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Receive satellite TV signals.
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Compact Inverted Microscope, 1mm Field Of View
Viewing transparent samples from below in a Petri dish, flask, well plate or cavity slide. The microscope is compact and can be put inside most incubators to view experiments without opening the door. Time-lapse images can be saved and viewed remotely.Ideal for use as a Bench Microscope in teaching applications.
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L Band Satellite over Fiber
Transport L Band signals from Satellite Dish to Receiver over Fiber Cable
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Thermal Microscope Stage
TS-4MP
With our TS-4MP Thermal Stage, a specimen on a microscope slide or culture dish can be maintained at any temperature between -20°C and +60°C. Setup is easy, takes little time, and the controller will regulate the stage temperature to within +/-0.1°C
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Thermal Microscope Stage For Large Petri Dish
TS-4LMP
Thermal Microscope Stage For Large Petri Dish
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Thermal Microscope Stage For Petri Dish
TS-4SMP
With our TS-4SMP Thermal Stage for Petri Dish, a specimen on a microscope slide or culture dish can be maintained at any temperature between -20°C and +60°C. Setup is easy, takes little time, and the controller will regulate the stage temperature to within +/-0.1°C. The collar on the stage is designed to accommodate a 35mm 'Nunc' petri dish. The collar may also be removed for use with slides.
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Mini Appliance Checker
880 AT
Standard Electric Works Co., Ltd
● The 880 AT is a simplified Version of an appliance tester which use low voltage and low current to perform it's checks.● Application Example The appliance is plugged into the mini appliance checker, then the probe make contact with the protective conductor.● Other appliance checking Washing Machine Toaster Iron Dish Washer Stove
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Cassegrain Antennas
In telecommunications and radar, a Cassegrain antenna is a parabolic antenna in which the feed antenna is mounted at or behind the surface of the concave main parabolic reflector dish and is aimed at a smaller convex secondary reflector suspended in front of the primary reflector. The beam of radio waves from the feed illuminates the secondary reflector, which reflects it back to the main reflector dish, which reflects it forward again to form the desired beam. The Cassegrain design is widely used in parabolic antennas, particularly in large antennas such as those in satellite ground stations, radio telescopes, and communication satellites.
