Raindrop size distribution
The raindrop size distribution (DSD), or granulometry of rain, is the distribution of the number of raindrops according to their diameter (D). Three processes account for the formation of drops: the accumulation of small drops on large drops and collisions between sizes. According to the time spent in the cloud, the vertical movement in it and the ambient temperature, the drops that have a very varied history and a distribution of diameters from a few micrometers to a few millimeters.
In general, the drop size distribution is represented as a truncated gamma function for diameter zero to the maximum possible size of rain dropplets. The number of drop with diameter is therefore :
with , and as constants.
The most well-known study about raindrop size distribution is from Marshall and Palmer done at McGill University in Montréal in 1948. They used stratiform rain with and concluded to an exponential drop size distribution. This Marshall-Palmer distribution is expressed as:
- N0 = 8000 m-3mm-1 ;
- = 4.1 R-0,21mm-1, R being the rainrate in stratiform precipitation ;
- D = raindrop diameter in mm
- Note: It should be noted that the units of N0 are sometimes simplified to cm -4 but this removes the information that this value is calculated per cubic meter of air.
As the different precipitations (rain, snow, sleet, etc...), and the different types of clouds that produce them vary in time and space, the coefficients of the drop distribution function will vary with each situation. The Marshall-Palmer relationship is still the most quoted but it must be remembered that it is an average of many stratiform rain events in mid-latitudes. The upper figure shows mean distributions of stratiform and convective rainfall. The linear part of the distributions can be adjusted with particular of the Marshall-Palmer distribution. The bottom one is a series of drop diameter distributions at several convective events in Florida with different precipitation rates. We can see that the experimental curves are more complex than the average ones, but the general appearance is the same.
Many other forms of distribution functions are therefore found in the meteorological literature to more precisely adjust the particle size to particular events. Over time researchers have realized that the distribution of drops is more of a problem of probability of producing drops of different diameters depending on the type of precipitation than a deterministic relationship. So there is a continuum of families of curves for stratiform rain, and another for convective rain.
The Marshall and Palmer distribution uses an exponential function that does not simulate properly drops of very small diameters (the curve in the top figure). Several experiments have shown that the actual number of these droplets is less than the theoretical curve. Carlton W. Ulbricht developed a more general formula in 1983 taking into account that a drop is spherical if D <1 mm and an ellipsoid whose horizontal axis gets flattened as D gets larger. It is mechanically impossible to exceed D = 10 mm as the drop breaks at large diameters. From the general distribution, the diameter spectrum changes, μ = 0 inside the cloud, where the evaporation of small drops is negligible due to saturation conditions and μ = 2 out of the cloud, where the small drops evaporate because they are in drier air. With the same notation as before, we have for the drizzle the distribution of Ulbricht:
Where is the liquid water content, water density, and 0.2 is an average value of the diameter in drizzle. For rain, introducing rainrate R (mm/h), the amount of rain per hour over a standard surface:
The first measurements of this distribution were made by rather rudimentary tool by Palmer, Marshall's student, exposing a cardboard covered with flour to the rain for a short time. The mark left by each drop being proportional to its diameter, he could determine the distribution by counting the number of marks corresponding to each droplet size. This was immediately after the Second World War.
Different devices have been developed to get this distribution more accurately:
Drop size versus radar reflectivity
Knowledge of the distribution of raindrops in a cloud can be used to relate what is recorded by a weather radar to what is obtained on the ground as the amount of precipitation. We can to find the relation between the reflectivity of the radar echoes and what we measure with a device like the disdrometer.
The rainrate (R) is equal to number of particules (), their volume () and their falling speed ():
The radar reflectivity Z is:
- where K is the Permittivity of water
Z and R having similar formulation, one can solve the equations to have a Z-R of the type:
- Where a and b are related to the type of precipitation (rain, snow, convective (like in thunderstorms) or stratiform (like from nimbostratus clouds)) which have different , K, N0 and .
- Paul T. Willis; Frank Marks; John Gottschalck (2006). "Rain Drop Size Distributions and Radar Rain Measurements in South Florida".
- Ondrej Fiser (February 1, 2010). "The Role of DSD and Radio Wave Scattering in Rain Attenuation". Geoscience and Remote Sensing New Achievements. InTech. doi:10.5772/9110. ISBN 978-953-7619-97-8.
- Marshall, J. S.; Palmer, W. M. (1948). "The distribution of raindrops with size" (pdf). J. Meteor. 5 (4): 165–166. doi:10.1175/1520-0469%281948%29005%3C0165%3ATDORWS%3E2.0.CO%3B2. ISSN 0095-9634. Retrieved January 16, 2012.
- Ulbrich, Carlton W. (1983). "Natural variation in the analytical form of the raindrop size distribution" (pdf). Journal of Climatology and Applied Meteorology. 22 (10): 1764–1775. doi:10.1175/1520-0450(1983)022<1764:NVITAF>2.0.CO;2. ISSN 0733-3021.
- "La mesure de la hauteur de précipitation grâce à la réflectivité radar". Glossaire météorologique (in French). Météo-France. Retrieved 2009-03-12.