solar thermogravimetry experiments at psi hfss facilities...4 + ½ o 2 2 mn 3 o 4 → 6 mno + o 2...

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Solar thermogravimetry experiments at PSI HFSS facilities José González-Aguilar 18 th SolarPACES Conference 11-14 September 2012. Marrakech. Morocco

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Page 1: Solar thermogravimetry experiments at PSI HFSS facilities...4 + ½ O 2 2 Mn 3 O 4 → 6 MnO + O 2 First proceeds at the temperature range between 800 ºC and 1060 ºC in nitrogen,

Solar thermogravimetry experiments

at PSI HFSS facilities

José González-Aguilar

18th SolarPACES Conference

11-14 September 2012. Marrakech. Morocco

Page 2: Solar thermogravimetry experiments at PSI HFSS facilities...4 + ½ O 2 2 Mn 3 O 4 → 6 MnO + O 2 First proceeds at the temperature range between 800 ºC and 1060 ºC in nitrogen,

Solar thermogravimetry experiments at PSI HFSS facilities

Contents

Context

Solar thermogravimetry – Experimental set-up

Analysis of Manganese oxides reduction

Conclusions

2/12

Page 3: Solar thermogravimetry experiments at PSI HFSS facilities...4 + ½ O 2 2 Mn 3 O 4 → 6 MnO + O 2 First proceeds at the temperature range between 800 ºC and 1060 ºC in nitrogen,

Solar thermogravimetry experiments at PSI HFSS facilities

Context

Mn2O3

MnO

NaMnO2

O2

H2

H2O

NaOH

Metal oxide

decomposition

(>1835 K)

Water splitting

(≥373 K)

Hydrogen

releasing step

(900 K)

Sturzenegger, M., Ganz, J., Nüesch, P., Schelling, T., 1998. Solar

hydrogen from manganese oxide- A new thermochemical cycle.

Hydrogen energy progress XII 1-3,801-805.

Manganese oxide based-on

thermochemical cycle

3/12

More details on 2nd and 3rd step in session THU-2-D: Solar Fuels and

Chemical Commodities next Thursday.

Factors Influencing Hydrogen Production and Sodium Recovery in the

NaOH-MnO Thermochemical Cycle, A. Bayón, IMDEA Energy

Page 4: Solar thermogravimetry experiments at PSI HFSS facilities...4 + ½ O 2 2 Mn 3 O 4 → 6 MnO + O 2 First proceeds at the temperature range between 800 ºC and 1060 ºC in nitrogen,

First-step manganese thermochemical cycle based for

hydrogen production:

3 Mn2O3 → 2 Mn3O4 + ½ O2

2 Mn3O4 → 6 MnO + O2

First proceeds at the temperature range between 800

ºC and 1060 ºC in nitrogen, air or oxygen (Tinsley and

Sharp, 1971).

Solar reduction tests have been previously carried out

by using concentrated radiation in a directly irradiated

reactor exposed to a solar furnace at above 1627 ºC

(Frey et al., 2001).

Thermogravimetry and a non-solar aerosol flow

reactor have been used (Francis, 2008; Francis et al.

2008). The Avrami-Erofeev mechanism was the best

at describing the kinetic model of the chemical

reaction (fractional extent of the reaction, a, between

0.15 and 0.85).

4/12

Solar thermogravimetry experiments at PSI HFSS facilities

Context

Mn3O4

Mn2O3

MnO

Page 5: Solar thermogravimetry experiments at PSI HFSS facilities...4 + ½ O 2 2 Mn 3 O 4 → 6 MnO + O 2 First proceeds at the temperature range between 800 ºC and 1060 ºC in nitrogen,

Characterization Of Solid-Gas Chemical Reactions by Solar TG

Context A deep knowledge of any solar thermochemical process

requires a detailed analysis of chemical reactions involved at

operating conditions close to those found under concentrating

solar radiation.

Thermal desorption in furnaces and thermogravimetric balances

are commonly used for that.

Solar thermogravimetry (in

solar furnace) has been

applied for analyzing solid-to-

gas chemical reactions

Schunk, L., Steinfeld, A., 2009. Kinetics of the thermal dissociation of ZnO exposed to

concentrated solar irradiation using a solar-driven thermogravimeter in the 1800 - 2100 K range.

AIChE Journal, vol. 55, no. 6, pp. 1497–1504. 5/12

Page 6: Solar thermogravimetry experiments at PSI HFSS facilities...4 + ½ O 2 2 Mn 3 O 4 → 6 MnO + O 2 First proceeds at the temperature range between 800 ºC and 1060 ºC in nitrogen,

http://solar.web.psi.ch/data/facilities/?pss

High Flux Solar Simulator (HFSS), PSI, Switzerland.

10 high-pressure Xe arcs, each close-coupled to

elliptical specular reflectors,

Capable of delivering 50 kW of continuous radiative

power, mostly in the visible and IR spectra

Peak flux intensities up to 11,000 suns.

