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Acta Astronautica 56 (2005) 35 – 43<br />

www.elsevier.com/locate/actaastro<br />

<strong>MAP<strong>SAR</strong></strong>: a <strong>small</strong> L-<strong>band</strong> <strong>SAR</strong> <strong>mission</strong> <strong>for</strong> <strong>land</strong> observation<br />

Reinhard Schröder a,∗ , Jürgen Puls a , Irena Hajnsek a , Fritz Jochim a , Thomas Neff a ,<br />

Janio Kono b , Waldir Renato Paradella b , Mario Marcos Quintino da Silva b ,<br />

Dalton de Morisson Valeriano b , Maycira Pereira Farias Costa b<br />

a German Aerospace Center, DLR, P.O. Box 1116, D-82230 Weßling, Germany<br />

b NationalInstitute <strong>for</strong> Space Research, INPE, Av. dos Astronautas 1758, Caixa Postal515, 12201-010 São José dos Campos, SP-Brazil<br />

Available online 14 October 2004<br />

Abstract<br />

This paper introduces Multi-Application Purpose <strong>SAR</strong> (<strong>MAP<strong>SAR</strong></strong>). A new Synthetic Aperture Radar (<strong>SAR</strong>) <strong>mission</strong> <strong>for</strong><br />

earth observation. <strong>MAP<strong>SAR</strong></strong> is the result of a joint pre-phase A study conducted by INPE and DLR targeting a <strong>mission</strong><br />

<strong>for</strong> assessment, management and monitoring of natural resources. The applicability of the sensor system was investigated<br />

<strong>for</strong> cartography, <strong>for</strong>estry, geology, geomorphology, hydrology, agriculture, disaster management, oceanography, urban studies<br />

and security. An L-<strong>band</strong> <strong>SAR</strong>, based on INPE’s multi-<strong>mission</strong> plat<strong>for</strong>m (MMP), has been chosen as payload of the satellite.<br />

The key component of the <strong>SAR</strong> instrument is the <strong>SAR</strong> antenna, which is designed as an elliptical parabolic reflector antenna.<br />

L-<strong>band</strong> (high spatial resolution, quad-pol) has been selected <strong>for</strong> the <strong>SAR</strong> sensor as optimum frequency accounting <strong>for</strong> the<br />

majority of Brazilian and German user requirements. At the moment, the pre-phase A has been concluded and the phase A<br />

is planned to start in early 2003.<br />

© 2004 Elsevier Ltd. All rights reserved.<br />

1. Introduction<br />

The ability of a <strong>SAR</strong> to provide high-resolution imagery<br />

independent of weather or sun light is particularly<br />

important <strong>for</strong> regions of the planet that present<br />

restrictions to the use of optical sensors due to the presence<br />

of rain, perennial clouds, haze and smoke (e.g.,<br />

the Amazon region) or where solar illumination is<br />

∗ Corresponding author. Tel.: +49 8153 28 2310;<br />

fax: +49 8153 28 1135.<br />

E-mailaddresses: reinhard.schroeder@dlr.de (R. Schröder),<br />

kono@dss.inpe.br (J. Kono).<br />

insufficient (Polar regions). Beside this, imaging<br />

radars also have the ability to penetrate a vegetation<br />

canopy, which is not possible using optical sensors.<br />

In general, the acquisition of in<strong>for</strong>mation in tropical<br />

regions, particularly in rain <strong>for</strong>ests is complicated due<br />

to the large continental extension, poor accessibility,<br />

and complex nature of the environment. In particular,<br />

Brazil has a vast territory with a tremendous need<br />

<strong>for</strong> resource management in<strong>for</strong>mation such as can be<br />

provided by satellite imaging radars. Many obstacles<br />

have been faced <strong>for</strong> the integration of the Amazon region<br />

to the rest of the country. This integration is necessary<br />

nowadays more than ever with respect to the<br />

0094-5765/$ - see front matter © 2004 Elsevier Ltd. All rights reserved.<br />

doi:10.1016/j.actaastro.2004.09.007


36 R. Schröder et al. / Acta Astronautica 56 (2005) 35 – 43<br />

increasing Brazilian population and the immense natural<br />

(renewable and non-renewable) resources available<br />

in the region. <strong>SAR</strong> systems have not only the capability<br />

to image but also to measure bio-/geophysical environmental<br />

parameters of such a “complex environment”<br />

in a systematic and repetitive manner in support of<br />

natural resource assessment and the monitoring processes<br />

that are essential parts of procedures <strong>for</strong> sustainable<br />

environmental management.<br />

In the range of wavelengths used by imaging<br />

radar, backscatter intensity from terrain surfaces is<br />

strongly controlled by decimetre-scale changes in surface<br />

slopes, or by centimetre-scale roughness of the<br />

surface. Thus, the sensitivity of <strong>SAR</strong> to the macrotopography<br />

