Click on the thumbnail at the bottom right of this page to go to the bitmap scan of this document. The text of this document appears immediately below.
THE ROYAL ASTRONOMICAL SOCIETY OF CANADA STANDING COMMITTEE ON OBSERVATIONAL ACTIVITIES Bulletin No. 3 METEOR SECTION THE GREAT LEONID METEOR STORM OF 1966 The Leonids have done it again! With practically all of Canada clouded out, and with many observers in the United States giving up too early, this unpredictable shower struck with the greatest intensity since 1833. In the western U.S., observers persevering after 3:00 a.m. Mountain Standard Time were rewarded with a display they never dared hope to see. Meteors kept arriving at a faster and faster rate, until the incredible value of 40 PER SECOND was reached at 5:00 a,m., LS.T. Of course, this was only an estimate - all recorders were in utter confusion before this occurred. Photographs taken in this period are covered with Leonid trails - one exposure recorded 43 in as many seconds. What a sight it must have beeni - read the accounts in "The Review of Popular Astronomy" (Jan/Feb-67) and "Sky and Telescrope" (Jan-67) and see what we missed! Mr. and Mrs. E.E. Bridgen, former stalwart observers in the Montreal Centre and now re- siding in Victoria, appear to have been the only ones in Canada to see anything of this meteor display, and they were badly hampered by clouds. Their report notes: "With 102 meteors in half an hour, there was little more than one observer - I was kept busy recording". METEOR SHOWERS OF LATE WINTER AND SPRING This is not a particularly good season for meteor observers. The weather is usually cold and/or cloudy and meteors few and far between. In fact, the strongest showers occur during the daytime and are observed only by radar techniques. Unless you are willing to accept an expensively high ratio of exposures per meteor, photography is not recommended durina this period. However, brilliant fireballs are just as likely to happen now as at other times. Of the night-time showers, only the two noted below have enough visual mete ors to emerge noticeably from the background of "sporadics". The LYRIDS (21-22 April) have a single observer hourly rate of 15. The diffuse radiant is dose to Vega (a. Lyra), and culminates (reaches its highest point in the sky) at 4:00 a.m. local time. Although a weak shower now, it was formerly much stronger, reaching a near-storm value in 1803. On the night of 21 April, 1922, the observed rate per hour was a miserable in the United Kingdom, but a magnificent 96 in Greece. Observing ccnditions will not be favourable this year - a full moon featuring a total eclipse occurs 2 days after the maximum. The k AQUARIDS (5-6 May) have a single observer hourly rate of 20. The radiant culminates at 7:00 a.m. local time- not a shower for those who like to retire early! Observing conditions will be favourable with the moon well past last quarter. This shower is thought to be associated with Halley' s Comet, as is the Orionid shower of 21 October. However, this cattaxy association is stifl in doubt as there are many uncertainties about the orbital characteristics of both showers. SUGGESTIONS ON SETTING UP A VISUAL OBSERVING STATION As more dust, smoke and light reach the skies above our cities, the selection of a site for a meteor observing station becomes difficult. It is necessary to accept less than perfect sky conditions in return for the convenience of accessibility and electric power. The site should be chosen and "checked out" both in daylight and at night before the station is established.