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    s

    October 2011 For the Engineer, by the EngineerSatcomT E C H N O L O G Y

    www.viasatellite.com

    Accessing

    Content OntheMove

    Presents New Opportunities

    for Satellite

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    2 Satcom Technology October 2011

    Vice President and Group Publisher Via Satellite

    Joe Rosone

    Divisional President, Business Information Group

    Heather Farley

    Associate Editor Via Satellite

    Mark Holmes

    Director, Satellite Online

    Julie Blondeau Samuel

    Managing Editor Via Satellite

    Debra Richards

    News Editor Satellite Today

    Jeff Hill

    Senior Graphic Designer Via Satellite

    Vince Lim

    Production Manager Via Satellite

    Sophie ChanWood

    Chief Executive Officer Access Intelligence, LLC.

    Don Pazour

    Accessing Content

    on-the-Move Presents New

    Opportunities for Satellite

    W

    hether users are on arplanes, cruse shps or trans,

    one thng s untng them the demand for data com-

    muncaton and vdeo servces on ther moble or tabletdevces. Wth most users utlzng data and vdeo servces as

    much as voce servces on ther moble devces, ths s presentng a new range of opportun-

    tes for satellte technology vendors as they look to supply the technology that wll enable

    users to have connectvty pretty much wherever they are.

    Amplier technology companes must rase ther game to meet the next set of demands, as

    users are expectng qualty connectvty servces on-the-move. It s a challenge they are enthusas-

    tcally embracng, as many see ths as a potentally lucratve opportunty for satellte companes,

    both on the operator sde and the technology sde.

    Certanly, Ka-band satelltes wll have a huge mpact on enablng the next generaton of commu-

    ncatons on-the-move servces. One company that ams to be at the forefront of provdng the nec-

    essary technology to power these servces s Wavestream. The company has hgh hopes for ts

    Grd Amplier, whch t sees as becomng an ntegral pece of the equaton for satellte operators

    nvestng aggressvely nto Ka-band satelltes. Wth a number of Ka-band satelltes gettng ready to

    launch, Wavestream s conident that ts amplier technology wll play a key role.

    However, state-of-the-art connectvty s about more than just Ka-band, although t s a key part

    of the debate. ITS Electroncs, a company based n Greater Toronto, Canada, whch also plays

    n the Ka-band space, s also lookng to offer a wder range of solutons. Its range of Sold State

    Power Ampliers (SSPAs) am to provde compellng and eficent solutons to satellte operators

    delverng on-the-move servces.

    The latest edton of Satcom Technology contnues our pledge to brng you nformaton for the

    engneer, by the engneer, and we are sure you wll ind t

    nformatve and a great resource when consderng your next

    moves n mprovng your communcatons nfrastructure.

    M E S S A G E F R O M T H E E D I T O R

    4 Choke Cherry Road, 2nd FloorRockville, MD 20850Phone: 301/354-2000, Fax: 301/340-3169Email: [email protected]: www.viasatellite.com

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    October 2011 Satcom Technoogy 3

    Demand for high-speed, reliable connectivity to the Internet is being driven by a worldwide expectation that plat-

    forms and applications will provide that access anytime, anywhere. Ka-band satellite services are coming online at

    just the right time to address this exponential growth.

    The Ka-band Revolution

    Gary Echo, VP Busness Deveopment at Wavestream, [email protected]

    B

    ack n 1968, the Beates

    asked us f we wanted a

    Revouton. Ive spent neary30 years n satcom and have wt-

    nessed many technoogca chang-

    es n that tme. Some of these

    changes have arguaby been revo-

    utonary, but most of these have

    been transparent to peope outsde

    our ndustry. I beeve that s about

    to change n a dramatc, revouton-

    ary way. The advent of hgh-band-

    wdth, Ka-band satete servces s

    gong to brng satcom drecty nto

    the hands of a arge percentage of

    the word popuaton.

    Why now? you mght ask. Ka-

    band has been around for more

    than a decade. What about the

    attempts by Teedesc, Astronk,

    Ceestr, Skybrdge and others?

    What s so dfferent now?

    What s dfferent now s that

    we are at a convergence of

    technooges both from the

    demand sde and from the

    suppy sde. Demand for bts

    s ncreasng exponentay, not

    ony n the amount of bts beng

    consumed, but aso n the number

    of ndvduas consumng them

    and reachng nto ther waets

    to pay for them. Meanwhe,

    satcom technoogsts from many

    satcom ieds (modem, encoder,

    antenna, satete) have mproved

    ther wdgets to the pont where

    deverng bts can be done at aprce that both the user s wng

    to pay and at a prce a servce

    provder s wng to dever or,

    n an subsdzed stuaton, togenerate ncrementa revenue.

