By Wing-Huen Ip, Anil Bhardwaj

Advances in Geosciences is the results of a concerted attempt in bringing the most recent effects and making plans actions on the topic of earth and area technological know-how in Asia and the overseas enviornment. the quantity editors are all top scientists of their examine fields overlaying six sections: Hydrological technology (Hs), Planetary technology (Ps), sun Terrestrial (St), strong Earth (Se), Ocean technology (Os) and Atmospheric technological know-how (As). the most objective is to spotlight the clinical concerns necessary to the research of earthquakes, tsunamis, atmospheric dirt storms, weather swap, drought, flood, typhoons, monsoons, area climate, and planetary exploration.

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Thin carbon foil is placed at the entrance of the LEF TOF mass analyzer, which generates start electrons when ions pass through the carbon foil. The start electrons are accelerated by the electric field inside the mass analyzer and their positions are detected by one-dimensional circular resistive anode that is placed behind the MCP. These start electrons also generate start signals when they pass through a May 29, 2007 6:55 spi-b486 AOGS 2006 - PS Volume 40 9in x 6in Y. Saito et al. Fig. 3. Cross section of IEA.

These signals are used as stop signals. The mass/charge of the incident ions can be calculated from its energy/charge and the TOF. Some of the incident ions enter the analyzer as ions. These ions are reflected by the linear electric field whose intensity is proportional to the distance from the entrance point. The reflected ions generate secondary electrons when they collide with the top part of the mass analyzer. These electrons are accelerated and detected by the center anode, which generate the stop signals.

Kuroda, N. Hashimoto, D. Sakai and M. Takahashi, Simulation of the Martian atmosphere using a CCSR/NIES AGCM, J. Meteorol. Soc. Jpn. 83 (2005) 1. 11. A. S. Medvedev and P. Hartogh, Winter polar warmings and the meridional transport on Mars simulated with a general circulation model, Icarus 186 (2007) 97. 12. O. A. Gusev and A. A. Kutepov, Non-LTE gas in planetary atmospheres, in Stellar Atmosphere Modeling, eds. I. Hubeny, D. Mihalas and K. Werner, ASP Conf. Ser. 288 (2003) 318. 13. T. Nakajima and M.

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