TDMPMN | DIAG | UPMEAN |
5 | 215 | TOTAL SNOWFALL RATE: LS+CONV KG/M2/ | TDMPMN | DIAG | UPMEAN |
5 | 216 | TOTAL PRECIPITATION RATE KG/M2/ | TDMPMN | DIAG | UPMEAN |
5 | 231 | CAPE TIMESCALE (DEEP) | TDMPMN | DIAG | UPMEAN |
5 | 238 | SO2 SCAVENGED BY CONV PPN KG/M2/SEC | TDMPMN | DIAG | UPMEAN |
5 | 239 | SO4 AIT SCAVNGD BY CONV PPN KG/M2/S | TDMPMN | DIAG | UPMEAN |
5 | 240 | SO4 ACC SCAVNGD BY CONV PPN KG/M2/S | TDMPMN | DIAG | UPMEAN |
5 | 241 | SO4 DIS SCAVNGD BY CONV PPN KG/M2/S | TDMPMN | DIAG | UPMEAN |
5 | 269 | DEEP CONVECTION INDICATOR | TDMPMN | DIAG | UPMEAN |
5 | 270 | SHALLOW CONVECTION INDICATOR | TDMPMN | DIAG | UPMEAN |
5 | 272 | MID LEVEL CONVECTION INDICATOR | TDMPMN | DIAG | UPMEAN |
5 | 277 | DEEP CONV PRECIP RATE KG/M2/ | TDMPMN | DIAG | UPMEAN |
5 | 278 | SHALLOW CONV PRECIP RATE KG/M2/ | TDMPMN | DIAG | UPMEAN |
5 | 279 | MID LEVEL CONV PRECIP RATE KG/M2/ | TDMPMN | DIAG | UPMEAN |
5 | 320 | MASS FLUX DEEP CONVECTION | TDMPMN | D52TH | UPMEAN |
5 | 322 | MASS FLUX SHALLOW CONVECTION | TDMPMN | D52TH | UPMEAN |
5 | 323 | MASS FLUX MID-LEVEL CONVECTION | TDMPMN | D52TH | UPMEAN |
6 | 201 | X COMPONENT OF GRAVITY WAVE STRESS | TDMPMN | DALLTH | UPMEAN |
8 | 23 | SNOW MASS AFTER HYDROLOGY KG/M | TDMPMN | DIAG | UPMEAN |
8 | 208 | SOIL MOISTURE CONTENT | TDMPMN | DIAG | UPMEAN |
8 | 223 | SOIL MOISTURE CONTENT IN A LAYER | TDMPMN | DSOIL | UPMEAN |
8 | 225 | DEEP SOIL TEMP. AFTER HYDROLOGY DEG | TDMPMN | DSOIL | UPMEAN |
8 | 234 | SURFACE RUNOFF RATE KG/M2/ | TDMPMN | DIAG | UPMEAN |
8 | 235 | SUB-SURFACE RUNOFF RATE KG/M2/ | TDMPMN | DIAG | UPMEAN |
16 | 4 | TEMPERATURE ON THETA LEVELS | TDMPMN | DALLTH | UPMEAN |
16 | 222 | PRESSURE AT MEAN SEA LEVEL | TDMPMN | DIAG | UPMEAN |
30 | 112 | WBIG Set to 1 if w GT 1.0m/s | TDMPMN | DALLTH | UPMEAN |
30 | 114 | WBIG Set to 1 if w GT 0.1m/s | TDMPMN | DALLTH | UPMEAN |
30 | 201 | U COMPNT OF WIND ON P LEV/UV GRID | TDAYM | DP36CCM | UPA |
30 | 201 | U COMPNT OF WIND ON P LEV/UV GRID | TDMPMN | DP36CCM | UPMEAN |
30 | 202 | V COMPNT OF WIND ON P LEV/UV GRID | TDAYM | DP36CCM | UPA |
30 | 202 | V COMPNT OF WIND ON P LEV/UV GRID | TDMPMN | DP36CCM | UPMEAN |
30 | 203 | W COMPNT OF WIND ON P LEV/UV GRID | TDAYM | DP36CCM | UPA |
30 | 203 | W COMPNT OF WIND ON P LEV/UV GRID | TDMPMN | DP17 | UPMEAN |
30 | 203 | W COMPNT OF WIND ON P LEV/UV GRID | TDMPMN | DP36CCM | UPMEAN |
30 | 204 | TEMPERATURE ON P LEV/UV GRID | TDAYM | DP36CCM | UPA |
30 | 204 | TEMPERATURE ON P LEV/UV GRID | TDMPMN | DP36CCM | UPMEAN |
30 | 205 | SPECIFIC HUMIDITY ON P LEV/UV GRID | TDAYM | DP36CCM | UPA |
30 | 205 | SPECIFIC HUMIDITY ON P LEV/UV GRID | TDMPMN | DP36CCM | UPMEAN |
30 | 206 | RELATIVE HUMIDITY ON P LEV/UV GRID | TDAYM | DP36CCM | UPA |
30 | 206 | RELATIVE HUMIDITY ON P LEV/UV GRID | TDMPMN | DP36CCM | UPMEAN |
30 | 207 | GEOPOTENTIAL HEIGHT ON P LEV/UV GRI | TDAYM | DP36CCM | UPA |
30 | 207 | GEOPOTENTIAL HEIGHT ON P LEV/UV GRI | TDMPMN | DP36CCM | UPMEAN |
30 | 208 | OMEGA ON P LEV/UV GRID | TDAYM | DP36CCM | UPA |
30 | 208 | OMEGA ON P LEV/UV GRID | TDMPMN | DP17 | UPMEAN |
30 | 208 | OMEGA ON P LEV/UV GRID | TDMPMN | DP36CCM | UPMEAN |
30 | 301 | HEAVYSIDE FN ON P LEV/UV GRID | TDAYM | DP36CCM | UPA |
30 | 301 | HEAVYSIDE FN ON P LEV/UV GRID | TDMPMN | DP36CCM | UPMEAN |
30 | 310 | RESIDUAL MN MERID. CIRC. VSTARBAR | TDAYM | DP36CCM | UPA |
30 | 310 | RESIDUAL MN MERID. CIRC. VSTARBAR | TDMPMN | DP36CCM | UPMEAN |
30 | 311 | RESIDUAL MN MERID. CIRC. WSTARBAR | TDAYM | DP36CCM | UPA |
30 | 311 | RESIDUAL MN MERID. CIRC. WSTARBAR | TDMPMN | DP36CCM | UPMEAN |
30 | 312 | ELIASSEN-PALM FLUX (MERID. COMPNT) | TDAYM | DP36CCM | UPA |