    Indeed, smartphones, Pads and

    other Internet-enabed devces are

    becomng ubqutous. Consumers

    are demandng contnua access

    to the Internet and streamng

    servces, and are wng to

    pay a szeabe porton of ther

    dscretonary ncome to secure that

    access. The average ce phone b

    has been rsng steady and today,

    many spend more on ther data

    pan than they do on voce. The ce

    phone s now more about stayng

    connected va ema, Facebook

    and Twtter, and much ess about

    makng phone cas. Ths s very

    true for busness users. It s hard

    to ind, even n the nerd herd,

    someone wth an antquated ce

    phone wth no keyboard. I take

    notce of these thngs. There are

    st some hodouts (weve had

    them at Wavestream) but some

    of these foks secrety keep a

    Backberry n ther brefcase, I just

    know t. A these users want to

    reman connected wth hgh-speed,

    reabe servce whether they are

    n ther homes, cars, on a tran, on

    a cruse or on a pane. Asde from

    the fact there s a stranger sttng

    next to us n 23E, on the arpane

    we want the same streamng

    Netlx experence to our Pad aswe have whe sttng n our vng

    room. Arnes are gearng up to

    dever that experence and more.

    The demand for bts snt justcomng from consumers and bus-

    ness peope. The mtary, home-

    and securty, NGOs (FEMA, Red

    Cross) are a adoptng technoogy

    to better perform ther dutes and

    keep us safe. These technooges

    requre ever ncreasng bandwdth

    and tmey devery. Specicay,

    magery s a sgnicant bandwdth

    hog. Around the word, demand for

    connectvty s ceary vsbe n the

    vast use of soca meda to com-

    muncate. Aggregated, thousands

    of users dong text, ema and

    soca networkng, s a ot of bts

    to get to/from the Internet from a

    manner of ocaes.

    Ka-band

    Ready for Prime Time

    The chaenge to the satcom ndus-

    try s how to dever hgh-bandwdth

    to users wherever they may be. For

    many patforms, the satcom ndustry

    aone owns ths chaenge. We are

    not gong to see fber to Fght 99.

    Terrestra can provde some servce

    to arcraft over and, but speeds are

    mted. Recenty, a terrestra-based

    servce to arcraft had to bock a

    users from upoadng mages to

    ther Facebook pages. That s not

    gong to fy, teray. If you just fn-

    shed your vacaton and rushed to

    the pane, you are gong to want toupoad those mages. Users w

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    4 Satcom Technology October 2011

    demand, and wll get, full connectv-ty by talkng wth ther wallets ether

    by payng for hgh-speed access

    drectly or by payng extra to fly on

    arlnes that support ther lfestyles.

    Ku-band can delver mproved ser-

    vce to n-moton platforms and n

    fact s dong so today to a lmted,

    but growng extent. Bandwdth,

    however, has become the lmtng

    factor. Ku-band satellte slots are

    practcally fully populated and the

    satelltes n these slots are hghlyutlzed today. 750 MHz of capacty

    n each polarzaton wth regonal or

    hem beams s not a lot of capacty

    when you consder the aggregated

    demand from moble users.

    Ka-band s the key to delverng

    to ths consumer mandate. Frst,

    Ka-band has 3.5 GHz of avalable

    bandwdth per polarzaton vce

    0.75 GHz for Ku. Ka-band further

    augments ts basc bandwdth ad-

    vantage wth the use of spot beams

    and frequency re-use (colors as they

    are called). Ka-Sat s advertsed

    at 70 Gbps throughput; VaSat-1,

    at 130 Gbps. That s almost 100

    tmes the capacty of a Ku-band

    brd. The space sde of the ndustry

    s posed to delver a vast amount

    of Ka-band bandwdth. One satellte

    s around 100 Gbps.

    Now multply ths per-

    satellte throughput by

    the number of roughly

    150 open orbtal slots

    (and that just counts

    the GEOs), and you see

    a true revoluton n the

    access to bts and the

    cost per bt.

    Revolutionary

    Technology

    Wavestream is Born

    Rewnd to the 1990sand the efforts of Teledesc and

    other large constellaton Ka-bandefforts. That s the geness of

    Wavestream. A couple of PhDs from

    Caltech set out to commercalze a

    technology they had been workng

    on n the Caltech labs called quas-

    optcal combnng. They took some

    angel nvestment and boldly set

    out to go where no one had gone

    before: take a free-space

    confguraton and condense t

    nto WR-28 wavegude. Some

    mght call ths effort noble.Fgure 1 shows an early test

    setup usng a one-foot lens to

    llumnate one of ther devces

    n the Caltech lab.

    The resultng technology s

    called the Grd amplier. The

    name comes from the struc-

    ture of the amplier tself: a

    grd of unt cells. Each unt cell

    has a par of antennas wth a

    par of transstors between.

