solar laser energy cycle - magnesium as energy 2012

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  • 8/13/2019 Solar Laser Energy Cycle - Magnesium as Energy 2012

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    3he University of okyo

    So l a r En e r g y C yc l e U s i n g M a g n e s i um

    a n d L a s e r T e c h n o l o g ie s

    2012.11.19 & 12.10

    Given by

    Shigeaki Uchida / Global Solar Initiative (GS+I), The University of Tokyo

    also at Pegasos Electra Co. Ltd.

    I n v i t e d L e c t u r e s o n

    M ag n e s i um e n e r g y c y c l e d r i v e n b y s o la r

    e n e r g y

    E l em e n t a l t e c h n o lo g i e s c o n s t i t u t i n g t h e

    c y c l e

    So l a r p um p e d l a s e r

    MgO r e d u c t i o n

    Mg c om b u s t i o n /b a t t e r y

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    4he University of okyo

    De f i n i t i o n o f t h e p r o b l em

    So la r p o w e r (r a d ia t i o n ) i s t h e u l t i m a t e

    r en e w a b le e n e r g y s o u rc e

    H ow e v e r

    Lo c a l ize d in t i m e a n d lo c a t i o n

    M i sm a t c h i n g b e t w e e n su p p l y a nd

    d em a n d N e e d m e a n s o f c o n v e n ie n t s t o r a g e

    Mg i s a p r om i s i n g c a n d id a t e f o r t h e s t o r i n g

    m a t e r i a l Mg

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    5he University of okyo

    World annual energy demand: 1.21014 kWh 2000s = 32,000 km2 of Solar energy200200 km desert equivalent

    Assume annual hours of sunshine3,000 hour/yearIssues to be Considered

    Typical sunshine hours in Japan: Four hours Need energy storing means for the rest of 20 hours Need transportation from the Sun Belt Region Construction cost & Energy Payback Time of those infrastructure

    A b u n d a n t s o la r po w e r o n t h e e a r t h

    Solar Radiation

    1kW m2 1 km2A thermal power stationSa h a r a d e s e r t 8 .61 06k m2Sa h a r a d e s e r t 8 .61 06k m2

    Gob i d e s e r t 1 .31 06k m2Gob i d e s e r t 1 .31 06k m2

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    6he University of okyo

    Mo r e t h a n 1 0 h o u r s o f s u n s h in e i s

    e x p e c t e d i n d e se r t a r ea

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    7he University of okyo

    En e rg y p r o d u c t i o n a n d p ow e r c o n t r o l

    f r o m M g c om b u s t i o n

    H2 combustion Power, Turbine

    MgOHOHMg 22 ++

    OHO

    2

    1H

    222 +

    +361 kJ/650+244 kJ/600

    Co n t r o l l i n g R e a c t i o n S p e e d a n d Pow e r Slow Reaction no H2 combustion) Rapid Reaction with H2 combustion)

    H2 (fuel cell) and reaction heat generation

    kJ/mol

    Easily generates steam at a few hundreds degree

    A s i m i la r e n e rg y o u t p u t i s e x p e c t e d f r om Mg -A i r b a t t e r y

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    8he University of okyo

    Ma g n e s i um a s e n e r g y s t o r a g e

    A bu nd an c e o f M a g n es iu m

    1 .2 x 10 1 5 t o n M g i n s e a w a t e r

    Fo s s i l f ue l c o n s u m p t i o n : 7 x 1 0 9 t o n /y e a r < = T h i s i s t h ea m o u n t w e n e ed f o r t h e c y c l e

    Sp e c i f ic e n e rg y (J /k g * ) c o m p a ra b le t o c o a l

    2 5 M J /k g (J e t f u e l : 4 3 M J /k g , C o a l: 3 0 M J /k g )

    En e r g y d en s i t y (c o m p a c t )

    4 3 GJ /m 3 4 .3 GJ /m3 (H2a t 7 00 a t m )

    H y d r og en s t o r ag e (e qu iv a l e n t )

    8 .3 w t % 5 -1 0 w t% (H 2

    t a n k f o r 35 0 a t m )

