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Access Tools--Processing, Display and Download


The View archived quicklook images command displays a page with one-month of of thumbnails images. Lidar images are generated automatically at the end of each hour. Calibration coefficients are computed using data from the radiosonde launched at the begining of the time period and a default system calibration scan file. For data acquired from Madison, WI the Green Bay, Wisconsin sounding is used. Data from Barrow uses the BRW sounding and data from Eureka uses the YEU sounding. MMCR, PAERI, and MWR quicklook images are also generated for each 12-hour period. However, these data are typically recieved one-day after they are acquired.

The customize image generation code computes images and line plots directly from the raw netcdf lidar data archive. By default it reads data from the last two hours; however, it can be used to generate custom images from any time or altitude interval within the archive. Calibration coefficients are computed from a default calibration scan and the radiosondes nearest in time to the data. The web interface activates a Python script which in turn launches a Matlab image processing program. This program: 1)locates and reads the raw data, 2) locates and reads the nearest time radiosonde files, 3) locates and reads the default system calibration files for the selected time period, 4) computes the inversion coefficients used to separate particulate and molecular scattering from the radiosonde and calibration files, 5) performs time and altitude averaging to match data to the display resolution, 6) generates the inverted data, 6) generates the plots. The delay between the web request and the image display increases as the time interval and/or altitude range is increased. Images of MMCR, PAERI and MWR data are also generated if requested. Data for these images are interpolated if the pixel spacing is smaller than the instrument resolution and averaged if the pixel spacing is larger than the instrument resolution. Once again it takes approximately one day for these data sets to appear in the archive. If selected, data from the lidar and radar are used together to compute cloud microphysical quantities. These assume a default crystal type of 'bullet rosette'.

The generate housekeeping data command produces plots of internal lidar parameters for the selected time period. This is mostly of interest to the lidar operators.

TheView System Online LogBook provides a record of lidar system hardware maintenance.

The Process and Export Data as NetCDF creates a downloadable NetCDF data file containing data from all instruments placed on a common time and altitude grid. Lidar data are processed from raw data files with time and altitude resolutions selected by the user. Data from the MMCR, PAERI, and MWR are interpolated if the selected resolution is higher that the instrument resolution and averaged if the selected resolution is less than the instrument resolution. After a NetCDF is created the user can create data mask fields using Matlab compatible logical statements to select data on basis of variables contained in the NetCDF. Quick look images are generated to guide the selection process. These show selected data points in color with the rest of the image depicted in shades of gray. The mask fields allow the user to isolate particular cloud types or signal regimes. The mask fields do not modify the data, but are provided in the NetCDF as arrays of ones and zeros having the same dimension as the data arrays. Cloud microphysical properties can also be computed from the lidar and radar data. A gamma size distribution is assumed along with power law representation of the particle volume and area relative to a sphere as presented by Mitchell JAS Vol 53,no 12, 1996. The parameters of the the size distribution and the power law coefficents can be selected from preset values or entered by the user.

The Download Archived Instrument Data as Received option allows users to download data received from instruments other than the lidar exactly as it was received from NOAA or the University of Idaho.


The Pre-processed monthly data files option provides access to HSRL, and MMCR data that has been processed using a 3-minute time and 45 m range averaging. Results are stored in monthly NetCDF files that extend from the surface to an altitude of 20km. The netcdf files include a default data quality mask field "qc_mask" that that can be used to reject flawed data. However it is unlikely that the default selection criteria will match any particular users requirements. To aid users we have provided a set of Matlab routines to read, display and compute data quality mask fields using user selected thresholds. Matlab routines for use with NetCDF files downloaded from this site.. Note: Rather than use these pre-processed monthly data files, most users will benefit by creating custom processed data files with time and altitude averaging selected to best match their needs. This will also assure use of the latest version of the data processing code.


Sample data from 14-Jan-2004


An attenuated backscatter image observed with the combined channel of the AHSRL on 14-Jan-04. A well calibrated conventional lidar would produce an identical image. Notice how the cirrus cloud at 7km by is shadowed by 3.4km water cloud which appears at 6:10 UTC. Also notice the strong lidar return seen below the clouds as a result of the combined effect of aerosol and molecular scattering. Data gaps at 8 and 12 UTC occur during system calibrations. The calibration sequences will be shortened in the future. (click on image to enlarge)

The backscatter cross section image computed for the 14-Jan-04 data shown above. This image is absolutely calibrated and molecular scattering has been removed. Areas with insufficient signal for the HSRL inversion are indicated by black shadows; everywhere else attenuation has been removed. Notice the effect of attenuation correction on the appearance of 7km cirrus cloud.

The circular depolarization image for the 14-Jan-04 case shown above. Water clouds produce little depolarizations and appear blue in this logrithmic display. Ice crystals produce large depolarizations allowing easy identification of both cirrus clouds and ice crystal virga which appear red in this image. An insturment bias is evident in regions of small backscatter cross section where the measured depolarizations are slightly too large(eg. in the boundary aerosol layer before 10 UTC). Laser light scattered inside of the instrument seems to be responsible. Corrective measures are underway.

The optical depth profile measured between 6:40 and 6:50 UTC for the data shown above. Blue and red symbols show 150 m and 600 m vertical averages respectively. The water cloud at 3.8k m has an optical depth of 0.4 while an optical depth of 2.8 is measured between the base of the cirrus cloud at 4.8km and the point where the signals fall into the noise at ~8.5km. Column optical depth measurements are currently limited to values of less than ~4 (even with long averages) by the system noise floor and systematic errors. The current noise floor is slightly larger than that which is expected based on photon counting statistics. This suggests that optical depth measurement limit may increase slightly as we gain more experience with the instrument.

Warning


Major improvements in the stability of system calibrations have been achieved after additional optical isolation was installed between the seed-laser and the main laser cavity(Dec 03). However, system characterization and software is not complete. Known and unknown errors exist. !!!

note


Unrealistically large values of depolarization appear at low altitudes in regions of low backscatter cross section. We now believe that this is caused by laser light scattered within the instrument. This effect can be seen in most current images. It is very apparent below 6 km after 5:00 UTC in the following image. Notice that more reasonable values (but still biased to larger values) of depolarization are seen before 5:00 UTC when the scattering cross section is larger.


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eloranta@lidar.ssec.wisc.edu