atmos:citation:research:iccp-cloudprobe2024
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atmos:citation:research:iccp-cloudprobe2024 [2024/07/30 17:56] – klinman | atmos:citation:research:iccp-cloudprobe2024 [2024/07/31 20:50] (current) – klinman | ||
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===== ICCP 2024 Cloud Probe Workshop ===== | ===== ICCP 2024 Cloud Probe Workshop ===== | ||
- | [[.: | + | [[.: |
- | + | ||
- | [[.: | + | |
- | + | ||
- | ===== Probe Processing Notes ===== | + | |
- | - Synthetic data is in the directory / | + | |
- | - Downloaded the Input/ | + | |
- | * Stored under Jeju_Cloud_Probe_Workshop_Simulations. | + | |
- | - Comparison between ADPAA scripted output and SODA GNU generated files. | + | |
- | * Run - python3 / | + | |
- | * When not 100 % match on rejectionflag is because of bins size difference. | + | |
- | + | ||
- | | Probe | ADPAA-SODA probe_type (Calling Initialized Structure) | | + | |
- | | SPEC 2D-S | 2ds | | + | |
- | | Spec HVPS-3 | + | |
- | | DMT PIP | pip | | + | |
- | | DMT CAPS-CIP | cipgs15 | + | |
- | + | ||
- | * Do two methods | + | |
- | * Use ADPAA method=" | + | |
- | * Use method=" | + | |
- | + | ||
- | ==== PROCESSING INSTRUCTIONS COMMENTS (Number Same as Instructions | + | |
- | - Extract information from the header. Generate a PbP file that contains the image time from header for each particle, count in buffer, W, L, A, D, P, end diode shadow flag. | + | |
- | - HVPS3 | + | |
- | - ~/ | + | |
- | - PIP | + | |
- | - ~/ | + | |
- | - Run python3 Extraxt_Header_Information.py | + | |
- | - Creates Output_Files/ | + | |
- | - View/Plot with ncview 20100101_HVPS3_columns_step1.pbp.nc | + | |
- | - ncplot and ncdump should also work. | + | |
- | - Determine counts recorded by probe as function of time before any corrections for particle size are made or before the sample volume is computed. | + | |
- | - run python3 Counts_per_second.py | + | |
- | - Creates files Steps/ | + | |
- | - Need to add plotting to programming and add resulting plots here. | + | |
- | + | ||
- | + | ||
- | + | ||
- | + | ||
- | ===== ICCP 2024 Cloud Probe Workshop ===== | + | |
- | + | ||
- | [[.: | + | |
[[.: | [[.: | ||
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* ./ | * ./ | ||
+ | * Data is processed using the System for OAP Data Analysis (SODA) created by Aaron Bansemer [[https:// | ||
* A comparison of the SODA_gui and the ADPAA_commandline was performed to verify that the command line wrapper works properly. | * A comparison of the SODA_gui and the ADPAA_commandline was performed to verify that the command line wrapper works properly. | ||
* The script ./ | * The script ./ | ||
+ | * Example command, ./ | ||
* All variables in the particle-by-particle (pbp) netcdf files are a 100% match except for the rejectionflag. The reason the rejectionflag does not match 100% is because the bin sizes specified in the wrapper are slightly different than the bin sizes specified in the SODA gui (lazy processing on my part). This leads to an out of size range rejection for a lot of smaller particles. | * All variables in the particle-by-particle (pbp) netcdf files are a 100% match except for the rejectionflag. The reason the rejectionflag does not match 100% is because the bin sizes specified in the wrapper are slightly different than the bin sizes specified in the SODA gui (lazy processing on my part). This leads to an out of size range rejection for a lot of smaller particles. | ||
Line 61: | Line 21: | ||
| Probe | ADPAA-SODA probe_type (Calling Initialized Structure) | | | Probe | ADPAA-SODA probe_type (Calling Initialized Structure) | | ||
| SPEC 2D-S | 2ds | | | SPEC 2D-S | 2ds | | ||
- | | Spec HVPS-3 | + | | SPEC HVPS-3 |
| DMT PIP | pip | | | DMT PIP | pip | | ||
| DMT CAPS-CIP | cipgs15 | | DMT CAPS-CIP | cipgs15 | ||
Line 70: | Line 30: | ||
* method=" | * method=" | ||
* Uses fastcircle, but applies a " | * Uses fastcircle, but applies a " | ||
+ | |||
+ | To process the synthetic data using the ADPAA wrapper for SODA, navigate into Probe_Processing_Init/ | ||
+ | |||
+ | ===== Processing Instructions ===== | ||
+ | All steps currently operational can be run by executing " | ||
+ | |||
+ | - Extract information from the header. Generate a PbP file that contains the image time from header for each particle, count in buffer, W, L, A, D, P, end diode shadow flag. | ||
+ | - Program: Extract_Header_Information.py | ||
+ | - To run on individual file: python3 Extract_Header_Information.py filename | ||
+ | - Generated file looks like: Output_Files/ | ||
+ | - View/plot with, ncview filename | ||
+ | - ncplot and ncdump should also work. | ||
+ | - Determine counts recorded by probe as function of time before any corrections for particle size are made or before the sample volume is computed. | ||
+ | - Program: Counts_per_second.py | ||
+ | - To run on individual file: python3 Counts_per_second.py filename | ||
+ | - Generated file looks like: Output_Files/ | ||
+ | - View/plot with, ncview filename | ||
+ | - ncplot and ncdump should also work. | ||
+ | - Determine counts recorded by probe as a function of time after corrections for particle size based on out of focus particles are made (Assume we need to use “water-processing flag in SODA) | ||
+ | - Program: Counts_per_second.py | ||
+ | - To run on individual file: python3 Counts_per_second.py filename | ||
+ | - Generated file looks like: Output_Files/ | ||
+ | - View/plot with, ncview filename | ||
+ | - ncplot and ncdump should also work. | ||
+ | - Number distribution functions before corrections for particle size (we will use counts per bin per second so that assumptions about the sample volume dependence on maximum dimension don't affect the results). | ||
+ | - Program: Number_Distribution.py | ||
+ | - To run on individual file: python3 Number_Distribution.py filename | ||
+ | - Generated file looks like: Output_Files/ | ||
+ | - View/plot with, ncview filename | ||
+ | - ncplot and ncdump should also work. | ||
+ | - Work is in progress to make matplotlib plots of the distributions for each second. | ||
+ | |||
atmos/citation/research/iccp-cloudprobe2024.1722362196.txt.gz · Last modified: 2024/07/30 17:56 by klinman