狮子王辛巴的荣耀

寒流袭击的那天,没有冬天的广州突然出奇的寒冷。面对中国百年不遇的寒冷天气,我选择了逃离。连续飞行了14小时,穿越了5个时区,我降落在南半球被阳光燃烧着的肯尼亚首都内罗毕(NAIROBI)。我和一个中国人以及两个法国人,带上本地的黑人司机、厨师和充足的食品、水以及扎营设备,开着那辆带天窗的专业狩猎远征(SAFARI)越野车,做一次彻底的狩猎远征。     

伊朗 谜一样的国度

电视中,每天都有关于伊朗的报道,伴随美国要打击伊朗的叫嚣,让人有种大战迫在眉睫的紧张。我唯恐伊朗再不去,这个国家就会像伊拉克一样,彻底改变当今的面貌。于是在好友的帮助下,展开了这次向往已久的伊朗之行。     

Bow shock: Power aspects

It is clear that the primary energy source for magnetospheric processes is the solar wind, but the process of energy transfer from the solar wind into the magnetosphere, or rather, to convecting magnetospheric plasma, appears to be rather complicated. Bow shock is a powerful transformer of the solar wind kinetic energy into the gas dynamic and electromagnetic energy. A jump of the magnetic field tangential component at front crossing means that the front carries an electric current. The solar wind kinetic energy partly transforms to gas kinetic and electromagnetic energy during its passage through the bow shock front. The transition layer (magnetosheath) can use part of this energy for accelerating of plasma, but can conversely spend part its kinetic energy on the electric power generation, which afterwards may be used by the magnetosphere. Thereby, transition layer can be both consumer (sink) and generator (source) of electric power depending upon special conditions. The direction of the current behind the bow shock front depends on the sign of the IMF Bz-component. It is this electric current which sets convection of plasma in motion.     

From the Solar Wind to the Magnetospheric Substorm

This paper gives a brief outline of the progression from the first substorm model developed in Ref.[4] and[8] based on Kennel's ideas[3], to the present views about the mechanism by which solar wind kinetic energy is converted to electromagnetic energy at the Bow Shock and by which this energy is transferred to the magnetosphere in the form of current; about the transformation of the energy of this current to gas kinetic energy of convecting plasma tubes, and, finally, the back transformation of gas kinetic energy to electromagnetic energy in secondary magnetospheric MHD generators. The questions of the formation of the magnetospheric convection system, the nature of substorm break-up, and of the matching of currents in the magnetosphere-ionosphere system are discussed.