30 | 312 | ELIASSEN-PALM FLUX (MERID. COMPNT) | TDMPMN | DP36CCM | UPMEAN |
30 | 313 | ELIASSEN-PALM FLUX (VERT. COMPNT) | TDAYM | DP36CCM | UPA |
30 | 313 | ELIASSEN-PALM FLUX (VERT. COMPNT) | TDMPMN | DP36CCM | UPMEAN |
30 | 314 | DIVERGENCE OF ELIASSEN-PALM FLUX | TDAYM | DP36CCM | UPA |
30 | 314 | DIVERGENCE OF ELIASSEN-PALM FLUX | TDMPMN | DP36CCM | UPMEAN |
30 | 315 | MERIDIONAL HEAT FLUX | TDAYM | DP36CCM | UPA |
30 | 315 | MERIDIONAL HEAT FLUX | TDMPMN | DP36CCM | UPMEAN |
30 | 316 | MERIDIONAL MOMENTUM FLUX | TDAYM | DP36CCM | UPA |
30 | 316 | MERIDIONAL MOMENTUM FLUX | TDMPMN | DP36CCM | UPMEAN |
30 | 403 | TOTAL COLUMN DRY MASS RHO GRID | TDMPMN | DIAG | UPMEAN |
30 | 404 | TOTAL COLUMN WET MASS RHO GRID | TDMPMN | DIAG | UPMEAN |
30 | 405 | TOTAL COLUMN QCL RHO GRID | TDMPMN | DIAG | UPMEAN |
30 | 406 | TOTAL COLUMN QCF RHO GRID | TDMPMN | DIAG | UPMEAN |
30 | 419 | ENERGY CORR P GRID IN COLUMN W/M2 | TDMPMN | DIAG | UPMEAN |
30 | 451 | Pressure at Tropopause Level | TDMPMN | DIAG | UPMEAN |
30 | 452 | Temperature at Tropopause Level | TDMPMN | DIAG | UPMEAN |
30 | 453 | Height at Tropopause Level | TDMPMN | DIAG | UPMEAN |
34 | 1 | O3 MASS MIXING RATIO AFTER TIMESTEP | TDAYM | DALLTH | UPA |
34 | 1 | O3 MASS MIXING RATIO AFTER TIMESTEP | TDMPMN | DALLTH | UPMEAN |
34 | 2 | NO MASS MIXING RATIO AFTER TIMESTEP | TDMPMN | DALLTH | UPMEAN |
34 | 3 | NO3 MASS MIXING RATIO AFTER TIMESTE | TDMPMN | DALLTH | UPMEAN |
34 | 5 | N2O5 MASS MIXING RATIO AFTER TSTEP | TDMPMN | DALLTH | UPMEAN |
34 | 6 | HO2NO2 MASS MIXING RATIO AFTER TSTE | TDMPMN | DALLTH | UPMEAN |
34 | 7 | HONO2 MASS MIXING RATIO AFTER TSTEP | TDMPMN | DALLTH | UPMEAN |
34 | 8 | H2O2 MASS MIXING RATIO AFTER TSTEP | TDMPMN | DALLTH | UPMEAN |
34 | 9 | CH4 MASS MIXING RATIO AFTER TSTEP | TDMPMN | DALLTH | UPMEAN |
34 | 10 | CO MASS MIXING RATIO AFTER TSTEP | TDMPMN | DALLTH | UPMEAN |
34 | 11 | HCHO MASS MIXING RATIO AFTER TSTEP | TDMPMN | DALLTH | UPMEAN |
34 | 12 | MeOOH MASS MIXING RATIO AFTER TSTEP | TDMPMN | DALLTH | UPMEAN |
34 | 13 | HONO MASS MIXING RATIO AFTER TSTEP | TDMPMN | DALLTH | UPMEAN |
34 | 14 | C2H6 MASS MIXING RATIO AFTER TSTEP | TDMPMN | DALLTH | UPMEAN |
34 | 15 | EtOOH MASS MIXING RATIO AFTER TSTEP | TDMPMN | DALLTH | UPMEAN |
34 | 16 | MeCHO MASS MIXING RATIO AFTER TSTEP | TDMPMN | DALLTH | UPMEAN |
34 | 17 | PAN MASS MIXING RATIO AFTER TSTEP | TDMPMN | DALLTH | UPMEAN |
34 | 18 | C3H8 MASS MIXING RATIO AFTER TSTEP | TDMPMN | DALLTH | UPMEAN |
34 | 19 | n-PrOOH MASS MIXING RATIO AFTER TS | TDMPMN | DALLTH | UPMEAN |
34 | 20 | i-PrOOH MASS MIXING RATIO AFTER TS | TDMPMN | DALLTH | UPMEAN |
34 | 21 | EtCHO MASS MIXING RATIO AFTER TSTEP | TDMPMN | DALLTH | UPMEAN |
34 | 22 | Me2CO MASS MIXING RATIO AFTER TSTEP | TDMPMN | DALLTH | UPMEAN |
34 | 23 | MeCOCH2OOH MASS MIXING RATIO AFT TS | TDMPMN | DALLTH | UPMEAN |
34 | 24 | PPAN MASS MIXING RATIO AFTER TSTEP | TDMPMN | DALLTH | UPMEAN |
34 | 25 | MeONO2 MASS MIXING RATIO AFTER TSTE | TDMPMN | DALLTH | UPMEAN |
34 | 27 | C5H8 MASS MIXING RATIO AFTER TSTEP | TDMPMN | DALLTH | UPMEAN |
34 | 28 | ISOOH MASS MIXING RATIO AFTER TSTEP | TDMPMN | DALLTH | UPMEAN |
34 | 29 | ISON MASS MIXING RATIO AFTER TSTEP | TDMPMN | DALLTH | UPMEAN |
34 | 30 | MACR MASS MIXING RATIO AFTER TSTEP | TDMPMN | DALLTH | UPMEAN |
34 | 31 | MACROOH MASS MIXING RATIO AFTER TS | TDMPMN | DALLTH | UPMEAN |
34 | 32 | MPAN MASS MIXING RATIO AFTER TSTEP | TDMPMN | DALLTH | UPMEAN |
34 | 33 | HACET MASS MIXING RATIO AFTER TSTEP | TDMPMN | DALLTH | UPMEAN |
34 | 34 | MGLY MASS MIXING RATIO AFTER TSTEP | TDMPMN | DALLTH | UPMEAN |
34 | 35 | NALD MASS MIXING RATIO AFTER TSTEP | TDMPMN | DALLTH | UPMEAN |
