Characteristics of Pi 2 magnetic pulsations observed at the CPMN stations: A review of the STEP results
Author:
Publisher
Springer Science and Business Media LLC
Subject
Space and Planetary Science,Geology
Link
http://link.springer.com/content/pdf/10.1186/BF03351695
Reference41 articles.
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2. Chen, L. and A. Hasegawa, A theory of long-period magnetic pulsations, 2, Impulse excitation of surface eigenmode, J. Geophys. Res., 79, 1033–1037, 1974b.
3. Cheng, C.-C., J.-K. Chao, and K. Yumoto, Spectral power of low-latitude Pi 2 pulsations at the 210° magnetic meridian stations and plasmaspheric cavity resonances, Earth Planets Space, 52, 615–627, 2000.
4. Lester, M., H. J. Singer, D. P. Smits, and W. J. Hughes, Pi 2 pulsations and the substorm current wedge: Low-latitude polarization, J. Geophys. Res., 94, 17133–17141, 1989.
5. Li, Y., K. Yumoto, M. Itonaga, M. Shinohara, T.-I. Kitamura, and the 210° MM group, Equatorial Pi 2’s as indicators of substorms and the relation between dayside and nightside Pi 2’s, in SUBSTORMS-4, Edited by S. Kokubun and Y. Kamide, pp. 555–558, Terra Scientific Publ. Comp/Kluwer Academic Publ., 1998a.
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