Temperatures exceeding 2000 ºC at heating rates

exceeding 1000 ºC/s are achievable.

6/12

Solar thermogravimetry experiments at PSI HFSS facilities

Experimental set-up

New adaptation for using in the HF solar

simulator:

Temperature probe measurement by

pyrometer on the rear side after effective

emissivity determination.

Simultaneous gas analysis and mass

measurement.

Solar simulator focal plane placed on

reactor aperture.

Page 7: Solar thermogravimetry experiments at PSI HFSS facilities...4 + ½ O 2 2 Mn 3 O 4 → 6 MnO + O 2 First proceeds at the temperature range between 800 ºC and 1060 ºC in nitrogen,

Reactor cavity

Pyrometer

Scale cavity

Reactor gas outlet

Solar thermogravimetry experiments at PSI HFSS facilities

Experimental set up

7/12

Reactor cavity

Page 8: Solar thermogravimetry experiments at PSI HFSS facilities...4 + ½ O 2 2 Mn 3 O 4 → 6 MnO + O 2 First proceeds at the temperature range between 800 ºC and 1060 ºC in nitrogen,

Sample holder: Al2O3 99 % purity; inner diameter, 17

mm; outer diameter, 25 mm; length, 45 mm

Mn2O3 powder 99 % purity, -325 mesh, Sigma-Aldrich.

Samples were prepared by mixing the oxide powder

with water in order to obtain a thick paste that was

introduced inside the alumina tube and dried at 130 ºC

for 1 hour.

Complete conversion after

treatment (confirmed by XRD).

Melting on sample front partial

melting due to strong radiation

transfer.

8/12

Solar thermogravimetry experiments at PSI HFSS facilities

Mn2O3 reduction

Page 9: Solar thermogravimetry experiments at PSI HFSS facilities...4 + ½ O 2 2 Mn 3 O 4 → 6 MnO + O 2 First proceeds at the temperature range between 800 ºC and 1060 ºC in nitrogen,

1 cm

Solar thermogravimetry experiments at PSI HFSS facilities

Complete solar thermogravimetry

9/12

Page 10: Solar thermogravimetry experiments at PSI HFSS facilities...4 + ½ O 2 2 Mn 3 O 4 → 6 MnO + O 2 First proceeds at the temperature range between 800 ºC and 1060 ºC in nitrogen,

10/12

Solar thermogravimetry experiments at PSI HFSS facilities

First reduction

Page 11: Solar thermogravimetry experiments at PSI HFSS facilities...4 + ½ O 2 2 Mn 3 O 4 → 6 MnO + O 2 First proceeds at the temperature range between 800 ºC and 1060 ºC in nitrogen,

Best fitting for an nth order kinetic rate with n = 0.93 for a conversion range between 1 and 99%.

Pre-exponential factor compatible with a temperature uncertainty of 50 ºC.

)(exp)( aaa

fRTEAfkdt

d

a

n

f aa 1

11/12

Solar thermogravimetry experiments at PSI HFSS facilities

Mn2O3 reduction

if

i

mm

mm

a

Page 12: Solar thermogravimetry experiments at PSI HFSS facilities...4 + ½ O 2 2 Mn 3 O 4 → 6 MnO + O 2 First proceeds at the temperature range between 800 ºC and 1060 ºC in nitrogen,

Kinetics of reduction chemical reaction of manganese oxides been

successfully determined.

New improvements on sample holders design are necessary for solar

thermogravimentry.

Gas analysis is enough for characterizing chemical reactions if plug-flow is

assured.

12/12

Solar thermogravimetry experiments at PSI HFSS facilities

Conclusions

More details on solar plug-flow reactors in session WED-2-C: Solar

Fuels and Chemical Commodities tomorrow.

Thermal Performance and Residence Time Distribution Determination in

a Solar Reactor for Chemical Kinetics Analysis, E. Alonso, IMDEA Energy

Page 13: Solar thermogravimetry experiments at PSI HFSS facilities...4 + ½ O 2 2 Mn 3 O 4 → 6 MnO + O 2 First proceeds at the temperature range between 800 ºC and 1060 ºC in nitrogen,

Characterization Of Solid-Gas Chemical Reactions by Solar TG

Acknowledgments

Financial support by the Access to Research Infrastructures activity in the

7th Framework Program of the EU (SFERA Grant Agreement n. 228296) is

gratefully acknowledged.

The authors wish to thank ‘‘Comunidad de Madrid’’ and “European Social

Fund” for its financial support to the SOLGEMAC Project through the

Program of Activities between Research Groups (S2009/ENE-1617).

The authors are also grateful for the technical assistance of C. Hutter, Y.

Baeuerle and D. Wuillemin and the collaboration of F. Frick and G. Putzi at

the Solar Technology Lab of PSI

13/12