34 | 36 | HCOOH MASS MIXING RATIO AFTER TSTEP | TDMPMN | DALLTH | UPMEAN |
34 | 37 | MeCO3H MASS MIXING RATIO AFTER TSTE | TDMPMN | DALLTH | UPMEAN |
34 | 38 | MeCO2H MASS MIXING RATIO AFTER TSTE | TDMPMN | DALLTH | UPMEAN |
34 | 40 | ISO2 MASS MIXING RATIO AFTER TSTEP | TDMPMN | DALLTH | UPMEAN |
34 | 41 | Cl MASS MIXING RATIO AFTER TIMESTEP | TDMPMN | DALLTH | UPMEAN |
34 | 42 | ClO MASS MIXING RATIO AFTER TSTEP | TDMPMN | DALLTH | UPMEAN |
34 | 43 | Cl2O2 MASS MIXING RATIO AFTER TSTEP | TDMPMN | DALLTH | UPMEAN |
34 | 44 | OClO MASS MIXING RATIO AFTER TSTEP | TDMPMN | DALLTH | UPMEAN |
34 | 45 | Br MASS MIXING RATIO AFTER TIMESTEP | TDMPMN | DALLTH | UPMEAN |
34 | 47 | BrCl MASS MIXING RATIO AFTER TSTEP | TDMPMN | DALLTH | UPMEAN |
34 | 48 | BrONO2 MASS MIXING RATIO AFTER TSTE | TDMPMN | DALLTH | UPMEAN |
34 | 49 | N2O MASS MIXING RATIO AFTER TIMESTE | TDMPMN | DALLTH | UPMEAN |
34 | 51 | HOCl MASS MIXING RATIO AFTER TSTEP | TDMPMN | DALLTH | UPMEAN |
34 | 52 | HBr MASS MIXING RATIO AFTER TIMESTE | TDMPMN | DALLTH | UPMEAN |
34 | 53 | HOBr MASS MIXING RATIO AFTER TSTEP | TDMPMN | DALLTH | UPMEAN |
34 | 54 | ClONO2 MASS MIXING RATIO AFTER TSTE | TDMPMN | DALLTH | UPMEAN |
34 | 55 | CFCl3 MASS MIXING RATIO AFTER TSTEP | TDMPMN | DALLTH | UPMEAN |
34 | 56 | CF2Cl2 MASS MIXING RATIO AFTER TSTE | TDMPMN | DALLTH | UPMEAN |
34 | 57 | MeBr MASS MIXING RATIO AFTER TSTEP | TDMPMN | DALLTH | UPMEAN |
34 | 58 | N MASS MIXING RATIO AFTER TIMESTEP | TDMPMN | DALLTH | UPMEAN |
34 | 59 | O3P MASS MIXING RATIO AFTER TIMESTE | TDMPMN | DALLTH | UPMEAN |
34 | 60 | MACRO2 MASS MIXING RATIO AFTER TSTE | TDMPMN | DALLTH | UPMEAN |
34 | 70 | H2 MASS MIXING RATIO AFTER TIMESTEP | TDMPMN | DALLTH | UPMEAN |
34 | 71 | DMS MASS MIXING RATIO AFTER TIMESTE | TDMPMN | DALLTH | UPMEAN |
34 | 72 | SO2 MASS MIXING RATIO AFTER TIMESTE | TDMPMN | DALLTH | UPMEAN |
34 | 73 | H2SO4 MASS MIXING RATIO AFTER TSTEP | TDMPMN | DALLTH | UPMEAN |
34 | 74 | MSA MASS MIXING RATIO AFTER TIMESTE | TDMPMN | DALLTH | UPMEAN |
34 | 75 | DMSO MASS MIXING RATIO AFTER TSTEP | TDMPMN | DALLTH | UPMEAN |
34 | 76 | NH3 MASS MIXING RATIO AFTER TIMESTE | TDMPMN | DALLTH | UPMEAN |
34 | 77 | CS2 MASS MIXING RATIO AFTER TIMESTE | TDMPMN | DALLTH | UPMEAN |
34 | 78 | COS MASS MIXING RATIO AFTER TIMESTE | TDMPMN | DALLTH | UPMEAN |
34 | 79 | H2S MASS MIXING RATIO AFTER TIMESTE | TDMPMN | DALLTH | UPMEAN |
34 | 80 | H MASS MIXING RATIO AFTER TIMESTEP | TDMPMN | DALLTH | UPMEAN |
34 | 81 | OH MASS MIXING RATIO AFTER TIMESTEP | TDMPMN | DALLTH | UPMEAN |
34 | 82 | HO2 MASS MIXING RATIO AFTER TIMESTE | TDMPMN | DALLTH | UPMEAN |
34 | 83 | MeOO MASS MIXING RATIO AFTER TSTEP | TDMPMN | DALLTH | UPMEAN |
34 | 84 | EtOO MASS MIXING RATIO AFTER TSTEP | TDMPMN | DALLTH | UPMEAN |
34 | 85 | MeCO3 MASS MIXING RATIO AFTER TSTEP | TDMPMN | DALLTH | UPMEAN |
34 | 86 | n-PrOO MASS MIXING RATIO AFTER TSTE | TDMPMN | DALLTH | UPMEAN |
34 | 87 | i-PrOO MASS MIXING RATIO AFTER TSTE | TDMPMN | DALLTH | UPMEAN |
34 | 88 | EtCO3 MASS MIXING RATIO AFTER TSTEP | TDMPMN | DALLTH | UPMEAN |
34 | 89 | MeCOCH2OO MASS MIXING RATIO AFTER T | TDMPMN | DALLTH | UPMEAN |
34 | 90 | MeOH MASS MIXING RATIO AFTER TSTEP | TDMPMN | DALLTH | UPMEAN |
34 | 91 | MONOTERPENE MASS MIXING RATIO AFT T | TDMPMN | DALLTH | UPMEAN |
34 | 92 | SEC_ORG MASS MIXING RATIO AFTER TS | TDMPMN | DALLTH | UPMEAN |
34 | 94 | SO3 MASS MIXING RATIO AFTER TIMESTE | TDMPMN | DALLTH | UPMEAN |
34 | 98 | LUMPED N (as NO2) MMR AFTER TIMESTE | TDMPMN | DALLTH | UPMEAN |
34 | 99 | LUMPED Br (as BrO) MMR AFTER TSTEP | TDMPMN | DALLTH | UPMEAN |
34 | 100 | LUMPED Cl (as HCl) MMR AFTER TSTEP | TDMPMN | DALLTH | UPMEAN |
