Showing results: 16 - 20 of 20 items found.
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Apollo 1.0 -
Labino AB
Labino’s Apollo 1.0 Radiometer/Photometer is an instrument for ACCURATE measurement of UV-A irradiation and visible illumination. Extra engineering effort is taken to make an accurate measurement of visible light emission from a UV-A lamp by incorporating a su-perior band pass filter stack containing only non-fluorescent filters. The instrument pro-vides fast measurement as it offers auto ranging and concurrent measuring of visible light and UV-A irradiation. Apollo 1.0 is traceable to NIST (USA’s National Institute of Standards and Technology). - See more at: http://labino.com/portfolio_item/labino-uv-meter/#sthash.yzHXJamq.dpuf
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Signals & Systems India Private Limited
In order to implement a 100 % stator earth fault protection based on subharmonic injection, a 20Hz voltage is injected into the generator star point. The 20-Hz generator SGEN-1001 is used in combination with the Band Pass Filter SBPF-1001 in the Stator Earth fault protection. The injection can be performed by connecting the SGEN-1001 and the SBPF-1001 to the load resistor of an earthing or neutral transformer. If an earth fault occurs in the generator star point, the 20 Hz voltage drives a current through the fault resistance. From the driving voltage and the fault current, the protective relay determines the fault resistance.
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Pulse Electronics
Pulse’s complete offering of LTCC based Band Pass Filters, Balun’s, Diplexer’s and Couplers used in conjunction with our wireless antenna products will enhance your devices performance keeping attenuation and noise to a minimum. Many of Pulse’s IPD components are already qualified or referenced on various radio designs, so please contact us about the components already qualified on the radio you are using. From Wifi Networking devices, to smart phones and tablets, Pulse’s offering of IPD Components has you completely covered. Using the table below you can search our complete IPD Component offering.
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LM-AS -
Eddy Co.
The short light source is compatible with the LM-101 or the LMC-20. The light is supplied with a 50 watt tungsten halogen convection cooled light source which provides suffcient energy for use with narrow band pass filters or monochronomators in the wave length range of .35 to 2.5 microns. The light beam is chopped at 200 hz by a quiet, vibration free, synchronous motor. The housing also contains a secondary LED light source and detector for synchronization of the amplifier, plus an electro-mechanical shutter to block the light output when the instrument is zeroed. An internal collimating lens produces a narrow beam (<1") so the LM-AS can be used in bell-jar and large coating systems.
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LM-A -
Eddy Co.
The long light source is compatible with the LM-101 or the LMC-20. The light is supplied with a 50 watt tungsten halogen convection cooled light source which provides suffcient energy for use with narrow band pass filters or monochronomators in the wave length range of .35 to 2.5 microns. The light beam is chopped at 200 hz by a quiet, vibration free, synchronous motor. The housing also contains a secondary LED light source and detector for synchronization of the amplifier, plus an electro-mechanical shutter to block the light output when the instrument is zeroed. An internal collimating lens produces a narrow beam (<1") so the LM-A can be used in bell-jar and large coating systems.
