GPM Ground Validation Autonomous Parsivel Unit (APU) at the NSSTC

Table of Contents

Introduction
Campaign
Instrument Description
File Naming Convention
Data Format
Contact Information

Introduction

The Autonomous Parsivel Unit (APU) is an optical disdrometer based on single particle extinction that measures particle size and fall velocity. This APU consists of the Parsivel, which was developed by OTT Messtechnik in Germany, and its support systems, which were designed and built by the University of Alabama in Huntsville. This parsivel dataset gathers data at the National Space Science and Technology Center (NSSTC) , Huntsville, AL when they are not deployed to other sites for the Global Precipitation Measurement (GPM) mission Ground Validation (GV) campaign.

Campaign

The Global Precipitation Measurement (GPM) mission Ground Validation (GV) campaign will use a variety of methods for validation of GPM satellite constellation measurements prior to launch of the GPM Core Satellite, which is currently scheduled for July 2013. The validation effort will entail numerous GPM-specific and joint-agency/international external field campaigns, using state of the art cloud and precipitation observational infrastructure (polarimetric radars, profilers, rain gauges, disdrometers). Surface rainfall will be measured by very dense rain gauge and disdrometer networks at various field campaign sites. These field campaigns will account for the majority of the effort and resources expended by Global Precipitation Measurement (GPM) mission Ground Validation (GV).

Instrument Description

The primary instrument is the parsivel disdrometer, produced by OTT Messtechnik, Germany. The OTT parsivel disdrometer is a modern, laser-based optical system for measuring all types of precipitation completely and reliably. The transmitter unit of the sensor generates a flat, horizontal beam of light, which the receiver converts into an electrical signal. The signal changes whenever a hydrometeor falls through the beam anywhere within the measurement area. The degree of dimming is a measure of the size of the hydrometeor, and together with the duration of the signal, the fall velocity can be derived. Extinction measurement technique directly measures size and velocity of each single hydrometeor, then derives size spectrum, amount of rainfall, equivalent radar reflectivity, visibility, kinetic energy, and precipitation type.

File Naming Convention

Data are in daily tared files of the form:

apuxx_<site>_yyyymmdd.tar

which contain hourly data files of the form:

apuxx_<site>_apuxx_yyyymmddhh.dat

where,

apu =  Autonomous Parsivel Unit
xx =   A unique notation, to further identify the instrument
site =   Represents the location of the instrument (NSSTC, Huntsville, AL.)
yyyymmdd =   Is the year, month and day of the data
hh = hour
tar =   Unix "tape archive" fromat
dat = ASCII data file

Data Format

The Parsivel data is recorded every 10 seconds and time stamped by the APU software. The data format is ASCII and organized as follows:

YYYYmmDDHHMMSS;APUXX,ST,TEMP,RAW_DATA

where

YYYY = 4-digit year
mm = 2-digit month
DD = 2-digit day
HH = 2-digit hour
MM = 2-digit minute
SS = 2-digit second
APUXX = station name (xx == 2-digit APU number)
ST = Parsivel sensor status ranging from 0-3

0 = Everything OK;
1 = Laser protective glass is dirty, but measurements still possible
2 = Laser protective glass is dirty, partially covered. No further measurements are possible
.3 = Laser damaged
TEMP = 3-digit Sensor temperature in °C
RAW_DATA = particle counts in each bin of the 32 x 32 (diameter x velocity) matrix (consult OTT Present Weather Sensor manual for classification of bins)


Example:

20100610000003;APU03,0,026,000,000,000,000,000,000,000,000,000,000,000,000,0
00,000,000,000,000,000,000,000,000,000,000,000,000,000,000,000,000,000,000,0
00,000,000,000,000,000,000,000,000,000,000,000,000,000,000,000,000,000,000,0
00,000,000,…

New format as of Feb 25, 2011:

YYYYmmDDHHMMSS;APUXX,ST,TEMP,N,R,Z,VIS,WX4680,WX4677,RAW_DATA

where

N = Number of detected particles
R = Rain intensity (32bit, mm/hr)
Z = Reflectivity factor (16bit, dBZ)
VIS = MOR Visibility in the precipitation (m)
WX4680 = 2-digit weather code according to SYNOP wawa Tbl 4680
WX4680 = 2-digit weather code according to SYNOP w.w. Tbl 4677

A PDF version of the format can be downloaded from here.
Information detailing APU Parsivel operating instructions can be found here.

Contact Information

The data producers are:

Walter A.Petersen
NASA Marshall Space Flight Center
Huntsville, Alabama, 35805

Larry Carey
Earth Systems Science Center
UAHuntsville
Huntsville, AL 35805

To order these data or for further information, please contact:

Global Hydrology Resource Center
User Services
320 Sparkman Drive
Huntsville, AL 35805
Phone: 256-961-7932
E-mail: ghrc@eos.nasa.gov
Web: http://ghrc.nsstc.nasa.gov/