115 lines
6.7 KiB
Plaintext
115 lines
6.7 KiB
Plaintext
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SUBJECT: SETI OPTICAL SEARCH BEST ? FILE: UFO1001
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PART 1
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SETI How and Where?
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Copying or reprinting of the EJASA, in part or in whole, is
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encouraged, provided clear attribution is made to the Astronomical
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Society of the Atlantic, the Electronic Journal, and the author(s).
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Opinions expressed in the EJASA are those of the authors' and not
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necessarily those of the ASA. This Journal is Copyright (c) 1993
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by the Astronomical Society of the Atlantic, Incorporated.
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CONFERENCE PREVIEW
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THE SEARCH FOR EXTRATERRESTRIAL INTELLIGENCE (SETI)
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IN THE OPTICAL SPECTRUM
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by Dr. Stuart A. Kingsley
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Fiberdyne Optoelectronics, Columbus, Ohio
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From the author of the January 1992 six-part EJASA (THE ELECTRONIC
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JOURNAL OF THE ASTRONOMICAL SOCIETY OF THE ATLANTIC) article (Vol. 3,
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No. 6A-6F) on Optical SETI (OSETI).
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The author would like to acknowledge that this Electronic Journal
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has been instrumental in the organization of this conference, for
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without last January's publication, this author would not have been
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invited by SPIE to put this conference together.
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You are encouraged to remail this material to anyone you know with
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interests in SETI or to print it out and pin it up on your astronomical
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society, company, faculty, or school notice board. Some of the
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following material was featured in the October 1992 issue of EJASA
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(Vol. 4, No. 3) and the December 1992 issue of SPIE's OE REPORTS:
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Almost three years ago I began "lobbying" the scientific community
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to reconsider the optical approach to the electromagnetic search for
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extraterrestrial intelligence (SETI), first described by Nobel laureate
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Charles Townes (1964 - masers/lasers) in 1961. Unfortunately, many of
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the strongest proponents for electromagnetic SETI have become dogmatic
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and will not countenance open discussion of alternatives to microwave
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SETI, believing that the issue of the relative efficiencies of microwave
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and optical SETI was settled years ago in favor of microwaves. Optical
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SETI has received very poor press ever since the skewed ETI laser
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transmitter assumptions in the Project Cyclops report, two decades ago.
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This NASA design study report described a microwave array consisting of
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up to nine hundred 100-meter diameter dishes which if fully built would
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have occupied an area 6.4 kilometers in diameter and cost, in 1970s
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currency, some ten billion dollars. This grand project was never fun-
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ded but the report itself has had a profound effect on SETI thinking.
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In the comparison table that appeared on page 50 of that report, the
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optical system modeled described an interstellar laser communication
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system that employed a 1.06 micron Nd:YAG laser, and a 22.5 cm diameter
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transmitting telescope. There were various reasons for limiting the
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aperture of the ETI transmitter. One reason arose out of unnecessarily
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constraining both parts of the system to operate on a planetary surface,
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within an atmosphere, and thus be limited by the atmospheric coherence
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cell size. Another reason was to avoid the production of beams that
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were smaller than the zones of life around nearby targeted stars.
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However, the net effect was to cripple the potential very high Effective
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Isotropic Radiated Power (EIRP) of the optical transmitters.
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It would be far better to build larger transmitting telescopes and
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defocus them when targeting nearby stars, if, in the unlikely event,
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the ETI civilization did not possess the technical prowess to aim narrow
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beams into nearby stars. In this way, the long-range EIRP would not be
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unnecessarily degraded. The modeled "toy" ETI uplink telescopes put
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the onus on the young and technically immature receiving civilization
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(humanity) to build very large and expensive telescopes to receive weak
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signals from mature ETI civilizations, instead of the converse. It
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was this part of an otherwise excellent report that so distorted its
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conclusions concerning the efficacy and relative cost (to us) of the
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optical approach to SETI.
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If we allow for transmitting and receiving apertures to be 10 meters
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in diameter or larger, it can be shown for transmitter powers comparable
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to those for microwave systems that relatively small diffraction-
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limited laser systems are capable of supporting far higher signal-to-
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noise ratios and data rates than the much larger microwave systems. The
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extremely high gains of optical antennas more than make up for the
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additional quantum noise and stellar background radiation noise. The
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lack of (currently) easily identifiable "magic optical frequencies",
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equivalent to the microwave waterhole between 1.420 and 1.662 GHz, save
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for the major CO2 transition at 10.6 microns, is not a reason to
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conclude that ETIs would not use lasers to signal Earth. Indeed, the
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effectiveness of pulsed laser signals is so high that there is less
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need to be concerned about the exact laser frequency.
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Indeed, from the viewpoint of communications with extraterrestrial
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intelligences (CETI), which is not presently being proposed, terrene SDI
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lasers of the late Twentieth Century are certainly capable of "reaching
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out and touching ETIs" across one thousand or more light years. The
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problem today is that we do not know where to point our lasers and we
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lack the means to provide precise forward predictive targeting of
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extrasolar planets. Even more basic to this problem is that direct
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visual observations of other planets around nearby star systems await
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the technological developments of the next century. In the meantime,
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we must take the passive and perhaps safer approach of listening for
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ETI signals.
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Let it be noted here that the word "optical" is used in a manner
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familiar to optoelectronics (photonics) engineers and scientists, as
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an umbrella term. It is a superset of both "visible" and "infrared."
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The word "optical" is not to be taken as being synonymous with the word
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"visible", since the former (for communication engineers) covers all
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electromagnetic frequencies from the far-infrared to the ultra-violet.
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**********************************************
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* THE U.F.O. BBS - http://www.ufobbs.com/ufo *
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**********************************************
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