Titlebook: High-Latitude Space Plasma Physics; Bengt Hultqvist,Tor Hagfors Book 1983 Springer Science+Business Media New York 1983 Plasma.earth.plane

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書(shū)目名稱High-Latitude Space Plasma Physics影響因子(影響力)




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onlooker

thrombus

The Role of the Auroral Ionosphere in Magnetospheric Substormsects such as the strengthening of electrojets and the motion and intensification of auroral forms were central elements in the development of the concept of the substorm (see, e.g., Akasofu, 1968). The purpose of this paper is not to discuss the obvious ionospheric manifestations of a substorm. Inst

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Characteristics of the Polar Cap at Ionospheric Levels and Present Understanding of the Physical Proents between various authors concerning these systems is given. In particular is attention focused on the relationship between the interplanetary magnetic field and the various current systems proposed. A short presentation is also given of the various techniques used in deriving the polar cap E-fie

Firefly

The Low Altitude Cleft: Plasma Entry and Magnetospheric Topologyr the confirmation of “relatively uninhibited access” of magnetosheath plasma to the earth’s magnetosphere, in a region referred to as the polar cusp, we can pose the following question. Have we advanced our knowledge of the detailed access mechanism and place of entry of solar wind plasma into the

才能

Incoherent-Scatter Radar Measurements of Electric Field and Plasma in the Auroral Ionosphererties of the auroral-zone ionosphere. This paper summarizes Chatanika radar measurements of electric fields and currents, and their relation to E-region ionization and conductivity. Several outstanding questions are discussed that pertain to electric-field coupling between the ionosphere and magneto

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木訥

犬儒主義者

Postmenopause

Dependence of the High-Latitude Ionospheric Fields and Plasma Characteristics on the Properties of ty (1961), the interplanetary magnetic field (IMF) modulated the transfer of energy from the solar wind to the magnetosphere. In particular, it was evident that the transfer function for the solar-terrestrial interaction was dependent on the direction of the IMF with respect to magnetopause field lin