Multistatic Small Satellite Network for Oil Monitoring in Nigeria

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    IAC-12-B4.1.6 MULTISTATIC SMALL SAR SATELLITE NETWORK FOR OIL MONITORING IN

    NIGERIA

    Abdul Duane Lawal

    Space Advanced Research Team, Aerospace Department University of Glasgow, G12 8QQ,

    [email protected]

    Radice, G

    Space Advanced Research Team, Aerospace Department University of Glasgow, G128QQ

    [email protected]

    The requirement for more sophisticated methods for monitoring the widespread oil resources within Nigeria has

    been evident. The use of Synthetic Aperture Radar (SAR) systems is particularly appealing since this payload is

    unaffected by adverse weather conditions and independent of sunlight for its operation. The all-weather

    capability of SAR makes it the most suitable remote sensing platform for monitoring environmental disasters

    such as oil spillage which could be highly elusive to optical sensors such as those onboard NigeriaSat-2. The

    application of interest for this proposed mission is the detection of oil spillage and assistance in monitoring

    illegal oil bunkering activities within and around the Gulf of Guinea region. In this paper, we present aspects of

    the mission design, including the mission objectives and a preliminary satellite design. The user requirement of

    high resolution SAR images, near-real-time data, low revisit time and low mission cost are the main drivers of

    the mission. The paper also describes the analysis for the selection of SAR frequency, consistent with providing

    high resolution images and low spacecraft mass. A discussion of the trade-off analysis between a near polar

    orbit and near equatorial orbit for reduced revisit time is presented. Altitude selection as a function of available

    pulse repetition frequency (PRF), consistent with range and azimuth ambiguities is also highlighted.

    Furthermore, to meet coverage and revisit time requirements with due consideration for cost of the mission, a

    system consisting of a few number of small SAR satellites is described. Satellites within the constellation will

    fly in close formation and maintain fixed across track and radial baseline distances that enable possible

    interferometric applications. Finally, the paper will conclude with a brief description of the small SAR network

    system operating solely within the equatorial region, for monitoring oil spillage disaster and oil bunkering

    activities within and around the Gulf of Guinea.

    mailto:[email protected]
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    INTRODUCTION

    The benefits of space generated data has seen wide

    spread application areas [1, 2, 3], and has benefited

    mankind for over five decades. Space missions

    have provided support in areas such as disaster

    monitoring and mitigation, telecommunications,

    meteorological forecasting and Earth Observations.

    However, even with the apparent contributions of

    space science and technology in driving state-of-

    the-art advancements, several nations are yet to

    embrace grass-root space science and technology

    as a possible solution for economic growth and

    urban development.

    Furthermore, the net contribution of space science

    to education, offers a different dimension in regards

    to the application of fundamental studies acquired

    from educational institutions. The breadth of space

    science spans across multi-disciplinary aspects of

    education, encompassing also law, business studies

    and medicine.

    As a source of revenue, space business has become

    an alternative to terrestrial solutions by providing

    service packages over a plethora of business

    models. The most common being the use of

    satellite communications for the mass market

    services such as television, telephony and

    broadband. Others include the creation of niche

    markets for radio, messaging (Little LEOs) and

    imaging (Remote Sensing), as well as infrastructure

    business by way of capacity leasing,

    manufacturing, launch services and ground

    equipment [5].

    From a security point of view, the most developed

    nations depend on their space resources to protect

    their territorial integrity. This is epitomised by the

    rate at which acquired satellite data is processed

    into information and disseminated to the

    appropriate authorities, thereby supporting the

    process of quick and timely decision making.

    Decisions taken are then relayed to commanders on

    the battle field for onward implementation. In

    addition to reducing troops causality rate, it also

    increases their chances of victory [6].

