posted on 2021-09-29, 13:46authored byMD Campbell-Brown, G Stober, C Jacobi, J Kero, A Kozlovsky, M Lester
The Draconid meteor shower shows strong bursts of activity at irregular intervals, with nearly no activity in intervening years. Five outbursts of the Draconid meteor shower were observed with specular meteor radars in Canada and Europe between 1999 and 2018. The outbursts generally lasted between 6 and 8 h, and most were not fully visible at a single geographical site, emphasizing the need for observations at multiple longitudes for short-duration shower outbursts. There is at least a factor of two difference in the peak flux as measured on different radars; the initial trail radius effect is undercorrected for Draconid meteors, which are known to be fragile.
Funding
Funding for this work was provided through NASA cooperative agreement 80NSSSC18M0046 and the Natural Sciences and Engineering Research Council of Canada (Grant no. RGPIN-2018-05474). The Esrange meteor radar operation, maintenance and data collection is provided by Esrange Space Center of Swedish Space Corporation (SSC). GS is a member of the Oeschger Center for Climate Change Research. The Andenes and Juliusruh meteor radar data were collected under the grant STO 1053/1-1 of the Deutsche Forschungsgemeinschaft (DFG). We thank Jorge L. Chau and R. Latteck for their support of the AHEAD project.
History
Citation
Monthly Notices of the Royal Astronomical Society, Volume 507, Issue 1, October 2021, Pages 852–857, https://doi.org/10.1093/mnras/stab2174
Author affiliation
Department of Physics and Astronomy
Version
VoR (Version of Record)
Published in
Monthly Notices of the Royal Astronomical Society
Volume
507
Issue
1
Pagination
852 - 857
Publisher
Oxford University Press (OUP) for Royal Astronomical Society