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Corrigendum to "Development of the mesospheric Na layer at 69 degrees N during the Geminids meteor shower 2010", published in Ann.Geophys., 31, 61-73, 2013

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Ann. Geophys., 33, 197, 2015 www.ann-geophys.net/33/197/2015/

doi:10.5194/angeo-33-197-2015

© Author(s) 2015. CC Attribution 3.0 License.

Corrigendum to

“Development of the mesospheric Na layer at 69 N during the Geminids meteor shower 2010”, published in Ann. Geophys., 31, 61–73, 2013

T. Dunker1, U.-P. Hoppe1, G. Stober2, and M. Rapp3

1Department of Physics and Technology, University of Tromsø – The Arctic University of Norway, 9037 Tromsø, Norway

2Leibniz-Institute of Atmospheric Physics e.V. at the University Rostock, Schlossstraße 6, 18225 Ostseebad Kühlungsborn, Germany

3German Aerospace Center (DLR), Institute of Atmospheric Physics, Münchner Straße 20, 82234 Oberpfaffenhofen-Wessling, Germany

Correspondence to: T. Dunker ([email protected])

0 10 20 30

1.5 2.0 2.5 3.0 3.5 4.0 4.5

0 10 20 30

Day of December 2010 1.5

2.0 2.5 3.0 3.5 4.0 4.5

Normalized number [1013 ]

Na column density MSP column density Sporadic meteor echoes

Figure 10. Comparison of sporadic meteor echoes (blue dash-dot line), Na column density (black asterisks; error bars indicate the standard deviation of the geophysical variability), and MSP col- umn (red diamonds) in December 2010. Theyaxis is correct for Na column density in m−2. The values must be multiplied by 1.51×10−2for absolute MSP column density. The values multi- plied by 2.5×10−10give the correct number of observed sporadic meteor echoes. The number of meteor echoes on 17 to 19 December is interpolated, because the radar was out of order on these days.

Due to a programming error, all sodium column densities given in Dunker et al. (2013) are systematically too small by exactly 1.5. Data from each day are affected equally by this error. The reported daily median Na column densities in Ta- ble 3, as well as the tick marks of Figs. 3, 4, 5, 7, and 8, must be multiplied by 1.5. We provide the corrected Fig. 10 here together with the normalization values. On average, there were∼66 free Na atoms per meteoric smoke particle.

This correction is important only and alone when compar- ing the absolute Na column density values in Dunker et al.

(2013) with other absolute Na column densities. Other state- ments and conclusions by Dunker et al. (2013) remain un- changed.

References

Dunker, T., Hoppe, U.-P., Stober, G., and Rapp, M.: Development of the mesospheric Na layer at 69N during the Geminids meteor shower 2010, Ann. Geophys., 31, 61–73, doi:10.5194/angeo-31- 61-2013, 2013.

Published by Copernicus Publications on behalf of the European Geosciences Union.

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