    The scientific community has continued to make

    remarkable progress by using space research

    programs in protecting humanity. Such examples

    include the contributions of the European space

    systems for monitoring climate changes and its

    effects [7]. Others include the Global Monitoring

    for Environment and Security (GMES) programme

    used for managing natural resources and

    biodiversity, with a recent mission adapted for real-

    time fire monitoring using satellite imagery as one

    of the sources of data into a GIS platform [8].

    The high cost of space missions has been a key

    factor to determining the nations that partake in

    space activities. The Space Shuttle Endeavour, the

    orbiter built to replace the Space Shuttle

    Challenger, cost approximately 1.7 billion US

    dollars [10], while a typical space mission program

    can costs hundreds of millions of dollars [11].

    Although the launch phase plays a huge role in the

    determination of the mission cost as highlighted on

    Figure 1, recent approaches have been taken to

    reduce spacecraft mass. The design, launch and

    operations of low cost, high data space missions

    has recently become a niche market with

    recognised companies like Surrey Satellite

    Technology Limited (SSTL), UK considered as a

    major stake-holder. With over 20 years of

    experience in launching and operating highly

    capable and cost effective small satellite missions,

    with 39 missions recorded, SSTL provides access

    to space for a fractional price normally associated

    with space missions [14, 15].

    Most nations yet to embrace the relevance of space

    missions as a multi-dimensional avenue for

    development, due to the relatively unaffordable

    cost, are mainly classified as developing

    countries. There are 156 countries classified as

    developing nations according to the International

    Monetary Funds World Economic Outlook Report

    given April 2012 [17], with Cuba and North Korea

    not included. According to Sheffrin et al (2003),

    these countries are known as less developed

    countries (LDC), with low living standards,

    undeveloped industrial base, and low Human

    Development index (HDI) relative to other

    countries[16].

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    Figure 1: Spacecraft mass vs mission cost [11]

    For the purpose of this paper, the Equatorial

    Region (ER), is defined as the area geographically

    located within 10 degrees of the Equator.

    Subsequently, there are 49 countries located within

    the ER with only Singapore classified as a

    developed country [18]. Furthermore, in this

    region, only Brazil, Indonesia, Malaysia and

    Nigeria have space capabilities at different levels

    defined under the framework of four major

    technology categories as defined by Wood, D.

    (2011).

    To address the highlighted issues preventing most

    developing nations from acquiring space

    capabilities, this paper proposes an approach that

    encourages the collaboration between countries

    within the ER. The approach suggests the

    establishment of a network of space systems

    dedicated and operated by member states within the

    ER. To define the overall mission concept, this

    paper uses Nigeria as a case-study.

    To this end, baseline mission objectives for

    Master_SAR_01 (M01) will be outlined, leading to

    a discussion on its mission design. A brief

    description of pulse repetition frequency (PRF) and

    orbit selection process is presented. Coverage

    analysis comparing the use of a near polar orbit

    (NigeriaSat-2) and a near equatorial orbit (M01) for

    the proposed mission is conducted. Furthermore the

    proposed sites for locating the ground segments for

    the network will be highlighted.

    Finally a system for a network of satellites

    operating within the ER will be described.

    MISSION OBJECTIVES

    The recent environmental disaster experienced in

    New Zealand as a result of a cargo ship running

    aground, with over 340 tonnes of oil spilled is

    regarded as New Zealands worst in decades [20].

    In 2010, the Gulf of Mexico oil spill, also regarded

    as the worst US environment disaster saw at least

    20 million gallons flow into the Gulf of Mexico

    and affecting more than 70 miles of the Louisiana

    coastline. The accident that led to explosion and

    fire which killed 11 people, caused wide spread oil

    pollution in the Gulf of Mexico [21, 22, 23].

    It is estimated that between 100,000 and 130,000

    barrels per day (bbl/d) of crude oil, worth an

    estimate of $3billion is stolen from Nigeria via

    illegal oil bunkering activities within and around

    the Gulf of Guinea [24]. The Gulf of Guinea

    stretches through Central and West Africa and is

    increasingly identified as one of the worlds most

    poorly governed maritime stretches [25]. It has

    been reported to be used for various forms of

    nefarious activities such as human trafficking from

    Senegal to Europe, drug trafficking and oil related

    crimes [25, 26, 27, 28].