    V e rs a t i l i t y in p ow e r g en e r a t i on

    1 kW (2 .5 g /m i n , 2 0 X 4 0 X 0 .3m m ) ~ >MW /k g M g r a n g e (f l a k e d M g )

    Re t r ie v a l c o m b u s t i o n re s id u e , s o l i d M gO (c o m p a re d t o CO 2)

    Co n v e n i e n c e

    B u lk M g is n on f l a m m a b le (N e e d >6 5 0

    f o r i g n i t i o n ) Se l f ru n n in g re a c t i o n (Ex o t h e r m i c r e ac t i o n c o n t r o l l ed b yw a t e r f l o w )

    C an b e u s e d a s a ba t t e r y f u e l , M g -A i r b a t t e r y

    T ec h n o lo gy t o b e d ev e l o pe d

    En e rg y e f f ic i e n t r e d uc t i o n o f M gO

    So la r d r i v en l as e r t e c h n o lo g y fo r t h e re d u c t i o n

    * Oxidizer is not included

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    9he University of okyo

    Re n ew a b le En e rg y Cy c l e w i t h

    M g a n d So la r Pum p e d L a se r

    MgO

    Mg

    Retrieve

    Reuse

    Fresh Water

    Mg

    Desalination

    Plant

    Mg Reduction

    by Solar Laser

    Mg Reduction

    by Solar Laser

    Mg Engine

    H2 Fuel Cell

    Mg Fuel Cell

    Mg Engine

    H2 Fuel Cell

    Mg Fuel Cell

    Mg resource in ocean 1800 Tril lion-tons

    (=300,000 years of oil )

    Laser Cutting, WeldingRefinement

    (Fe, Al, Mg, Ti )

    Chemical Assistant

    Laser-related

    Manufacture

    Laser Cutting, WeldingRefinement

    (Fe, Al, Mg, Ti )

    Chemical Assistant

    Laser-related

    Manufacture

    Conversion efficiency

    30-40%

    Reduction efficiency

    40-50%

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    10he University of okyo

    -80

    -60

    -40-20

    0

    20

    40

    0 1000 2000 3000 4000 5000MgO Temperature [K]

    Mg, MgOMgOReductionAnalysis.xls

    2Mg O 2 2MgO

    2MgO 2Mg O 2

    Temperature for spontaneous MgO reduction

    Tokyo Inst. of Technology

    ChangeofGibbsFreeEnergy

    [kJ/mol]

    Change of Gibbs

    Free Energy of a

    Reaction

    G = H TSIf the change is

    negative, the

    reaction is

    spontaneous

    H: Enthalpy

    T: Temperature

    S: Entropy

    Gibbs Free Energy for MgO Formation

    Mg oxidizationtakes place

    MgO reduction

    takes place

    =RT

    GK exp

    Eq u i l i b r i um c o n s t a n t

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    11he University of okyo

    0

    Exothermic

    Endothermic

    273K1/2273K

    -601.8

    E [kJ/mol]

    MgO(s)

    Mg(g)(4000K)+O(g)(4000K)478

    152 Mg(g)(923K)

    Mg(g)(4000K)191

    1/2O2(g)(4000K)39

    602602 + 478

    Maximum Possible

    Energy Efficiency 56

    O(g)(4000K)288Dissociation

    Heating

    HeatingVaporization

    Heating

    MgO,Mg&H2O&H2.cvx

    Maximum Energy Storage Efficiency through MgO ReductionThermo Chemical Evaluation

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    12he University of okyo

    Pow e r B a l a n c e o f MgO V a p o r i za t i o n

    MgO Heated region

    Laser, Ilaser

    Ilaser(105W/cm2)Ivap(105W/cm2) + Irad (2103W/cm2) + Icond(103W/cm2)

    Ivap includes heat capacity 0.9 J/Kg, melting(1.9kJ/g), vaporization(8.2kJ.g), and dissociation9.2 kJ/g energies of MgO. Heat conduction measured. Vaporization rate0.05 g/sis measured Solar radiation concentration limit, 103 W/cm2

    Laser intensity wil l be required to maintain MgO reduction > 100Natural Sun Power Power Conversion rather than Beam Quality

    Heat Conduction, Icond

    Radiation Loss, Irad

    Vaporization, Ivap

    Laser Irradiation

    Power = 1 kW cw

    Spot = 1 mm = 10.6 m

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    13he University of okyo

    Why So l a r Pum p e d L a s e r ?

