presentation technion 2009

Upload: hphmhphm

Post on 04-Apr-2018

225 views

Category:

Documents


0 download

TRANSCRIPT

  • 7/30/2019 Presentation Technion 2009

    1/29

    1

    A NON-POLLUTING SOLAR CHEMICAL

    PROCESS FOR PRODUCTION OFHYDROGEN AND CARBON BLACK BY

    SOLAR THERMAL METHANE

    SPLITTINGA. Kogana , M. Koganb, S. Barak, M. Epstein, A. Segal, R. Rubin,

    Y. Yeheskel, D. Lieberman, R. Arielic, Y. Hlopovitzd

    a. Department of Aerospace Engineering, Technion IIT, Israel

    Visiting Scientist at Solar Research Facilities Unit, Weizmann Institute of Science.b. Solar Research Facilities Unit, Weizmann Institute of Science, Rehovot, Israel

    c. Department of Aerospace Engineering, Technion IIT, Israel

    d. Department of Computer Science, Technion IIT, Israel

    49th Israel Annual Conference on Aerospace Sciences

    Tel Aviv - March 4, 2009

  • 7/30/2019 Presentation Technion 2009

    2/29

    2

    HYDROGEN IS THE CHOICEFUEL OF THE 21ST CENTURY

    ITS COMBUSTION IN AIR RELEASESGREAT QUANTITIES OF ENERGY PER

    UNIT MASS.

    ITS COMBUSTION PRODUCT IS ONLYWATER.

    IT IS A NON-POLLUTING FUEL ANDTHEREFORE ITS USE ISENVIRONMENTALLY ACCEPTABLE.

  • 7/30/2019 Presentation Technion 2009

    3/29

    3

    HYDROGEN PRODUCTION BYMETHANE-STEAM REFORMING

    CH4+H2O CO+3H2

    PRODUCTION OF 1 TON H2 IS ASSOCIATED WITHCONSUMPTION OF 2.6 TON CH4 AND DUMPING OF 7.15 TON

    CO2 TO THE ENVIRONMENT.

    THE PRESENT GLOBAL H2 DEMAND IS ABOUT 50106 TON.

    THE CONCOMITANT CO2 PRODUCTION AMOUNTS TO MORETHAN 350106 TON.

    800C

    30 atm

    CO+H2O CO2+H2400C

  • 7/30/2019 Presentation Technion 2009

    4/29

    4

    2gr42HCCH C1500

    HYDROGEN PRODUCTION

    BY METHANE SPLITTING

  • 7/30/2019 Presentation Technion 2009

    5/29

    5

    Three problems must be solved during thedevelopment of a Solar Thermal Methane

    Splitting reactor based on direct heating of CH4

    1. PROTECTION OF THE REACTOR WINDOWFROM CONTACT WITH SOLID CARBONPARTICLES GENERATED BY THE STMSREACTION.

    2. PREVENTION OF PYROCARBON DEPOSITIONON THE REACTOR WALLS.

    3. DEVELOPMENT OF ADEQUATE MEANS TOENABLE EFFICIENT ABSORPTION OFCONCENTRATED RADIATION BY METHANE,WHICH IS A TRANSPARENT GAS.

  • 7/30/2019 Presentation Technion 2009

    6/29

    6

    Fig. 1. REACTOR MODEL M2B-CPC ASSEMBLY

    Impeller-like disc

    Insulation

    Auxiliary stream inMain stream in

    First annularpassage

    Second annularpassage

    Window

    Exit port

  • 7/30/2019 Presentation Technion 2009

    7/29

    7Fig. 2. IMPELLER RING INSTALLED IN FLANGE GROOVE

  • 7/30/2019 Presentation Technion 2009

    8/29

    8

    Smoke charged radial auxiliary flow 2 L/M

    Fig. 3. CONSECUTIVE STAGES IN THE EVOLUTION OF ATORNADO FLOW PATTERN IN A REACTION CHAMBER

  • 7/30/2019 Presentation Technion 2009

    9/29

    9

    Fig. 5. FLOW OF A REAL LOW-VISCOSITY FLUID PAST

    A CIRCULAR CYLINDER

  • 7/30/2019 Presentation Technion 2009

    10/29

  • 7/30/2019 Presentation Technion 2009

    11/29

    11

    Fig 6. SMOKE FLOW VISUALIZATIONOF AN UNSTABLE TORNADO

    FLOW CONFIGURATION

    Fig. 7. SMOKE FLOW VISUALIZATION

    OF A DEGENERATED TORNADO

    FLOW CONFIGURATION

  • 7/30/2019 Presentation Technion 2009

    12/29

    12

    It has been shown by a room temperature experiment that this

    flow configuration remains stable in our laboratory-scale

    reactor model when operated at a gas flow rate of up to 20 L/Mcorresponding to a minimum Ekman number

    5

    max

    min104.3

    swirlVD

    E

    Under actual conditions of operation of a STMS plant, say at

    T=2000 K, the kinematic viscosity of Methane goes up by a

    factor of 25, as compared to its value at room temperature. This

    indicates the potential for upscaling the reactor for industrial use.

    The small laboratory reactor mentioned above could be operated

    at 2000 K with a maximum gas flowrate close to 500 L/M, with the

    quartz window protected by the confined tornado flow effect

  • 7/30/2019 Presentation Technion 2009

    13/29

    13

    Fig. 9. THE QUARTZ INSERT TUBEBECAME CLOGGED WITH CARBON

    Fig. 8. CROSS SECTION OFREACTOR M4-3, USED DURINGTEST CH4-9

  • 7/30/2019 Presentation Technion 2009

    14/29

    14

    A sequence of such tests was performed

    with the same reactor at similar insulation,

    but with the quartz insert tube replaced by a

    zirconia tube and then by a copper tube of a

    similar geometry.In all these cases the testsended due to heavy clogging of the inserts

    with carbon, while the rest of the reactor

    walls were free of Pyrocarbon deposition.