    The capacity to monitor the local maritime traffic

    and infrastructures involving oil exploitation rigs

    and platforms provides addition benefits which

    include: information on geographical location of

    ships, ship size (resolution dependent), ship route

    and speed.

    With the stage set for a low-cost sophisticated

    approach to addressing the aforementioned issues,

    the use of a spaceborne remote sensing system for

    complimenting terrestrial efforts has become

    paramount. Although Nigeria current has 3

    spaceborne optical remote sensing platforms

    (NigeriaSat-1, NigeriaSat-2 and NigeriaSat-X),

    their operation is limited by daylight and adverse

    weather conditions. Additionally, to ensure rapid

    response in the event of oil spills, and to maintain

    continuous vigilance over the Gulf of Guinea, 24

    hour surveillance is required.

    The primary mission objective is the use of

    interferometric operation for generation of high

    resolution data for the Equatorial Region. The

    following are the mission design drivers:

    Low cost space mission

    24 hour surveillance of Gulf of Guinea

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    Monitor oil resources/ detection of oil

    spill

    High resolution data

    Near-real-time data acquisition

    Low temporal resolution

    M01 MISSION DESIGN

    The baseline operational orbit is a circular LEO at

    an altitude of 700km and inclination of 10 degrees.

    The orbit and system parameters are listed in Table

    1 [41].

    Orbit and System Parameters

    Altitude (m) 700

    Revolutions/day 14.5

    Inclination 10

    Period (mins) 98.6

    RAAN (deg) 0 Table 1: Orbit and System Parameters

    The choice of PRF for a spaceborne SAR is an

    important parameter that influences many other

    system parameters. PRF selection is affected by

    several factors which include antenna length,

    incidence angle, swath width, platform velocity,

    platform altitude and transmitter pulse length. The

    system parameters affected by PRF include duty

    factor, peak transmit power and raw data rate.

    Ultimately, the selected PRF constraints must be

    satisfied to ensure the combination of swath width

    and antenna length are compatible by ensuring the

    Nyquist requirement and ambiguity constraints do

    not conflict [39, 40].

    The baseline mode of operation for M01 is the

    stripmap mode. To meet the Nyquist criteria, the

    selected PRF must be greater than the Doppler

    bandwidth of the imaged scene. The Doppler

    bandwidth is given by:

    [ ]

    Where Vsc is the platform velocity, az is the half

    power beamwidth angle and is wavelength.

    The beamwidth is related to the antenna length by

    [2]

    Substituting [2] into [1] yields a minimum PRF

    given by:

    [ ]

    where laz, is the antenna length in the along track

    direction.

    The maximum PRF dictates that the maximum

    echo duration must be less than the interpulse

    period. A system with pulse length p, and scene

    echo duration s, the maximum PRF is calculated as

    follows:

    [4]

    where s is given by

    [5]

    and, SWsr is the slant range extent calculated from

    the difference Rf Rn [39]

    Rf - is the slant range to the far end of the swath

    Rn - is the slant range to near end of swath.

    Although the selected PRF will between the

    PRFmin and PRFmax, other factors such as eclipsing

    and nadir returns must be considered. To avoid

    eclipsing (blind ranges) resulting from isolation

    issues inherent in radar systems, such that returning

    echoes coincide with transmit times, the following

    inequality must be satisfied [39].

    [6]

    where:

    B are whole numbers (1,2)

    corresponding to pulses.

    The other issue that must be avoided are echoes

    from nadir returns, since for every transmit pulse,

    there is a nadir echo. These time of occurrence

    nadir commences from the beginning of the

    transmit pulse. nadir is calculated from

    [ ]

    Where h is the platform altitude above the nadir

    point.

