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Corrigendum to "Geotail observations of temperature anisotropy of the two-component protons in the dusk plasma sheet" published in Ann. Geophys., 25, 769?777, 2007

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HAL Id: hal-00318329

https://hal.archives-ouvertes.fr/hal-00318329

Submitted on 29 Jun 2007

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Corrigendum to ”Geotail observations of temperature

anisotropy of the two-component protons in the dusk

plasma sheet” published in Ann. Geophys., 25, 769?777,

2007

M. N. Nishino, M. Fujimoto, T. Terasawa, G. Ueno, K. Maezawa, T. Mukai,

Y. Saito

To cite this version:

M. N. Nishino, M. Fujimoto, T. Terasawa, G. Ueno, K. Maezawa, et al.. Corrigendum to ”Geotail observations of temperature anisotropy of the two-component protons in the dusk plasma sheet” published in Ann. Geophys., 25, 769?777, 2007. Annales Geophysicae, European Geosciences Union, 2007, 25 (6), pp.1233-1233. �hal-00318329�

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Ann. Geophys., 25, 1233, 2007 www.ann-geophys.net/25/1233/2007/ © European Geosciences Union 2007

Annales

Geophysicae

Corrigendum to

“Geotail observations of temperature anisotropy of the

two-component protons in the dusk plasma sheet” published in

Ann. Geophys., 25, 769–777, 2007

M. N. Nishino1, M. Fujimoto1, T. Terasawa2, G. Ueno3, K. Maezawa1, T. Mukai4, and Y. Saito1 1ISAS/JAXA, Kanagawa 229-8510, Japan

2Tokyo Institute of Technology, Tokyo 152-8551, Japan 3Institute of Statistical Mathematics, Tokyo 106-8569, Japan 4JAXA, Tokyo 100-8260, Japan

By accident, Fig. 4 of the mentioned paper contains an error. In the fourth panel from the top, which shows the per-pendicular and parallel temperatures of the hot proton com-ponent, the values on the vertical axis was half as high as the correct ones. Figure 4 should be replaced, although de-scriptions of the hot component temperatures in the text were correct.

The postal code of ISAS/JAXA, which some of the authors belong to, should be corrected to 229-8510.

Correspondence to: M. N. Nishino (nishino@stp.isas.jaxa.jp)

Fig. 4. The upper panel shows the Geotail observations between

07:40–08:00 UT on 23 September 1995, in the same format as Fig 2. The lower panel shows a cut of ion phase space density for the 12-s interval 07:43:40–07:43:52 UT.

Figure

Fig. 4. The upper panel shows the Geotail observations between 07:40–08:00 UT on 23 September 1995, in the same format as Fig 2.

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