34 | 101 | NUCLEATION MODE (SOLUBLE) NUMBER | TDMPMN | DALLTH | UPMEAN |
34 | 102 | NUCLEATION MODE (SOLUBLE) H2SO4 MMR | TDMPMN | DALLTH | UPMEAN |
34 | 103 | AITKEN MODE (SOLUBLE) NUMBER | TDMPMN | DALLTH | UPMEAN |
34 | 104 | AITKEN MODE (SOLUBLE) H2SO4 MMR | TDMPMN | DALLTH | UPMEAN |
34 | 105 | AITKEN MODE (SOLUBLE) BC MMR | TDMPMN | DALLTH | UPMEAN |
34 | 106 | AITKEN MODE (SOLUBLE) OC MMR | TDMPMN | DALLTH | UPMEAN |
34 | 107 | ACCUMULATION MODE (SOLUBLE) NUMBER | TDMPMN | DALLTH | UPMEAN |
34 | 108 | ACCUMULATION MODE (SOL) H2SO4 MMR | TDMPMN | DALLTH | UPMEAN |
34 | 109 | ACCUMULATION MODE (SOL) BC MMR | TDMPMN | DALLTH | UPMEAN |
34 | 110 | ACCUMULATION MODE (SOL) OC MMR | TDMPMN | DALLTH | UPMEAN |
34 | 111 | ACCUMULATION MODE (SOL) SEA SALT MM | TDMPMN | DALLTH | UPMEAN |
34 | 113 | COARSE MODE (SOLUBLE) NUMBER | TDMPMN | DALLTH | UPMEAN |
34 | 114 | COARSE MODE (SOLUBLE) H2SO4 MMR | TDMPMN | DALLTH | UPMEAN |
34 | 115 | COARSE MODE (SOLUBLE) BC MMR | TDMPMN | DALLTH | UPMEAN |
34 | 116 | COARSE MODE (SOLUBLE) OC MMR | TDMPMN | DALLTH | UPMEAN |
34 | 117 | COARSE MODE (SOLUBLE) SEA SALT MMR | TDMPMN | DALLTH | UPMEAN |
34 | 119 | AITKEN MODE (INSOLUBLE) NUMBER | TDMPMN | DALLTH | UPMEAN |
34 | 120 | AITKEN MODE (INSOLUBLE) BC MMR | TDMPMN | DALLTH | UPMEAN |
34 | 121 | AITKEN MODE (INSOLUBLE) OC MMR | TDMPMN | DALLTH | UPMEAN |
34 | 126 | NUCLEATION MODE (SOLUBLE) OC MMR | TDMPMN | DALLTH | UPMEAN |
34 | 127 | AITKEN MODE (SOLUBLE) SEA SALT MMR | TDMPMN | DALLTH | UPMEAN |
34 | 149 | PASSIVE O3 MASS MIXING RATIO | TDMPMN | DALLTH | UPMEAN |
34 | 151 | O(1D) MASS MIXING RATIO | TDMPMN | DALLTH | UPMEAN |
34 | 152 | O(3P) MASS MIXING RATIO | TDMPMN | DALLTH | UPMEAN |
34 | 154 | BrO MASS MIXING RATIO AFTER TSTEP | TDMPMN | DALLTH | UPMEAN |
34 | 155 | HCl MASS MIXING RATIO AFTER TSTEP | TDMPMN | DALLTH | UPMEAN |
34 | 156 | Cly MASS MIXING RATIO AFTER TSTEP | TDMPMN | DALLTH | UPMEAN |
34 | 157 | AEROSOL SURFACE AREA | TDMPMN | DALLTH | UPMEAN |
34 | 158 | NAT PSC MASS MIXING RATIO AFTER TS | TDMPMN | DALLTH | UPMEAN |
34 | 159 | OZONE COLUMN | TDAYM | D1TH | UPA |
34 | 159 | OZONE COLUMN | TDMPMN | DALLTH | UPMEAN |
34 | 160 | Heterogenous Rate for N2O5 | TDMPMN | DALLTH | UPMEAN |
34 | 161 | Heterogenous Rates for HO2+HO2 | TDMPMN | DALLTH | UPMEAN |
34 | 162 | TOTAL CLOUD DROPLET NO. CONC. (m^-3 | TDMPMN | DALLTH | UPMEAN |
34 | 163 | <CLOUD DROPLET NO CONC^(-1/3)> (m) | TDMPMN | DALLTH | UPMEAN |
34 | 342 | RXN FLUX: NO3+C5H8->ISON | TMMNUKCA | DALLTH | UPB |
34 | 343 | RXN FLUX: NO+ISO2->ISON | TMMNUKCA | DALLTH | UPB |
34 | 344 | RXN FLUX: H2O2 PRODUCTION | TMMNUKCA | DALLTH | UPB |
34 | 345 | RXN FLUX: ROOH PRODUCTION | TMMNUKCA | DALLTH | UPB |
34 | 346 | RXN FLUX: HONO2 PRODUCTION (HNO3) | TMMNUKCA | DALLTH | UPB |
34 | 352 | TENDENCY: O3 (TROP ONLY) | TMMNUKCA | DALLTH | UPB |
34 | 353 | TROPOSPHERIC O3 | TMNMEAN | DALLTH | UPB |
34 | 354 | TENDENCY: O3 (WHOLE ATMOS) | TMMNUKCA | DALLTH | UPB |
34 | 363 | AIR MASS DIAGNOSTIC (WHOLE ATMOS) | TDMPMN | DALLTH | UPMEAN |
34 | 363 | AIR MASS DIAGNOSTIC (WHOLE ATMOS) | TMNMEAN | DALLTH | UPB |
34 | 371 | CO BUDGET: CO LOSS VIA OH+CO | TMMNUKCA | DALLTH | UPB |
34 | 372 | CO BUDGET: CO PROD VIA HCHO+OH/NO3 | TMMNUKCA | DALLTH | UPB |
34 | 373 | CO BUDGET: CO PROD VIA MGLY+OH/NO3 | TMMNUKCA | DALLTH | UPB |
34 | 374 | CO BUDGET: CO MISC PROD&O3+MACR/ISO | TMMNUKCA | DALLTH | UPB |
34 | 375 | CO BUDGET: CO PROD VIA HCHO PHOT RA | TMMNUKCA | DALLTH | UPB |
34 | 376 | CO BUDGET: CO PROD VIA HCHO PHOT MO | TMMNUKCA | DALLTH | UPB |
34 | 377 | CO BUDGET: CO PROD VIA MGLY PHOTOL | TMMNUKCA | DALLTH | UPB |