    L a se r t e c h n o lo g y g iv e s s o lu t i o n s t o o ve r c om e t w o m a jo r

    o b s t a c l e s i n u t i l i z i n g s o l a r l i g h t e n e r g y

    A u t o -r e du c t i o n o f M gO w i t h 4 0 0 0 -K h ig h t em p e ra t u r e

    Ad v a n t a g e o ve r c o n v e n t i on a l M g m e t a l lu r g y p ro c e s s e s

    Pow e r c o n c e n t r a t i o n is a s m a n y o rd e r s o f m a g n i t u d e

    l a r g e r t h a n t h e n a t u r a l s u n l ig h t

    Ad v a n t a g e o v e r a h u ge h e l io s t a t f a c i l i t y

    On l y la s e r c a n p r o v i d e t h e p ow e r d e n s i t y

    n e e d e d f o r t h e s p o n t a n e o u s MgO r ed u c t i o n

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    14he University of okyo

    A h u g e f a c i l i t y i s n e e d e d f o r d i r e c t s u n l ig h t

    a p p l ic a t i o n t o h ig h t em p e r a t u r e

    So la r p ow e r e ng in e i n Fo n t Rom e u Fr a nc e

    N a t i o n a l Re n ew a b le En e rg y La b o r a t o r y , U SA

    3 0 0 0 -K s o l a r f u r n ac e r eq u i r e s a 5 0 -m s o la r c o n c e n t r a t o r a r r a y

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    15he University of okyo

    L a s e r c a n be v e r y c om p a c t

    T he la se r a bo ve c a n he a t m a gn e s ia t o 40 00 K

    Ra d i a n c e o r B r i g h t n e s s c h a ra c t e r i ze s t h e p o w e r d en s i t y a n dc om p a c t n e s s o f a l ig h t s o u r c e i n W /c m 2s r

    L a se r v s . So la r = 1 0 1 4

    : 1 07

    , in W/m2

    s r

    4 kW o u t p u t p ow e rc a n b e d e l iv e r e df r om t h i s c om p a c tl a s e r h e a d

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    16he University of okyo

    L i g h t B e am Qu a l i t y

    ~Fo c u s a b l e Pow e r De n s i t y

    Co he re n t a nd I n c o h e r e n t L ig h t so u r c e

    >1 kW

    Beam divergence : 1 mraddiffraction limitted

    Coherent Light Source;Laser Mediumsuch as optical fiber laser Incoherent light sourceThe Sun

    1.4109 m

    3.81026 W

    ConcentratorVery tiny angle

    Etendue, an opt ical invariant: The smaller, the better

    (Light source size)(Solid angle of light flux)

    10

    -3

    m

    10

    -3

    rad = 10

    -6

    mrad 10

    -2

    m

    0.05 rad ~ 10

    -3

    mrad

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    17he University of okyo

    Sun

    6.96108m6.96108m

    L

    1.501011m

    AspotA

    lens

    Distance to the Sun (1.51011 m) Focal Length of the Sun Collector (L m)

    Sun Collector

    (Fresnel Lens)

    Why Laser? Why not Sun?Natural Limit of Sun Light Intensity

    I0Solar intensity on the ground0.1 [W/cm2] LnSun-earth distance normalized by sun diamer100

    number1Ispot 10,000I0 1000 W/cm2 Two orders of magnitude less thanrequired for MgO reduction