    One set of antennas grabs ts

    pece of the ncomng sgnal,

    and the amplied sgnal s

    put out nto the wavegude by

    the output antennas. A grd

    of unt cells s mounted co-planar

    on a ceramc carrer, whch s then

    mounted to a heat spreader. The unt

    cells are spaced closely together

    such that they effectvely operaten concert on an entre wave. The

    result s an amplicaton devce that

    takes a plane wave mpngng on

    ts backsde and puts an amplied

    verson out ts front. Ths devce s

    placed nsde a WR-28 wavegude as

    shown n Fgure 2. The igure actually

    shows a two-stage amplier module.

    The Grd amp rotates the sgnal 90

    degrees due to the orthogonal rela-

    tonshp between nput and output

    antennas. By usng two stages, the

    wavegude stays n the module n

    the same orentaton as the output.

    Havng two stages allows for basng

    the irst stage for gan and second

    for output power. The Grd amplier

    s a unque, and obvously patented,

    archtecture that provdes hgh-power

    at hgh frequences. Whle ths artcle

    s focused manly on Ka-band, the

    Grd amplier s also well suted to

    frequences up to 100 GHz.

    Fgure 3 compares the Grd to

    10 ndvdual devces currentlyon the market. The red dot sFigure1: Illuminating Early Grid Amps

    Figure2: Illuminating Early Grid Amps

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    October 2011 Satcom Technoogy 5

    Wavestreams devce at 22W outputpower wth 17 percent Power Added

    Eficency (PAE).

    A Grd modue wth WR-28 output

    provdes 15W saturated power wth

    8W of near power n a 4-ounce

    package. When addressng cha-

    engng mobe coniguratons, t s

    crtca to mount the ampier as

    cose to the antenna as possbe.

    Ths mnmzes osses, whch, at

    Ka-band, are sgnicant even over

    wavegude (0.75 dB per meter). Theghter the ampier, the easer fe s

    for the antenna postonng system.

    As the market moves to lat pane

    arrays, the sze of the ampier starts

    to become more mportant, and the

    Grd ampiers compact power has

    added beneits.

    An advantage of the Grd archtec-

    ture s the devce mountng to the

    heat spreader wth rada transfer of

    heat to a surfaces. Ths mountng

    coniguraton provdes fary eficent

    therma transfer, whch mantans

    ower juncton temperatures and

    yeds hgher Mean Tme Between

    Faures (MTBF). Comparatvey,

    wth tradtona MMIC devces the

    majorty of the heat s n the astbnary stage as depcted n Fgure 5

    (eft). The ampier desgners usng

    these devces are forced to get heat

    out of that tny strp. In these MMIC

    devces, gettng that heat out can

    be a rea chaenge partcuary for

    GaN devces that have hgher power

    denstes as compared to GaAs.

    Another advantage of the Grd s

    that the sgna never transts a bond

    wre. The ony bond wres on a Grd

    amp are used for DC, and there are

    redundant bond wres

    from each edge. For

    the ampier to ose

    any power t woud

    take two bond wres

    to fa and they woud

    have to be both on the

    same coumn. Even n

    ths unkey scenaro,

    the ampier woud

    ose ony 1/11th of ts

    power. I know, remarkabe.

    Demand to In-Hand

    Up to now we have taked about

    the scence of the ampfer, but

    t s mportant to understand the

    appcaton of the scence. Scence

    by nature s hard and not every

    good dea yeds usabe resuts.

    For the nventor/desgner (and

    obvousy to the nvestor) t s aways

    rewardng when a good dea and

    a the effort pays off. In the caseof the Grd amp, we beeve we

    have succeeded. Snce the frstdevery n 2008, Wavestream has

    shpped more than 4,000 Ka-band

    ampfers. If we excude ampfers

    for consumer broadband (

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    8 Satcom Technology October 2011

    power supply wth, other nstruments

    on one platform. As a result, the HPAs requred to have low conducted

    and radated

    emssons for

    electromagnetc

    compatblty

    (EMC) wth other

    equpment. The

    demand on

    system EMC af-

    fects the choce

    of TWTA or SSPA. A TWTA requres very

    hgh voltage DC sources, rangng from10 kV to 18 kV, to bas the cathode

    and the helx col. It requres a power

    converter that steps up the AC lne

    voltage to the klovolt range, and rect-

    ies t wth hgh breakdown swtchng

    crcuts. In contrast, SSPAs utlze GaAs

    or GaN transstor technologes that op-

    erate at low voltages, e.g. 6 V for Ka-

    band 0.15 m pHEMT transstors, 10

    V for X-band GaAs FETs and up to 50

    V DC for GaN. It s a challenge to sup-

    press the hgh voltage rpples present

    n the TWTA power converters. Further-

    more, the choce of large capactors

    and ilters that can wthstand tens of

    klovolts breakdown s lmted. On the

    other hand, EMI ilters n SSPAs can be

    desgned usng a wde varety of com-

    ponents, such as electrolytc, tantalum

    and ceramc capactors, together wth

    common-mode chokes to suppress

    the rpples. As a result, the TWTAs

    generally have nferor EMC compared

    to SSPAs. Fnally, the hgh voltages n

    TWTAs cause more stresses to the cr-

    cut components. Therefore, the power

    supples used n SSPAs generally enjoy

    hgher MTBFs than those n TWTAs.

