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Correction to 'Radiation belt electron precipitation by man-made VLF transmissions'

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HAL Id: hal-00383346

https://hal.archives-ouvertes.fr/hal-00383346

Submitted on 10 Apr 2017

HAL is a multi-disciplinary open access archive for the deposit and dissemination of sci- entific research documents, whether they are pub- lished or not. The documents may come from teaching and research institutions in France or abroad, or from public or private research centers.

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Correction to ’Radiation belt electron precipitation by man-made VLF transmissions’

R. Gamble, C.J. Rodger, M.A. Clilverd, J.-A. Sauvaud, N.R. Thomson, S.L.

Stewart, R.J. Mccormick, Michel Parrot, Jean-Jacques Berthelier

To cite this version:

R. Gamble, C.J. Rodger, M.A. Clilverd, J.-A. Sauvaud, N.R. Thomson, et al.. Correction to ’Radiation belt electron precipitation by man-made VLF transmissions’. Journal of Geophysical Research Space Physics, American Geophysical Union/Wiley, 2009, 114 (A5), pp.A05205. �10.1029/2009JA014304�.

�hal-00383346�

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Correction to ‘‘Radiation belt electron precipitation by man-made VLF transmissions’’

Rory J. Gamble, Craig J. Rodger, Mark A. Clilverd, Jean-Andre´ Sauvaud, Neil R. Thomson, S. L. Stewart, Robert J. McCormick, Michel Parrot, and Jean-Jacques Berthelier

Received 27 March 2009; published 8 May 2009.

Citation: Gamble, R. J., C. J. Rodger, M. A. Clilverd, J.-A. Sauvaud, N. R. Thomson, S. L. Stewart, R. J. McCormick, M. Parrot, and J.-J. Berthelier (2009), Correction to ‘‘Radiation belt electron precipitation by man-made VLF transmissions,’’ J. Geophys. Res., 114, A05205, doi:10.1029/2009JA014304.

[

1

] In the paper ‘‘Radiation belt electron precipitation by man-made VLF transmissions’’ by Rory J. Gamble et al.

(Journal of Geophysical Research, 113, A10211,

doi:10.1029/2008JA013369, 2008), Figures 2 and 7 were switched. The correct figures and their captions are shown here.

Figure 2. Typical UT variation in transmissions from the VLF station NWC, received at Dunedin, New Zealand, 21 – 27 August 2005. Nighttimes correspond to the periods with higher amplitudes. This plot presents 1-min average amplitudes, demonstrating the near-constant operation of this transmitter.

JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 114, A05205, doi:10.1029/2009JA014304, 2009

Copyright 2009 by the American Geophysical Union.

0148-0227/09/2009JA014304

A05205 1 of 2

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Figure 7. Variation with L of the first-order cyclotron resonant energy with waves of 19.8 kHz (solid line) and the plasmaspheric electron number density used in this calculation (dashed line). The crosses mark the mean L and energy for typical wisps as described in Table 2.

A05205 GAMBLE ET AL.: CORRECTION

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