    Focused intensity, Ispot is determined by F numberalone

    02

    2

    02

    2

    02

    2

    0 I

    F

    LI

    DL

    DL

    I

    LLD

    D

    A

    IAI n

    lens

    sun

    sun

    sun

    sun

    lens

    spot

    lensspot

    =

    ==

    Laser Pumping Aperture

    ~Size of Laser Medium

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    18he University of okyo

    L a s e r i s a n e s s e n t i a l t o o l fo r t h e

    M g -S o l a r Ene r g y C y c l e S umm a r y

    Re n ew a b le e n e rg y c y c l e n e ed s a g oo d e ne rg y s t o r i n g

    m a t e r i a l

    M g is a p r o m i s i n g m a t e r i a l

    U se c h e m i c a l p o t e n t ia l c h a n ge b e t w e en M g an d M gO

    En e rg y c h a rg in g p r o c e s s , M gO r e du c t i o n n ee d s 4 0 0 0 K

    Di r e c t s o la r p o w e r c a n n o t su s t a in t h e t e m p e ra t u re

    L a se r t e c h n o l o g y p r ov id e s c om p a c t a n d e f f i c i e n t s o lu t i o n

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    3The Universit o Tok o

    So l a r En e r g y C yc l e U s i n g M a g n e s i um

    a n d L a s e r T e c h n o l o g ie s

    2012.11.19 & 12.10 at Tokyo University

    Given by

    Shigeaki Uchida / Global Solar Initiative (GS+I), The University of Tokyo

    also at Pegasos Electra Co. Ltd.

    T o p i c a l L ec t u r e s o n

    M ag n e s i um e n e r g y c y c l e d r i v e n b y s o la r

    e n e r g y

    E l em e n t a l t e c h n o lo g i e s c o n s t i t u t i n g t h e

    c y c l e

    So l a r p um p e d l a s e r

    Mg c om b u s t i o n

    MgO r e d u c t i o n

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    36The Universit o Tok o

    So l a r Pum p e d L a s e r

    Me c h a n i sm o f Co n v e r t i n g So l a r L i g h t t o

    L a s e r R a d i a t i o n =

    Fo u r L e v e l L a s e r M o d e l

    De s i g n Pr i n c i p l e o f So l i d St a t e L a s e r =T h e rm a l A n a l y s i s

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    38The Universit o Tok o

    a s i c Com p o n e n t s o fSo l a r Pum p e d L a s e r

    Solar pumped lasers use sun light to

    directly pump (activate or excite)

    laser media and convert it to

    coherent laser radiationun

    Sun lightLightcollector

    Laser mediumLaser

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    37The Universit o Tok o

    Sun

    6.96108 m6.96108 m

    L

    1.501011m

    AspotA

    lens

    Distance to the Sun (1.51011 m) Focal Length of the Sun Collector (L m)

    Sun Collector(Fresnel Lens)

    Why Laser? Why not Sun?Natural Limit of Sun Light Intensity

    I0Solar intensity on the ground0.1 [W/cm2] LnSun-earth distance normalized by sun diameter100

    number1Ispot 10,000I0 1000 W/cm2 Two orders of magnitude less thanrequired for MgO reduction

    Focused intensity, Ispot is determined by F numberalone

    02

    2

    02

    2

    02

    2

    0 IF

    LI

    DL

    DL

    I

    LLD

    D

    A

    IAI n

    lens

    sun

    sun

    sun

    sun

    lens

    spot

    lensspot

    =

    ==

    Laser Pumping Aperture

    ~Size of Laser Medium

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    39The Universit o Tok o

    Ba s i c E l em e n t s o f So l a r L a se r

    L a s e r Os c i l la t o r

    Fr e s n e l l e n s

    So l a r r a d i a t i o n

    Laser

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    40The Universit o Tok o

    Laser Devise :Laser Devise : solar pumped lasersolar pumped laser

    Cr:Cr:NdNd:YAG:YAG ~Economical and efficient~Economical and efficient

    Negligible amount ofresource for lasermaterial

    Water for powerconcentration andcooling

    low manufacturingcost 0

    0.5

    1

    1.5

    2

    400 500 600 700 800(nm)

    (/cm)

    Nd absorption

    Cr + Nd absorption

    Wave length (nm)

    Absorptio

    n

    coefficien

    t(cm-1)

