Micro Spectro-Gonio Radiometer
(8 intermediate revisions by one user not shown) | |||
Line 26: | Line 26: | ||
'''General description''' | '''General description''' | ||
− | The new spectro-gonio radiometer currently under developement will be optimized for the measurement at low temperature of bidirectional reflectance spectra, over the visible and near-IR (at least from | + | The new micro spectro-gonio radiometer currently under developement will be optimized for the measurement at low temperature of bidirectional reflectance spectra, over the visible and near-IR (at least from 350 to 4800 nm), of dark and very small samples (organics, meteorites…) down to a few mm3 in volume. |
[[sample holders]]: | [[sample holders]]: | ||
Line 32: | Line 32: | ||
It will have 2 major sample holder configurations: | It will have 2 major sample holder configurations: | ||
− | - Open sample holders (various sizes | + | - '''''Open sample holders''''' (various sizes) in '''''cold chamber''''' over -20°C ─ +20°C temperature range. |
− | - The SERAC environmental cell (-40°C ─ +80°C | + | - The '''''SERAC environmental cell''''' with cryostats, pumps, pressure and temperature controllers, which allows us to introduce gas(es) of known composition and pressure (10-6 mb - 1 bar) over the sample and controlling and measuring the temperature over the -40°C ─ +80°C range. It will have a set of sample holders (small sizes) adapted to this new setup. |
[[Tools and sub-systems]]: | [[Tools and sub-systems]]: | ||
Line 40: | Line 40: | ||
A number of sample preparation tools and experiment sub-systems are available to the facility: | A number of sample preparation tools and experiment sub-systems are available to the facility: | ||
− | - For samples preparation: another cold chamber (down to -20°C), set of sample holders, several specific tools for ice sample preparation, | + | - For samples preparation: another cold chamber (down to -20°C), set of sample holders, several specific tools for ice sample preparation, 2 sets of sieves, grinders, mortars, saw, balances, microscope, owen, ultra-pure water, several pure gasses, wet chemistry materials a, several owens (up to 1200°C) for sample treatments. |
- For the experiment: a thermodynamic volumetric system with high accuracy pressure gauges (10-6 to 1 bar), a flow meter (1-10 sccm) and pumps. He-Ne laser + detectors, camera for sample monitoring, … | - For the experiment: a thermodynamic volumetric system with high accuracy pressure gauges (10-6 to 1 bar), a flow meter (1-10 sccm) and pumps. He-Ne laser + detectors, camera for sample monitoring, … | ||
Line 49: | Line 49: | ||
'''Technical characteristics''': | '''Technical characteristics''': | ||
− | [[Spectral range]] : 0. | + | [[Spectral range]] : 0.35 - 4.5 µm (< 0.35 & > 4.8 µm: lower S/N) (4.2-4.3µm: atm. CO2 limited) |
[[Spectral resolution]] : variable | [[Spectral resolution]] : variable | ||
Line 55: | Line 55: | ||
- mini: < 0.1 nm (but S/N limited) | - mini: < 0.1 nm (but S/N limited) | ||
− | - maxi: | + | - maxi: 3 nm (<700nm), 7 nm (<1600nm), 12 nm (<3000nm), 26nm (>3000nm) [May change with future new monochromator] |
[[Bidirectional Reflectance]] | [[Bidirectional Reflectance]] | ||
− | - ''Incidence angle'': 0° to | + | - ''Incidence angle'': 0° to 75° ; resolution: 2° (can be reduced to 1°) ; maximum sampling : 0.1° |
- ''Emergence angle'': 0° to 80° for dark / fine grained samples ; resolution : ± 2° (may be reduced to < ± 0.5°, but S/N limited) ; max. sampling : 0.1° | - ''Emergence angle'': 0° to 80° for dark / fine grained samples ; resolution : ± 2° (may be reduced to < ± 0.5°, but S/N limited) ; max. sampling : 0.1° | ||
Line 65: | Line 65: | ||
- ''Azimuth angle'': 0° to 180° ; resolution : ± 2° (may be reduced to < ± 0.5°, but S/N limited) ; max. sampling : 0.1° | - ''Azimuth angle'': 0° to 180° ; resolution : ± 2° (may be reduced to < ± 0.5°, but S/N limited) ; max. sampling : 0.1° | ||
