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Science, 1980 Some of the next articles are maybe not open access.
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Terrestrial Magnetism and Atmospheric Electricity, 1948
In a recent paper, “Critical Survey of Recent Theoretical Work on the Ionosphere” by Pande [Terr. Mag., 52, 375–396 (1947)], the author discusses a number of the many papers dealing with the temperature of the upper atmosphere. He indicates that a good deal of confusion exists regarding the meaning of the word temperature in this case.
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In a recent paper, “Critical Survey of Recent Theoretical Work on the Ionosphere” by Pande [Terr. Mag., 52, 375–396 (1947)], the author discusses a number of the many papers dealing with the temperature of the upper atmosphere. He indicates that a good deal of confusion exists regarding the meaning of the word temperature in this case.
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2012
The momentum equation of the ion species j moving in a plasma in the presence of an electric (E) and a magnetic (B) field can be expressed as: $$ \rho j \frac{d {\mathbf{v}_{j}}}{dt} = -\nabla\,p_{j}\,+\, \rho_{j}\mathbf{g}\,+ \frac{q_{j}\rho_{j}}{m_{j}}(\mathbf{E}\,+\,\mathbf{v}_{j} \times \mathbf{B}) - \sum\limits_{k j\neq k}\rho_{j}\nu_{j}k ...
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The momentum equation of the ion species j moving in a plasma in the presence of an electric (E) and a magnetic (B) field can be expressed as: $$ \rho j \frac{d {\mathbf{v}_{j}}}{dt} = -\nabla\,p_{j}\,+\, \rho_{j}\mathbf{g}\,+ \frac{q_{j}\rho_{j}}{m_{j}}(\mathbf{E}\,+\,\mathbf{v}_{j} \times \mathbf{B}) - \sum\limits_{k j\neq k}\rho_{j}\nu_{j}k ...
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1971
The ionosphere begins at an altitude of about 50 km and extends to beyond 1000 km. It is formed by interactions between the components of the atmosphere and the solar radiation. Let us begin by examining the characteristics of the latter. We shall then consider the various processes it causes and their consequences with regard to the Earth’s atmosphere.
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The ionosphere begins at an altitude of about 50 km and extends to beyond 1000 km. It is formed by interactions between the components of the atmosphere and the solar radiation. Let us begin by examining the characteristics of the latter. We shall then consider the various processes it causes and their consequences with regard to the Earth’s atmosphere.
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