The International Year of Astronomy 2009 is a global effort initiated by the International Astronomical Union and UNESCO to help the citizens of the world rediscover their place in the Universe through the day- and night-time sky, and thereby engage a personal sense of wonder and discovery.
The goal of Solar physics Task Group is to help IYA2009 with solar matters. It aims to communicate the link between the Sun and the rest of the Universe, and so the place of solar science in astronomy. Our means are the suggestion, organisation and support of solar related events for IYA2009 and being the reference desk for solar matters. | Taurids 2008 |
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| Written by Confedration of Indian Amateur astronomers | |||||||||||||||||||||||||||||||||
| Wednesday, 07 July 2004 | |||||||||||||||||||||||||||||||||
Southern Taurids (STA)
Northern Taurids (NTA)
These two streams form part of the complex associated with Comet 2P/Encke. Defining their radiants is best achieved by careful visual or telescopic plotting, or imaging recordings, since they are large and diffuse. Each radiant should be considered an oval area of ~ 20° by 10°, α by δ, centred on the radiant position for that date, for shower association. Their activity very clearly dominates the Antihelion Source area's during the northern autumn, so much so that the ANT is considered inactive while they are present. The brightness and relative slowness of many shower meteors makes them ideal targets for still-imaging, while these factors coupled with low, steady, combined Taurid rates makes them excellent subjects for newcomers to practice their plotting techniques on. The activity of both showers produces an apparently plateau-like maximum for about ten days in early November, and they have a reputation for producing some excellently bright fireballs at times, although seemingly not in every year. Studies by David Asher have indicated that increased Taurid fireball rates may result from a 'swarm' of larger particles within the Taurid stream complex, and he suggested such 'swarm' returns might happen in 1995, 1998 and 2005 most recently. In 1995, an impressive crop of bright Taurids occurred between late October to mid November, while in 1998, Taurid ZHRs reached levels comparable to the usual maximum rates in late October, together with an increased flux of brighter Taurids generally. The 2005 event was the most impressive and best-observed yet, with a lot of, occasionally very brilliant, fireballs, and enhanced combined ZHRs of ~ 10 — 15, that persisted from about October 29 to November 10. Another 'swarm' return is predicted for 2008, while late October into early November has a new to first quarter Moon, so all observers should be alert to cover whatever happens (but do remember that nothing is ever guaranteed in meteor astronomy!). The Southern Taurid maximum will have relatively little lunar interference, but the Northern peak falls just a day before full Moon, so will likely be missed this time. The near-ecliptic radiants for both shower branches mean all meteoricists can observe these streams, albeit northern hemisphere observers are somewhat better-placed, as here suitable radiant zenith distances persist for much of the night. Even in the southern hemisphere, a good 3 — 5 hours' watching around local midnight is possible with Taurus well above the horizon, however.
Source :IMO.Net |
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