34 | 378 | CO BUDGET: CO PROD VIA MISC PHOTOL | TMMNUKCA | DALLTH | UPB |
34 | 379 | CO BUDGET: CO DRY DEPOSITION (3D) | TMMNUKCA | DALLTH | UPB |
34 | 381 | LIGHTNING NOx EMISSIONS 3D | TDMPMN | DALLTH | UPMEAN |
34 | 382 | LIGHTNING DIAGNOSTIC: TOT FLASHES 2 | TDMPMN | DIAG | UPMEAN |
34 | 383 | LIGHTNING DIAG: CLD TO GRND FLSH 2D | TDMPMN | DIAG | UPMEAN |
34 | 384 | LIGHTNING DIAG: CLD TO CLD FLSH 2D | TDMPMN | DIAG | UPMEAN |
34 | 385 | LIGHTNING DIAG: TOTAL N PRODUCED 2D | TDMPMN | DIAG | UPMEAN |
34 | 391 | STRATOSPHERIC OH PRODUCTION | TMMNUKCA | DALLTH | UPB |
34 | 392 | STRATOSPHERIC OH LOSS | TMMNUKCA | DALLTH | UPB |
34 | 401 | STRAT O3 PROD: O2+PHOTON->O(3P)+O(3 | TMMNUKCA | DALLTH | UPB |
34 | 402 | STRAT O3 PROD: O2+PHOTON->O(3P)+O(1 | TMMNUKCA | DALLTH | UPB |
34 | 403 | STRAT O3 PROD: HO2 + NO | TMMNUKCA | DALLTH | UPB |
34 | 404 | STRAT O3 PROD: MeOO + NO | TMMNUKCA | DALLTH | UPB |
34 | 411 | STRAT O3 LOSS: Cl2O2 + PHOTON | TMMNUKCA | DALLTH | UPB |
34 | 412 | STRAT O3 LOSS: BrO + ClO | TMMNUKCA | DALLTH | UPB |
34 | 413 | STRAT O3 LOSS: HO2 + O3 | TMMNUKCA | DALLTH | UPB |
34 | 414 | STRAT O3 LOSS: ClO + HO2 | TMMNUKCA | DALLTH | UPB |
34 | 415 | STRAT O3 LOSS: BrO + HO2 | TMMNUKCA | DALLTH | UPB |
34 | 416 | STRAT O3 LOSS: O(3P) + ClO | TMMNUKCA | DALLTH | UPB |
34 | 417 | STRAT O3 LOSS: O(3P) + NO2 | TMMNUKCA | DALLTH | UPB |
34 | 418 | STRAT O3 LOSS: O(3P) + HO2 | TMMNUKCA | DALLTH | UPB |
34 | 419 | STRAT O3 LOSS: O3 + H | TMMNUKCA | DALLTH | UPB |
34 | 420 | STRAT O3 LOSS: O(3P) + O3 | TMMNUKCA | DALLTH | UPB |
34 | 421 | STRAT O3 LOSS: NO3 + PHOTON | TMMNUKCA | DALLTH | UPB |
34 | 422 | STRAT O3 LOSS: O(1D) + H2O | TMMNUKCA | DALLTH | UPB |
34 | 423 | STRAT O3 LOSS: HO2 + NO3 | TMMNUKCA | DALLTH | UPB |
34 | 424 | STRAT O3 LOSS: OH + NO3 | TMMNUKCA | DALLTH | UPB |
34 | 425 | STRAT O3 LOSS: NO3 + HCHO | TMMNUKCA | DALLTH | UPB |
34 | 431 | STRAT MISC: O3 DRY DEPOSITION (3D) | TMMNUKCA | DALLTH | UPB |
34 | 432 | STRAT MISC: NOy DRY DEPOSITION (3D) | TMMNUKCA | DALLTH | UPB |
34 | 433 | STRAT MISC: NOy WET DEPOSITION (3D) | TMMNUKCA | DALLTH | UPB |
34 | 447 | Monoterp + OH => Sec_org | TMMNUKCA | DALLTH | UPB |
34 | 448 | Monoterp + O3 => Sec_org | TMMNUKCA | DALLTH | UPB |
34 | 449 | Monoterp + NO3 => Sec_org | TMMNUKCA | DALLTH | UPB |
34 | 451 | SO2 + H2O2 => NULL0 | TMMNUKCA | DALLTH | UPB |
34 | 452 | SO2 + O3 => NULL1 | TMMNUKCA | DALLTH | UPB |
34 | 453 | SO2 + O3 => NULL2 | TMMNUKCA | DALLTH | UPB |
34 | 454 | SO2 DRY DEPOSITION (3D) | TMMNUKCA | DALLTH | UPB |
34 | 455 | SO2 WET DEPOSITION (3D) | TMMNUKCA | DALLTH | UPB |
34 | 460 | CS2+O(3P)->COS+SO2+CO BIMOL | TMMNUKCA | DALLTH | UPB |
34 | 461 | CS2+OH->COS+SO2 BIMOL | TMMNUKCA | DALLTH | UPB |
34 | 462 | DMS+OH->SO2 BIMOL | TMMNUKCA | DALLTH | UPB |
34 | 463 | DMS+OH->MSA+SO2 BIMOL | TMMNUKCA | DALLTH | UPB |
34 | 464 | DMS+NO3->SO2 BIMOL | TMMNUKCA | DALLTH | UPB |
34 | 465 | DMS+O(3P)->SO2 BIMOL | TMMNUKCA | DALLTH | UPB |
34 | 466 | H2S+O(3P)->OH+SO2 BIMOL | TMMNUKCA | DALLTH | UPB |
34 | 467 | H2S+OH->SO2+H20 BIMOL | TMMNUKCA | DALLTH | UPB |
34 | 468 | COS+O(3P)->CO+SO2 BIMOL | TMMNUKCA | DALLTH | UPB |
34 | 469 | COS+OH->COS+SO2 BIMOL | TMMNUKCA | DALLTH | UPB |
34 | 470 | SO2+O3->SO3 BIMOL | TMMNUKCA | DALLTH | UPB |
34 | 471 | SO3+H2O->H2SO4+H2O BIMOL | TMMNUKCA | DALLTH | UPB |
34 | 472 | CS2->COS+SO2 PHOTOL | TMMNUKCA | DALLTH | UPB |
34 | 473 | COS->CO+SO2 PHOTOL | TMMNUKCA | DALLTH | UPB |
34 | 474 | H2SO4->SO3+OH PHOTOL | TMMNUKCA | DALLTH | UPB |
34 | 475 | SO3->SO2+O(3P) PHOTOL | TMMNUKCA | DALLTH | UPB |
34 | 476 | SO2+OH->SO3+HO2 | TMMNUKCA | DALLTH | UPB |
