USING SOLAR ENERGY CONTINUOUSLY THROUGH DAY AND NIGHT FOR METHANE REFORMING – AN EXPERIMENTAL...
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USING SOLAR ENERGY CONTINUOUSLY THROUGH DAY AND NIGHT FOR METHANE REFORMING – AN
EXPERIMENTAL DEMONSTRATION
J. L. Lapp, M. Lange, M. Roeb, C. Sattler
ECCE10 – 1701 01.10.2015
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200 300 400 500 600 700 800 900
Temperature in °C
Mo
le-%
CH4
CO2CO
H2
H2O
Background on Methane Reforming
• Primary source of industrial hydrogen• Feedstock is typically natural gas
• Other possible feedstocks: biogas, refinery gas, coke oven gas
• Heat input needed at 700-900 C• Products (syngas) useful for synthesis of
other fuels (Fischer-Tropsch)• Catalyst required for kinetic reasons
04 2 2 298CH H O 3H CO 206 kj/molKH
04 2 2 298CH CO 2H 2CO 247 kj/molKH
Steam Reforming:
Dry Reforming:
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Traditional Methane Reforming
04 2 2 298CH H O 3H CO 206 kj/molKH
800 °C30%
800 °C
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Solar Methane Reforming
04 2 2 298CH H O 3H CO 206 kj/molKH
800 °C30%
42% increased output
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Why use solar energy to produce chemical fuels?
1)Long term storage
2)Easy to transport
3)Compatible with current infrastructure
4)Uses in transportation
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Solar Methane Reforming Background
Directly irradiated Indirectly heated
Source: R. Tamme, 2002, SOLASYS – Final Report
+ High efficiency– High cost– Technically challenging
+ Consists of existing / simplerprocess units
Technically easy? Efficiency potential unknown
Concept first proposed in 1982 by Chubb of U.S. Naval Research Laboratory
ECCE10-1701 01 October 2015 Lapp et al.
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Indirect Experimental Studies
ASTERIX (CIEMAT/DLR, 1991)170 kW, 68-93% Conversion
DCORE (CSIRO, 2009) 200 kWSCORE (CSIRO, 1999) 25 kW
WIS, 2003, 480 kW
Sodium Vapor HTF (WIS/SNL 1983)20 kW
ECCE10-1701 01 October 2015 Lapp et al.
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Direct Experimental Studies
INHA-DISH1, 20105 kW 60% conversion
DIAPR (porcupine), WIS, 201085% conversion
Particle concept, WIS, 2009
SOLBIOPOLYSY, 2008, 250 kW, landfill gas
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CAESAR – SNL/DLR 1987 – 100kW
Solar Power (kW)
Receiver Efficiency (%)
Chemical Efficiency (%)
Methane Conversion (%)
Radially Uniform Absorber74.8 21.7 20.8 60.078.7 43.8 28.5 51.686.3 39.7 25.2 48.888.8 44.0 29.0 45.6105.7 79.3 50.7 45.9115.7 85.6 54.4 39.1Radially Non-Uniform Absorber64.1 67.3 46.3 66.072.1 65.9 44.9 68.576.9 62.7 43.6 69.597.3 68.7 45.3 52.4
ECCE10-1701 01 October 2015 Lapp et al.
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SOLASYS: DLR/WIS/Ormat, 220 kW, >90% conversion
Source: R. Tamme, 2002, SOLASYS – Final Report
4.9 bar 7.5 barMeasured CH4 Conversion 72.0% 70.5%Calculated CH4 Conversion 73.2% 65.0%
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SOLREF: DLR/WIS – 400 kW, 950 °C, 15 bar
Included novel catalytic system suitable for biogas, landfill gas, and high CO2 natural gas
94.6% Conversion
ECCE10-1701 01 October 2015 Lapp et al.