(slopes, tilts, broad undulations in the<br />

terrain), the surface roughness (roughness on the scale<br />

of the <strong>SAR</strong> wavelength) and to the presence of moisture<br />

or liquid water content of a medium affecting the<br />

complex dielectric constant, makes it an ideal instrument<br />

<strong>for</strong> thematic mapping and resource management<br />

purposes in the tropical region, and when stereoscopic<br />

capabilities are available, <strong>for</strong> topographic mapping.<br />

In addition, the large ratio of <strong>SAR</strong> return from <strong>land</strong><br />

versus water is primarily a function of contrast of<br />

dielectric properties and surface roughness, providing<br />

a striking interface which also facilitates coastal<br />

delineation and related mapping application (flooding,<br />

wet<strong>land</strong> and hydrological studies in the Brazilian<br />

Amazon).<br />

On the other hand, <strong>for</strong>est biomass is today one of<br />

the most unknown parameters in dynamic ecosystem<br />

change especially with respect to a reliable global<br />

Carbon-flux modelling. In many regions of our planet<br />

even a mere <strong>for</strong>est classification is missed. Parallel to<br />

the ecological dimension, and under the light of the<br />

Kyoto protocol, this problem has also a political dimension<br />

that increases the responsibility of the scientific<br />

community to provide exact answers. The fact that<br />

biomass in<strong>for</strong>mation is especially missed in remote<br />

areas (i.e. tropical and boreal <strong>for</strong>est ecosystems) combined<br />

with the fact that these ecosystems contain the<br />

biggest amount of <strong>for</strong>est biomass make remote sensing<br />

techniques a challenge. However, optical remote<br />

sensing sensors are in general not capable of measuring<br />

<strong>for</strong>est biomass or monitoring the dynamics of de<strong>for</strong>estation<br />

and biomass regeneration. An alternative<br />

methodology is the estimation of <strong>for</strong>est biomass based<br />

on the estimation of <strong>for</strong>est height from radar remote<br />

sensing data. One of the key challenges facing imaging<br />

radars is to <strong>for</strong>ce evolution from high-resolution<br />

qualitative imaging to accurate high-resolution quantitative<br />

measurement. One very promising way to extend<br />

the observation space is the combination of interferometric<br />

and polarimetric observations. <strong>SAR</strong> interferometry<br />

is today an established technique <strong>for</strong> the<br />

estimation of the height location of scatterers through<br />

the phase difference in images acquired from spatially<br />

separated locations at either end of a baseline.<br />

The initiative of the joint study of a <strong>small</strong><br />

spaceborne <strong>SAR</strong> is a consequence of a long-term<br />

Brazilian–German scientific and technical cooperation<br />

that was initiated between INPE and DLR in the<br />

1970s. The decision to per<strong>for</strong>m a pre-phase A study<br />

<strong>for</strong> <strong>MAP<strong>SAR</strong></strong> was established in 2001 following<br />

several meetings in both agencies ([1,2]). Based on<br />

the specific and complementary experience of both<br />

partners, the sharing of the thematic responsibilities<br />

within the study was agreed. Brazil is responsible<br />

<strong>for</strong> the plat<strong>for</strong>m and integrated satellite analysis and<br />