    The PRF that coincides with returning scene echoes

    is described by the inequality [39].

    where:

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    N are whole numbers (1,2)

    corresponding to pulses.

    [8]

    There are other approaches to avoiding nadir

    echoes such as:

    Changing the slope of the chirp waveform

    polarity from positive to negative on an

    interpulse basis.

    Designing antenna to have low gain in the

    nadir direction

    Phase coding the transmit signal to ensure

    filtering of energy from different transmit

    pulses.

    M01 SYSTEM PARAMETERS

    Oil spill modifies surface tension and therefore it

    has a strong impact on radar backscatter level [32].

    The effect on the sea surface is the reduction of the

    surface roughness by damping the waves. This

    results in decreased radar backscatter which appear

    as dark patches on SAR images when compared to

    the surroundings [28, 29].

    Several factors such as oil characteristics and

    environmental factors play key roles in oil spill

    detection in addition to the radar properties. The

    choice of the operational frequency is informed by

    the results obtained from studies which conducted

    multi-frequency scatterometer measurements. The

    results showed that as frequency increases, the sea

    contrast ration of oily/clean sea also increases.

    Therefore, for applications such as oil spill

    detection, higher radar frequencies are expected to

    provide better contrast ratio [30, 31].

    Previous SAR missions like the Radarsat-2, ALOS

    and Envisat missions have used the C-band

    frequency for operations. However, with the recent

    emergence of several X-band Earth observation

    missions notably TerraSAR, COSMO SkyMed and

    Tandem-X, it can be argued that better contrast

    ration is amongst the factors influencing the

    paradigm shift. For the chosen application area, this

    paper selects X-band for its operational frequency.

    Table 2 summarizes the characteristics and

    corresponding values of the M01 system parameters.

    System Parameters

    Frequency (GHz) 10

    Band X

    PRF (kHz) 2.7

    Bandwidth (MHz) 44

    Polarization VV

    Look direction Left

    Antenna width (m)

    Antenna length (m) 6

    Incidence angle range (deg) 45

    Resolution (m) 3 Table 2: M01 System Parameters

    COVERAGE ANALYSIS FOR M01

    Coverage analysis of the ER was first conducted

    using one master satellite (M01) and then using two

    master satellites (M01 & M 11). The simulation was

    carried out over 7 days period, using Satellite Tool

    Kit (STK), with granularity set to 2 degrees. Table

    3 summarizes the result of the coverage analysis of

    M01 over the ER. An average time of 12% is spent

    covering each latitude range within the defined

    region, thereby increasing the possibility of

    increasing the number of looks at any area of

    interest in addition to the benefits of short revisit

    time.

    Latitude

    (deg)

    Time covered

    (%)

    Total time covered

    (mins)

    -9 12.76 183.75

    -7 13.20 190.15

    -4 15.51 194.54

    -2 13.69 197.14

    0 13.76 198.08

    2 13.71 197.38

    4 13.54 195.02

    7 13.26 190.89

    9 12.83 184.78

    Table 3: Summary of coverage analysis for M01 over the ER

    Figure 2 show that M01 potentially has access to

    100 percentage of the ER on a daily basis

    depending on the sensor swath.

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    Figure 2: Coverage analysis of ER using M01

    Coverage over Nigeria

    With Nigeria as the primary focus of this paper, a

    coverage assessment was conducted over 7 days.

    Figure 3 show that M01 makes contact with the

    existing ground station in Abuja on each of its

    passes. The average duration of each pass is 13

    minutes. This is in contrast to the average of 4

    passes made by existing missions such NigeriaSat-

    2, whose mission involves global coverage.

    NigeriaSat-2 is a near polar orbit at an altitude of

    700km [37, 38].

    Figure 3: Typical M01 daily access to Abuja groundstation

    Therefore, for applications that do not require the

    acquisition of global coverage data, a near

    equatorial orbit is better suited when compared to a

    near polar orbit. Table 4 compares the difference

    between the access times to the Abuja

    groundstation in Nigeria, between NigeriaSat-2

    (near polar orbit) and M01 (near equatorial orbit).

