Description - Esa 2009i |
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Revolutionary way of bringing a powerful analytical tool to solve problems in urgent forensic, R&D or QA cases in production monitoring Removal of the instrument background and substantial reduction of the second order analyser aberrations made it possible to achieve the best energy resolution spectrometer for its size High resolution imaging is a combination of superior focusing properties of the analyzer , lens system and resolution of the imaging detector. Our software has an intuitive customer interface , is flexible and easy to use. Its standardized data transfer is ready to accommodate future developments. Comprehensive analysis by combining XPS spectra , XPS snap-shots and XPS imaging in one instrument . |
Capabilities - Esa 2009i combination of 3 techniques in one portable instrument |
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XP Spectrometry (XPS): |
Specification - Esa 2009i Analyser | |
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Analytical techniques (depending on appropriate sources being fitted) | XPS, AES, SAM, UPS, ISS |
Type | An analyser of proprietary design with variable slits |
Mean radius (diameter) | 180 mm |
CE Conformity | Meets Electromagnetic Compatibility Directive 89/336/EEC and Low |
Detector | Multi channel detector with 20, 40 & 60 channels; with minimum 14 channels |
Magnetic shielding & vacuum envelope | Vacuum envelope constructed from mu-metal to reduce outgassing in vacuum |
Analyser operating modes | CAE (constant analyser energy) CRR (constant retard ratio) |
Energy range | Continuous |
Pass energy range | Continuous |
Retard ratio values | Continuous |
Minimum step size under computer control | +- 1 LSB of the full scale |
Analyser ultimate resolution | 5 meV |
Analyser machining | manufacture to a tolerance of 0.005 mm (0.0002”) |
Mounting flange size | C150 mm (6”) o.diamater |
Recommended working distance |
30 mm. Longer distances easily accommodated by simple lens control potentiometer adjustment. |
Slit mechanism operation | Single rotary drive |
Spectrometer control unit ripple level | As specified |
Spectrometer control unit output voltage drift | +/-LSD of 16 bit on FSD; over 5 hours after 1 hour warm up |
Maximum Bake-out Temperature | 250 C |
White Documents |
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ESA 2009i Product Range & Specification |
Performance - Esa 2009i | |||
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XPS large area MgKa Ag3d5 at 300W |
dE(eV) | I(cps) | |
0.81 | 1500000 | ||
0.85 | 6000000 | ||
0.87 | 8000000 | ||
1.00 | 15000000 | ||
1.40 | 36000000 | ||
Selected Area XPS | dE(eV) | I(cps) | |
MgKa Ag3d5 300W Sample dia 150um |
0.81 | 75000 | |
0.99 | 300000 | ||
Sample dia 1000um | 0.81 | 950000 | |
0.99 | 9200000 | ||
Imaging XPS Resolution MgKa Ag3d5 300W |
dX (um) | Pixel cps | |
dE=1.4eV | 10 | 16 | |
dE=2.0eV | 2 | 1 | |
Imaging XPS Ultimate Resolution | < 200 nm | ||
UPS He I | dE(eV) | I(cps) | |
Ag val. Band 300K | 0.14 | 20000000 | |
AES | dE(eV) | I(cps) | |
Cu 920eV 20nA/5kV | 0.50% | 4000000 | |
ISS | dE(eV) | I(cps) | |
( He+) 500nA/2kV | 0.50% | 12000000 | |