By R.L. Xu, A.T.Y. Lui
Launches of numerous significant magnetospheric learn satellites (i.e., Polar, Wind, and Interball) set the scene for wide multi-platform investigations of the Earth's plasma setting within the period of the overseas Solar-Terrestrial Physics application. intriguing new effects from this software and the continuing cutting edge advances to medical instrumentation and spacecraft know-how are extremely important for the overseas house group in getting ready for destiny plans within the upcoming new millenium. This quantity is a made from the COSPAR Colloquium held in Beijing on April 15-19, 1996 aimed to consolidate those achievements. It includes state of the art articles within the 4 parts of contemporary magnetospheric strategies, particularly, (1) lively scan in house, (2) leading edge dimension method, (3) multi-point commentary, and (4) numerical simulation and theoretical research. Researchers within the area neighborhood, either beginners and specialists, are anticipated to learn from this selection of articles
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Additional resources for Magnetospheric research with advanced techniques: proceedings of the 9th COSPAR Colloquium held in Beijing, China, 15-19 April, 1996
With UON in coop. with NIPR in coop. with NIPR in coop. with NIPR in coop. with NIPR Abbreviation of Organizations: BO CAMS CRIRP CSSAR IAP IG NIPR PRIC UON Beijing Observatory, Academia Sinica, Beijing 100080 Chinese Academy of Meteorological Sciences, Beijing 100081 China Research Institute of Radiowave Propagation, Xinxiang 453003 Center for Space Science and Applied Research, Academia Sinica, Beijing 100080 Institute of Atmospheric Physics, Academia Sinica, Beijing 100029 Institute of Geophysics, Academia Sinica, Beijing 100101 National Institute of Polar Research, Japan Polar Research Institute of China, Shanghai 200129 University of Newcastle, Australia Most of the measurement instruments in Table 1 are used in regular observation and long-term monitoring.
1993) and Doke et al. (1994). For the easy reference we briefly describe the principal features of the instrument: HEP-LD is an advanced energetic particle spectrometer with time-of-flight(T) and energy(E) detection systems which determine the mass of incident nuclear particles. The novel design of the sensor head as a 'projection' camera allows the linear imaging of particle distributions in the polar angle (reference axis is the satellite spin vector pointing approximately towards ecliptic north): Twelve contiguous angular intervals over a range of 180 ~ Combined with the sectored spin plane of the spacecraft the unit sphere in phase space is covered with a total of 192 contiguous angular pixels (the satellite spin rate is 20 rpm).
Ilb. The plasma conditions at ISEE 2 from 0840 to 1018 UT on April 22, 1979. From top to bottom this figure shows the plasma velocity toward and away from the Earth; the number density; the ratio of the maximum to minimum ion temperature in one spin of the spacecraft, the average ion temperature and the plasma thermal and magnetic pressures, and their sum. 0 m =.. 0 08:40 09:00 09:20 09:40 10:00 Universal Time 79 Apr 22 THE HARRIS C U R R E N T SHEET S T R U C T U R E The Harris model is a simple analytical description of a one-dimensional current sheet model and is self-consistent using either MHD or kinetic theory.