Germany <strong>for</strong> the payload and orbit analysis.<br />

2. User requirements<br />

The <strong>MAP<strong>SAR</strong></strong> <strong>mission</strong> is tailored to optimally support<br />

the potential user groups in both countries taking<br />

into account distinct aspects of specific applications.<br />

Thus, in April 2002, a working group of Brazilian<br />

<strong>SAR</strong> scientists and technical experts (potential <strong>SAR</strong><br />

end-users) met on the campus of INPE (São José dos<br />

Campos) to per<strong>for</strong>m a review of the use of imaging<br />

radar to derive surface characteristics important <strong>for</strong><br />

tropical applications. The first workshop of potential<br />

end-users of <strong>MAP<strong>SAR</strong></strong> was structured <strong>for</strong> the purpose<br />

of (1) per<strong>for</strong>ming an assessment of the current understanding<br />

of the applications of <strong>SAR</strong> in Brazil and (2)<br />

developing end-user requirements and recommendations<br />

aiming at a joint INPE–DLR <strong>small</strong> spaceborne<br />

<strong>SAR</strong> program.<br />

The consensus of the Brazilian working group<br />

was that a spaceborne <strong>SAR</strong> <strong>mission</strong> will provide a<br />

powerful new tool to acquire data and to derive important<br />

and unique in<strong>for</strong>mation of vegetated terrain<br />

of the Amazon Region. Due to the enormous scarcity<br />

of up-to-date in<strong>for</strong>mation, which is fundamental<br />

<strong>for</strong> planning and strategic decision-making about


R. Schröder et al. / Acta Astronautica 56 (2005) 35 – 43 37<br />

environmental assessment, management and monitoring<br />

of natural resources in the Brazilian Amazon, the<br />

proposed <strong>small</strong> spaceborne <strong>SAR</strong> initiative should be<br />

strongly oriented to a quasi-operational (“applicationoriented”)<br />

system. This is dedicated to thematic<br />

mapping purposes <strong>for</strong> topography, vegetation and<br />

de<strong>for</strong>estation, geology, hydrology, etc. Furthermore,<br />

it was strongly recommended to have a series of<br />

satellites aiming at the operational aspects and the<br />

program continuity. In addition, the <strong>MAP<strong>SAR</strong></strong> concept<br />

should also address aspects of integration with<br />

the Brazilian “Surveillance of the Amazon System”<br />

(SIVAM/SIPAM), due to the complementary nature of<br />

both sources (spaceborne/airborne) of multi-polarized<br />

and fully polarimetric L-<strong>band</strong> data. Finally, although<br />

recognised in most application fields, the effects of<br />

polarimetry and interferometry on the image in<strong>for</strong>mation<br />

content are not well understood in some of those<br />

fields.<br />

The Brazilian applications are of high interest <strong>for</strong><br />

the German potential user community. Additional applications,<br />

which are of specific importance <strong>for</strong> the<br />

German user side, as biomass estimation, disaster<br />

monitoring and security complement the Brazilian<br />

disciplines. The common aim is a global biomass<br />

mapping <strong>mission</strong> covering major <strong>for</strong>ests biomes of<br />

the globe (tropical and boreal regions). This requires<br />

the capability of polarimetric <strong>SAR</strong> interferometry <strong>for</strong><br />

<strong>for</strong>est height estimation which is directly related to<br />

<strong>for</strong>est biomass using allometry. The Brazilian and the<br />

German requirements have been merged resulting in<br />

the final user requirements <strong>for</strong> <strong>MAP<strong>SAR</strong></strong> presented<br />

in Table 1(a) and (b).<br />

Due to several restrictions related to INPE’s multi<strong>mission</strong><br />

plat<strong>for</strong>m (mass, power generation, geometric<br />

envelope and data rate) the following main limitations<br />

were imposed upon the satellite configuration: use of<br />

a single frequency and use of a light weight antenna.<br />

The resulting antenna concept limits the maximum<br />

instantaneous swath width to approximately 55 km.<br />

Table 2 summarizes the final specification.<br />

3. Payload configuration<br />

Based on these user requirements and plat<strong>for</strong>m limitations<br />

the design of the L-<strong>band</strong> <strong>SAR</strong> sensor is based<br />

on a reflector antenna concept. The main advantage<br />

is the possibility to realize full polarization and high<br />

<strong>band</strong>width with low technological risk at low costs.<br />

The main drawbacks are the limited instantaneous<br />

swath width and the lack of an electronic beam steering<br />

capability.<br />

3.1. <strong>SAR</strong> antenna<br />

A key problem <strong>for</strong> a L-<strong>band</strong> <strong>SAR</strong> is the large antenna<br />

