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    A Concept for an Advanced Reflector-Based

    Space Surveillance Radar

    A. Patyuchenko, M. Younis, G. Krieger, M. Weigel

    German Aerospace Center (DLR)

    European Space Surveillance Conference07-09 June, 2011

    Madrid, Spain

    Slide 2

    Outline

    Introduction

    Conventional Radar for Space Debris Detection

    Concept of the Reflector-Based DBF Radar System

    Aspects of the Improved DBF Radar Performance

    Prototype Development

    Conclusion

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    Slide 3

    Outline

    Introduction

    Conventional Radar for Space Debris Detection

    Concept of the Reflector-Based DBF Radar System

    Aspects of the Improved DBF Radar Performance

    Prototype Development

    Conclusion

    Slide 4

    Space Debris Environment

    Space debris orbital man-made space junk is a many-sided problem becoming more

    and more critical nowadays.

    Low Earth Orbit (LEO)

    debris population

    SSA has to guarantee the safe and stable space environment.

    Reliable and operationally flexible source of information for SSA are required.

    Technical requirements for the measurement systems are becoming more stringent.

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    Slide 5

    Detection of Space Debris

    Various ground based radar systems are used to detect space debris at LEO:

    Reflector systems are chosen for their high directivity and a low side lobe level.

    Classical radar measuring systems have limitations of physical and technical nature.

    In particular, reflector systems performance is limited in terms of a mechanical

    steering of an antenna and a search volume.

    HAX, USMU Radar, Japan

    TIRA, Germany

    TRADEX, US

    Slide 6

    Outline

    Introduction

    Conventional Radar for Space Debris Detection

    Concept of the Reflector-Based DBF Radar System

    Aspects of the Improved DBF Radar Performance

    Prototype Development

    Conclusion

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    Slide 7

    Earth rotation

    Operational Modes I

    Antenna elevation angle is fixed.

    Volume density of space objects is observed

    as the Earth rotates.Information on non-cataloged objects is

    obtained:

    Objects size

    Orbit data

    Observation methods are translated into two main operational modes:

    Beam-Park Mode and Tracking Mode

    Beam-Park Mode

    Data precision is poor.

    Slide 8

    Operational Modes II

    Antenna pointing direction follows a target.

    Target directed observation is performed.

    Accurate information on cataloged

    objects is obtained:

    Tracking Mode

    Object characteristics

    and orbit data

    Initial orbit data are required.

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    Slide 9

    Elevation view Azimuth view

    1c

    Lp

    1c

    Lp

    Performance Aspects: Capture Probability

    Geometrical representation of the tracking operational mode:

    - Cross-Track Orbit Uncertainty

    Probability of a target capture depends on the HPBW of the antenna and a slantrange to the target and thus, it is proportional to the observation volume.

    Slide 10

    Performance Aspects: Antenna Elevation Angle Impact

    Peak transmit power = P1

    Peak transmit power = P2P1 > P2

    Antenna elevation angle [deg.]

    Increase of the antenna elevation angle leads to:

    - decrease of the beam spatial extension => capture probability decreases;

    - decrease of the free space attenuation => detection probability increases.

    L-Band

    S-Band

    X-Band

    Ku-Band

    Orbit height: 1000 km

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    Slide 11

    Performance Aspects: Operational Frequency Impact

    Capture probability is directly proportional to the HPBW.

    Detection probability is directly proportional to the gain.

    G2

    G1

    3dB2

    3dB1

    G1 < G2

    3dB1>3dB2

    L-Band

    X-Band

    03dB

    c

    Df

    2

    0

    DfG

    c

    D

    - antenna shape and illumination parameter

    - antenna diameter

    - frequency

    - net efficiency

    HPBW and gain are inversely dependent in terms of frequency.

    Slide 12

    Conventional System Performance

    3200

    Sphere

    (10 cm diameter)

    30m/L

    30m/S

    30m/X

    Target is orbiting the Erath at 1000 km height.

    The slant range of 3200 km is equivalent to the 5 antenna elevation angle for theconsidered system

    1/ 42 2

    max 3

    min(4 )

    t

    s

    G PR

    kT L SNR

    Maximum detection range:

    G

    tP

    sT

    L

    - pulse length

    - gain

    - RCS

    - wavelength

    - Tx peak power

    - loss factor

    - system noise temp.

    min 11dBSNR

    0.99dp

    0.01fap

    The largest maximum detection range is achieved at X-Band.

