CRUST
发表于 2025-3-21 19:10:56
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onlooker
发表于 2025-3-21 20:33:02
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thrombus
发表于 2025-3-22 01:52:47
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
不公开
发表于 2025-3-22 06:04:30
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
发表于 2025-3-22 08:56:53
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
发表于 2025-3-22 14:03:09
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
同步信息
发表于 2025-3-22 19:39:43
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木讷
发表于 2025-3-23 00:02:44
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犬儒主义者
发表于 2025-3-23 05:10:54
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Postmenopause
发表于 2025-3-23 06:32:39
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