size required compared to higher earth observation<br />

frequencies. Fig. 1 shows an approximation <strong>for</strong><br />

the minimum antenna size required to access various<br />

incidence angles at different orbit heights taking into<br />

account a sufficient ambiguity suppression of approximately<br />

−20 dB.<br />

It is obvious that a low orbit height reduces the<br />

antenna size requirements significantly. On the other<br />

hand, orbit heights below 500 km can become critical<br />

with respect to maintainability and drag compensation.<br />

To achieve a maximum incidence angle of 45 ◦<br />

an antenna aperture of at least 27 m 2 is necessary at<br />

600 km orbit height. Lower orbit heights would allow<br />

to reduce the antenna aperture, higher orbit heights<br />

would require to increase it. A reduction of the antenna<br />

dimensions as far as possible is mandatory taking<br />

into account the launcher and plat<strong>for</strong>m limitations.<br />

There<strong>for</strong>e, an orbit height as low as possible is advantageous<br />

<strong>for</strong> the <strong>SAR</strong> sensor design. Considering<br />

the requirements of the Brazilian multi <strong>mission</strong> plat<strong>for</strong>m<br />

it was agreed between the partners to concentrate<br />

the investigations on orbits with a height between 600<br />

and 650 km. There<strong>for</strong>e, the basis <strong>for</strong> the <strong>SAR</strong> sensor<br />

design was chosen to be at a height over ground of<br />

620 km. Variations of ±30 km do not affect the design<br />

significantly.<br />

The final choice of the antenna size is a trade-off between<br />

various parameters. We considered a Cassegrain<br />

configuration with an elliptical parabolic main reflector<br />

with 7.5 m length in azimuth and 5 m width in elevation.<br />

Neither the subreflector mounting nor the horntype<br />

prime radiator need to be folded. The resulting<br />

antenna gain in combination with a low orbit allows<br />

very good sensitivity with a reasonable power budget.<br />

3.2. Access region of the <strong>SAR</strong> sensor<br />

The antenna configuration and the restrictions imposed<br />

by a sufficient ambiguity suppression in azimuth


38 R. Schröder et al. / Acta Astronautica 56 (2005) 35 – 43<br />

Table 1<br />

<strong>MAP<strong>SAR</strong></strong> user requirements<br />

(a)<br />

Application/<strong>MAP<strong>SAR</strong></strong> parameters Agriculture Cartography Disaster monitoring Forestry<br />

Frequency LLC L ∗ ,C<br />

L C L L<br />

Polarization/polarimetry quad. pol N.E. VV, HH quad. pol.<br />

quad. polN.E. quad. pol quad. pol.<br />

Incidence interval Variable 25–45 ◦ variable (45 ◦∗ ) 20 ◦ –30 ◦ /45 ◦ –60 ◦ 20 ◦ –45 ◦<br />

45 ◦∗ variable 20 ◦ –45 ◦<br />

Spatial resolution 30 m 5 m 30–50/15 m 10 m<br />

3–5 m 3–5 m 3–5 m 10 m<br />

Swath 30 km N.A. 150–350 km 100 km<br />

30 km variable variable variable<br />

Orbit inclination N.A. sun-syn sun-syn sun-syn<br />

sun-syn sun-syn sun-syn sun-syn<br />

Look direction N.A. asc/desc asc/desc N.A.<br />

asc/desc asc/desc asc/desc asc/desc<br />

Revisit 15 days N.A. < 1 day monthly<br />


R. Schröder et al. / Acta Astronautica 56 (2005) 35 – 43 39<br />

Table 2<br />

<strong>MAP<strong>SAR</strong></strong> final specification taking into account user requirements<br />