34 | 477 | DMSO DRY DEP | TMMNUKCA | DALLTH | UPB |
34 | 478 | NH3 DRY DEP | TMMNUKCA | DALLTH | UPB |
34 | 479 | Monoterp DRY DEP | TMMNUKCA | DALLTH | UPB |
34 | 480 | SEC_ORG DRY DEP | TMMNUKCA | DALLTH | UPB |
34 | 481 | O3 WET DEP | TMMNUKCA | DALLTH | UPB |
34 | 482 | DMSO WET DEP | TMMNUKCA | DALLTH | UPB |
34 | 483 | NH3 WET DEP | TMMNUKCA | DALLTH | UPB |
34 | 484 | SEC_ORG WET DEP | TMMNUKCA | DALLTH | UPB |
35 | 1 | O3 MASS MIX RATIO ON PRESS LEVELS | TDAYM | DP36CCM | UPA |
35 | 1 | O3 MASS MIX RATIO ON PRESS LEVELS | TDMPMN | DP36CCM | UPMEAN |
35 | 173 | HEAVYSIDE FUNC FOR P LEVEL DIAGS | TDAYM | DP36CCM | UPA |
35 | 173 | HEAVYSIDE FUNC FOR P LEVEL DIAGS | TDMPMN | DP36CCM | UPMEAN |
35 | 341 | FLUX: OH+CH4 REACTION ON PLEVS | TDAYM | DP36CCM | UPA |
35 | 341 | FLUX: OH+CH4 REACTION ON PLEVS | TDMPMN | DP36CCM | UPMEAN |
38 | 201 | PRIMARY SO4 TO AITKEN (SOL) | TMMNUKCA | DALLTH | UPB |
38 | 202 | PRIMARY SO4 TO ACCUMULATION (SOL) | TMMNUKCA | DALLTH | UPB |
38 | 203 | PRIMARY SO4 TO COARSE (SOL) | TMMNUKCA | DALLTH | UPB |
38 | 204 | PRIMARY SEA-SALT TO ACCUMULTN (SOL) | TMMNUKCA | DALLTH | UPB |
38 | 205 | PRIMARY SEA-SALT TO COARSE (SOL) | TMMNUKCA | DALLTH | UPB |
38 | 207 | PRIMARY BLACK CARBON TO AITKEN (INS | TMMNUKCA | DALLTH | UPB |
38 | 209 | PRIMARY ORG. CARBON TO AITKEN (INS | TMMNUKCA | DALLTH | UPB |
38 | 214 | DRY DEPOSITION SO4 NUCLEATION (SOL) | TMMNUKCA | DALLTH | UPB |
38 | 215 | DRY DEPOSITION SO4 AITKEN (SOL) | TMMNUKCA | DALLTH | UPB |
38 | 216 | DRY DEPOSITION SO4 ACCUMULTN (SOL) | TMMNUKCA | DALLTH | UPB |
38 | 217 | DRY DEPOSITION SO4 COARSE (SOL) | TMMNUKCA | DALLTH | UPB |
38 | 218 | DRY DEPOSITION SEA-SALT ACC (SOL) | TMMNUKCA | DALLTH | UPB |
38 | 219 | DRY DEPOSITION SEA-SALT COARSE (SOL | TMMNUKCA | DALLTH | UPB |
38 | 220 | DRY DEPOSITION BLK CARB AITKEN (SOL | TMMNUKCA | DALLTH | UPB |
38 | 221 | DRY DEPOSITION BLK CARB ACCUM. (SOL | TMMNUKCA | DALLTH | UPB |
38 | 222 | DRY DEPOSITION BLK CARB COARSE (SOL | TMMNUKCA | DALLTH | UPB |
38 | 223 | DRY DEPOSITION BLK CARB AITKEN (INS | TMMNUKCA | DALLTH | UPB |
38 | 224 | DRY DEPOSITION ORG CARB NUCLN. (SOL | TMMNUKCA | DALLTH | UPB |
38 | 225 | DRY DEPOSITION ORG CARB AITKEN (SOL | TMMNUKCA | DALLTH | UPB |
38 | 226 | DRY DEPOSITION ORG CARB ACCUM. (SOL | TMMNUKCA | DALLTH | UPB |
38 | 227 | DRY DEPOSITION ORG CARB COARSE (SOL | TMMNUKCA | DALLTH | UPB |
38 | 228 | DRY DEPOSITION ORG CARB AITKEN (INS | TMMNUKCA | DALLTH | UPB |
38 | 239 | NUC SCAVENGING SO4 ACCUMULTN (SOL) | TMMNUKCA | DALLTH | UPB |
38 | 240 | NUC SCAVENGING SO4 COARSE (SOL) | TMMNUKCA | DALLTH | UPB |
38 | 241 | NUC SCAVENGING SEA-SALT ACCUM. (SOL | TMMNUKCA | DALLTH | UPB |
38 | 242 | NUC SCAVENGING SEA-SALT COARSE (SOL | TMMNUKCA | DALLTH | UPB |
38 | 243 | NUC SCAVENGING BLK CARB AITKEN (SOL | TMMNUKCA | DALLTH | UPB |
38 | 244 | NUC SCAVENGING BLK CARB ACCUM. (SOL | TMMNUKCA | DALLTH | UPB |
38 | 245 | NUC SCAVENGING BLK CARB COARSE (SOL | TMMNUKCA | DALLTH | UPB |
38 | 246 | NUC SCAVENGING BLK CARB AITKEN (INS | TMMNUKCA | DALLTH | UPB |
38 | 247 | NUC SCAVENGING ORG CARB NUCLN. (SOL | TMMNUKCA | DALLTH | UPB |
38 | 248 | NUC SCAVENGING ORG CARB AITKEN (SOL | TMMNUKCA | DALLTH | UPB |
38 | 249 | NUC SCAVENGING ORG CARB ACCUM. (SOL | TMMNUKCA | DALLTH | UPB |
38 | 250 | NUC SCAVENGING ORG CARB COARSE (SOL | TMMNUKCA | DALLTH | UPB |
38 | 251 | NUC SCAVENGING ORG CARB AITKEN (INS | TMMNUKCA | DALLTH | UPB |
38 | 261 | IMP SCAVENGING SO4 NUCLN. (SOL) | TMMNUKCA | DALLTH | UPB |
38 | 262 | IMP SCAVENGING SO4 AITKEN (SOL) | TMMNUKCA | DALLTH | UPB |
38 | 263 | IMP SCAVENGING SO4 ACCUMULTN (SOL) | TMMNUKCA | DALLTH | UPB |
