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RADIOMETRIC CALIBRATION OF FULL-WAVEFORM
SMALL-FOOTPRINT AIRBORNE LASER SCANNERS
W. Wagner a ’ *, J. Hyyppä b , A. Ullrich c , H. Lehner 3 , C. Briese 3 , S. Kaasalainen b
Christian Doppler Laboratory, Institute of Photogrammetry and Remote Sensing, Vienna University of Technology,
Gusshausstrasse 27-19, 1040 Wien, Austria - ww@ipf.tuwien.ac.at
b Finnish Geodetic Institute, Geodeetinrinne 2, 02431 Masala, Finland-juha.hyyppa@fgi.fi
c RIEGL Laser Measurement Systems GmbH, Riedenburgstraße 48, 3580 Horn, Austria - aullrich@riegl.co.at
KEY WORDS: Laser scanning, Lidar, Calibration, Radiometry, Point Cloud, Classification
ABSTRACT:
Small-footprint airborne laser scanners (ALS) are lidar instruments originally developed for topographic mapping. In recent years
ALS sensors are increasingly used also in other applications (forest mapping, building extraction, power line modelling, etc.) and
their technical capabilities are steadily improving. While the first ALS systems only allowed determining the range from the sensor
to the target, current ALS sensors also record the amplitude of the backscattered echoes (peak power of the received echo), or even
the complete echo waveform. To fully utilise the potential of the echo amplitude and waveform measurements in applications, it is
necessary to perform a radiometric calibration. The calibration process involves the definition of the physical quantities describing
the backscattering properties of objects and the development of practical calibration techniques. These issues are currently addressed
by an EuroSDR (http://www.eurosdr.net/) project which aims at developing ALS calibration standards. This paper reviews the
definition of common scattering (reflectance) parameters and concludes that in the case of small-footprint airborne laser scanning,
the cross section <j[m 2 ] and the backscattering coefficient /[m 2 m 2 ], which is defined as the cross section normalised with the cross-
section of the beam hitting the larget, are the preferred quantities for describing the scattering properties. Hence, either a or /should
be used in the calibration. Also, some results of converting full-waveform data acquired with the R1EGL LMS-Q560 to cross section
data over urban and rural test sites in Austria are shown.
1. INTRODUCTION
Airborne laser scanners (ALS) designed for topographic
mapping - also referred to as topographic lidar - transmit
narrow-beam laser pulses with a high pulse repetition frequency
and measure the round-trip time of the pulses travelling from
the sensor to the ground and back (Wehr and Lohr, 1999). After
converting the time measurements to range and precise
geolocation, an irregular but dense 3D point cloud representing
the scatterers is obtained. While first ALS systems only
measured the round-trip time, more advanced systems also
record the echo amplitude (peak power of the received echo,
most commonly referred to as “intensity”) or the complete echo
waveform (Wagner et al., 2004). In this. way, not only
information about the 3D location of the scatterers is collected,
but also information about the physical backscattering
characteristics. This opens the possibility for identifying target
classes (e.g. vegetation, asphalt, or gravel) and target properties
(size, reflectivity and orientation of scatterers). However, the
echo amplitude and waveform measurements depend not only
on the backscattering properties of the targets but also on sensor
and flight parameters such as the flying altitude, beam
divergence, laser pulse energy, atmospheric conditions, etc.
(Hopkinson, 2007). Therefore, amplitude and waveform
measurements from different sensors, acquisition campaigns
and flight strips are not directly comparable. It may even not be
possible to compare the measurements taken within one
individual flight strip because of topographic height variations
and variable atmospheric conditions along the flight path.
For segmentation and classification purposes it would in
general be sufficient to perform a relative correction of the ALS
amplitude and waveform measurements. Relative correction
methods such as proposed by (Coren and Sterzai, 2006),
(Ahokas et al., 2006) and (Hofle and Pfeifer, 2007) aim at
reducing echo amplitude variations by correcting the
measurements relative to some reference, e.g. relative to a
reference range R ref . However, it is much more desirable to
convert the echo amplitude and waveform measurements into
physical parameters describing the backscatter properties of the
scatterers in a quantitative way. As pointed out by (Freeman,
1992) for the case of Synthetic Aperture Radar (SAR) imaging,
this is because one would like to compare measurements from
different sensors and/or flight strips, extract geophysical
parameters from the backscatter measurements using models,
carry out multi-temporal studies over large areas, and build up a
database of backscatter measurements for different types of
land cover and incidence angles.
To convert the sensor raw data into physical parameters it is
necessary to apply calibration procedures. In remote sensing,
calibration normally involves monitoring of sensor functions
(internal calibration) and correction of the measurements with
the help of known external reference targets (external
calibration). Because current ALS instruments do not monitor
sensors functions crucial for the radiometric calibration of the
measurements (e.g. laser pulse energy), their calibration has yet
to rely solely on external reference targets. First results using
external reference targets have been presented by (Ahokas et al.,
2006; Kaasalainen et al., 2005; Kaasalainen et al., 2008;
* Corresponding author