TerraSAR-X and TanDEM-X:
Revolution in Spaceborne Radar
Ralf Düring, Fifame N. Koudogbo, and Marco Weber,
Infoterra GmbH, 88039 Friedrichshafen, Germany
INTRODUCTION
While Earth Observation from space in the past was mainly
focused on scientific purposes, today data and the derived
information products are increasingly used for various
commercial applications. Potential users are planning and
consulting offices, food and natural resource industries,
insurance companies or agencies. New data of enhanced quality,
available quickly and reliably, independently of daylight and
weather conditions, are required for an increasing and sustained
commercial exploitation of Earth Observation data.
The design and performance of TerraSAR-X, high resolution
satellite X-band satellite, built on a public-private-partnership
agreement between the German Aerospace Centre DLR and
EADS Astrium GmbH will exactly meet these requirements.
Launched on the 15 th June 2007 from the Russian Cosmodrome
in Baikonur (Kazakhstan), the Synthetic Aperture Radar (SAR)
instruments of the spacecraft supply radar images of high quality,
day and night and under nearly all weather conditions; leaving
thus the way open for the establishment of a worldwide
commercial EO-market and the development of numerous
applications, products and services.
Those services include highly sophisticated client-specific image
interpretation, topographic maps up to a scale of 1:10,000, geo
spatial databases and terrain analysis in demand for a wide scope
of applications. Other purposes comprise environmental
planning, land cover and natural resource exploration, regional
and urban development, insurance, risk assessment and
humanitarian objectives, particularly in time-critical situations,
as well as applications in border control, security and defence.
Moreover the smallest movements of the Earth's surface due to
tectonics, volcanism, earthquakes, and land slides are further
challenging fields of application of TerraSAR-X interferometry.
1. TERRASAR-X BASIC IMAGE PRODUCTS
The TerraSAR-X is a Synthetic Aperture Radar instrument
based on an active phased array technology. The radar carrier
frequency is of 9.65GHz (X-band). The nominal range
bandwidth is 150 MHz, the maximum one 300 MHz. The
spacecraft was successfully launched into a sun-synchronous
dusk-dawn orbit with a nominal orbit height at the equator of
514 km. It is flying at a velocity of about 7,6km/s; this results in
about 15 revolutions around the Earth per day and in a revisit
time of 11 days. Fehler! Verweisequelle konnte nicht
gefunden warden, presents an overview of the TerraSAR-X
main orbit parameters.
Parameter
Mission Orbit
_ Qrbit type
Sun-synchronous repeat orbit
Repeat Period
11 days
Repeat cycle
167 orbits in the repeat
Orbits per day
15%
Equatorial crossing
time
18:00 ± 0.25h (local time)
Inclination
97.4438°
Altitude at equator
514.8 km
TerraSAR-X Orbit parameters
1.1 TerraSAR-X imaging Modes
TerraSAR-X sensor is designed for multiple imaging modes and
can acquire in StripMap, SpotLight and ScanSAR modes with
single-, dual- or full polarization. The characteristics of each
imaging mode are described in the following subsections.
1.1.1 The StripMap mode
The ground swath is illuminated with continuous sequence of
pulses while the antenna beam is fixed in elevation and azimuth
(Fig. 1). This results in an image strip with a continuous image
quality in the flight direction. Besides dual polarization
StripMap images will even be available as quadruple
polarisation data that are still under investigation.
Satellite Orbit
Fig. 1: The StripMap imaging geometry
Single pol SM
Dual pol SM
Polarizations
HH or VV
HH/VV, HH/HV
or VV/VH
Scene dimensions
50km x 30km
50km x 15km
Full performance
range
20° - 45°
20° - 45°
Azimuth
resolution
3.3m
6.6m
Ground range
resolution
1.70-3.49m
(@45°...20°inc)
1.70-3.49m
(@45°...20°inc)
The SpotLight (SL) and High Resolution SpotLight (HS) modes
Two variants of the spotlight mode (Spotlight (SL) and High
Resolution SpotLight (HS)) are designed with different values
for azimuth resolution and scene size. As depicted in Fig. 2, SL
and HS modes use electrical beam steering in azimuth direction
in order to increase the illumination time, i.e. the size of the
synthetic aperture. The larger aperture results in a higher
azimuth resolution at the cost of azimuth scene size.