    Cross-track beam extension at 1000 km distance:

    X-Band: 0.96 km, S-Band: 5.3 km, L-Band: 9.38 km.

    X-Band system allows the lowest probability of capture.

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    Slide 13

    Outline

    Introduction

    Conventional Radar for Space Debris Detection

    Concept of the Reflector-Based DBF Radar System

    Aspects of the Improved DBF Radar Performance

    Prototype Development

    Conclusion

    Slide 14

    Reflector Based DBF Radar Structure

    The concept originates from the spaceborne system [1].

    Multiple independent digital channels with ADCs.Application of innovative DBF techniques.

    Reflector antenna: high directivity and a low side lobe level.

    [1] G. Krieger, el al., Advanced concepts for ultra-wide swath SAR imaging, in Proceedings of the 7th European

    Conference on Synthetic Aperture Radar (EUSAR 08), Friedrichshafen, Germany, June 2008.

    Feed System

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    Slide 15

    12

    1

    2

    Indicesofthefee

    delements

    1

    2

    1

    2

    Wide Tx low-gain beam illuminates the volume in space.

    Narrow Rx high-gain beams follow targets digitally by combining weighted data from

    signal channels.

    Reflector Based DBF SAR Operation

    Slide 16

    Outline

    Introduction

    Conventional Radar for Space Debris Detection

    Concept of the Reflector-Based DBF Radar System

    Aspects of the Improved DBF Radar Performance

    Prototype Development

    Conclusion

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    Slide 17

    Relaxed Requirements for Mechanical Steering

    =16

    TxRx

    16

    The corresponding classical radar has a HPBW of 0.36 only and thus needs to be

    mechanically steered in the tracking mode.

    The DBF system requires no mechanical steering over the angular range of 16(example) and can perform tracking digitally.

    L-Band system using 30 m reflector dish and 34 digital channels:

    Slide 18

    Advanced Operational Modes

    Multiple independent digital channels:

    Advanced operational modes are possible:

    - Track While Scan mode with enhanced efficiency.

    - Effective tracking of several targets over a large angular range.

    The measurement time can be considerably reduced.

    Catalogued and non-catalogued objects: simultaneous capability.

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    Slide 19

    Improved Capture Probability I

    X-Band DBF Radar

    30 m

    48 channels

    Cross-track beam extension at 1000 km is larger by a factor of 45 compared to the

    classical X-Band radar.

    However the detection probability and thus the maximum detection range is lower

    for the DBF Radar due to the decreased gain on transmit.

    0.08

    3.5

    Conventional system

    Slide 20

    Improved Capture Probability II

    The detection probability can be improved by increasing transmit power, using multiple

    PAs or by means of sequential switching of channels:

    1 2 3

    2

    1

    2

    max ( )

    t

    average

    t

    P P u t dt

    - pulse train waveform( )u t

    tavP

    receive window

    P

    1t 2t

    P

    tmaxP

    receive window

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    Slide 21

    Outline

    Introduction

    Conventional Radar for Space Debris Detection

    Concept of the Reflector-Based DBF Radar System

    Aspects of the Improved DBF Radar Performance

    Prototype Development

    Conclusion

    Slide 22

    Prototype Development

    1 personal computer, 2 data storage device, 3 analog-to-digital

    converters with an embedded PC, 4 analog signal generator, 5 arbitrary

    waveform generator, 6 coupler, 7 reflector antenna.

    Multichannel DBF Radar Demonstrator based on the cPCI architecture.

    Development and test of the advanced operational modes.

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    Slide 23

    Outline

    Introduction

    Conventional Radar for Space Debris Detection

    Concept of the Reflector-Based DBF Radar System

    Aspects of the Improved DBF Radar Performance

    Conclusion

    Slide 24

    The new concept allows better performance in terms of a search area and has

    relaxed requirements imposed on the mechanical steering of the antenna.

    Advanced operational Track While Scan mode with efficient tracking of several

    targets simultaneously is possible.

    DBF radar system allows high detection probability and large search volume

    at higher frequencies.

    The prototype system is under development.

    The suggested concept has a high operational flexibility and an improved

    performance. It opens a wide range of problems which must be further

    considered and solved.

    Conclusion

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    Slide 25

    Thank you!