Copyright Resonance Ltd., December 2011 143 Ferndale Drive North, Barrie, ON L4N 9V9       Tel: 705-733-3633         Fax: 705-733-1388      Email:sales@resonance.on.ca 
Contact us for more information Home Products Services Downloads Library Heritage Contact
24W RF-Powered Light Sources Manual Page 2
Appendices Specifications for Hydrogen and Deuterium Light Sources HHeLCMM-L, DHeLCMM-L The Hydrogen or Deuterium Light sources comes standard with everything needed to produce VUV radiation in the 110 to 200 nm region. A heater on the light source bulb generates H2 or D2 in the light source. This allows the user to operate the light source at low H2/D2 levels for an “optically thin” Lyman-Alpha line or a multiple-lined H2 or D2 spectrum in the 110 to 165 nm region and a continuum between 165 and 375 nm. Continuously variable heater temperature setting that allows: o “Optically thin” source of Lyman-Alpha radiation (121.6 nm) or with heater adjustment a broadband VUV UV light source with output from 112 to 400 NM. o Hydrogen/Deuterium spectral output from 112 to 6000 NM. Air-cooled, optically stable (Typically < 1% drift per hour) Longer lifetime than most available Lyman-Alpha sources owing to an internal source of hydrogen Breakout box for RS-232 telemetry, BNC modulation input (if equipped), power switch, and USB interface for interface software (see software manual) “Smart Light Source” software allows for precise control and monitoring of light source parameters (heater, RF power etc.) o Visible NIR source emission intensity graphing and logging for tracking source stability. o Temperature and RF power logging and graphing via graphical chart-recorder interface o  Excel-friendly .csv output format for data saving Hydrogen Light Source VUV and UV Output Spectra Lamp spectrum with Heater set to 45 C Heater set to 60 C Hydrogen Light Source VUV and UV Output Spectra Heater Set to 60C UV Spectrum D2 Spectrum with VM300 monochromator at 1 Ang. Resolution General Specifications for all Rare-Gas LIght Sources Models ArLL-L, KrLM-L, XeLM-L, KrLM-LDQ12, XeLM-LDQ12, ArCM-L, KrCM-L, XeCM-L Rare Gas Light Sources The Resonance Argon Krypton and Xenon Rare Gas Light source comes standard with everything needed to produce VUV radiation in the 110 to 200 nm region. They employ RF-excited bulbs with Magnesium Fluoride windows in EMI shielded enclosures.   The line sources are filled to a few Torr and emit narrow emission lines in the VUV.  The continuum sources are filled to 30 to 400 Torr Ar, Kr or Xe and emit both lines and continua in the VUV (see spectra below). Air-cooled, optically stable (Typically < 1% drift per hour) Longer lifetime than most available Rare gas sources sources owing to an internal source getters and “hard seal windows”. Breakout box for RS-232 telemetry, BNC modulation input (if equipped), power switch, and USB interface for interface software (see software manual) “Smart Light Source” software allows for precise control and monitoring of light source parameters (heater, RF power etc.) o Visible NIR source emission logging and graphing for tracking source stability. o Temperature and RF power logging and graphing via graphical chart-recorder interface o Excel-friendly .csv output format for data saving General Specifications for all Rare-Gas Light Sources Models ArLL-L, KrLM-L, XeLM-L, KrLM-LDQ12, XeLM-LDQ12, ArCM-L, KrCM-L, XeCM-L Calibration of Krypton Source Lamp SN 679 Typical Spectra KrCM-L XeLM-L XeCM-L HgArLQ-L
View Next