− | - ''Phase angle'': | + | - ''Phase angle'': up to to 155° ; mini : ~ 7° for dark / fine grained samples |
− | - ''Illumination diameter'' (nadir): | + | - ''Illumination diameter'' (nadir): 7.5 mm |
- ''Observation diameter'' (nadir): 20 mm | - ''Observation diameter'' (nadir): 20 mm | ||
Line 74: | Line 74: | ||
''Absolute'': [will be determined during calibration and test phase end 2015 - 2016] | ''Absolute'': [will be determined during calibration and test phase end 2015 - 2016] | ||
− | - 0. | + | - 0.35-1.0 µm: expected better than 1% over all configurations (relative to a calibrated Spectralon 0.99 reference panel) |
- 1.0-2.5 µm: expected better than 1% over all configurations | - 1.0-2.5 µm: expected better than 1% over all configurations | ||
Line 82: | Line 82: | ||
''Relative'' : | ''Relative'' : | ||
− | - better than 0.5% (0. | + | - better than 0.5% (0.35-4.5 µm) |
+ | |||
+ | |||
+ | [[File:micro-gonio_design-optique.jpg|500px]] | ||
+ | |||
+ | ''Picture'': sketch of the micro spectro-gonio radiometer under building at IPAG | ||
[[Samples]] | [[Samples]] | ||
− | + | ''Types'': cosmo-materials, synthetic and terrestrial carbonaceous materials, minerals | |
− | + | ''Texture'': compact (dark) or granular (dark and/or fine grained < 200µm) | |
− | + | ''Grain size'': sub-µm to a 200 µm | |
− | + | ''Size'': | |
− | + | - 32 mm diameter (for full BRDF down to 75° observation) | |
− | + | - 8 mm x 32 mm (for principal plane observation down to 75°) | |
+ | - 8 mm x 16 mm (for principal plane observation down to 60°) | ||
+ | |||
+ | ''Thickness'': | ||
− | + | - 0.1 mm for dark & fine grained samples (< 20 µm) | |
− | '' | + | - up to 5 mm for 'gray' & medium grained samples (< 200 µm) |
− | + | - up to 10 mm for bright & medium/fine grained samples (< 100 µm) | |
− | |||
[[Temperature]]: | [[Temperature]]: | ||
Line 129: | Line 136: | ||
[[Current state of system]]: | [[Current state of system]]: | ||
− | - 0.3 - | + | - Visible 0.3 - 1 µm range: under development, testing and buiding [2013-2015]. Ready for full testing end of 2015 |
+ | |||
+ | - Infrared 1 - 4.8µm range: extension planned in 2015-2017 (if EPN2020-RI program accepted) | ||
− | + | - low temperature: to be tested in cold room down to -20°C (end 2015) | |
− | + | ||
− | - low temperature: to be tested in cold room down to -20°C | + | |
* Characteristics: [[File:Micro-Spectro-Gonio_characteristics.pdf]] | * Characteristics: [[File:Micro-Spectro-Gonio_characteristics.pdf]] | ||
Line 139: | Line 146: | ||
− | '''Availability to community:''' | + | '''Availability to community:''' |
+ | |||
+ | '''''2016-2017''''': | ||
+ | |||
+ | - Technical improvements/calibration (40%) | ||
+ | |||
+ | - IPAG + associated laboratories measurements (60%) | ||
+ | |||
+ | '''''after 2017''''': | ||
- Technical improvements/calibration (20%) | - Technical improvements/calibration (20%) |
Latest revision as of 23:21, 3 December 2014
[edit] Laboratory Experiment facility
Facility name:
Micro Spectro-Gonio Radiometer
Location:
Institut de Planétologie et Astrophysique de Grenoble
CNRS - Université Grenoble Alpes
Saint Martin d’Hères, France
Persons in charge:
- Scientific : Pierre Beck, Assistant Professor & Bernard Schmitt, Research director
- Technical : Olivier Brissaud, Engineer
General description
The new micro spectro-gonio radiometer currently under developement will be optimized for the measurement at low temperature of bidirectional reflectance spectra, over the visible and near-IR (at least from 350 to 4800 nm), of dark and very small samples (organics, meteorites…) down to a few mm3 in volume.
It will have 2 major sample holder configurations:
- Open sample holders (various sizes) in cold chamber over -20°C ─ +20°C temperature range.
