By Wing-huen Ip
"Advances in Geosciences" is the results of a concerted attempt in bringing the most recent effects and making plans actions concerning earth and area technological know-how in Asia and the overseas area. the quantity editors are all top scientists of their learn fields masking 5 sections: strong Earth (SE), sun Terrestrial (ST), Planetary technology (PS), Hydrological technology (HS), and Oceans and Atmospheres (OA). the most function is to spotlight the clinical concerns necessary to the research of earthquakes, tsunamis, weather switch, drought, flood, typhoons, area weathers, and planetary exploration.
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Extra resources for Advanced in Geoscience, V3: Planetary Science(Ps) (2006)(en)(416s)
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Fraction of Mercury’s surface that is characterized by open magnetic ﬁeld lines, mapping on the dayside magnetopause, as calculated by means of both the T96* (left panels) and the TH93* (right panels) models. Upper panels: open ﬁeld area as a function of the IMF Bz component, for ﬁxed solar wind pressure (Pdyn = 20 nPa): the black lines mark the IMF B = (0, 0, Bz ) conﬁgurations, while the gray lines show the results obtained with the IMF aligned along the nominal Parker’s spiral direction (TH93* only, since T96* is independent from Bx ).
P. T. Newell, Y. I. Feldstein, Y. I. -I. Meng, J. Geophys. Res. 101 (1996) 10,737. 13. K. Seki, N. Terada, D. C. Delcourt and T. Ogino (abstract), SGEPSS, Kyoto, Japan (2005). 14. G. L. Siscoe, N. F. Ness and C. M. Yeates, J. Geophys. Res. 80 (1975) 4359. 15. J. G. Luhmann, C. T. Russell and N. A. Tsyganenko, J. Geophys. Res. 103 (1998) 9113. 16. -H. Ip, Adv. Space Res. 19 (1997) 1615. 17. D. C. Delcourt, K. Seki, N. Terada and Y. Miyoshi, Annales Geophys. 24 (2006). 18. D. C. Delcourt, K. Seki, N.
Advanced in Geoscience, V3: Planetary Science(Ps) (2006)(en)(416s) by Wing-huen Ip