    Parameter NigeriaSat-2 M01

    Payload MRI/VHRI SAR

    Classification Passive Active

    Period of operation Daylight 24 hours

    Altitude (Km) 700 700

    Inclination (deg) 98 10

    Orbital period 98 98

    Average number of daily passes 4 14

    Average duration of pass (min) 10 13.5

    Total average daily access (min) 40 189

    Table 4: Comparing daily access to groundstation in Abuja, between NigeriaSat-2 (near polar orbit) and M01 (near equatorial

    orbit)

    Improving Coverage of Nigeria

    The busy nature of the Gulf of Guinea and the

    territorial waters around Nigeria owing to seafaring

    oil related activities prompts the need of frequent

    surveillance. The approach taken to meet this

    requirement involves the introduction of M11, an

    identical monostatic SAR satellite to M01 in

    configuration. M11 also shares the same orbital

    elements as M01, but are separated by mean

    anomaly of 180 degrees.

    Figure 4: Coverage analysis of ER using M01 and M11.

    Figure 4 shows that the introduction of M11, flying

    in the same orbit as M01, doubles the percentage of

    time available for covering the ER when compared

    to Figure 2.

    Furthermore, the access time to the Abuja

    groundstation in Nigeria also increases two-folds

    with a total of 28 passes and a total average time of

    364 minutes daily. Figure 5 outlines a typical

    access to Abuja groundstation for both M01 and M11

    on a daily basis. Each pair of passes per orbit is

    separated by approximately 49 minutes.

    Figure 5: Typical daily access to Abuja groundstation for M01

    and M11

    CONSTELLATION DESIGN

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    The requirement for a low cost mission capable of

    providing all-weather imaging and high revisit time

    while exploring the possibility of collaboration

    with other developing nations prompted the choice

    of using a constellation of several small SAR

    satellites flying in close formation. The

    implementation of a semi-active SAR configuration

    provides an avenue to reduce launch cost, by using

    receiver-only platforms within the constellation. It

    is envisaged that the receiver-only (slave) platforms

    will invariably weight less in mass.

    Another benefit of proposing a constellation is the

    opportunity to promote cooperation between

    several nations within the ER. This could

    potentially involve pooling together various

    resources such as: personnel, ground segment

    location and equipment as well as space segment.

    The overall cost of mission is then shared with

    maximum benefit of various forms of data for

    several application areas leading to a Data-Full

    consortium.

    The constellation includes two groups of multi-

    static satellites in a pendulum configuration. The

    pendulum configuration has been reported to be

    well suited for providing multiple baselines at fixed

    baseline ratio along the whole orbit cycle [34, 35,

    36, 42]. The configuration allows the independent

    selection of along-track baselines and is well suited

    for velocity measurements. The pendulum

    configuration consists of three slave satellites with

    the same inclination but different values of right

    ascension of ascending nodes (RAAN). For

    operational safety, it is typical to apply slight

    offsets to the eccentricity vectors when flying near

    polar orbits, as this ensures vertical separation at

    the poles. For near equatorial region applications,

    this eccentricity difference may not be necessary,

    as the spacecraft maintain their relative distance

    and orientation through the orbit cycle when flying

    in close formation. Figure 6 highlights the

    pendulum configuration.

    Figure 6: Pendulum configuration showing Group 0 flying over

    the Equatorial region

    Each group consists of one Master satellite (Mnm)

    and three Slave satellites (Snm). Where n is the

    satellite number within a group and m is the

    group within the constellation. Table 5 summarizes

    the satellite constellation orbit parameters for group

    0. However, group 1will have the same parameters

    but with true anomaly offset by 180 deg.

