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Optical SETI Survey - Ground-Based and DaylightOptical SETI (Part F)Radobs 7FVersion 1.0 1. Optical SETI is best done in space, and probably has a higher chance of success if space-based. The costs given below are very approximate. Do you think that one or more observatories should be built? The following options are available, depending on mankind's commitment and depth of his wallet (tick off the one that you would prefer): (a) A large second-generation Space Telescope at a cost of about $10 billion, possibly associated with Space Station Freedom. (b) Two purpose-built ground-based Optical SETI Observatories, one in the northern and one in the southern hemisphere, at a total cost of about $200 million. (c) The recommissioning of large ground-based telescopes for Optical SETI that have been previously decommissioned because of severe light pollution effects, at a cost of about $20 million per telescope. (d) Adapting existing telescopes and telescopes yet to see first light, so that they can be shared with Optical SETI activities, with SETI activities being largely relegated to the daytime. This might also be done at a cost of about $20 million per telescope. YES DON'T KNOW NO 2. I have suggested that FIBERDYNE OPTOELECTRONICS & OSU propose to NASA, NSF and/or to some private philanthropic organization, to fund a project that will develop the receiving and signal processing technology for a prototype Optical SETI Observatory. This might well be much smaller than the observatories indicated above. The optical receivers may use heterodyne techniques and PIN photodetector arrays, or tunable high-Q Fabry-Perot filters with photon-counting arrays. Do you think that proposing a series of Optical SETI research and development programs would be sensible? YES DON'T KNOW NO 3. Do you think a prototype observatory would be useful for perfecting the technology? The prototype Optical SETI Observatory could be built around one of the following (tick off the one that you would prefer). Members of RADOBS may have a natural preference for (c), even considering the number of overcast days in Columbus. Remember, night- time light pollution should not affect SETI observations, and Perkins, outfitted with a new larger telescope, could be made available around the clock. There is plenty of room within the observatory dome to house all the needed equipment. It should be appreciated, that for most of the night-time observation periods, it will be possible to conduct conventional astronomy and SETI investigations simultaneously on the same part of the sky. The super high resolution light science spectral analysis capability of the telescope, will yield valuable new data about natural objects in the heavens. (a) The new Columbus Telescope, which is to be constructed on Mt. Graham in Arizona. (b) The decommissioned Mt. Wilson Observatory. (c) The Perkins Observatory, adjacent to OSU's "Big Ear" Radio Observatory. YES DON'T KNOW NO 4. At the present time, only one of the two 8 meter diameter mirrors for the new Columbus Telescope has been paid for. Do you think it a reasonable suggestion that if Optical SETI could make use of this telescope, that it might also fund the second mirror? YES DON'T KNOW NO 5. In the visible spectrum, dye lasers look very promising for very coherent, easily tunable local-oscillator heterodyning sources. Companies like Coherent & Spectra-Physics manufacture these highly coherent tunable dye laser systems. For example, the Coherent Model 899 Dye Laser can be made to function over the visible and near- infrared 380 nm to 1100 nm wavelength band with single-mode linewidths as small as 10 kHz, and powers > 200 mW. The cost of such a system with a high-power Ion Laser pump, is likely to be of the order of $200,000. Do you think such a laser has merit for Optical SETI receivers? YES DON'T KNOW NO 6. Are you an amateur (optical) astronomer? YES DON'T KNOW NO 7. If the answer to the above question was YES, it may be possible for you to get involved with Optical SETI in the visible spectrum in an amateur way. I would warn, however, that some sophisticated and expensive equipment will be required at the receiving end of the telescope. It could be done without (dye) laser local-oscillators and photon-counting arrays, though a "poor man's" incoherent approach would require the minimum of a high-Q Fabry-Perot interferometer spectrum analyzer and a single photon-counting receiver. A complete Burleigh CF-500 Confocal Etalon Fabry-Perot system operating over the wavelength range 400 - 1400 nm with up to 1.2 MHz resolution, costs about $13,000. Each mirror set, which has a bandwidth of about 100 nm, costs about $1,300. Alternatively, the Burleigh HiFASE Etalon System can operate over the wavelength region 450 - 1800 nm, with a maximum resolution of < 15 MHz, and costs about $ 25,000. This bandwidth is compatible with the maximum bandwidth requirement for satisfactory daylight optical SETI. Each mirror set for this system, which covers a bandwidth of about 60 nm, costs about $2,000. Initial wavelengths and mirror sets selected would be based on known laser or Fraunhofer lines. Other optical filters or spectrographs would be required in order to pre-filter the light and overcome problems caused by the Free Spectral Range properties of Fabry-Perot interference filters. Newport Corporation makes a cheaper system called the SR Series (465 - 1550 nm), which has a 1.2 MHz passband with a 63% throughput, and costs about $7,500. A single photon-counting detector system would cost about $2,000. In reality, you would have to be a fairly rich "poor-man", and considering the flexibility of the laser heterodyne approach and no requirement for a photon-counting array, it could be argued that the laser approach is by far the best, albeit somewhat more costly! The cost of the hardware not withstanding, would you be interested in amateur Optical SETI? YES DON'T KNOW NO Score out of 7: YES = DON'T KNOW = NO = January 1, 1991 RADOBS.07F BBOARD No. 299 * * * * * * * * * * * * * * * * * * * * * * * * * * * * * * * * * * * * * * * Dr. Stuart A. Kingsley Copyright (c), 1991 * * AMIEE, SMIEEE * * Consultant "Where No Photon Has Gone Before" * * __________ * * FIBERDYNE OPTOELECTRONICS / \ * * 545 Northview Drive --- hf >> kT --- * * Columbus, Ohio 43209 \__________/ * * United States .. .. .. .. .. * * Tel. (614) 258-7402 . . . . . . . . . . . * * skingsle@magnus.ircc.ohio-state.edu .. .. .. .. .. * * CompuServe: 72376,3545 * * * * * * * * * * * * * * * * * * * * * * * * * * * * * * * * * * * * * * *
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