    Concept

    Solar spectrum

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    41The Universit o Tok o

    Qua l i t a t i v e d e s c r i p t i o n o f l a s e r

    O s c i l l a t i o n ~ Sp o n t a n e o u s & S t i m u l a t e d

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    42The Universit o Tok o

    Four-Energy-Level Model of Nd Ion

    Most important: To form a population inversion between the upper and

    lower laser level

    Population inversion: status that upper level has more ions than the

    lower level against the thermal equil ibrium condit ion

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    43The Universit o Tok o

    Upper level

    Lower level

    Pumping

    Stimulated EmissionLaser Photon) Spontaneous EmissionPower Loss)

    Nd:YAG

    Fo u r L e v e l L a s e r Eq u a t i o n s

    The equations deal with the number densities of

    population inversion, N2 and laser photon,

    2

    2

    2 N

    NBRdt

    dN

    p =

    =

    caNBVdt

    d 1

    2

    HR mirror Output mirror

    Laser photons are generated from

    stimulated emission and lost through the

    output mirror

    Population inversion, N2 is added the

    pumping and reduced by both stimulated

    and spontaneous emission

    At oscillation condition, steady state is realized, i.e. d/dt = 0

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    44The Universit o Tok o

    Laser Power as a Function of Pumping

    Power in Oscillation Condition

    ( )

    ( )

    +

    +

    =

    +

    +

    =

    =

    a

    sT

    photon

    T

    med

    aT

    pa

    T

    T

    med

    pca

    e

    out

    Vf

    P

    f

    A

    chl

    fRV

    f

    f

    lRVh

    L

    cP

    1

    11

    1

    1

    2

    2

    Expression for Laser Power

    Solar Power(Input)

    Slope

    Efficiency

    Threshold Photon Lifetime in Cavityc

    Lec

    ( ) aTa f

    122

    ++ Cavity Loss

    a

    Tf

    2

    2 Ratio of Output Coupling toMedium Loss

    medefcta AlV Mode Volume=Gain lengthGain cross section

    T he Ex p r es s i o n In c l u d e s

    Tw o L a s e r Os c i l l a t i o n

    C h a r a c t e r i s t i c s ;

    S lo p e Ef f i c i e n c y

    T h r e sh o l d

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    45The Universit o Tok o

    Axial PumpingAxial Pumping ConfigurationConfiguration

    A x i a l p um p i n g c o n f i g u r a t i o n w i t h t a p e r e d l i g h t c a v i t y h a s

    b e e n d e s i g n e d fo r e f f i c i e n t s o l a r p ow e r c o n c e n t r a t i o n

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    46The Universit o Tok o

    01020304050607080

    800 1000 1200 1400 1600 1800 2000 [W]

    Calculation

    Experiments

    Model Calculation Well ReproducesModel Calculation Well Reproduces

    Experimental ResultsExperimental Results

    Both Slope

    Efficiency and

    Threshold are wellreproduced by

    theoretical model

    LaserOutput[W]

    Solar Input [W]

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    47The Universit o Tok o

    L im i t o n L a s e r M e d i a T h i c k n e s s T h e rm a l s h o c k l i m i t

    Qt h[W/m3]Wa s t e h e a t

    Fs h a p e Sh a p e f a c t o r 1 28 / s l abr o d

    RT[W /m ] T h e rm a l sh o c k p a ra m e t e r 700 / YAG

    t [m ] Me d i um d i m e n s i o n a lo n g t em p e r a t u r e g r a d ie n t

    SSa f e fa c t o r 0 .10 .3

    PumpPpumpWaste heatQthV

    Laser radiationPlaser

    Laser medium (volume V)

    t

    SQ

    RF

    tth

    Tshape

    M d i t h i k d d

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    48The Universit o Tok o

    Me d i um t h i c k n e s s de p e nd e n c e

    o f L a s e r Pow e r

    0

    10

    20

    30

    40

    50

    60

    70

    80

    600 800 1000 1200 1400 1600 1800

    Input Solar Power [W]