    Orbit & System

    Parameters

    M01/11 S01/S11 S02/12 S03/12

    Altitude (km) 700 700 700 700

    Revs/day 14.5 14.5 14.5 14.5

    Inclination () 10 10 10 10

    Period (mins) 98.6 98.6 98.6 98.6

    RAAN () 0 0.00752 0.00182 0.00282

    Mean Anomaly () 0 5 5 5

    Table 5: Constellation orbit parameters

    The satellites in each group of the pendulum

    formation are evenly distributed along two 2 major

    orbits. One orbit consists of the master satellites

    M01 and M11 separated by 180 degrees mean

    anomaly. The second orbit contains six slave

    satellites, with S01, S02 and S03 separated from S11,

    S12 and S13 by 180 degrees mean anomaly

    respectively. Figure 6 shows a simulation of group

    0 satellites flying in pendulum configuration over

    the ER.

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    Figure 7: Simulation of in-orbit pendulum configuration of group 0, showing M01, S01, S02 and S03

    GROUND SEGMENT SITES

    As mentioned in section 1, there are over 45

    countries within the ER, with only 5 selected as

    possible locations for ground segment sites. These

    locations are subject to flexibility although certain

    criteria such as having existing space agency, and

    proximity to Equator were considered. Figure 8

    shows a Northerly oriented view of the locations of

    the selected groundstations.

    Figure 8: Selected locations for Ground Segment View from the North Pole

    The distance between subsequent locations varies;

    however, the maximum time between successive

    contacts with groundstation must be less than 10

    minutes. Table 6 details the location of the selected

    ground station sites. Sites can be flexibly selected

    provided the out of communication time with

    satellites is less than 10 minutes.

    Country Latitude Longitude

    Accra 5 30' N 0 10' W

    Cayenne 4 56' N 52 20'W

    Mogadishu 2 04' N 45 22'E

    Singapore 1 17' N 103 51'E

    Tarawa 1 19' N 172 58'E Table 6: Location of selected ground segment sites with ER

    Figure 9 shows a screen capture of the simulation

    conducted over groundstation locations.

    Figure 9: Ground segment location showing M01 making contact with groundstation in Accra

    Access to selected Ground Segment Sites

    The access to the selected ground segment location

    allows each group of the satellite constellation to

    always be in view of one ground station.

    Figure 10: Access report of M01 to selected ground sites within

    ER

    Figure 10 summarizes a daily access report for M10

    to each ground segment. A total of 70 accesses

    daily are available to download captured data, or

    upload telecommand to each spacecraft as required.

    This configuration serves to usher a new approach

    in data generation.

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    A line of sight constraint of a minimum of 6

    degrees elevation angle is applied to each

    groundstation.

    CONCLUSION

    The enormous benefits of oil to Nigeria were

    highlighted, and so were the potential hazards if not

    properly monitored. The current loses incurred due

    to inadequate surveillance of Nigerias oil resource

    were also mentioned. The approach adopted to

    meet a series of developed mission objectives, was

    the use of a SAR satellite for surveillance of illegal

    oil activities, and the detection of oil spills within

    the territorial waters.

    The benefits include over 20% increase access time

    to the existing ground station in Nigeria when

    compare to NigeriaSat-2 mission, as well as the

    possibility for 24 hours surveillance divulge of

    lighting or bad weather conditions. Furthermore,

    the potential to cover the territorial waters where

    oil resources are located in every pass exists.

    Other neighbouring countries in similar

    circumstances were identified using classification

    by latitude. An approach to solving Nigerias

    pending problem as well as meeting several other

    mission objectives was suggested. This is the use of

    a Multisatic SAR system dedicated to monitoring

    the equatorial region, which Nigeria lays herein.

    An approach suggesting the formation of a

    consortium of developing nations within the ER

    was also proposed. Advantages of the consortium

    include further reduction in cost of space mission,

    due to shared cost, availability of cheaper data,

    availability of a variety of data, and opportunity to

    apply the data for various form of development.

    Five sites were selected as locations for ground

    segments, which will facilitate a nearly 24 hours

    availability of data with a total of 70 access passes

    to the ground segments.

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