IPHEX Cloud Microphysics This data set consists of data collected from three instruments on the UND Citation aircraft, the PMS Two-Dimensional Cloud probe (2D-C), the SPEC Two-Dimensional Stereo probe (2D-S), and the SPEC High Volume Precipitation Spectrometer 3 (HVPS-3). All instruments are two-dimensional optical array probes which record images of particles that travel through their sampling area. The recorded images are then analyzed to produce particle size distributions from 50 microns to 3 centimeters in diameter. Probe specifications: 2D-C: 32-element diode array, 30 microns per pixel 2D-S: Two 128-element diode arrays, 10 microns per pixel HVPS-3: 128-element diode array, 150 microns per pixel The 2D-S records particles from two separate arrays, one with a vertical (top view) orientation, and one with a horizontal (side view) orientation. They are treated as two separate instruments in this data set. The HVPS-3 was oriented vertically for flights between May 9 and May 29. The instrument was then rotated to a horizontal orientation for flights between June 5 and June 12. The 2D-C was oriented vertically for all flights. Processing details: Particle size distributions are given in terms of particle diameter, which is defined as the diameter of the smallest circle than can completely enclose the particle image. Images that touch a side of the array are allowed. The technique described in Field et al. (2006) has been applied to mitigate shattering artifacts on the 2D-C and 2D-S. The 2D-C and 2D-S also had modified probe tips to minimize the amount of shattering. Optical depth of field for the 2D-C follows the manufacturer's specifications. Depth of field for the 2D-S and HVPS follows Lawson et al. (2006). For each flight a "comb.spectrum" file has been produced, which is a combination of a small-particle instrument (either the 2DS-H or 2DS-V) for particles smaller than 1mm in diameter, and a large-particle instrument (HVPS-3) for particles larger than 1mm in diameter. The 2DS-V was used when the HVPS-3 was oriented vertically, and the 2DS-H was used when the HVPS-3 was oriented horizontally. Bulk ice water content (IWC) is derived in the size distribution files for the convenience of data users, using a mass-size parameterization of mass=0.0061*(D^2.05) from Heymsfield et al. (2004). Note that this has been indiscriminately applied, and will not be valid in cases of rain, graupel, or ice habits that are not well represented by this mass-size parameterization. The total number concentration (Nt) given in the files is for particles larger than 100 microns for the 2D-C and 2D-S, and larger than 1mm for the HVPS-3. File naming convention: The size distributions are written in ASCII files (using the NASA Ames format specification) with each instrument's data in a separate file. The two arrays on the 2D-S are identified by an 'H' for the horizontal array, and a 'V' for the vertical array. Files are named with the following convention: YYYYMMDD_HHMMSS.2DC.1Hz YYYYMMDD_HHMMSS.2DS_H.1Hz YYYYMMDD_HHMMSS.2DS_V.1Hz YYYYMMDD_HHMMSS.HVPS3.1Hz YYYYMMDD_HHMMSS.comb.spectrum.1Hz The particle image files are named with the following convention: YYYYMMDD_HHMMSS_2DC7.png YYYYMMDD_HHMMSS_HVPS3.png YYYYMMDD_HHMMSS_2DS_H.png YYYYMMDD_HHMMSS_2DS_V.png where YYYYMMDD = year, month and day HHMMSS = hour, minutes, and seconds at data start time comb.spectrum = combined spectrum (2D-S, HVPS-3) png = portable network graphics, a raster graphics file format References: Field, P. R., A. J. Heymsfield, A. Bansemer, 2006: Shattering and Particle Interarrival Times Measured by Optical Array Probes in Ice Clouds. J. Atmos. Oceanic Technol., 23, 1357–1371. Heymsfield, A.J, Aaron Bansemer, Carl Schmitt, Cynthia Twohy, and Michael R. Poellot, 2004: Effective Ice Particle Densities Derived from Aircraft Data. J. Atmos. Sci., 61, 982–1003. Lawson, R.P., Darren O’Connor, Patrick Zmarzly, Kim Weaver, Brad Baker, Qixu Mo, and Haflidi Jonsson, 2006: The 2D-S (Stereo) Probe: Design and Preliminary Tests of a New Airborne, High-Speed, High-Resolution Particle Imaging Probe. J. Atmos. Oceanic Technol., 23, 1462–1477.