Experimentalist
- Name
- Zuriñe Yoldi
- ORCID
- 0000-0003-3938-8332
Previous
- Name
- Space Research & Planetary Sciences Division of the University of Bern (WP Unibe)
- Experimentalist status
- Master student
- Dates
- From 2014-03-01 to 2014-06-01
- Name
- Space Research & Planetary Sciences Division of the University of Bern (WP Unibe)
- Experimentalist status
- Phd student
- Dates
- From 2014-07-01 to 2018-07-31
- Name
- Space Research & Planetary Sciences Division of the University of Bern (WP Unibe)
- Experimentalist status
- Post-doc
- Dates
- From 2018-08-01
Previous
Current
- zurine.yoldi@space.unibe.ch
- Phone
- +41 31 631 32 33
- Samples
-
- Water ice spherical particles 4.5±2.5 μm at 223 K
- Water ice spherical particles 4.5±2.5 μm at 173 K
- Water ice spherical particles 67±31 μm at 223 K
- Water ice spherical particles 67±31 μm at 173 K
- Water ice spherical particles about 2 to 100 μm at 173 K
- Dark basalt (Original)
- Dark basalt (grains larger than 400 µm)
- Dark basalt (200-400 µm grains)
- Dark basalt (100-200 µm grains)
- Dark basalt (grains smaller than 100 µm)
- Water frost (~13 µm thick) on Dark basalt (grains larger than 400 µm)
- Water frost (~52 µm thick) on Dark basalt (grains larger than 400 µm)
- Water frost (~75 µm thick) on Dark basalt (grains larger than 400 µm)
- Water frost (~13 µm thick) on Dark basalt (200-400 µm grains)
- Water frost (~52 µm thick) on Dark basalt (200-400 µm grains)
- Water frost (~75 µm thick) on Dark basalt (200-400 µm grains)
- Water frost (~13 µm thick) on Dark basalt (100-200 µm grains)
- Water frost (~52 µm thick) on Dark basalt (100-200 µm grains)
- Water frost (~75 µm thick) on Dark basalt (100-200 µm grains)
- Water frost (~13 µm thick) on Dark basalt (grains smaller than 100 µm)
- Water frost (~52 µm thick) on Dark basalt (grains smaller than 100 µm)
- Water frost (~75 µm thick) on Dark basalt (grains smaller than 100 µm)
- Water frost (~14 µm thick) on JSC Mars-1 (grains larger than 400 µm)
- Water frost (~33 µm thick) on JSC Mars-1 (grains larger than 400 µm)
- Water frost (~50 µm thick) on JSC Mars-1 (grains larger than 400 µm)
- Water frost (~14 µm thick) on JSC Mars-1 (200-400 µm grains)
- Water frost (~33 µm thick) on JSC Mars-1 (200-400 µm grains)
- Water frost (~50 µm thick) on JSC Mars-1 (200-400 µm grains)
- Water frost (~14 µm thick) on JSC Mars-1 (100-200 µm grains)
- Water frost (~33 µm thick) on JSC Mars-1 (100-200 µm grains)
- Water frost (~50 µm thick) on JSC Mars-1 (100-200 µm grains)
- Water frost (~14 µm thick) on JSC Mars-1 (grains smaller than 100 µm)
- Water frost (~33 µm thick) on JSC Mars-1 (grains smaller than 100 µm)
- Water frost (~50 µm thick) on JSC Mars-1 (grains smaller than 100 µm)
- Water ice spherical particles 4.5±2.5 μm at about 120 K
- Water ice spherical particles 67±31 μm at about 120 K
- JSC Mars-1 mixed with 10 wt% Water ice particles (4.5±2.5 μm)
- JSC Mars-1 mixed with 35 wt% Water ice particles (4.5±2.5 μm)
- JSC Mars-1 mixed with 50 wt% Water ice particles (4.5±2.5 μm)
- JSC Mars-1 mixed with 75 wt% Water ice particles (4.5±2.5 μm)
- JSC Mars-1 mixed with 10 wt% Water ice particles (67±31 μm)
- JSC Mars-1 mixed with 35 wt% Water ice particles (67±31 μm)
- JSC Mars-1 mixed with 50 wt% Water ice particles (67±31 μm)
- JSC Mars-1 mixed with 75 wt% Water ice particles (67±31 μm)
- Dark basalt mixed with 35 wt% Water ice particles (67±31 μm)
- Dark basalt mixed with 50 wt% Water ice particles (67±31 μm)
- Dark basalt mixed with 75 wt% Water ice particles (67±31 μm)