and MMP constraints<br />

Off-nadir angle<br />

Frequency<br />

Polarization<br />

Incidence interval<br />

Spatial resolution<br />

Swath<br />

Orbit inclination<br />

Coverage<br />

Look direction<br />

Revisit<br />

Data access<br />

Additional requirement<br />

L-<strong>band</strong><br />

Single, dual and quad<br />

20 ◦ –45 ◦<br />

3–20 m<br />

20–55 km<br />

Sun-synchronous<br />

Global<br />

Ascending/descending<br />

Weekly<br />

Near real time<br />

Stereoscopy and interferometry<br />

620 km<br />

Incidence angle<br />

20˚<br />

48,1˚<br />

Nadir<br />

204 km<br />

395 km<br />

Fig. 3. Access region of the <strong>SAR</strong> sensor.<br />

Nadir Zone<br />

20 30 40 50 60<br />

30<br />

Orbit height= 500 km<br />

Orbit height= 600 km<br />

Orbit height= 700 km<br />

L-Band (f=1.3 GHz)<br />

5<br />

Ambiguities appr. -20 dB<br />

0<br />

0 10 20 30 40 50 60<br />

Incidence angle / deg<br />

Fig. 1. Minimum antenna size in L-<strong>band</strong>.<br />

25<br />

20<br />

15<br />

10<br />

Minimum antenna area /m 2<br />

between 20 ◦ and 48.1 ◦ incidence angle covering an<br />

area of 395 km on both sides of the satellite nadir track.<br />

In full polarization mode the PRF must be doubled,<br />

leading to a useful range between 5200 and 6000 Hz.<br />

The corresponding field of view is between 20 ◦ and<br />

39.3 ◦ incidence angle, covering an area of 245 km on<br />

both sides of the satellite nadir track.<br />

Fig. 3 illustrates the whole access region. Since the<br />

sensor has no electronic beam steering the current<br />

swath is selected by rolling the whole satellite in the<br />

necessary position. The same is done to change between<br />

left or right looking configuration. This results<br />

in certain restrictions to image regions within the same<br />

orbit which are close to each other in flight direction<br />

but separated in elevation by more than one instantaneous<br />

swath width.<br />

3.3. <strong>MAP<strong>SAR</strong></strong> radar modes<br />

Offnadir angle/ deg<br />

60<br />

50<br />

40<br />

30<br />

20<br />

transmit interference<br />

nadir interference<br />

PRF-RESTRICTIONS<br />

10<br />

2200 2400 2600 2800 3000 3200<br />

PRF / Hz<br />

Fig. 2. PRF <strong>band</strong>s with interference.<br />

DLR<br />

Based on the user requirements, <strong>MAP<strong>SAR</strong></strong> offers<br />

three different resolution modes (3, 10, and 20 m) operated<br />

in the conventional stripmap mode. The chirp<br />

<strong>band</strong>width is designed to operate in the full 85 MHz allowed<br />

by the World Administrative Radio Conference<br />

(WARC). This enables a high-resolution (HR) mode<br />

in the order of 3 m without increasing the complexity<br />

of the front-end and the antenna. For lower resolution<br />

modes the <strong>band</strong>width is reduced accordingly. A single<br />

polarization mode (SPM), a dual polarization mode<br />

(DPM) and a quad polarization mode (QPM) are <strong>for</strong>eseen<br />

<strong>for</strong> all of these resolution modes. Table 3 lists the<br />

sensor and per<strong>for</strong>mance parameters <strong>for</strong> some of these<br />