    Fig. 10 CROSS SECTIONOF REACTOR M4-5, USEDDURING TEST CH4-11

    The insert tube was then replaced by a longcopper tube that reached down to the bottom

    of the quenching chamber. The tube was

    cooled strongly by water sprays. In this case

    there was no carbon deposition inside the

    reactor.The test lasted for half an hour and was

    terminated because of a cloud in the sky.

  • 7/30/2019 Presentation Technion 2009

    15/29

    15

    Next we studied some gas dynamics methods to facilitate evacuation of

    particles from the reaction chamber [5].

    By rebuilding of the Fig. 8 reactor by assembling the three components (a),

    (b) and (c) shown in Fig. 11 and by installing an additional annular plenum

    chamber (Fig. 12), it became possible to apply radial blowing along thebase of the reaction chamber.

    Fig. 11. COMPONENTS OF

    REACTOR D2

    Fig. 12. AXIAL CROSS SECTIONOF REACTOR D2

  • 7/30/2019 Presentation Technion 2009

    16/29

    16

    The exit port section from the chamber was rounded by insertion of

    flared metal inserts (Fig. 13).

    Fig. 14 illustrates the reduction of powder sedimentation at the reactor cavity

    bottom by activation of the tertiary flow during a test at room temperature.

    Fig. 14. REDUCTION OF POWDER SEDIMENTATION TEST# 204

    (A) F3=0; (B) F3=3 SLM.

    Fig. 13

  • 7/30/2019 Presentation Technion 2009

    17/29

    17

    FIG. 15. COMPONENTS OF

    REACTOR D3FIG. 16. AXIAL CROSS SECTION

    OF REACTOR D3

  • 7/30/2019 Presentation Technion 2009

    18/29

    18

    4. Some technical problems connected with the replacement of the smallsecondary concentrator by the 155 cm paraboloid mirror.

    At this stage we acquired a 155 cm secondary concentrator (SC) to replace

    the old 63 cm SC, in order to upgrade our solar power input to 10 kW. The

    reactor window had to be increased and moved from the reactor aperture in

    order to prevent its overheating (Fig. 18).

    Fig. 18. ENLARGED WINDOW Fig. 19. TWO SS FLANGES REPLACED

    BY ZIRCONIA INSULATION BOARD

    Window

    Aperture

    plane

  • 7/30/2019 Presentation Technion 2009

    19/29

    19

    Fig. 21. Contours of Stream function

    F2 (He) 2 L/M

    F1 (N2) = 26.3 L/M; =55

    F1(CH4) = 20 L/M; =55

    T4 = 1300 K

    F3,2(N2) = 20 L/M

  • 7/30/2019 Presentation Technion 2009

    20/29

    20

    The updated design of the STMS

    reactor is illustrated in Fig. 22. In this

    design part of the zirconia structure at

    the exit end of the reactor is replaced bya shaped cylinder made of copper (a).

    The temperature of the external

    surfaces of shaped cylinder (a) is kept

    down by out-of-contact water cooling.

    The inner surface (b) of the zirconia

    insulation is partly cooled by blowing atertiary stream of gas F(N2) at room

    temperature in a direction tangential to

    surface (b). The blowing stream

    entrains any solid particles in gas

    suspension in region (b) and thus

    prevents the formation of a Pyrocarbondeposit.

    F(N2)

    Boundary layerblowing

    F(N2-CB)

    F1(CH4)

    F1(N2)

    F2(He)

    F1(CA)

    F(CW)

    Shaped coppercylinder,water-cooled

    Window

    Aperturedd

    Fig.22. AXIAL CROSS SECTION

    OF THE WIS 10 Kw REACTOR

    b

    a

  • 7/30/2019 Presentation Technion 2009

    21/29

    21

  • 7/30/2019 Presentation Technion 2009

    22/29

    22

  • 7/30/2019 Presentation Technion 2009

    23/29

    23

  • 7/30/2019 Presentation Technion 2009

    24/29

    24

  • 7/30/2019 Presentation Technion 2009

    25/29

    25

  • 7/30/2019 Presentation Technion 2009

    26/29

    26

    TEM magnifications of two additional CB samples collected from

    the product filter after the same test.

  • 7/30/2019 Presentation Technion 2009

    27/29

    27

  • 7/30/2019 Presentation Technion 2009

    28/29

    28

    A spot of formation of nano-tubes that

    could be building blocks in the

    formation of nearby Fulerenes

  • 7/30/2019 Presentation Technion 2009

    29/29

    29

    CONCLUDING REMARKAS MENTIONED ABOVE, THE CONFINED

    TORNADO FLOW CONFIGURATION COULD BEAPPLIED WITH THE WIS REACTOR DESIGNWITH A MAXIMUM FLOW RATE OF SWIRLINGGAS UP TO 510 L/M.

    SUCH AN ENLARGED STMS INSTALLATIONWILL HAVE TO BE POWERED BY SOME 80 KWCONCENTRATED SOLAR RADIATION.TO DO THIS ONE WOULD HAVE TO USE A

    CLUSTER OF AT LEAST 8 WIS HELIOSTATSCOUPLED WITH A NON-IMAGINGCONCENTRATOR, SUCH AS A COMPOUNDPARABOLIC CONCENTRATOR.