    3 53 9

    9

    100

    World Record of Solar Pumped Laser

    Thicker media are preferable but

    Also medium broke

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    49The Universit o Tok o

    T h e h i gh e s t p o w e r r e c o r d e d c o r r e sp o n d s t o

    t h e t h e r m a l l i m i t o f t h e r o d m e d i um

    80 W is close to the highest power that the 9 medium canaccommodate

    St

    RFQ

    Tshape

    th 2=

    Measured medium effective (activated) volume, V

    Extraction efficiency, (Model Calculation)Maximum output power would be

    WVQ

    I th 90

    11max =

    =

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    51The Universit o Tok o

    A n o t h e r h ig h e s t T A P h a s b e e n a c h i e ve d

    3. M.Landoat alOptics Communication 2003

    1.M.Weksler,at alIEEE J QE 1988

    2. V.Krupkin,.at alProc.SPIE 1993

    4. Our Study, Yabe LabTokyo Inst of Tech,Okamoto Opt

    Laser Output[W]Collector Size[m2] TAP [W/m2]

    24.4 16.66.6

    60500

    46

    38.56606.851.47

    1.550.76

    6.7

    Totaltal Areaea Performancerformance Laser outputaser output [W]W]Collector area [mollector area [m2]Reflects the future plant cost effectiveness

    80 20.00.0.0. Our Study, Yabe LabTokyo Inst of Tech,Okamoto Opt

    Set in March 07

    New!

    Currentperformance:

    30%

    absorption

    Limited by

    thermal load

    =>More and

    distributed

    absorption

    A t h ib i l i t

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    52The Universit o Tok o

    An o t h e r p o s s ib i l i t y Sl a b t y p e l a s e r m e d i a

    Design laser media that absorbs pumping power

    through its wide area

    Principle of design

    Achieve high absorption while avoiding

    thermal fracture

    Laser oscillation

    Solar power

    T h i c k n e s s a n d n um b e r o f m e d ia d e p e n d o n

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    53The Universit o Tok o

    T h i c k n e s s a n d n um b e r o f m e d ia d e p e n d o n

    p um p in g p o w e r

    Thick

    Small pump power

    Less media Thin

    Large pump power

    More media

    Stacked laser media for the areal pump power absorption scheme

    Thin

    With reflection

    More media

    % f

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    54The Universit o Tok o

    9 0% a b s o r p t i o n f o r w h o l e la s e r m e d i a sy s t em

    0.00.20.40.60.81.01.2

    1.41.6

    2

    4

    6

    8

    10

    0.5 0.6 0.7 0.8 0.9 1Absorption

    Blue: 200 W/cm 2Red : 400 W/cm 2

    Thickness

    Number of Media

    No reflection

    Thickness&Number.qpc

    S i d i t h i t h 1

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    55The Universit o Tok o

    S i x m e d ia t h i n n e r t h a n 1 c m

    0.5

    1.0

    1.5

    2.0

    2.5

    2

    345678910

    50 100 150 200 250 300 350 400Pumping power [W]

    Number

    Thickness

    Thickness&Numbre-Pump

    Blue: without reflectionRed : with reflection

    Current performance

    More than 1500 Wis absorbed in thestacked media1 kW laser outputcan be expected

    [W/cm2]

    P t t f h l f i l t k i t

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    Pr o t o t y p e o f h a l f -p i p e s o l a r t r a c k i n g s y s t em

    Master-Slave Sun Tracking System has been tested

    Driving power 30W (to be 1% of laser output)

    Master

    (active tracker)Slave

    Lens1Lens2

    Laser1Laser2

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    57The Universit o Tok o

    Pr e l im i n a ry d e v i c e f o r s l a b m e d i um

    Radiator

    Laser medium

    Window

    Solarlight

    Cu holder

    G l f t h R& D

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    58The Universit o Tok o

    Go a l o f t h e R& D

    Conversion efficiency

    30-40%

    To MgO reduction plant

    Solar Laser Array

    680 t M d ti /d / 2 5k 2

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    59The Universit o Tok o

    680-ton Mg production /day /2.5km2