Precipitation

 

Cloud ice and small precipitation particles were imaged with a PMS optical array probe (OAP) providing two-dimensional shadow images of particles with a vertical window height of 0.8 mm (2D-C).  This probe produces shadow images of precipitation-size particles with 0.2 mm resolution. 

 

A brief discussion of the probe is given in Detwiler and Hartman (1991). This probe performed very well during the project.  An example of the recordings for the flight 781 on June 11, 2002, is shown in Figure 1, and the particle size distribution for the buffer shown is displayed in Figure 2.

 

Flight 813 – 2DC Images

 

 

Figure 1: 2DC images recorded during flight 813 (July 23, 2003).  The red arrow shows the portion of the T-28 flight track where the shown 2DC buffer was collected.

 

 

Figure 2: Particle size distribution for the buffers shown in figure 1.

 

 

 

Larger precipitation particles were imaged and counted by the custom-built Optical Array Hail Spectrometer, sensitive to particles between 0.9 mm and 12 cm in diameter.  The automated counting and sizing circuitry includes only particles in the size range 4.5 mm to 4.5 cm.  The probe performed well during the project, except during descent.  It is not de-iced, and descent from cooler to warmer layers of the atmosphere caused condensation on the windows and loss of data.

 

 

Additional information on large particles can be inferred from the recorded videotape with the camera mounted under the right wing of the airplane.  If the video camera housing window is not iced-over, the video can be used to view precipitation particle impacts and some judgement can be made about the character of the precipitation (liquid, soft ice, hard ice, etc.). In addition, the windscreen microphone, recorded on one of the two audio tracks, can be used to verify when hail is striking the windscreen. Mushy hailstones produce muffled sounds, while hard hailstones sound almost like a hammer hitting the windscreen.

 

The HVPS (High Volume Particle Sampler) measures the size, shape and concentration of precipitation size particles.  It operates by taking a two-dimensional shadow digital picture of the particles that pass through a 4.5 x 20.3 cm laser light plane that is normal to the direction of aircraft flight. The sheet of light is imaged onto a linear array of 256 photo-elements, so that the HVPS has 200 mm pixel resolution when measured across the array.  In order to keep the pixel resolution along the flight path constant, the system clock frequency is adjusted according to the detected True Air Speed (TAS) by the data system itself.

 

The maximum clock frequency for the HVPS is 240 kHz.  The HVPS data recorded during this project has 400 mm resolution along the flight path.  An example of the data obtained with the HVPS instrument is presented below (Flight 813 July 23, 2003).

 

 

 

 

The above figure shows a typical display of the software developed in IDL to display the T-28  HVPS data for each flight.  On the lower right corner, you can see a display of the particle size distribution, while on the lower left corner the track of the T28 and the position of the buffer displayed above are shown. The large blotchy images in the upper center and left of the window are examples of images of hydrometeors that have hit the upper plate or one of the probe arms, and been broken and accelerated forward  as the pieces move through the sample volume. Because the pieces are moving in the same direction as the aircraft, they move through the sample volume more slowly than hydrometeors falling through the air, and appear stretched.