38 | 264 | IMP SCAVENGING SO4 COARSE (SOL) | TMMNUKCA | DALLTH | UPB |
38 | 265 | IMP SCAVENGING SEA-SALT ACCUM. (SOL | TMMNUKCA | DALLTH | UPB |
38 | 266 | IMP SCAVENGING SEA-SALT COARSE (SOL | TMMNUKCA | DALLTH | UPB |
38 | 267 | IMP SCAVENGING BLK CARB AITKEN (SOL | TMMNUKCA | DALLTH | UPB |
38 | 268 | IMP SCAVENGING BLK CARB ACCUM. (SOL | TMMNUKCA | DALLTH | UPB |
38 | 269 | IMP SCAVENGING BLK CARB COARSE (SOL | TMMNUKCA | DALLTH | UPB |
38 | 270 | IMP SCAVENGING BLK CARB AITKEN (INS | TMMNUKCA | DALLTH | UPB |
38 | 271 | IMP SCAVENGING ORG CARB NUCLN. (SOL | TMMNUKCA | DALLTH | UPB |
38 | 272 | IMP SCAVENGING ORG CARB AITKEN (SOL | TMMNUKCA | DALLTH | UPB |
38 | 273 | IMP SCAVENGING ORG CARB ACCUM. (SOL | TMMNUKCA | DALLTH | UPB |
38 | 274 | IMP SCAVENGING ORG CARB COARSE (SOL | TMMNUKCA | DALLTH | UPB |
38 | 275 | IMP SCAVENGING ORG CARB AITKEN (INS | TMMNUKCA | DALLTH | UPB |
38 | 285 | INCLOUD SO4 (H2O2) TO ACCUMLTN (SOL | TMMNUKCA | DALLTH | UPB |
38 | 286 | INCLOUD SO4 (H2O2) TO COARSE (SOL) | TMMNUKCA | DALLTH | UPB |
38 | 288 | INCLOUD SO4 (O3) TO ACCUMULTN (SOL) | TMMNUKCA | DALLTH | UPB |
38 | 289 | INCLOUD SO4 (O3) TO COARSE (SOL) | TMMNUKCA | DALLTH | UPB |
38 | 290 | CLOUDPROC SU AITSOL --> ACCSOL | TMMNUKCA | DALLTH | UPB |
38 | 291 | CLOUDPROC BC AITSOL --> ACCSOL | TMMNUKCA | DALLTH | UPB |
38 | 292 | CLOUDPROC OC AITSOL --> ACCSOL | TMMNUKCA | DALLTH | UPB |
38 | 294 | CONDENSATION SO4 TO NUCLEATION (SOL | TMMNUKCA | DALLTH | UPB |
38 | 295 | CONDENSATION SO4 TO AITKEN (SOL) | TMMNUKCA | DALLTH | UPB |
38 | 296 | CONDENSATION SO4 TO ACCUMULTN (SOL) | TMMNUKCA | DALLTH | UPB |
38 | 297 | CONDENSATION SO4 TO COARSE (SOL) | TMMNUKCA | DALLTH | UPB |
38 | 298 | CONDENSATION SO4 TO AITKEN (INSOL) | TMMNUKCA | DALLTH | UPB |
38 | 301 | CONDENSATION OC1 TO NUCLEATION (SOL | TMMNUKCA | DALLTH | UPB |
38 | 302 | CONDENSATION OC1 TO AITKEN (SOL) | TMMNUKCA | DALLTH | UPB |
38 | 303 | CONDENSATION OC1 TO ACCUMULTN (SOL) | TMMNUKCA | DALLTH | UPB |
38 | 304 | CONDENSATION OC1 TO COARSE (SOL) | TMMNUKCA | DALLTH | UPB |
38 | 305 | CONDENSATION OC1 TO AITKEN (INSOL) | TMMNUKCA | DALLTH | UPB |
38 | 319 | NUCLEATION OF SO4 (TO NUC-SOL) | TMMNUKCA | DALLTH | UPB |
38 | 320 | COAG SO4 NUCLTN-SOL TO AITKEN-SOL | TMMNUKCA | DALLTH | UPB |
38 | 321 | COAG SO4 NUCLTN-SOL TO ACCUMULN-SOL | TMMNUKCA | DALLTH | UPB |
38 | 322 | COAG SO4 NUCLTN-SOL TO COARSE-SOL | TMMNUKCA | DALLTH | UPB |
38 | 323 | COAG SO4 NUCLTN-SOL TO AITKEN-INSOL | TMMNUKCA | DALLTH | UPB |
38 | 326 | COAG OC1 NUCLTN-SOL TO AITKEN-SOL | TMMNUKCA | DALLTH | UPB |
38 | 327 | COAG OC1 NUCLTN-SOL TO ACCUMULN-SOL | TMMNUKCA | DALLTH | UPB |
38 | 328 | COAG OC1 NUCLTN-SOL TO COARSE-SOL | TMMNUKCA | DALLTH | UPB |
38 | 329 | COAG OC1 NUCLTN-SOL TO AITKEN-INSOL | TMMNUKCA | DALLTH | UPB |
38 | 338 | COAG SO4 AITKEN-SOL TO ACCUMULN-SOL | TMMNUKCA | DALLTH | UPB |
38 | 339 | COAG SO4 AITKEN-SOL TO COARSE-SOL | TMMNUKCA | DALLTH | UPB |
38 | 342 | COAG BC AITKEN-SOL TO ACCUMULN-SOL | TMMNUKCA | DALLTH | UPB |
38 | 343 | COAG BC AITKEN-SOL TO COARSE-SOL | TMMNUKCA | DALLTH | UPB |
38 | 346 | COAG OC1 AITKEN-SOL TO ACCUMULN-SOL | TMMNUKCA | DALLTH | UPB |
38 | 347 | COAG OC1 AITKEN-SOL TO COARSE-SOL | TMMNUKCA | DALLTH | UPB |
38 | 354 | COAG SO4 ACCUMULN-SOL TO COARSE-SOL | TMMNUKCA | DALLTH | UPB |
38 | 356 | COAG BC ACCUMULN-SOL TO COARSE-SOL | TMMNUKCA | DALLTH | UPB |
38 | 358 | COAG OC1 ACCUMULN-SOL TO COARSE-SOL | TMMNUKCA | DALLTH | UPB |
38 | 360 | COAG SEA-SALT ACC-SOL TO COARSE-SOL | TMMNUKCA | DALLTH | UPB |
38 | 366 | COAG BC AITKEN-INS TO ACCUMULN-SOL | TMMNUKCA | DALLTH | UPB |
38 | 367 | COAG OC1 AITKEN-INS TO ACCUMULN-SOL | TMMNUKCA | DALLTH | UPB |
