Documents / Hearing transcript
This NICAP extract reproduces the statement of Dr. Robert M. L. Baker, Jr., a Computer Sciences Corporation scientist and UCLA engineering faculty member, to the House Committee on Science and Astronautics symposium on unidentified flying objects on July 29, 1968. Baker reviews his analyses of the Utah, Montana, Venezuela and Vandenberg films. He argues that current radar and optical sensors are poorly suited to detecting anomalistic phenomena and urges a well-funded, long-term interdisciplinary research program. The extract ends with panel discussion including Hynek and Hall.
“UFO Research Society”2 pages
4. Markowitz, William, letters dated November 10 and December 6, 1967. According to Markowitz the panel consisted of H. L. Robertson, L. Alvarez, L. V. Berkner, S. A. Goudsmit, and T. W. Page. 5. Ruppelt, E. J., The Report on Unidentified Flying Objects. (Doubleday & Company, Inc., Garden City, New York, 1956), pp. 286 to 288 and p. 292. 6. The maximum speed (achieved during a dive) of the F-94 is 602 mph, its landing speed is 130 mph, and its stalling speed is 108 mph. 7. McKinley, D. W. R., Meteor Science and Engineering, (McGraw-Hill Book Company, New York, 1961), page 128. 8. Baker, Robert M. L., Jr., "Future Experiments on Anomalistic Observational Phenomena," J. Astronaut. Sci. XV, No. 1, January-February, 1968. [[182]] The Journal of the Astronautical Sciences Vol. XV, No, 1, pp. 44 - 45 Jan.-Feb., 1968 Future Experiments on Anomalistic Observational Phenomena The requirement for additional experiments in the area of anomalistic phenomena is given, based upon the paucity of "hard data"; relevant data collected by astronomers, meteoriticists, and meteorologists, which would be either overlooked or not detected; and the possible "filtering" and/or "editing" out of pertinent data by our various space surveillance systems prior to its evaluation. An experiment involving two cameras slaved to a detection radar is outlined broadly and it is concluded that such a system should be constructed for use in meteoritic, meteorological, astronautical, psychological, and "UFO" study programs. The majority of our astronomical equipment (e.g., conventional photographic telescopes, Baker-Nunn cameras, meteor cameras, Markowitz dual-rate Moon Cameras, etc.) are special-purpose by their very nature and would probably not detect the anomalous luminous phenomenon reported by the casual observer if it were indeed present. Their photographic speed, field of view, etc. put definite limits on their capability to collect data on objects other than those for which they have been specially designed. Even if such data WCPP collected, the recognition of their uniqueness or anomalous character by an experimenter is improbable. Examples abound in celestial mechanics of minor planets being detected on old astronomical plates that had been measured for other purposes and then abandoned. Tombaugh's discovery of Pluto from rather old astronomical plates in storage is a well-known example. The space surveillance systems are almost programmed to overlook anomalous data. Any hard-data arising from an object or manifestation that did not move on a nearly two-body orbit, had a low radar cross-section, or followed an erratic path would most probably be filtered out of the system by various data-editing, or data-weighting procedures [1], which are inherent in most of our sophisticated space surveillance systems. A representative space surveillance radar may have a beam width of 1/6° for detection and require accurate orbital information good to 0.01° for fine tracking. Needless to say, such radars often miss even well-known spacecraft and would be completely inadequate for "locking-on" to a hypothetical "UFO." To be sure, advanced radar systems are being developed for our missile defense systems, such as the ALTAR (ARPA Long-range Tracking and Instrumentation Radar), TRADEX (Target Resolution and Discrimination Experiments) and the phased array RESER (Re-entry System Evaluation Radar) system. Although they extend the field of view, they still are developed to filter out anomalous signals. As Cheettam [2] points out, "Power and aperture will be programmed after a learning measurement cycle to conserve and efficiently distribute available energy when and where (reentry) targets are estimated to exist." Not only are conventional sensors almost insensitive to anomalous data, but observations published by trained scientists, that could be hard-data records of anomalistic phenomena, are often too quickly categorized and then forgotten. The observation by Mohr [3] in a letter to Science in 1966 gave an account of a "most unusual fly" and described a very remarkable and almost bizarre event that might or might not have been ball lightning. The Tunguska event of 1908 may well have been a impacting comet [4] and is usually studied in the context of meteoritics [5], Similarly, the Canadian fireball procession of 9 February 1913 could have been an ephemeral natural satellite of the Earth [6] or it could have been something more involved. In most such cases, and as in also the situation in published UFO studies [7], [8], [10], information-rich hard-data of high quality are rather hard to come by. It therefore suggests itself that a special experimental program is in order. The scientific method usually dictates experiments in the face of anomalous data and, at the moment,
Hearing transcript, cited by the archive. The PDF is mirrored here; the original link is above. 68 pages are in the text index: search them above, or from the library's search.