ECCE10-1701 01 October 2015 Lapp et al. 12
Theoretical Efficiency Analysis
650 700 750 800 850 900 950 1000
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Eff
icie
ncy
Hot Air Temperature in °C
Overall Receiver-Reactor Process
-0.4
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ectr
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oduc
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Hot Air Temperature in °C
Overall Receiver Process
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oduc
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Indirect Direct
650 700 750 800 850 900 950 1000
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OVCR OVR TCR CVR
Pro
cess
Eff
icie
ncy
Hot Air Temperature in °C
• Energy balance (flow sheet) analysis
• Directly and indirectly heated receiver concepts (separate models)
• Annual efficiency calculated with hourly irradiation data
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Direct and Indirect Concepts
Directly Irradiated Catalyst Indirectly Heated with Air HTF
Technical Difficulties Window, Catalyst-Absorber Low Heat Transfer Rate
Dynamic Behavior Fast Slow
Heat Losses Moderate High
Heat Storage Difficult Easy
Hybridization (burners) Difficult Easy
Coupling with CSP Plant Difficult Easy
ECCE10-1701 01 October 2015 Lapp et al.
Reactor: SiSiC - honeycomb structure with catalyst coating (Rh)
Contisol Project
CO + H2 Hot air
Cold air CH4 + steam + CO2
ECCE10-1701 01 October 2015 Lapp et al. 14
Contisol Project
Thermal StorageDaytime
Thermal StorageNighttime
Hot air to storage
Hot air from storage
ECCE10-1701 01 October 2015 Lapp et al. 15
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Modeling Results
Concept 3D Computational DomainApplied Heat Flux
Reactants side Air side
Daytime Operation
Nighttime Operation
Reactants side Air side
ECCE10-1701 01 October 2015 Lapp et al.
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Experimental Setup
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Experimental Setup (simplified to thermal testing)
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Experimental PreparationPorous Silicon Carbide Monolith
Infiltrated (dense)Monolith
TC’s Mounted“Canning” Mounted
Channels Closed
Monolith Sealed and Mounted
ECCE10-1701 01 October 2015 Lapp et al.
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ExperimentsGas coolers ReactorAir Preheater Radiation Shield
Reactant Preheater
Pressure Sensors
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Experiments
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ExperimentalResults
06:00:00 09:00:00 12:00:00 15:00:00 18:00:000
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Time
Tem
pera
ture
(°C
)
Absorber FrontAbsorber Middle
Absorber Back
Side Inlet
Side Outlet
Straight InletStraight Outlet
06:00:00 09:00:00 12:00:00 15:00:00 18:00:00-400
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Time
T
(°C
)
Side Stream
Straight Stream
06:00:00 09:00:00 12:00:00 15:00:00 18:00:000
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Time
Flo
w R
ate
(l/m
in)
Straight Inlet
Side InletStraight Outlet
Side Outlet
ECCE10-1701 01 October 2015 Lapp et al.
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Experimental Investigation• Used statistical design of experiments procedure (using Origin software)• Identified key variables
• Gas flow rate (x2)• Gas inlet temperature (x2)• Monolith front temperature
• Even with 3 values of each variable, 243 runs needed to fully describe system (full factorial)
• Optimally distributed input parameter set over 23 runs• Regression and co-variance analysis used to determine impact on efficiency of
each varible• Performance prediction of receiver fit by statistical model with R2 > 0.99
𝑇 𝑓𝑟𝑜𝑛𝑡
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Experimental Investigation Results (all CI 95%)ECCE10-1701 01 October 2015 Lapp et al.
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Experimental Investigation Results (all CI 95%)
• Flow rates are less important at high monolith temperatures (re-radiation dominates)
• Flow rates are more important to the efficiency than inlet temperatures
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Leakage Problem
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Future Advancements• 3-D printing of Inconel monolith
Test Sample, DLR, 17.09.2015
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Future Advancements• 3-D printing of Inconel monolith• Acid etching of surface required
Test Sample, DLR, 17.09.2015
Before Etching
AfterEtching
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Conclusions
• 41% upgrade of useful fuel energy with solar energy• Indirect and direct concepts• High conversion demonstrated, flexibility has not• New concept (CONTISOL) has been modeled• Thermal experiments begun• Major challenge is leakage• Will address in next steps
Thermal Storage
ECCE10-1701 01 October 2015 Lapp et al.