Full text: Proceedings, XXth congress (Part 4)

/er, 
z. This 
tly for 
ensing 
| sofar, 
d. The 
F small 
tes for 
ally as 
depend 
litional 
erefore 
F small 
International Archives of the Photogrammetry, Remote Sensing and Spatial Information Sciences, Vol XXXV, Part B4. Istanbul 2004 
  
3. REQUIRED COMPONENTS FOR OPERATION OF 
A SMALL SATELLITE FOR EARTH OBSERVATION 
3.1 Launch 
For satellite launches several competitive possibilities exist. 
They can be launched by a separate mission or in piggyback. 
Recently retrievable launch vehicles, such as the German 
Phoenix are under development. Traditionally, launchers have 
been used in the Russian Federation, in India, from ESA, and in 
the United States. A launch cost estimate is about 10 000 $ per 
| kg of mass. A retrievable launcher would cut this cost to 
about half. 
3.2 Choice of Orbit 
The choice of the orbit is crucial for the performance of an 
earth observation satellite. 
Geostationary orbits at 36 000 km are preferred for 
communication satellites. Earth observation satellites prefer 
sunsynchronous polar orbits at orbital heights between 400 and 
1000 km. If the observations are aimed at specific areas of the 
globe, then lower inclinations combined with elliptical orbits 
(150 to 500 km) can be chosen. Such orbits do not provide ideal 
illumination conditions, however. The choice of the orbit 
determines repeatability of sensing. 
3.3 Attitude and Orbit Controls 
The orbit can best be monitored by an on-board GPS satellite 
receiver. The positions of the satellite are downlinked and 
monitored in the ground facilities. Orbit corrections are possible 
by hydrocyne propulsion systems with the need to carry this 
fuel on board. 
The attitude of the satellite is warranted first by 3 axes gyros. 
For higher precisions a sun sensor is required. After monitoring 
the attitude on the ground the propulsion systems can carry out 
the attitude corrections for pointing of sensors. For smaller 
corrections the sensor my be reoriented. 
3.4 Sensors 
For earth observations sensors are required, which sense 
reflections of the earth within the range of the electromagnetic 
spectrum. Optical and thermal (passive) sensors require 
sensitive elements, which need to be read out and transmitted to 
earth. Onboard processing by microprocessors is possible. 
Active sensors (such as radar) require antennas for transmission 
of electromagnetic pulses and for reception of the backscattered 
reflections from the ground. Obviously passive sensors require 
less mass. 
The sensor limitations for use in small satellites have been 
discussed in detail in the paper *High resolution mapping with 
small satellites" by Rainer Sandau, presented to the ISPRS 
2004 Congress (1). They refer mainly to optical and thermal 
sensors. They are: 
- Spatial resolution by the optical system, which is 
governed by the diffraction limitation; 
- sensitivity of the detector elements requiring a minimum 
exposure time of about 1 msec; 
581 
- image motion, due to the forward motion of the satellite 
movement in the order of 7.4 km/sec or 7.4 m/msec. 
If higher resolutions than 7 m are desired, then image motion 
compensation must be applied. This is possible by time delay 
integration sensors (TDI), in which instead of a single array of 
detector elements across the platform motion a number of 
arrays in direction of the platform motion are utilized, over 
which the detector signals are averaged before readout. High 
resolution sensors with ground resolutions better than 7 m 
therefore not only need smaller resolution elements, e.g. by 
staggered arrays, but also means of image motion 
compensation, wither by TDI arrays or by rotation of the 
satellite sensor during the exposure time. 
3.5 Power 
For the requirements of on-board sensing, processing and the 
reception and transmission of sensing and auxiliary data, as 
well as for the control options of the satellite power systems 
must be provided. The principal source are batteries (NiCd, 
NiH or Li-Ion). For longer duration missions they need to be 
charged by solar energy, which has to be collected by solar 
panels. 
3.6 Data Readout 
The charges received at the sensor elements of the arrays need 
to be transmitted at appropriate readout rates to the ground 
stations during a ground station contact time of about 10 
minutes. At a rate of 100 Mb/s up to 60 GB of data can be 
transmitted. If higher data rates are required data compression 
must be utilized for transmission. 
3.7 Ground Station Processing 
The received signals at a ground antenna must be stored and 
processed at the ground station facility. 
4. CONCLUSIONS 
Simple imaging of the ground requires a linear array sensor 
perpendicular to satellite motion. Images of such a sensor 
system require geocoding. This is possible using the transmitted 
GPS and attitude orbital data within accuracy limitations. 
Ground control points can increase the accuracy of geocoding. 
However, the images cannot be orthorectified onto a 
cartographic projection unless a digital elevation model of the 
terrain is known from other sources, and used in the ground 
processing chain. 
To be independent of the knowledge of the digital elevation 
model stereo sensing can be utilized, using at least two sensor 
systems operating with a forward and a backward inclination 
along the orbital path against the nadir. Rainer Sandau 
describes the possible stereo sensing configurations in his 
paper, which have been utilized in satellite systems (1). 
As the swath widths for small satellite sensors are usually small 
due to the use of narrow angle optical systems optimal 
base/height ratios of 1:1 permitting to acquire digital elevation 
models with sufficient accuracy are difficult to achieve. 
  
  
 
	        
Waiting...

Note to user

Dear user,

In response to current developments in the web technology used by the Goobi viewer, the software no longer supports your browser.

Please use one of the following browsers to display this page correctly.

Thank you.