    Many ITSs SSPAs are desgned to

    comply wth EMC standards such as

    EN55022 and MIL-STD-461E for ml-

    tary applcatons. These SSPAs utlzes

    EMC certied AC-to-DC step-down

    converters or DC-to-DC step-down con-

    verters to provde the bas voltages tothe transstors. Lnear regulators are

    utlzed to enhance the lne regulaton

    (mmunty to the power supply rpple)and the load regulaton of crtcal bas

    crcuts for the power transstors.

    To acheve hgh avalablty for a

    satellte communcaton lnk, SSPAs,

    whch have graceful degradaton

    characterstcs, are the preferred

    choce over TWTAs. When a TWTA fals,

    the tube s usually damaged beyond

    meanngful usage. Buldng a 2-to-1

    redundant HPA wth TWTA also doubles

    the cost and sze because two TWTAs

    are requred nstead of one. Therefore,redundancy may not be feasble n

    hghly moble (.e. portable) SATCOM

    termnals. The redundancy mplemen-

    taton also mposes addtonal loss

    to the output power of the TWTA. The

    repar s also costly, because the entre

    travellng wave tube must be replaced.

    The above problems can be mtgated

    by usng SSPAs nstead of TWTAs.

    Although the output power of a tran-

    sstor s clearly nferor to one mghty

    TWTA, numerous sold-state amplier

    modules can be combned together

    to acheve graceful degradaton. For a

    SSPA comprsng N amplier modules,

    the power drop due to one faled mod-

    ule s 20*log10((N-1)/N). For example,

    f a hgh-power SSPA comprses eght

    amplier modules and one module

    fals, the output power wll only drop

    by 1.2 dB. The falure of the SSPA s

    graceful not only n the mnor output

    power degradaton, but the reman-

    ng seven modules contnuously and

    fathfully transmt every sngle RF cycle

    of the symbols before, durng and after

    the module falure. Snce no IF symbol

    are mssed durng symbol recovery

    by the recever, the satellte lnk s

    not dsrupted by the mssng data. As

    mentoned prevously, the mnor power

    drop does not readly degrade the BER

    of QPSK or 8PSK demodulaton. ITS

    Electroncs SSPAs have the beneit

    of graceful degradaton because theyutlze multple transstors for power

    amplicaton. The companys patented

    nnovatve solutons n hgh-frequencyhgh-power combnng technques

    make ts products attractvely scalable,

    thanks to hgh-eficency, and small

    sze and weght.

    ITS hgh-power SSPA technology ut-

    lzes amplier modules that are com-

    pact and often hot-swappable. A power

    module, whch s attractvely prced at

    a fracton of the overall SSPA, provdes

    an economc opton for n-stu repar.

    For example, a warshp patrollng on

    open sea can be equpped wth extralow-cost amplier modules. In the un-

    lkely event of a SSPA module falure,

    t s unacceptable that the satellte

    lnk s down untl

    the shp must be re-

    turned to port for the

    repar. Instead, the

    repar can be per-

    formed rght on the

    sea. The on-shp

    crews can replace

    the SSPA module

    wthn 15 mnutes,

    whle the satellte lnk s unnterrupted

    durng the entre msson. The redun-

    dancy advantages can be extended

    by usng hot-swappable power supply

    modules and fan modules for cost-

    effectve mantenance.

    ITS Electroncs products serve the

    government, defense and commer-

    cal communcaton markets n the

    L, X, Ku/K/Ka and Q/V frequency

    bands. ITS equpment has been

    desgned and certied complant to

    MIL-STD-188-164A

    to operate wth the

    Wdeband Global

    SATCOM (WGS)

    satelltes. The

    companys equp-

    ment powers gate-

    ways for Ka-Sat,

    Spaceway, IPSTAR,

    WINDS, Vasat-1among others.

    Figure 2: ITS 90W 29.1-29.3GHz SSPA replacement ofTWTA in IRIDIUM Gateways,year 1999

    Figure 3: ITS 40- to60-Watt Ka-bandSatcom Block UpConverter

    Figure 4: ITS airborneKu-band 20-Watt HPA,

    High IP3 LNA and LowLoss Diplexer