38 | 368 | COAG BC AITKEN-INS TO COARSE-SOL | TMMNUKCA | DALLTH | UPB |
38 | 371 | AGEING SO4 AITKEN-INS TO AITKEN-SOL | TMMNUKCA | DALLTH | UPB |
38 | 372 | AGEING BC AITKEN-INS TO AITKEN-SOL | TMMNUKCA | DALLTH | UPB |
38 | 373 | AGEING OC1 AITKEN-INS TO AITKEN-SOL | TMMNUKCA | DALLTH | UPB |
38 | 375 | MERGE SO4 NUCLTN-SOL TO AITKEN-SOL | TMMNUKCA | DALLTH | UPB |
38 | 376 | MERGE OC1 NUCLTN-SOL TO AITKEN-SOL | TMMNUKCA | DALLTH | UPB |
38 | 378 | MERGE SO4 AITKEN-SOL TO ACCUMULN-SO | TMMNUKCA | DALLTH | UPB |
38 | 379 | MERGE BC AITKEN-SOL TO ACCUMULN-SO | TMMNUKCA | DALLTH | UPB |
38 | 380 | MERGE OC1 AITKEN-SOL TO ACCUMULN-SO | TMMNUKCA | DALLTH | UPB |
38 | 382 | MERGE SO4 ACCUMULN-SOL TO COARSE-SO | TMMNUKCA | DALLTH | UPB |
38 | 383 | MERGE SEA_SALT ACC-SOL TO COARSE-SO | TMMNUKCA | DALLTH | UPB |
38 | 384 | MERGE BC ACCUMULN-SOL TO COARSE-SO | TMMNUKCA | DALLTH | UPB |
38 | 385 | MERGE OC1 ACCUMULN-SOL TO COARSE-SO | TMMNUKCA | DALLTH | UPB |
38 | 401 | DRY PARTICLE DIAMETER NUCLEATION-SO | TMMNUKCA | DALLTH | UPB |
38 | 402 | DRY PARTICLE DIAMETER AITKEN-SOL | TMMNUKCA | DALLTH | UPB |
38 | 403 | DRY PARTICLE DIAMETER ACCUMULATN-SO | TMMNUKCA | DALLTH | UPB |
38 | 404 | DRY PARTICLE DIAMETER COARSE-SOL | TMMNUKCA | DALLTH | UPB |
38 | 405 | DRY PARTICLE DIAMETER AITKEN-INS | TMMNUKCA | DALLTH | UPB |
38 | 408 | WET PARTICLE DIAMETER NUCLEATION-SO | TMMNUKCA | DALLTH | UPB |
38 | 409 | WET PARTICLE DIAMETER AITKEN-SOL | TMMNUKCA | DALLTH | UPB |
38 | 410 | WET PARTICLE DIAMETER ACCUMULATN-SO | TMMNUKCA | DALLTH | UPB |
38 | 411 | WET PARTICLE DIAMETER COARSE-SOL | TMMNUKCA | DALLTH | UPB |
38 | 412 | WATER CONTENT FOR NUCLEATION-SOLUBL | TMMNUKCA | DALLTH | UPB |
38 | 413 | WATER CONTENT FOR AITKEN -SOLUBL | TMMNUKCA | DALLTH | UPB |
38 | 414 | WATER CONTENT FOR ACCUMULTN.-SOLUBL | TMMNUKCA | DALLTH | UPB |
38 | 415 | WATER CONTENT FOR COARSE -SOLUBL | TMMNUKCA | DALLTH | UPB |
38 | 437 | CN NUMBER CONCENTRATION | TMMNUKCA | DALLTH | UPB |
38 | 438 | CCN NO. CONCENTRN. (ACC+COR) | TMMNUKCA | DALLTH | UPB |
38 | 439 | CCN NO. CONCENTRN. (ACC+COR+AIT>25r | TMMNUKCA | DALLTH | UPB |
38 | 440 | CCN NO. CONCENTRN. (ACC+COR+AIT>35r | TMMNUKCA | DALLTH | UPB |
38 | 441 | CD NUMBER CONCENTRATION | TMMNUKCA | DALLTH | UPB |
38 | 469 | ACTIVE CLOUD DROP NO CONC (NUC-SOL) | TMMNUKCA | DALLTH | UPB |
38 | 470 | ACTIVE CLOUD DROP NO CONC (AIT-SOL) | TMMNUKCA | DALLTH | UPB |
38 | 471 | ACTIVE CLOUD DROP NO CONC (ACC-SOL) | TMMNUKCA | DALLTH | UPB |
38 | 472 | ACTIVE CLOUD DROP NO CONC (COR-SOL) | TMMNUKCA | DALLTH | UPB |
38 | 476 | CLOUD LIQUID FRACTION | TMMNUKCA | DALLTH | UPB |
38 | 477 | TOTAL CDNC * CLOUD LIQ FRACTION | TMMNUKCA | DALLTH | UPB |
Contributions and Acknowledgements
Luke Abraham would like to thank the following people (in no particular order) for their help in creating this job:
- Mohit Dalvi, Met Office
- Alex Archibald, NCAS/University of Cambridge
- Graham Mann, NCAS/University of Leeds
- Colin Johnson, Met Office
- Fiona O'Connor, Met Office
- Nick Savage, Met Office
- Sandip Dhomse, University of Leeds
- Martyn Chipperfield, NCAS/University of Leeds
- James Keeble, University of Cambridge
- Paul Telford, NCAS/University of Cambridge
- Maria Russo, NCAS/UNiversity of Cambridge
- John Pyle, NCAS/University of Cambridge
- Zak Kipling, University of Oxford
- Rosalind West, University of Oxford
- Philip Stier, University of Oxford
- Karthee Sivalingam, NCAS/University of Reading
- Kirsty Pringle, University of Leeds
- Ken Carslaw, NCAS/University of Leeds
- Ben Johnson, Met Office
- Jane Mulcahy, Met Office
- Nicolas Bellouin, University of Reading