Physics
Scientific paper
Feb 1999
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999jimo...27...30l&link_type=abstract
WGN, Journal of the International Meteor Organization, vol. 27, no. 1, p. 30-32
Physics
2
Scientific paper
Following a prominent activity peak of bright meteors peaking about 0.75 days earlier, the Leonid outburst recurrence of 1998 displayed a second pronounced activity peak in the hours around passage through the node of parent comet 55P/Tempel-Tuttle on November 17.82. Here, we report preliminary video results from two observational networks established in China by the 1998 Sino-Dutch Leonid Expedition. The results suggest that two separate activity structures might have been responsible for the short-lived activity around nodal passage: a B=5 background peaking near 19h20m UT (lambda=235.260, eq. 2000.0) and a B=30 narrow structure peaking near 20h40m UT (lambda=235.316). These come in addition to the broader structure that produced the fireball activity on November 16-17. The two structures near nodal passage appear similar in shape and equivalent width (but not in activity level) to the two structures in the historic 1866 storm display.
de Lignie Marc
Langbroek Marco
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