The 1999 Quadrantids and the lunar Na atmosphere |
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Authors: | S Verani C Barbieri CR Benn G Cremonese M Mendillo |
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Institution: | 1International Space Science Institute, Hallerstrasse 6, 3012 Bern, Switzerland;2Department of Astronomy, University of Padova, Vic. Osservatorio 2, 35122 Padova, Italy;3Isaac Newton Group, Apartado 321, 38700 Santa Cruz de La Palma, Tenerife, Spain;4Astronomical Observatory of Padova, Vic. Osservatorio 5, 35122 Padova, Italy;5Center for Space Physics, Boston University, Boston, MA 02215, USA |
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Abstract: | Enhancements of the Na emission and temperature from the lunar atmosphere were reported during the Leonid meteor showers of 1995, 1997 and 1998. Here we report a search for similar enhancement during the 1999 Quadrantids, which have the highest mass flux of any of the major streams. No enhancements were detected. We suggest that different chemical–physical properties of the Leonid and Quadrantid streams may be responsible for the difference. |
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Keywords: | meteors meteoroids Moon |
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