- Water frost (~80 µm) over Dark basalt mixed with 35 wt% Water ice particles (67±31 μm)
- Water frost (~80 µm) over Dark basalt mixed with 50 wt% Water ice particles (67±31 μm)
- Water frost (~80 µm) over Dark basalt mixed with 75 wt% Water ice particles (67±31 μm)
- JSC Mars-1 (Original)
- JSC Mars-1 (grains larger than 400 µm)
- JSC Mars-1 (200-400 µm grains)
- JSC Mars-1 (100-200 µm grains)
- JSC Mars-1 (grains smaller than 100 µm)
- Frozen water saturated (87 wt%) JSC Mars-1 (grains smaller than 100 µm) after 3h of sublimation
- Frozen water saturated (87 wt%) JSC Mars-1 (grains smaller than 100 µm) after 7h of sublimation
- Frozen water saturated (87 wt%) JSC Mars-1 (grains smaller than 100 µm) after 14h of sublimation
- Frozen water saturated (87 wt%) JSC Mars-1 (grains smaller than 100 µm) after 17h of sublimation
- Frozen water saturated (90 wt%) Dark basalt (grains smaller than 100 µm) after 3h of sublimation
- Frozen water saturated (90 wt%) Dark basalt (grains smaller than 100 µm) after 3.5h of sublimation
- Frozen water saturated (90 wt%) Dark basalt (grains smaller than 100 µm) after 4h of sublimation
- Frozen water saturated (90 wt%) Dark basalt (grains smaller than 100 µm) after 4.5h of sublimation
- Frozen water saturated (90 wt%) Dark basalt (grains smaller than 100 µm) after 4.6h of sublimation
- JSC-1AF Lunar Regolith simulant (fine fraction)
- Lunar regolith simulant JSC-1AF mixed with 10 wt.% spherical water ice particles
- Lunar regolith simulant JSC-1AF mixed with 35 wt.% spherical water ice particles
- Lunar regolith simulant JSC-1AF mixed with 50 wt.% spherical water ice particles
- Lunar regolith simulant JSC-1AF mixed with 75 wt.% spherical water ice particles
- Lunar regolith simulant JSC-1AF mixed with 10 wt.% fine-grained spherical water ice particles
- Lunar regolith simulant JSC-1AF mixed with 35 wt.% fine-grained spherical water ice particles
- Lunar regolith simulant JSC-1AF mixed with 50 wt.% fine-grained spherical water ice particles
- Lunar regolith simulant JSC-1AF mixed with 75 wt.% fine-grained spherical water ice particles
- Second location with water frost deposition (intermediate, estimated 150 microns) over the CO2 slab
- Third location with water frost deposition (thin, estimated 75 µm microns) over the CO2 slab
- First location with water frost deposition (thick, estimated 400 microns) over the CO2 slab
- Piece of compact CO2 ice slab
- Crushed CO2 ice: 400 to 800 microns
- Crushed CO2 ice: 200 to 400 microns
- Crushed CO2 ice: less than 200 microns
- Crushed CO2 ice (400 to 800 microns)
- Crushed CO2 ice (400 to 800 microns) mixed with 3 wt.% fine-grained spherical water ice (4.5 microns average diameter)
- Crushed CO2 ice (400 to 800 microns) mixed with 5 wt.% fine-grained spherical water ice (4.5 microns average diameter)
- Crushed CO2 ice (400 to 800 microns) mixed with 10 wt.% fine-grained spherical water ice (4.5 microns average diameter)
- 95 wt.% of JSC Mars-1, 5 wt.% of CO2 ice
- 90 wt.% of JSC Mars-1, 10 wt.% of CO2 ice
- 65 wt.% of JSC Mars-1, 35 wt.% of CO2 ice
- 50 wt.% of JSC Mars-1, 50 wt.% of CO2 ice
- 25 wt.% of JSC Mars-1, 75 wt.% of CO2 ice
- Pure crushed CO2 ice, 400 to 800 microns fraction
- CO2 frost (10-100 microns) produced by adiabatic expansion of gas
- CO2 frost (10-100 microns) intimately mixed with 3 wt.% fine-grained spherical water ice (4.5 microns average diameter)
- CO2 frost (10-100 microns) intimately mixed with 5 wt.% fine-grained spherical water ice (4.5 microns average diameter)
- CO2 frost (10-100 microns) intimately mixed with 10 wt.% fine-grained spherical water ice (4.5 microns average diameter)