modes.<br />

As a baseline a RF peak power of 1000 W was<br />

considered. Depending on the priority of the different


40 R. Schröder et al. / Acta Astronautica 56 (2005) 35 – 43<br />

Table 3<br />

<strong>MAP<strong>SAR</strong></strong> radar modes<br />

Parameter HR mode MR mode LR mode<br />

High resolution Medium resolution Low resolution<br />

SPM DPM QPM<br />

Access region near far near far near far<br />

Resolution<br />

Range/m 4,7 3,1 10 10 20 20<br />

Azimuth/m 3,1 3,1 10 10 20 20<br />

Off-nadir angle/ ◦ 20,0 41,8 20,0 41,8 20,0 32,1<br />

Incidence angle/ ◦ 20,3 47,6 20,0 48,1 20,0 36,8<br />

Ground swath width/km 38,3 20,5 45,1 35 43,4 28<br />

PRF/Hz 2650 2718 2660 2680 5320 5320<br />

Pulse <strong>band</strong>width/MHz 85 85 42,5 21,25 21,25 21,25<br />

Sampling frequency/MHz 96 96 2 × 48 2 × 24 2 × 24 2 × 24<br />

Pulse length/μs 25 25 10 10 10 10<br />

Data rate/Mbit/s 262 300 267 300 247 249<br />

RF peak power/W 1000 1000 1000 1000 1000 1000<br />

Average DC power/W ∼ 490 ∼ 500 ∼ 440 ∼ 440 ∼ 440 ∼ 440<br />

NESZ/dB<br />

Image center −23,6 −19 −28,9 −25,4 −34,6 −33,3<br />

Image edge −17,0 −18,3 −19,9 −23,3 −26,6 −30,9<br />

Number of looks<br />

Range 1 1,33 1,14 1,13 1,04 1,73<br />

Azimuth 1 1 3,3 3,3 6,6 6,6<br />

Radiometric res./dB


R. Schröder et al. / Acta Astronautica 56 (2005) 35 – 43 41<br />

Table 4<br />

Radar beam specification<br />

Beam number/ Incidence angle Swath width/ Eff. PRF/<br />

km range/ ◦ km Hz<br />

1 19,93–23,95 45,1 2660<br />

2 23,76–27,32 41,9 3010<br />

3 27,12–30,71 44,5 2660<br />

4 29,69–33,31 46,9 2660<br />

5 32,86–36,52 50,4 2910<br />

6 36,15–39,86 54,8 2660<br />

7 39,50–42,69 50,0 2900<br />

8 42,22–45,24 51,0 2640<br />

9 45,16–46,92 31,6 2870<br />

10 46,28–48,08 33,5 2680<br />

Fig. 6. Average revisit time over Brazil.<br />

Fig. 5. Maximum revisit time over Brazil.<br />

The actual concept of the <strong>MAP<strong>SAR</strong></strong> <strong>mission</strong> favours<br />

an orbit with a repeat cycle of 37 days and an altitude<br />

of about 620 km. This orbit has an inclination of<br />

about 97.86 ◦ . The sensor field of view <strong>for</strong> this orbit is<br />

between 20 ◦ and 48.1 ◦ to fulfil the specifications of<br />

the users. Fig. 5 shows the maximum revisit times <strong>for</strong><br />

Brazil. The highest value is 132 h, but most regions of<br />

Brazil will be reached in less than 100 h.<br />

In Fig. 6, the average value <strong>for</strong> the revisit times can<br />

be seen. The maximum value over the northern part of<br />

Brazil is 42.3 h, but most regions have average revisit<br />

times far less than 40 h.<br />

Because of the fact that the latitude of the German<br />

regions ranges between 47 ◦ and 55 ◦ , the revisit times<br />

are quite lower than <strong>for</strong> some Brazilian regions. In<br />

detail, the maximum values can be seen in Fig. 7, the<br />

average values <strong>for</strong> Germany are shown in Fig. 8.<br />

Fig. 7. Maximum revisit time over Germany.<br />

Fig. 8. Average revisit time over Germany.


42 R. Schröder et al. / Acta Astronautica 56 (2005) 35 – 43<br />

Fig. 9. <strong>MAP<strong>SAR</strong></strong> satellite configuration.<br />

Fig. 11. MMP pictorial view (blow-up).<br />

Table 5<br />

<strong>MAP<strong>SAR</strong></strong> payload nominal mass budget<br />

Sub-system<br />

Mass (kg)<br />

4. <strong>MAP<strong>SAR</strong></strong> satellite<br />

Fig. 10. MMP block diagram.<br />

Mechanical structure 30.0<br />

Thermal control 4.0<br />

Radar sensor & data acquisition 193.6<br />

Data storage & transmitter 42.5<br />

Total mass 270.1<br />

Specified mass 280.0<br />

Nominal margin 9.9<br />

4.1. Satellite concept<br />

The <strong>MAP<strong>SAR</strong></strong> satellite utilizes a modular concept<br />

(Fig. 9), consisting of a payload module and the Brazilian<br />

Multi-Mission Plat<strong>for</strong>m (MMP).<br />

The MMP concept provides <strong>for</strong> a capability to support<br />

a variety of low earth orbit <strong>mission</strong>s using the<br />

same basic three-axis stabilized plat<strong>for</strong>m with different<br />

payload modules. The MMP block diagram and<br />

pictorial view are shown in Figs. 10 and 11. The MMP<br />

is already being developed by INPE and its first flight<br />

model shall be ready by the end of 2005.<br />

Thermal Control<br />

1%<br />

Structure<br />

11%<br />

<strong>MAP<strong>SAR</strong></strong><br />

Nominal Mass Budget<br />

Radar Sensor<br />

69%<br />

Margin<br />

4%<br />

Data Storage<br />

15%<br />

4.2. Mass budget<br />

Table 5 presents a summary of the nominal mass<br />

budget <strong>for</strong> the <strong>MAP<strong>SAR</strong></strong> payload.<br />

The total mass <strong>for</strong> the <strong>MAP<strong>SAR</strong></strong> payload is<br />

270.1 kg. Compared to the specified value (280.0 kg),<br />

this leads to a margin of 9.9 kg. This shows that, in<br />

Fig. 12. <strong>MAP<strong>SAR</strong></strong> payload mass breakdown.<br />

terms of mass, the proposed configuration is feasible.<br />

Fig. 12 shows the payload mass breakdown in a pie<br />

diagram.