- The SERAC environmental cell with cryostats, pumps, pressure and temperature controllers, which allows us to introduce gas(es) of known composition and pressure (10-6 mb - 1 bar) over the sample and controlling and measuring the temperature over the -40°C ─ +80°C range. It will have a set of sample holders (small sizes) adapted to this new setup.
A number of sample preparation tools and experiment sub-systems are available to the facility:
- For samples preparation: another cold chamber (down to -20°C), set of sample holders, several specific tools for ice sample preparation, 2 sets of sieves, grinders, mortars, saw, balances, microscope, owen, ultra-pure water, several pure gasses, wet chemistry materials a, several owens (up to 1200°C) for sample treatments.
- For the experiment: a thermodynamic volumetric system with high accuracy pressure gauges (10-6 to 1 bar), a flow meter (1-10 sccm) and pumps. He-Ne laser + detectors, camera for sample monitoring, …
Technical characteristics:
Spectral range : 0.35 - 4.5 µm (< 0.35 & > 4.8 µm: lower S/N) (4.2-4.3µm: atm. CO2 limited)
Spectral resolution : variable
- mini: < 0.1 nm (but S/N limited)
- maxi: 3 nm (<700nm), 7 nm (<1600nm), 12 nm (<3000nm), 26nm (>3000nm) [May change with future new monochromator]
- Incidence angle: 0° to 75° ; resolution: 2° (can be reduced to 1°) ; maximum sampling : 0.1°
- Emergence angle: 0° to 80° for dark / fine grained samples ; resolution : ± 2° (may be reduced to < ± 0.5°, but S/N limited) ; max. sampling : 0.1°
- Azimuth angle: 0° to 180° ; resolution : ± 2° (may be reduced to < ± 0.5°, but S/N limited) ; max. sampling : 0.1°
- Phase angle: up to to 155° ; mini : ~ 7° for dark / fine grained samples
- Illumination diameter (nadir): 7.5 mm - Observation diameter (nadir): 20 mm
Absolute: [will be determined during calibration and test phase end 2015 - 2016]
- 0.35-1.0 µm: expected better than 1% over all configurations (relative to a calibrated Spectralon 0.99 reference panel)
- 1.0-2.5 µm: expected better than 1% over all configurations
- 2.5-4.5 µm : expected better than 2% over all configurations
Relative :
- better than 0.5% (0.35-4.5 µm)
Picture: sketch of the micro spectro-gonio radiometer under building at IPAG
Types: cosmo-materials, synthetic and terrestrial carbonaceous materials, minerals
Texture: compact (dark) or granular (dark and/or fine grained < 200µm)
Grain size: sub-µm to a 200 µm
Size:
- 32 mm diameter (for full BRDF down to 75° observation)
- 8 mm x 32 mm (for principal plane observation down to 75°)
- 8 mm x 16 mm (for principal plane observation down to 60°)
Thickness:
- 0.1 mm for dark & fine grained samples (< 20 µm)
- up to 5 mm for 'gray' & medium grained samples (< 200 µm)
- up to 10 mm for bright & medium/fine grained samples (< 100 µm)
- room temperature or heated
- down to -20°C (in cold room)
- down to -40°C (in SERAC environmental cell)
- PC/Windows, fully software controlled (LabView©). Automatic acquisition of all spectral/geometric configurations
Acquisition time: [will be determined during calibration and test phase end 2015 - 2016]
- typical: 1 mn for 200 spectral channels in visible (S/N dependent)
- total: <1 hour for 100 spectral channels and 100 geometries
- Visible 0.3 - 1 µm range: under development, testing and buiding [2013-2015]. Ready for full testing end of 2015
- Infrared 1 - 4.8µm range: extension planned in 2015-2017 (if EPN2020-RI program accepted)
- low temperature: to be tested in cold room down to -20°C (end 2015)
- Characteristics: File:Micro-Spectro-Gonio characteristics.pdf
- Article: [[File:]]
Availability to community:
2016-2017:
- Technical improvements/calibration (40%)
- IPAG + associated laboratories measurements (60%)
after 2017:
- Technical improvements/calibration (20%)
- IPAG + associated laboratories measurements (60%)
- open as facility or to specific collaborations w. funding (20%)
References: