Walesville-Westmorland (New York), . Météo : temps apparemment clair. Les signalements du 1er juillet 1954 arrivèrent au Dépot AF de Rome (New York), à propos d'un ovni ayant l'apparence d'un ballon. L'officier en charge dit croire qu'il s'agissait d'un ballon partiellement dégonflé, et que s'il était encore là le jour suivant, il déclencherait une enquête.
A le 2 juillet 1954, le F-94C 51-13559 décolla pour une mission d'entraînement de routine. Le GCI demanda à l'appareil de change sa mission pour intercepter un appareil inconnu à 10 000 pieds. Le pilote identifia un appareil C-47 par son marquage de queue, et il lui fut alors demandé de vérifier un second appareil non-identifié qui se était à basse altitude et apparently letting down pour atterrir à la base aérienne de Griffith. Le rapport de la FA indique :
Alors que le pilote commençait une descente, il remarqua que le température du cockpit augmenta brusquement. L'augmentation de température amena le pilote à scruter les instruments. La lumière d'alarme incendie était allumée et le pilote informa l'observateur radar de ce fait. La lumière d'alarme incendie resta allumée après que les gaz aient été mis sur "ralenti" et donc moteur fut arrêté et l'équipage s'éjecta avec succès.
L'appareil s'écrasa à "l'Intersection de Walesville" et fut détruit. L'appareil toucha une maison et une automobile, blessant mortellement 4 personnes.
Le récit ci-dessus est tiré du rapport d'accident officiel de l'USAF ("Résumé des circonstances"). Il n'existe pas de dossier Blue Book parce qu'aucun ovni ne fut impliqué.
Conclusion :
Wright-Patterson AFB, Ohio, août 1952, . Météo : nuages épars à 25 000 pieds. This case, occurring almost over Project Blue Book's home base, is a very good example of confusion or contradictory evidence tending to obscure the true nature of a UFO incident.
At 1051 LST an unidentified radar track appeared 20 mi. NNW of Wright Patterson AFB on the 664th AC&W Squadron's
GCI radar at Bellefontaine. The radar operator stated that the course was 240° at 400 knots. Elsewhere the report
states 450 knots; how he determined this is not made clear. Two F-86 aircraft from the 97th Fighter-Interceptor
Squadron, Wright-Patterson AFB, were vectored in and made visual contact at
1055 LST. Fighters stayed with the object until 1113 LST. The F-86s climbed to 48,000 ft., fell off, and made a second
climb. One aircraft had airborne radar activated and received a "weak" return. The object was described as "silver in
color, round in shape," and its altitude was estimated as 60,000-70,000 ft. The object appeared on the radar gunsight
film as a "fuzzy, small image ... with discernible motion ... that could be any darn thing
."
In this incident it is apparent that
All of the evidence points to a weather balloon except for the 400-450 knot speed, and the 240° flight path, which is against the prevailing upper winds. Known aircraft were ruled out because of the altitude. A U-2 would "fit," but the first one was not flown until 1955, and the visual appearance was all wrong. The radar returns eliminated astronomical objects, mirage was ruled out because of the high angles, and the sighting occurred "above the weather." The conclusion was: unknown.
However, buried deep in the report was the radar operator's note that At the time it was dropped
() object was 5 miles northwest of Springfield, Ohio
." This allows the UFO's course to be
plotted on a map; Figs 18 and 19, shows such a map plot. It is readily apparent from this that the UFO's true heading
was about 111° at an average speed of only 44 noeuds. Apparently no one thought to make this simple check. Since the
highest reported winds from the radiosonde launched at Dayton at were 260°/31 noeuds at 50 000
pieds and 270°/33 noeuds at 55 000 pieds the plotted track of the UFO is consistent with the observed upper winds. The
blip was first "painted" at a 240° azimuth, which may explain where that quantity originated in the UFO movement
report.
Conclusion: almost certainly a weather balloon. Note that the winds reported for the Wright-Patterson AFB 10:00 LST show winds blowing first from the east, then from the SSE, ultimately from the west at higher altitudes. These winds were blowing in such a manner that it is conceivable that Wright-Patterson's own radiosonde balloon may have been the UFO in this incident.
Near Charleston, W. Va., mai 1966, . Weather: Severe thunderstorms in area. Pilot of a Braniff Airlines Boeing 707 flying at 33 000 pieds observed on his left side what appeared to be a fast-flying aircraft with landing lights. Braniff's airborne radar recorded this unknown. Pilot requested the radar operator at Charleston sector of Indianapolis ARTC to look for traffic at his 8:30 or 9:00 position, and the radar picked up a track in this position. Return made a sweeping turn and disappeared off scope to the southwest.
An American Airlines pilot flying 20 miles behind the Braniff plane saw the object. It appeared to him to be a normal aircraft with landing lights. This pilot stated he had often seen such aircraft with lights during AF refueling missions.
Estimated speed of the unknown was 750-800 miles/h. No unusual maneuvers were performed or any that were beyond known military aircraft capabilities at the time. AF explanation is that the unknown was an aircraft with landing lights on. This is consistent with the reported facts.
Lakenheath (Angleterre), - août 1956, . Météo : globalement claire jusqu'à (pour les détails voir la section 4).
La probabilité qu'une propagation anormale de signaux radar puisse avoir été impliquée dans ce cas semble être faible. 1
ou 2 détails suggèrent une PA, en particulier la disparition rapportée de la première piste alors que l'ovni semblait
survoler le radar GCA de Bentwaters. A nouveau cela doit être soupesé avec la déclaration du contrôleur de Lakenheath
selon laquelle il y avait peu ou pas de traffic ou de cibles sur l'écran
, ce qui ne suggère pas du tout des
conditions de PA, et le comportement de la cible près de Lakenheath — apparemment continu et suivi sans difficulté. Le
"tailing" du chasseur de la RAF, à lui seul, semble indique la possibilité d'une image fantôme, mais ceci n'est
pas en accord avec le rapport selon lequel l'ovni arrêta de suivre le chasseur, alors que ce dernier retournait à sa
base, et partit dans une direction différente. Les opérateurs radar furent apparemment prudents pour calculer la vitesse de
l'ovni d'après les distances et heures estimées, et les vitesses furent rapportées comme étant cohérentes de course en
course, entre les épisodes stationnaires. Ce comportement serait relativement cohérent avec les réflexions depuis des
couches atmosphériques — mais pas dans tant de directions différentes.
Un mirage visuel à Bentwaters semble être hors de question en raison des observations combinées au sol et en l'air ; le pilote de C47 a apparemment vu l'ovni sous lui. Les objets visuels ne semblent pas avoir été des météores ; les déclarations d'observateurs selon lesquelles les météores étaient nombreux impliquent qu'ils étaient capables de différencier l'ovni de météores.
En résumé, il s'agit du cas plus intriguant et inhabituel des dossiers radar-visuels. Le comportement apparemment rationnel, intelligent de l'ovni suggère un appareillage mécanique d'origine inconnue comme l'explication la plus probable de cette observation. Cependant, au regard de la faillibilité inévitable des témoins, des explications plus conventionnelles de ce signalement ne peuvent être totalement exclues.
Sault Saint Marie, Michigan, 11-12 septembre 1967, . Météo : claire, plafond illimité, visibilité illimitée (au-delà de 20 miles), pas d'orages dans cette région, vent de surface de 140°/4 noeuds, en haut de 240°-270°/15-35 nœuds. Le profil de réfractivité radio de Sault Saint Marie pour l'heure la plus applicable est montré en figure 21.
This is a good example of moving radar targets that cannot be seen visually, where there is a "forbidden cone" over the radar site. Some of the returns were even seen to approach within 5-15 mi. of the radar and disappear, apparently subsequently reappearing on the other side of the radar scope at about the same range that they disappeared. This sort of behavior is symptomatic of AP-echoes.
The meteorological data tend to confirm this interpretation. The refractivity profile shown in Fig. 21 displays three peculiarities: a strong subrefractive layer at the surface, a strong elevated duct at 325-520 m (about 1100-1700 pieds) and a super-refractive layer at 1070-1360 m. (about 3500-4500 pieds). A ray-tracing is shown for this profile in figure 20. The ray shows noticeable changes in curvature as it passes through the different layers, an indication that strong partial reflections would be expected. With this profile, moving AP-echoes, produced in the manner described by Borden and Vickers (1953), could be expected to appear at apparent heights of between 2000-3000 pieds and 7000-9000 pieds. No height information was supplied with this report, so the calculation above cannot be verified.
In summary, it appears that this is a case of observations of moving AP-echoes produced by unusually well stratified atmospheric conditions.
Golfe du Mexique, Coast Guard Cutter "Sebago," 25"47'N 89° 24'W, novembre 1957, 05:10-15:37 LST. Météo : non fournie, mais apparemment quelques nuages dans la zone. The most applicable radio refractivity data available are for Key West (Floride). et , 5 novembre 1957. They are shown in Figs. 22 and 23. One visual and three radar objects were included in this case. The ship's heading was 23° true. The first contact was a radar blip picked up at at 290° true azimuth, 14 miles. It moved south, approached the ship within 2 mi., and returned north along ship's port side. Contact was lost at . Average speed of this UFO was calculated as 250 miles/h. At 05:16 LST a new blip was picked up at 188°, 22 mi.; this target departed at a computed 650 mph., disappearing at at 190°, 55 mi. The third radar target was acquired at at 350°, 7 mi.; it appeared to be stationary. While the third radar target was being watched on the scope, a visual object was observed for about 3 sec. at 05:21 LST travelling from south to north at about 31° elevation between 270° and 310° azimuth. The third radar target remained stationary for about 1 min. and then slowly moved to the northeast, finally accelerating rapidly and moving off scope at 15°, 175 miles.
The visual object was described as "like a brilliant planet;" it was undoubtedly a meteor, and in any event obviously was unrelated to radar target number three, the only radar target visible at the same time.
The radar targets were, with the possible exception of the first one, erratic and unpredictable in their movements. Les 2nd et 3ᵉs blips radar appeared suddenly, well within the normal pick-up range of the ship's radar. Ces 2 blips were probably caused by anomalous propagation. The two Key West profiles, although taken at some distance from the ship's position, are indicative of rather unusual atmospheric conditions in the area. Indeed, the profile is probably one of the most unusual radio refractive index profiles that has ever been observed. The atmospheric structure was apparently one of alternating very wet and very dry layers. Patterns of this sort are often very stable in these subtropical latitudes, and tend to extend in rather homogeneous form over large horizontal distances. The ray-tracing of this profile, Fig. 23a, shows even greater changes in ray curvature. Strong partial reflections should be expected under these conditions.
The first radar target behaved generally like an aircraft, and the AF investigators were of the opinion that it was an aircraft, probably from Eglin AFB to the north.
In summary, the weight of evidence points toward anomalous propagation as the cause of the radar echoes, the first possibly being an aircraft. The visual object was apparently a meteor.
Coincidentally, the ship, SS Hampton Roads, at 27° 50'N 91° 12'W sighted a round, glowing object high in the sky that faded as darkness approached at . This object appeared to move with the upper winds. AF investigators concluded that it was in all probability a weather balloon.
Canal Zone, novembre 1952, . Météo : temps globalement clair,
quelques nuages épars, plafond et visibilité illimités, la visibilité à 2000 pieds était de 50 miles. Radio
refractivity profiles for Balboa, 1000 and 25 November 1952, are shown in Figs. 24 and 25. Two
unidentified objects were tracked by gun-laying radar during the period . These objects,
never present simultaneously, could have represented two tracks of the same object. The radar returns were described
as "firm and consistent
," and the objects were said to maneuver in a "conventional manner
" at an average
speed of 275 knots. Apparently the track speeds were as high as 720-960 miles/h at times. Two B-26s, a B-17, and a PBM
were scrambled but no radar or visual contact could be made with the unknowns. The UFOs were not spotted from the
ground, with the exception of a single report that an officer saw, low in the sky, an "elongated yellow glow
"
giving a soft light like a candle. It moved quickly, disappearing in the west in about 3 sec. There were scattered
clouds. It seems possible that this was the sighting of a meteor seen through thin clouds producing the soft,
yellow-glow effect. In any event, the description does not correspond with the simultaneous radar track of the first
UFO.
Avec une visibilité de 50 miles, il semble étrange que l'appareil envoyé n'ai put observer aucun des ovnis. Le rapport de la Force Aérienne commente :
It is believed that due to radar units being slightly off calibration and due to delay in communication, interceptors did chase their own tail or were sent to intercept themselves.
It is also believed that the majority of the radar plots were legitimate unidentified objects.
The preparing officer knows of no object which flies at 275 noeuds, that could remain in the Canal Zone area for nearly six hours, maneuver from 1000 through 28 000 pieds d'altitude, make no sound, and evade interception.
In fact, it is difficult to imagine any material object that could accomplish all these feats. The strange radar tracks were probably the product of anomalous propagation conditions, an hypothesis that would account for the facts above. The atmospheric conditions were certainly favorable for AP, as can be seen from the A-profiles in Figs 24 and 25. However, there are two considerations that argue against this hypothesis.
Despite these two contradictions to the AP hypothesis, the lack of any visual corroboration of the 2 ovnis makes any other hypothesis even more difficult to accept. This case therefore seems to fall, albeit inconclusively, into the classification of probable AP radar returns.
Colorado Springs, Colorado, mai 1967, 15:40 LST (16:40 MDT). Météo : couvert, froid, averses éparses et averses de neige (graupel) dans le secteur, vents orientés nord d'environ 30 miles/h, rafales à 40 miles/h, visibilité air — plus de 15 miles (l'aéroport de Colorado Springs n'est pas limité par l'horizon ; des visibilités de 100 miles sont communément rapportées les jours clairs). Ceci est un cas uniquement radar, et est d'un intérêt particulier parce que l'ovni ne pouvait être vu, lorsqu'il y avait toute indication qu'il aurait dû être vu (voir section 4).
Du moment où l'ovni a été repéré pour la 1ʳᵉ fois au moment ou le vol Braniff a atterri sur la piste 35, la piste de l'ovni s'est comportée comme un écho fantôme, peut-être un retour du sol réfléchi depuis l'appareil. Ceci est indiqué par le fait que le blip de l'ovni apparût au double de la distance du blip de Braniff, et au même azimut, bien que l'angle d'élévation semble avoir été différent. Lorsque Braniff atterrit, cependant, la situation changea radicalement. Le blip de l'ovni tira vers la droite (l'est) et passa au-dessus de l'aéroport à une altitude indiquée d'environ 200 pieds. Comme indiqué par la FAA, ceci est précisément la procédure correcte pour un appareil en approche, ou un pratiquant une approche ILS mais n'ayant en fait pas l'intention d'atterrir. Bien que la trajectoire de l'ovni soit passée à moins de 1,5 mile de la tour de contrôle, et que le personnel présent ait été alerté de la situation, l'ovni n'était pas visible, même aux jumelles. Un vol de Continental Airlines, qui fut suivi 3 à 4 miles derrière l'ovni au 1er contact, et qui volait dans la même direction, ne le vit jamais non plus.
Les antennes transmettrices des radar PAR comme ASR sont situées à l'est de la piste 35, et elles sont à environ 1000 pieds éloignées de la ligne SO-NE. Un écho fantôme semble donc être exclu par au moins les considérations suivantes :
Les caractéristiques de vol au radar de l'ovni dans ce cas sont toutes compatibles avec l'hypothèse que l'inconnu était un jet de la série century (F100, F104, etc.), bien que rien n'ai jamais été vu ou entendu.
Ceci doit rester comme l'un des cas radar les plus intriguants connus, et aucune conclusion n'est possible à ce jour. Il semble inconcevable qu'un écho de propagation anormale se comporte de la manière décrite, en particulier concernant les changements d'altitude signalés, même si une PA était probable à ce moment. Au regard de la situation météorologique, il semblerait qu'une PA était plutôt improbable. A côté de cela, quelle est la probabilité qu'un retour de PA n'apparaisse qu'une seule fois, et à ce moment semble exécuter une parfaite approche d'entraînement ILS ?
Vandenberg AFB, Lompoc, Californie, 6-7 octobre 1967, . Météo : clair, bonne visibilité, fortes inversions de température près de la surface causées par une advection of very warm (80°-90°F), dry air over the cool ocean surface (water temperature 58°-59°F). This sighting begins with an apparent mirage (of a ship probably 60 miles beyond the normal horizon) and continues with a very large number of unknown targets that were found on tracking radars which were being used in a search mode (they normally are not used in this way). The project case file contains a good analysis of the probable nature of the radar targets, some of which were apparently birds and some apparently ships tracked at 80 mi. ranges as well as other AP-like returns that may have been associated with local intensification of the ducting layer. The nature of the visual objects is not as clear, although at least two of them appear to have been superior mirages of ships beyond the normal horizon. There were possibly some meteor sightings involved.
The meteorological conditions were quite interesting. The warm, dry air was apparently quite close to the water surface, at least in places. Data from Vandenberg and San Nicholas island indicate that in places the inversion was no thicker than about 90 m. (10 mb pressure difference). The contrast that may have existed can be calculated from these data:
A ou près de la surface de la mer | A 90 m ou moins | |
---|---|---|
Pression | 1004 mb | 994 mb |
Temperature °F | 58 °F | 90 °F |
Temperature °C | 14 °C | 32 °C |
Temperature °K | 287 °K | 305 °K |
Optical N (5570A) | 275 (ppm) | 256 (ppm) |
The optical refractive index gradient that may have existed at the time was therefore on the order of -210 ppm. km-1, or a somewhat greater negative value, depending upon the thickness chosen for the layer. The value above is computed as (256-275) /0,090, based on the 90 m. maximum thickness assumed. Since the critical value of the gradient for a superior mirage is -157 ppm. km-1, it is quite apparent that the conditions required for the formation of extended superior mirages were most likely present on the date in question. The only problem with this explanation is the reported elevation angle of 10°, but as pointed out in the conclusions to this chapter such estimates by visual observers are invariably over-estimated by a large factor.
In summary, the conclusions arrived at by the investigators in this case seem to be adequately supported by the meteorological data available.
L'observation signalée pour octobre 1967, , semble être un exemple classique de la description de l'image d'une étoile isolée et scintillante vue à travers une forte couche d'inversion. Notez particulièrement le ratio estimé des mouvements verticaux et horizontaux. 2 étoiles très brillantes auraient été proches de l'horizon à cette heure : Altair, de magnitude 0,9, aurait été à 277° d'azimut et environ 4° d'angle d'élévation ; Vega, de magnitude 0,1, aurait été à environ 313 ° d'azimut et environ 12 ° d'angle d'élévation. Des 2, Altair semble la cible la plus probable en raison de l'angle d'élévation plus petit ; les observateurs n'ont donné aucune estimation d'azimut ou d'angle d'élévation.