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Tweets by ApssLab
Tweets by WijewardaneK
RESOURCES
BRUKER ALPHA II
Available modules: Platinum-ATR, DRIFT, Front-Reflection, and Transmission
Wavelength range: 1,250 nm – 28,000 nm
Diode calibration laser with higher wavenumber accuracy
Detector: DLaTGS
RockSolid
TM
interferometer
IR source: CenterGlow
TM
technology
Ocean Insight NIRQuest+2.2 Spectrometers
Wavelength range: 900 nm – 2.2 μm
High resolution: 4 cm
-1
Detector: InGaAs linear array
Ocean Insight HR4PRO-XR-ES Spectrometer
Wavelength range: 200 nm – 1.1 μm
Optical resolution: 0.9 nm FWHM
Detector : linear silicon CCD array
Ocean Insight DH-2000-BAL Light Source
Light sources: UV-Vis-NIR
Wavelength range: 210 nm – 2.5 μm
Source: Deuterium & Tungsten Halogen
Fiber connects with SMA 905
Power requirement: 85-264 V, 50/60 Hz
ARCoptix FT-MIR Rocket Spectrometer
Mid-Infrared spectrometer
Wavelength range: 2 μm – 6 μm
Optical Resolution: 3.13 nm
Signal: >1:60,000 noise
Interferometer type: permanently aligned, double retro-reflector design
Cable: CIR (chalcogenide) fibers
Cable range: 1 μm – 6 μm
ARCoptix FT-MIR (2-12) Rocket Spectrometer
Mid-Infrared spectrometer
Wavelength range: 2 μm – 12 μm
Signal: > 1:40,000 noise
Interferometer type: permanently aligned, double retro-reflector design
Cable: PIR (polycrystalline) fiber
Cable range: 3 μm -17 μm
Neospectra Scanner
Near-Infrared spectrometer
Wavelength range: 1.35 μm – 2.50 μm
Portable FTIR spectrometer
Resolution at λ = 1,550 nm: 16 nm
IP65 ingress protection
Detector: InGAs photodetector
Retsch Mixer Mill 200
For size reduction, mixing, homogenization, cell disruption
Digital setting of vibrational frequency: 3 Hz – 30 Hz (180 – 1800 min
-1
)
Material feed size: <=8 mm
Final fineness: ~ 5 µm
No. of grinding stations = 2
Retsch Mixer Mill 500 VARIO
For size reduction, mixing, homogenization, cell disruption
Digital setting of vibrational frequency: 3 Hz – 35 Hz (180 – 2100 min
-1
)
Material feed size: <=8 mm
Final fineness: ~ 5 µm
No. of grinding stations = 6
METER SATURO Infiltrometer
Fully automated
Portable
Real time Ksat value calculation/ graphs
Integrated UV-VisNIR-MIR Scanning Chamber
Developed in APSS lab
Handle both intact and powder samples
Wavelength range: 250 nm – 6,000 nm
No. of integrated spectrometers: 3
Minimum background wave reflectance
Giddings Probe
#25-SCT model HDGSRPST
Hydraulic soil sampling, coring, and drilling machine
Powered by 35 HP Briggs and Stratton 2-cylinder air-cooled gas engine
Rotary head: 0-190 rpm (adjustable) and 1100 ft lbs torque
Master cylinder: 12000 lbs down force @ 1.1 ft/s and 7500 lbs pull force @ 1.72 ft/s