R. Schröder et al. / Acta Astronautica 56 (2005) 35 – 43 43<br />

The ground segment <strong>for</strong> <strong>MAP<strong>SAR</strong></strong>, as a bilateral<br />

project, has to fulfil the requirements and account <strong>for</strong><br />

the existing infrastructure of each individual partner.<br />

In principle, the ground segment is, as usually in all<br />

large Earth observation projects, comprised of two essential<br />

elements, the FOS (flight operations segment)<br />

and PDS (payload data segment). Being a multilateral<br />

program, a clear definition of the responsibilities and<br />

the data policy have to be developed during the (future)<br />

engineering phase, defining the operational responsibilities,<br />

duties and rights of the individual partner. The<br />

following guidelines are in principle assumed:<br />

• The scientific community will be served by national<br />

institutions, a possible commercial user community<br />

will be served by data distributors. Both have to be<br />

served by the PDS.<br />

• Each partner will serve its user community in<br />

its own region (e.g. Brazil—Latin America;<br />

Germany—Europe). The data distribution over<br />

other regions has to be decided during the next<br />

program phases.<br />

• The FOS will be arranged in a primary and a secondary<br />

satellite control center, with equal functions<br />

managing the spacecraft according to a jointly defined<br />

timely structure. Both control centres use a<br />

joint network of TT & C ground stations <strong>for</strong> the<br />

LEOP and operational phase.<br />

Fig. 13. <strong>MAP<strong>SAR</strong></strong> satellite and launcher fairings.<br />

5. Launcher<br />

In terms of dimensions, the <strong>MAP<strong>SAR</strong></strong> payload<br />

layout is compatible with the majority of MMP<br />

considered standard launcher family. Fig. 13 shows<br />

the <strong>MAP<strong>SAR</strong></strong> satellite inside the launcher fairing<br />

dynamic envelopes. Some candidate launchers are<br />

excluded due to the envelope constraints imposed by<br />

the stowed reflector antenna envelope.<br />

6. Ground segment<br />

7. Conclusions<br />

An innovative <strong>small</strong> satellite <strong>mission</strong> with an L-<strong>band</strong><br />

<strong>SAR</strong> was described. The study was prepared by INPE<br />

and DLR, taking into account Brazilian and German<br />

user requirements. The preliminary feasibility was<br />

demonstrated <strong>for</strong> a reflector antenna concept. A high<br />

degree of innovation is presented in the design considering<br />

the <strong>small</strong> <strong>SAR</strong> payload, the reflector antenna<br />

and the remarkable sensor per<strong>for</strong>mance. The applications<br />

will take advantage of high spatial resolution<br />

L-<strong>band</strong> <strong>SAR</strong> with enhanced capabilities (polarimetry,<br />

stereoscopy, interferometry), particularly suitable <strong>for</strong><br />

the Amazon region and Boreal <strong>for</strong>est operations.<br />

The deployment of the reflector antenna and the<br />

solid state power amplifier are main technological<br />

challenges <strong>for</strong> this project, but nevertheless, after<br />

careful analysis, the <strong>SAR</strong> sensor is considered feasible<br />

and its development is estimated in 5 years.<br />

<strong>MAP<strong>SAR</strong></strong> launch is envisaged <strong>for</strong> 2008.<br />

References<br />

[1] INPE/DLR, <strong>MAP<strong>SAR</strong></strong> Pre-Phase A: Final Report, National<br />

Institute <strong>for</strong> Space Research (INPE) and Deutsches Zentrum<br />

für Luft und Raumfahrt (DLR), December 2002, 142pp.<br />

[2] www.obt.inpe.br/mapsar/mapsarindex1.htm.

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