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Wireless for CELT? (Or: An astronomer thinks about BSAC and BWRC) Marshall Perrin Ay 250 1 Why consider it? • CELT requires a tremendous number of sensors and actuators: • 6200 segment edge sensors • 3000 segment position actuators • Other sensors: temperature, vibration, wind speed, ??? • Lots of interesting technology is being developed at Berkeley currently • Berkeley Sensor and Actuator Center (BSAC) • Berkeley Wireless Research Center (BWRC) • So what, if any, potential benefits can be gained for CELT? Wireless Sensors for CELT 2 Wireless Sensor Networks BSAC microsensors • Current “macro motes”: • • • temperature, humidity, barometric pressure, light intensity, tilt and vibration, and magnetic field sensors all in a cubic inch package, including the bi-directional radio, the microprocessor controller, and the battery! 20 meter communication range one week lifetime in continuous operation, 2 years with 1% duty cycling • Future “Smart Dust” • Pack everything into ~ 1 mm3. • Power: batteries, solar, vibration? • Estimates of a few nW power, or a few nJ per bit transmitted Wireless Sensors for CELT 3 Powering Wireless Sensors • Batteries – low tech, easily available but limited lifetime • Solar – probably not feasible inside • Sunlight is .14 W/cm2, but internal light levels down a few orders of magnitude. Solar cell efficiency ~ 15%. Result: ~ 10 mW/cm2 • Local generation from ambient vibrations • http://www-bsac.eecs.berkeley.edu/publications/pdf/pub1027468961.pdf http://www2.acae.cuhk.edu.hk/~aml/iros2000/li-2.pdf • Electrostatic or inductive power generation • ~ 10-100 10 mW/cm3 Wireless Sensors for CELT 4 Potential Benefits for CELT • Reduced wiring complexity on the telescope • Ease of maintenance for segment replacement? • Reduced weight • Reduced needs for cable wraps • Increased capabilities from additional sensors • Additional diagnostic capability at minimal cost and added complexity Wireless Sensors for CELT 5 Potential Negatives • Increased technological complexity • These technologies still require further development, but should be more mature by the ~2010 timescale for CELT • Reduced Reliability • Interference with other systems • Wireless transmissions at 2.4 GHz • Optical communications lasers (do we really want signal lasers bouncing around the back of our telescope primary?) Wireless Sensors for CELT 6 The Problem: Actuator Power • The current segment actuator candidate design requires approximately 2 W per actuator. • This is far in excess of what can feasibly be provided by batteries or local generation, so at bare minimum we’ve got to run a power cable to every single segment. • Might as well run data cables in the same cable runs at low cost and low complexity? • But power distribution is much less complex than multiplexing 6000 incoming and 3000 outgoing signals, so maybe wireless can be of benefit after all. • Requires comparison of more detailed designs than are currently available. • Power needs of edge sensors not clear (~ .1-1 W?). Could this be reduced further? Wireless Sensors for CELT 7 Additional possibilities • Distribute many temperature sensors throughout telescope and dome to measure dome seeing • Locate and track sources of heat inside the enclosure • Low duty cycle so can get substantial battery lifetimes • Vibration sensors for diagnostic purposes • Watch bearings for frequency signatures indicating immanent failures • Humidity sensors for operating conditions • Better knowledge of whether it’s safe to open the dome Wireless Sensors for CELT 8 An additional driver for low power… • 6 kW spread over the primary mirror due to the 3000 actuators, plus whatever the 6200 edge sensors use • For dry air at 0 degrees C on Mauna Kea, 6 kW will heat air at a rate of 8.3 m3/s/K • Or, spread over the 706 m2 area of CELT, that’s 1.2 cm3 heated by 1 degree per second per cm2 of mirror… • That can’t be good for dome seeing! (Particularly given as in reality it won’t be evenly distributed) Wireless Sensors for CELT 9