- Sample evolved by sublimation of an initial ternary mixture of CO2 frost with 3 wt.% fine-grained water ice and 0.2 wt.% of JSC Mars-1; texture: compacted;
- Sample evolved by sublimation of an initial ternary mixture of CO2 frost with 3 wt.% fine-grained water ice and 0.2 wt.% of JSC Mars-1; texture: powder;
- First location with water frost deposition (thick, estimated 400 microns) over the CO2 slab
- Sample evolved by sublimation of an initial ternary mixture of CO2 frost with 3 wt.% coarse-grained water ice and 0.2 wt.% of JSC Mars-1; texture: compacted;
- Sample evolved by sublimation of an initial ternary mixture of CO2 frost with 3 wt.% coarse-grained water ice and 0.2 wt.% of JSC Mars-1; texture: powder;
- Crushed CO2 ice (400 to 800 microns)
- Crushed CO2 ice (400 to 800 microns) mixed with 3 wt.% spherical water ice (70 microns average diameter)
- Crushed CO2 ice (400 to 800 microns) mixed with 5 wt.% spherical water ice (70 microns average diameter)
- Crushed CO2 ice (400 to 800 microns) mixed with 10 wt.% spherical water ice (70 microns average diameter)
- Second location with water frost deposition (intermediate, estimated 150 microns) over the CO2 slab
- Third location with water frost deposition (thin, estimated 75 µm microns) over the CO2 slab
- CO2 frost (10-100 microns) produced by adiabatic expansion of gas
- CO2 frost (10-100 microns) intimately mixed with 3 wt.% spherical water ice (70 microns average diameter)
- CO2 frost (10-100 microns) intimately mixed with 5 wt.% spherical water ice (70 microns average diameter)
- CO2 frost (10-100 microns) intimately mixed with 10 wt.% spherical water ice (70 microns average diameter)
- JSC1AF Lunar Regolith simulant (fine fraction)
- SPIPA-B spherical water ice (average diameter: 67 microns)
- SPIPA-A fine-grained spherical water ice (average diameter: 4.5 microns)
- Lunar regolith simulant JSC-1AF mixed with 10 wt.% spherical water ice particles
- Lunar regolith simulant JSC-1AF mixed with 35 wt.% spherical water ice particles
- Lunar regolith simulant JSC-1AF mixed with 75 wt.% spherical water ice particles
- Lunar regolith simulant JSC-1AF mixed with 50 wt.% spherical water ice particles
- Lunar regolith simulant JSC-1AF mixed with 10 wt.% fine-grained spherical water ice particles
- Lunar regolith simulant JSC-1AF mixed with 35 wt.% fine-grained spherical water ice particles
- Lunar regolith simulant JSC-1AF mixed with 75 wt.% fine-grained spherical water ice particles
- Lunar regolith simulant JSC-1AF mixed with 50 wt.% fine-grained spherical water ice particles
- Matters
-
- Water ice spherical particles 4.5±2.5 μm
- Water ice spherical particles 67±31 μm
- Water ice spherical particles 2 to 100 μm (possibly 35±20 µm, to be confirmed)
- JSC Mars-1 (grains larger than 400 µm)
- JSC Mars-1 (200-400 µm grains)
- JSC Mars-1 (100-200 µm grains)
- JSC Mars-1 (grains smaller than 100 µm)
- Dark basalt
- Dark basalt (grains larger than 400 µm)
- Dark basalt (200-400 µm grains)
- Dark basalt (100-200 µm grains)
- Dark basalt (grains smaller than 100 µm)
- CO2 slab
- CO2 ice crushed from a commercial slab and dry sieved to extract particles sizes between 200 and 400 microns
- CO2 ice crushed from a commercial slab and dry sieved to extract particles sizes smaller than 200 microns
- CO2 frost
- H2O frost deposited at the surface of compact CO2 ice
- CO2 ice crushed from a commercial slab and dry sieved to extract particles sizes between 400 and 800 microns
- JSC1AF Lunar regolith simulant (fine fraction)